@@ -359,10 +359,12 class JROData(GenericData): | |||
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359 | 359 | class Voltage(JROData): |
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360 | 360 | |
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361 | 361 | # data es un numpy array de 2 dmensiones (canales, alturas) |
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362 | data = None | |
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363 |
data |
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364 |
data |
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365 |
data |
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362 | data = None | |
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363 | dataPP_POW = None | |
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364 | dataPP_DOP = None | |
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365 | dataPP_WIDTH = None | |
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366 | dataPP_SNR = None | |
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367 | ||
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366 | 368 | def __init__(self): |
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367 | 369 | ''' |
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368 | 370 | Constructor |
@@ -421,6 +423,35 class Voltage(JROData): | |||
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421 | 423 | |
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422 | 424 | return noise |
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423 | 425 | |
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426 | def getNoisebyHildebrandDC(self, channel=None,DC=0): | |
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427 | """ | |
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428 | Determino el nivel de ruido usando el metodo Hildebrand-Sekhon | |
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429 | ||
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430 | Return: | |
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431 | noiselevel | |
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432 | """ | |
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433 | ||
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434 | if channel != None: | |
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435 | data = self.data[channel]-DC | |
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436 | nChannels = 1 | |
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437 | else: | |
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438 | data = self.data | |
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439 | nChannels = self.nChannels | |
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440 | ||
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441 | noise = numpy.zeros(nChannels) | |
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442 | power = data * numpy.conjugate(data) | |
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443 | ||
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444 | for thisChannel in range(nChannels): | |
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445 | if nChannels == 1: | |
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446 | daux = power[:].real | |
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447 | else: | |
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448 | daux = power[thisChannel, :].real | |
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449 | noise[thisChannel] = hildebrand_sekhon(daux, self.nCohInt) | |
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450 | ||
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451 | return noise | |
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452 | ||
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453 | ||
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454 | ||
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424 | 455 | def getNoise(self, type=1, channel=None): |
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425 | 456 | |
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426 | 457 | if type == 1: |
@@ -1262,15 +1293,19 class PlotterData(object): | |||
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1262 | 1293 | self.flagDataAsBlock = dataOut.flagDataAsBlock |
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1263 | 1294 | self.nProfiles = dataOut.nProfiles |
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1264 | 1295 | if plot == 'pp_power': |
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1265 |
buffer = dataOut.data |
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1296 | buffer = dataOut.dataPP_POWER | |
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1297 | self.flagDataAsBlock = dataOut.flagDataAsBlock | |
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1298 | self.nProfiles = dataOut.nProfiles | |
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1299 | if plot == 'pp_signal': | |
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1300 | buffer = dataOut.dataPP_POW | |
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1266 | 1301 | self.flagDataAsBlock = dataOut.flagDataAsBlock |
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1267 | 1302 | self.nProfiles = dataOut.nProfiles |
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1268 | 1303 | if plot == 'pp_velocity': |
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1269 |
buffer = dataOut.data |
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1304 | buffer = dataOut.dataPP_DOP | |
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1270 | 1305 | self.flagDataAsBlock = dataOut.flagDataAsBlock |
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1271 | 1306 | self.nProfiles = dataOut.nProfiles |
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1272 | 1307 | if plot == 'pp_specwidth': |
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1273 |
buffer = dataOut.data |
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1308 | buffer = dataOut.dataPP_WIDTH | |
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1274 | 1309 | self.flagDataAsBlock = dataOut.flagDataAsBlock |
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1275 | 1310 | self.nProfiles = dataOut.nProfiles |
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1276 | 1311 |
@@ -156,6 +156,8 class ScopePlot(Plot): | |||
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156 | 156 | thisDatetime = datetime.datetime.utcfromtimestamp(self.data.times[-1]) |
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157 | 157 | if self.CODE == "pp_power": |
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158 | 158 | scope = self.data['pp_power'] |
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159 | elif self.CODE == "pp_signal": | |
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160 | scope = self.data["pp_signal"] | |
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159 | 161 | elif self.CODE == "pp_velocity": |
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160 | 162 | scope = self.data["pp_velocity"] |
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161 | 163 | elif self.CODE == "pp_specwidth": |
@@ -191,6 +193,13 class ScopePlot(Plot): | |||
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191 | 193 | thisDatetime, |
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192 | 194 | wintitle |
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193 | 195 | ) |
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196 | if self.CODE=="pp_signal": | |
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197 | self.plot_weatherpower(self.data.heights, | |
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198 | scope[:,i,:], | |
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199 | channels, | |
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200 | thisDatetime, | |
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201 | wintitle | |
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202 | ) | |
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194 | 203 | if self.CODE=="pp_velocity": |
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195 | 204 | self.plot_weathervelocity(scope[:,i,:], |
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196 | 205 | self.data.heights, |
@@ -230,6 +239,13 class ScopePlot(Plot): | |||
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230 | 239 | thisDatetime, |
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231 | 240 | wintitle |
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232 | 241 | ) |
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242 | if self.CODE=="pp_signal": | |
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243 | self.plot_weatherpower(self.data.heights, | |
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244 | scope, | |
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245 | channels, | |
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246 | thisDatetime, | |
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247 | wintitle | |
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248 | ) | |
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233 | 249 | if self.CODE=="pp_velocity": |
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234 | 250 | self.plot_weathervelocity(scope, |
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235 | 251 | self.data.heights, |
@@ -249,7 +265,7 class ScopePlot(Plot): | |||
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249 | 265 | |
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250 | 266 | class PulsepairPowerPlot(ScopePlot): |
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251 | 267 | ''' |
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252 | Plot for | |
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268 | Plot for P= S+N | |
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253 | 269 | ''' |
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254 | 270 | |
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255 | 271 | CODE = 'pp_power' |
@@ -259,7 +275,7 class PulsepairPowerPlot(ScopePlot): | |||
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259 | 275 | |
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260 | 276 | class PulsepairVelocityPlot(ScopePlot): |
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261 | 277 | ''' |
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262 | Plot for | |
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278 | Plot for VELOCITY | |
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263 | 279 | ''' |
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264 | 280 | CODE = 'pp_velocity' |
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265 | 281 | plot_name = 'PulsepairVelocity' |
@@ -268,9 +284,19 class PulsepairVelocityPlot(ScopePlot): | |||
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268 | 284 | |
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269 | 285 | class PulsepairSpecwidthPlot(ScopePlot): |
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270 | 286 | ''' |
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271 | Plot for | |
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287 | Plot for WIDTH | |
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272 | 288 | ''' |
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273 | 289 | CODE = 'pp_specwidth' |
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274 | 290 | plot_name = 'PulsepairSpecwidth' |
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275 | 291 | plot_type = 'scatter' |
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276 | 292 | buffering = False |
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293 | ||
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294 | class PulsepairSignalPlot(ScopePlot): | |
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295 | ''' | |
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296 | Plot for S | |
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297 | ''' | |
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298 | ||
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299 | CODE = 'pp_signal' | |
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300 | plot_name = 'PulsepairSignal' | |
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301 | plot_type = 'scatter' | |
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302 | buffering = False |
@@ -360,21 +360,27 class SimulatorReader(JRODataReader, ProcessingUnit): | |||
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360 | 360 | fd = Fdoppler #+(600.0/120)*self.nReadBlocks |
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361 | 361 | d_signal = Adoppler*numpy.array(numpy.exp(1.0j*2.0*math.pi*fd*time_vec),dtype=numpy.complex64) |
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362 | 362 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·SeΓ±al con ancho espectralΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· |
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363 | #specw_sig = numpy.linspace(-149,150,300) | |
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364 | #w = 8 | |
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365 | #A = 20 | |
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366 | #specw_sig = specw_sig/w | |
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367 | #specw_sig = numpy.sinc(specw_sig) | |
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368 | #specw_sig = A*numpy.array(specw_sig,dtype=numpy.complex64) | |
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363 | if prof_gen%2==0: | |
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364 | min = int(prof_gen/2.0-1.0) | |
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365 | max = int(prof_gen/2.0) | |
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366 | else: | |
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367 | min = int(prof_gen/2.0) | |
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368 | max = int(prof_gen/2.0) | |
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369 | specw_sig = numpy.linspace(-min,max,prof_gen) | |
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370 | w = 4 | |
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371 | A = 20 | |
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372 | specw_sig = specw_sig/w | |
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373 | specw_sig = numpy.sinc(specw_sig) | |
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374 | specw_sig = A*numpy.array(specw_sig,dtype=numpy.complex64) | |
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369 | 375 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· DATABLOCK + DOPPLERΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· |
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370 | 376 | HD=int(Hdoppler/self.AcqDH_0) |
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371 | 377 | for i in range(12): |
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372 | 378 | self.datablock[0,:,HD+i]=self.datablock[0,:,HD+i]+ d_signal# RESULT |
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373 | 379 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· DATABLOCK + DOPPLER*Sinc(x)Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· |
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374 |
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375 |
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376 |
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377 |
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380 | HD=int(Hdoppler/self.AcqDH_0) | |
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381 | HD=int(HD/2) | |
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382 | for i in range(12): | |
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383 | self.datablock[0,:,HD+i]=self.datablock[0,:,HD+i]+ specw_sig*d_signal# RESULT | |
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378 | 384 | |
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379 | 385 | def readBlock(self): |
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380 | 386 | |
@@ -421,7 +427,8 class SimulatorReader(JRODataReader, ProcessingUnit): | |||
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421 | 427 | FixPP_CohInt= 1,Tau_0= 250,AcqH0_0 = 70 ,AcqDH_0=1.25, Bauds= 32, |
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422 | 428 | FixRCP_TXA = 40, FixRCP_TXB = 50, fAngle = 2.0*math.pi*(1/16),DC_level= 50, |
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423 | 429 | stdev= 8,Num_Codes = 1 , Dyn_snCode = None, samples=200, |
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424 |
channels=2,Fdoppler=20,Hdoppler=36,Adoppler=500, |
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430 | channels=2,Fdoppler=20,Hdoppler=36,Adoppler=500, | |
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431 | profilesPerBlock=300,dataBlocksPerFile=120,nTotalReadFiles=10000, | |
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425 | 432 | **kwargs): |
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426 | 433 | |
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427 | 434 | self.set_kwargs(**kwargs) |
@@ -447,14 +454,14 class SimulatorReader(JRODataReader, ProcessingUnit): | |||
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447 | 454 | codeType=0, nCode=Num_Codes, nBaud=32, code=Dyn_snCode, |
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448 | 455 | flip1=0, flip2=0,Taus=Tau_0) |
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449 | 456 | |
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450 |
self.set_PH(dtype=0, blockSize=0, profilesPerBlock= |
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451 |
dataBlocksPerFile= |
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457 | self.set_PH(dtype=0, blockSize=0, profilesPerBlock=profilesPerBlock, | |
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458 | dataBlocksPerFile=dataBlocksPerFile, nWindows=1, processFlags=numpy.array([1024]), nCohInt=1, | |
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452 | 459 | nIncohInt=1, totalSpectra=0, nHeights=samples, firstHeight=AcqH0_0, |
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453 | 460 | deltaHeight=AcqDH_0, samplesWin=samples, spectraComb=0, nCode=0, |
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454 | 461 | code=0, nBaud=None, shif_fft=False, flag_dc=False, |
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455 | 462 | flag_cspc=False, flag_decode=False, flag_deflip=False) |
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456 | 463 | |
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457 |
self.set_SH(nSamples=samples, nProfiles= |
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464 | self.set_SH(nSamples=samples, nProfiles=profilesPerBlock, nChannels=channels) | |
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458 | 465 | |
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459 | 466 | self.readFirstHeader() |
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460 | 467 |
This diff has been collapsed as it changes many lines, (2143 lines changed) Show them Hide them | |||
@@ -8,12 +8,12 import copy | |||
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8 | 8 |
import sys |
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9 | 9 |
import importlib |
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10 | 10 |
import itertools |
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11 |
from multiprocessing import Pool, TimeoutError |
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11 | from multiprocessing import Pool, TimeoutError | |
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12 | 12 |
from multiprocessing.pool import ThreadPool |
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13 | 13 |
import time |
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14 | 14 | |
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15 | 15 |
from scipy.optimize import fmin_l_bfgs_b #optimize with bounds on state papameters |
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16 |
from .jroproc_base import ProcessingUnit, Operation, MPDecorator |
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16 | from .jroproc_base import ProcessingUnit, Operation, MPDecorator | |
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17 | 17 |
from schainpy.model.data.jrodata import Parameters, hildebrand_sekhon |
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18 | 18 |
from scipy import asarray as ar,exp |
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19 | 19 |
from scipy.optimize import curve_fit |
@@ -48,13 +48,13 def _unpickle_method(func_name, obj, cls): | |||
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48 | 48 | |
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49 | 49 | |
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50 | 50 |
class ParametersProc(ProcessingUnit): |
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51 | ||
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51 | ||
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52 | 52 |
METHODS = {} |
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53 | 53 |
nSeconds = None |
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54 | 54 | |
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55 | 55 |
def __init__(self): |
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56 | 56 |
ProcessingUnit.__init__(self) |
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57 | ||
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57 | ||
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58 | 58 |
# self.objectDict = {} |
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59 | 59 |
self.buffer = None |
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60 | 60 |
self.firstdatatime = None |
@@ -63,14 +63,14 class ParametersProc(ProcessingUnit): | |||
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63 | 63 |
self.setupReq = False #Agregar a todas las unidades de proc |
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64 | 64 | |
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65 | 65 |
def __updateObjFromInput(self): |
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66 | ||
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66 | ||
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67 | 67 |
self.dataOut.inputUnit = self.dataIn.type |
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68 | ||
|
68 | ||
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69 | 69 |
self.dataOut.timeZone = self.dataIn.timeZone |
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70 | 70 |
self.dataOut.dstFlag = self.dataIn.dstFlag |
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71 | 71 |
self.dataOut.errorCount = self.dataIn.errorCount |
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72 | 72 |
self.dataOut.useLocalTime = self.dataIn.useLocalTime |
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73 | ||
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73 | ||
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74 | 74 |
self.dataOut.radarControllerHeaderObj = self.dataIn.radarControllerHeaderObj.copy() |
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75 | 75 |
self.dataOut.systemHeaderObj = self.dataIn.systemHeaderObj.copy() |
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76 | 76 |
self.dataOut.channelList = self.dataIn.channelList |
@@ -92,27 +92,43 class ParametersProc(ProcessingUnit): | |||
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92 | 92 |
self.dataOut.ippSeconds = self.dataIn.ippSeconds |
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93 | 93 |
# self.dataOut.windowOfFilter = self.dataIn.windowOfFilter |
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94 | 94 |
self.dataOut.timeInterval1 = self.dataIn.timeInterval |
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95 |
self.dataOut.heightList = self.dataIn.getHeiRange() |
|
|
95 | self.dataOut.heightList = self.dataIn.getHeiRange() | |
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96 | 96 |
self.dataOut.frequency = self.dataIn.frequency |
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97 | 97 |
# self.dataOut.noise = self.dataIn.noise |
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98 | ||
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98 | ||
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99 | 99 |
def run(self): |
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100 | 100 | |
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101 | 101 | |
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102 | 102 | |
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103 | 103 |
#---------------------- Voltage Data --------------------------- |
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104 | ||
|
104 | ||
|
105 | 105 |
if self.dataIn.type == "Voltage": |
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106 | 106 | |
|
107 | 107 |
self.__updateObjFromInput() |
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108 | 108 |
self.dataOut.data_pre = self.dataIn.data.copy() |
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109 | 109 |
self.dataOut.flagNoData = False |
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110 | 110 |
self.dataOut.utctimeInit = self.dataIn.utctime |
|
111 | self.dataOut.paramInterval = self.dataIn.nProfiles*self.dataIn.nCohInt*self.dataIn.ippSeconds | |
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111 | ||
|
112 | self.dataOut.paramInterval = self.dataIn.nProfiles*self.dataIn.nCohInt*self.dataIn.ippSeconds | |
|
113 | if hasattr(self.dataIn, 'dataPP_POW'): | |
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114 | self.dataOut.dataPP_POW = self.dataIn.dataPP_POW | |
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115 | ||
|
116 | if hasattr(self.dataIn, 'dataPP_POWER'): | |
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117 | self.dataOut.dataPP_POWER = self.dataIn.dataPP_POWER | |
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118 | ||
|
119 | if hasattr(self.dataIn, 'dataPP_DOP'): | |
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120 | self.dataOut.dataPP_DOP = self.dataIn.dataPP_DOP | |
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121 | ||
|
122 | if hasattr(self.dataIn, 'dataPP_SNR'): | |
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123 | self.dataOut.dataPP_SNR = self.dataIn.dataPP_SNR | |
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124 | ||
|
125 | if hasattr(self.dataIn, 'dataPP_WIDTH'): | |
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126 | self.dataOut.dataPP_WIDTH = self.dataIn.dataPP_WIDTH | |
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127 | ||
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112 | 128 |
return |
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113 | ||
|
129 | ||
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114 | 130 |
#---------------------- Spectra Data --------------------------- |
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115 | ||
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131 | ||
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116 | 132 |
if self.dataIn.type == "Spectra": |
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117 | 133 | |
|
118 | 134 |
self.dataOut.data_pre = (self.dataIn.data_spc, self.dataIn.data_cspc) |
@@ -126,243 +142,243 class ParametersProc(ProcessingUnit): | |||
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126 | 142 |
self.dataOut.spc_noise = self.dataIn.getNoise() |
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127 | 143 |
self.dataOut.spc_range = (self.dataIn.getFreqRange(1) , self.dataIn.getAcfRange(1) , self.dataIn.getVelRange(1)) |
|
128 | 144 |
# self.dataOut.normFactor = self.dataIn.normFactor |
|
129 |
self.dataOut.pairsList = self.dataIn.pairsList |
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|
145 | self.dataOut.pairsList = self.dataIn.pairsList | |
|
130 | 146 |
self.dataOut.groupList = self.dataIn.pairsList |
|
131 |
self.dataOut.flagNoData = False |
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|
132 | ||
|
147 | self.dataOut.flagNoData = False | |
|
148 | ||
|
133 | 149 |
if hasattr(self.dataIn, 'ChanDist'): #Distances of receiver channels |
|
134 | 150 |
self.dataOut.ChanDist = self.dataIn.ChanDist |
|
135 |
else: self.dataOut.ChanDist = None |
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|
136 | ||
|
151 | else: self.dataOut.ChanDist = None | |
|
152 | ||
|
137 | 153 |
#if hasattr(self.dataIn, 'VelRange'): #Velocities range |
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138 | 154 |
# self.dataOut.VelRange = self.dataIn.VelRange |
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139 | 155 |
#else: self.dataOut.VelRange = None |
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140 | ||
|
156 | ||
|
141 | 157 |
if hasattr(self.dataIn, 'RadarConst'): #Radar Constant |
|
142 | 158 |
self.dataOut.RadarConst = self.dataIn.RadarConst |
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143 | ||
|
159 | ||
|
144 | 160 |
if hasattr(self.dataIn, 'NPW'): #NPW |
|
145 | 161 |
self.dataOut.NPW = self.dataIn.NPW |
|
146 | ||
|
162 | ||
|
147 | 163 |
if hasattr(self.dataIn, 'COFA'): #COFA |
|
148 | 164 |
self.dataOut.COFA = self.dataIn.COFA |
|
149 | ||
|
150 | ||
|
151 | ||
|
165 | ||
|
166 | ||
|
167 | ||
|
152 | 168 |
#---------------------- Correlation Data --------------------------- |
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153 | ||
|
169 | ||
|
154 | 170 |
if self.dataIn.type == "Correlation": |
|
155 | 171 |
acf_ind, ccf_ind, acf_pairs, ccf_pairs, data_acf, data_ccf = self.dataIn.splitFunctions() |
|
156 | ||
|
172 | ||
|
157 | 173 |
self.dataOut.data_pre = (self.dataIn.data_cf[acf_ind,:], self.dataIn.data_cf[ccf_ind,:,:]) |
|
158 | 174 |
self.dataOut.normFactor = (self.dataIn.normFactor[acf_ind,:], self.dataIn.normFactor[ccf_ind,:]) |
|
159 | 175 |
self.dataOut.groupList = (acf_pairs, ccf_pairs) |
|
160 | ||
|
176 | ||
|
161 | 177 |
self.dataOut.abscissaList = self.dataIn.lagRange |
|
162 | 178 |
self.dataOut.noise = self.dataIn.noise |
|
163 | 179 |
self.dataOut.data_SNR = self.dataIn.SNR |
|
164 | 180 |
self.dataOut.flagNoData = False |
|
165 | 181 |
self.dataOut.nAvg = self.dataIn.nAvg |
|
166 | ||
|
182 | ||
|
167 | 183 |
#---------------------- Parameters Data --------------------------- |
|
168 | ||
|
184 | ||
|
169 | 185 |
if self.dataIn.type == "Parameters": |
|
170 | 186 |
self.dataOut.copy(self.dataIn) |
|
171 | 187 |
self.dataOut.flagNoData = False |
|
172 | ||
|
188 | ||
|
173 | 189 |
return True |
|
174 | ||
|
190 | ||
|
175 | 191 |
self.__updateObjFromInput() |
|
176 | 192 |
self.dataOut.utctimeInit = self.dataIn.utctime |
|
177 | 193 |
self.dataOut.paramInterval = self.dataIn.timeInterval |
|
178 | ||
|
194 | ||
|
179 | 195 |
return |
|
180 | 196 | |
|
181 | 197 | |
|
182 | 198 |
def target(tups): |
|
183 | ||
|
199 | ||
|
184 | 200 |
obj, args = tups |
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185 | ||
|
201 | ||
|
186 | 202 |
return obj.FitGau(args) |
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187 | ||
|
188 | ||
|
203 | ||
|
204 | ||
|
189 | 205 |
class SpectralFilters(Operation): |
|
190 | ||
|
206 | ||
|
191 | 207 |
'''This class allows the Rainfall / Wind Selection for CLAIRE RADAR |
|
192 | ||
|
208 | ||
|
193 | 209 |
LimitR : It is the limit in m/s of Rainfall |
|
194 | 210 |
LimitW : It is the limit in m/s for Winds |
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195 | ||
|
211 | ||
|
196 | 212 |
Input: |
|
197 | ||
|
213 | ||
|
198 | 214 |
self.dataOut.data_pre : SPC and CSPC |
|
199 | 215 |
self.dataOut.spc_range : To select wind and rainfall velocities |
|
200 | ||
|
216 | ||
|
201 | 217 |
Affected: |
|
202 | ||
|
218 | ||
|
203 | 219 |
self.dataOut.data_pre : It is used for the new SPC and CSPC ranges of wind |
|
204 |
self.dataOut.spcparam_range : Used in SpcParamPlot |
|
|
220 | self.dataOut.spcparam_range : Used in SpcParamPlot | |
|
205 | 221 |
self.dataOut.SPCparam : Used in PrecipitationProc |
|
206 | ||
|
207 | ||
|
222 | ||
|
223 | ||
|
208 | 224 |
''' |
|
209 | ||
|
225 | ||
|
210 | 226 |
def __init__(self): |
|
211 | 227 |
Operation.__init__(self) |
|
212 | 228 |
self.i=0 |
|
213 | ||
|
214 |
def run(self, dataOut, PositiveLimit=1.5, NegativeLimit=2.5): |
|
|
215 | ||
|
216 | ||
|
217 |
#Limite de vientos |
|
|
229 | ||
|
230 | def run(self, dataOut, PositiveLimit=1.5, NegativeLimit=2.5): | |
|
231 | ||
|
232 | ||
|
233 | #Limite de vientos | |
|
218 | 234 |
LimitR = PositiveLimit |
|
219 | 235 |
LimitN = NegativeLimit |
|
220 | ||
|
236 | ||
|
221 | 237 |
self.spc = dataOut.data_pre[0].copy() |
|
222 | 238 |
self.cspc = dataOut.data_pre[1].copy() |
|
223 | ||
|
239 | ||
|
224 | 240 |
self.Num_Hei = self.spc.shape[2] |
|
225 | 241 |
self.Num_Bin = self.spc.shape[1] |
|
226 | 242 |
self.Num_Chn = self.spc.shape[0] |
|
227 | ||
|
243 | ||
|
228 | 244 |
VelRange = dataOut.spc_range[2] |
|
229 | 245 |
TimeRange = dataOut.spc_range[1] |
|
230 | 246 |
FrecRange = dataOut.spc_range[0] |
|
231 | ||
|
247 | ||
|
232 | 248 |
Vmax= 2*numpy.max(dataOut.spc_range[2]) |
|
233 | 249 |
Tmax= 2*numpy.max(dataOut.spc_range[1]) |
|
234 | 250 |
Fmax= 2*numpy.max(dataOut.spc_range[0]) |
|
235 | ||
|
251 | ||
|
236 | 252 |
Breaker1R=VelRange[numpy.abs(VelRange-(-LimitN)).argmin()] |
|
237 | 253 |
Breaker1R=numpy.where(VelRange == Breaker1R) |
|
238 | ||
|
239 |
Delta = self.Num_Bin/2 - Breaker1R[0] |
|
|
240 | ||
|
241 | ||
|
254 | ||
|
255 | Delta = self.Num_Bin/2 - Breaker1R[0] | |
|
256 | ||
|
257 | ||
|
242 | 258 |
'''Reacomodando SPCrange''' |
|
243 | 259 | |
|
244 | 260 |
VelRange=numpy.roll(VelRange,-(int(self.Num_Bin/2)) ,axis=0) |
|
245 | ||
|
261 | ||
|
246 | 262 |
VelRange[-(int(self.Num_Bin/2)):]+= Vmax |
|
247 | ||
|
263 | ||
|
248 | 264 |
FrecRange=numpy.roll(FrecRange,-(int(self.Num_Bin/2)),axis=0) |
|
249 | ||
|
265 | ||
|
250 | 266 |
FrecRange[-(int(self.Num_Bin/2)):]+= Fmax |
|
251 | ||
|
267 | ||
|
252 | 268 |
TimeRange=numpy.roll(TimeRange,-(int(self.Num_Bin/2)),axis=0) |
|
253 | ||
|
269 | ||
|
254 | 270 |
TimeRange[-(int(self.Num_Bin/2)):]+= Tmax |
|
255 | ||
|
271 | ||
|
256 | 272 |
''' ------------------ ''' |
|
257 | ||
|
273 | ||
|
258 | 274 |
Breaker2R=VelRange[numpy.abs(VelRange-(LimitR)).argmin()] |
|
259 | 275 |
Breaker2R=numpy.where(VelRange == Breaker2R) |
|
260 | ||
|
261 | ||
|
276 | ||
|
277 | ||
|
262 | 278 |
SPCroll = numpy.roll(self.spc,-(int(self.Num_Bin/2)) ,axis=1) |
|
263 | ||
|
279 | ||
|
264 | 280 |
SPCcut = SPCroll.copy() |
|
265 | 281 |
for i in range(self.Num_Chn): |
|
266 | ||
|
282 | ||
|
267 | 283 |
SPCcut[i,0:int(Breaker2R[0]),:] = dataOut.noise[i] |
|
268 | 284 |
SPCcut[i,-int(Delta):,:] = dataOut.noise[i] |
|
269 | ||
|
285 | ||
|
270 | 286 |
SPCcut[i]=SPCcut[i]- dataOut.noise[i] |
|
271 | 287 |
SPCcut[ numpy.where( SPCcut<0 ) ] = 1e-20 |
|
272 | ||
|
288 | ||
|
273 | 289 |
SPCroll[i]=SPCroll[i]-dataOut.noise[i] |
|
274 | 290 |
SPCroll[ numpy.where( SPCroll<0 ) ] = 1e-20 |
|
275 | ||
|
291 | ||
|
276 | 292 |
SPC_ch1 = SPCroll |
|
277 | ||
|
293 | ||
|
278 | 294 |
SPC_ch2 = SPCcut |
|
279 | ||
|
295 | ||
|
280 | 296 |
SPCparam = (SPC_ch1, SPC_ch2, self.spc) |
|
281 |
dataOut.SPCparam = numpy.asarray(SPCparam) |
|
|
282 | ||
|
283 | ||
|
297 | dataOut.SPCparam = numpy.asarray(SPCparam) | |
|
298 | ||
|
299 | ||
|
284 | 300 |
dataOut.spcparam_range=numpy.zeros([self.Num_Chn,self.Num_Bin+1]) |
|
285 | ||
|
301 | ||
|
286 | 302 |
dataOut.spcparam_range[2]=VelRange |
|
287 | 303 |
dataOut.spcparam_range[1]=TimeRange |
|
288 | 304 |
dataOut.spcparam_range[0]=FrecRange |
|
289 | 305 |
return dataOut |
|
290 | ||
|
306 | ||
|
291 | 307 |
class GaussianFit(Operation): |
|
292 | ||
|
308 | ||
|
293 | 309 |
''' |
|
294 |
Function that fit of one and two generalized gaussians (gg) based |
|
|
295 |
on the PSD shape across an "power band" identified from a cumsum of |
|
|
310 | Function that fit of one and two generalized gaussians (gg) based | |
|
311 | on the PSD shape across an "power band" identified from a cumsum of | |
|
296 | 312 |
the measured spectrum - noise. |
|
297 | ||
|
313 | ||
|
298 | 314 |
Input: |
|
299 | 315 |
self.dataOut.data_pre : SelfSpectra |
|
300 | ||
|
316 | ||
|
301 | 317 |
Output: |
|
302 | 318 |
self.dataOut.SPCparam : SPC_ch1, SPC_ch2 |
|
303 | ||
|
319 | ||
|
304 | 320 |
''' |
|
305 | 321 |
def __init__(self): |
|
306 | 322 |
Operation.__init__(self) |
|
307 | 323 |
self.i=0 |
|
308 | ||
|
309 | ||
|
324 | ||
|
325 | ||
|
310 | 326 |
def run(self, dataOut, num_intg=7, pnoise=1., SNRlimit=-9): #num_intg: Incoherent integrations, pnoise: Noise, vel_arr: range of velocities, similar to the ftt points |
|
311 | 327 |
"""This routine will find a couple of generalized Gaussians to a power spectrum |
|
312 | 328 |
input: spc |
|
313 | 329 |
output: |
|
314 | 330 |
Amplitude0,shift0,width0,p0,Amplitude1,shift1,width1,p1,noise |
|
315 | 331 |
""" |
|
316 | ||
|
332 | ||
|
317 | 333 |
self.spc = dataOut.data_pre[0].copy() |
|
318 | 334 |
self.Num_Hei = self.spc.shape[2] |
|
319 | 335 |
self.Num_Bin = self.spc.shape[1] |
|
320 | 336 |
self.Num_Chn = self.spc.shape[0] |
|
321 | 337 |
Vrange = dataOut.abscissaList |
|
322 | ||
|
338 | ||
|
323 | 339 |
GauSPC = numpy.empty([self.Num_Chn,self.Num_Bin,self.Num_Hei]) |
|
324 | 340 |
SPC_ch1 = numpy.empty([self.Num_Bin,self.Num_Hei]) |
|
325 | 341 |
SPC_ch2 = numpy.empty([self.Num_Bin,self.Num_Hei]) |
|
326 | 342 |
SPC_ch1[:] = numpy.NaN |
|
327 | 343 |
SPC_ch2[:] = numpy.NaN |
|
328 | 344 | |
|
329 | ||
|
345 | ||
|
330 | 346 |
start_time = time.time() |
|
331 | ||
|
347 | ||
|
332 | 348 |
noise_ = dataOut.spc_noise[0].copy() |
|
333 | ||
|
334 | ||
|
335 |
pool = Pool(processes=self.Num_Chn) |
|
|
349 | ||
|
350 | ||
|
351 | pool = Pool(processes=self.Num_Chn) | |
|
336 | 352 |
args = [(Vrange, Ch, pnoise, noise_, num_intg, SNRlimit) for Ch in range(self.Num_Chn)] |
|
337 |
objs = [self for __ in range(self.Num_Chn)] |
|
|
338 |
attrs = list(zip(objs, args)) |
|
|
353 | objs = [self for __ in range(self.Num_Chn)] | |
|
354 | attrs = list(zip(objs, args)) | |
|
339 | 355 |
gauSPC = pool.map(target, attrs) |
|
340 | 356 |
dataOut.SPCparam = numpy.asarray(SPCparam) |
|
341 | ||
|
357 | ||
|
342 | 358 |
''' Parameters: |
|
343 | 359 |
1. Amplitude |
|
344 | 360 |
2. Shift |
|
345 | 361 |
3. Width |
|
346 | 362 |
4. Power |
|
347 | 363 |
''' |
|
348 | ||
|
364 | ||
|
349 | 365 |
def FitGau(self, X): |
|
350 | ||
|
366 | ||
|
351 | 367 |
Vrange, ch, pnoise, noise_, num_intg, SNRlimit = X |
|
352 | ||
|
368 | ||
|
353 | 369 |
SPCparam = [] |
|
354 | 370 |
SPC_ch1 = numpy.empty([self.Num_Bin,self.Num_Hei]) |
|
355 | 371 |
SPC_ch2 = numpy.empty([self.Num_Bin,self.Num_Hei]) |
|
356 | 372 |
SPC_ch1[:] = 0#numpy.NaN |
|
357 | 373 |
SPC_ch2[:] = 0#numpy.NaN |
|
358 | ||
|
359 | ||
|
360 | ||
|
374 | ||
|
375 | ||
|
376 | ||
|
361 | 377 |
for ht in range(self.Num_Hei): |
|
362 | ||
|
363 | ||
|
378 | ||
|
379 | ||
|
364 | 380 |
spc = numpy.asarray(self.spc)[ch,:,ht] |
|
365 | ||
|
381 | ||
|
366 | 382 |
############################################# |
|
367 | 383 |
# normalizing spc and noise |
|
368 | 384 |
# This part differs from gg1 |
@@ -370,60 +386,60 class GaussianFit(Operation): | |||
|
370 | 386 |
#spc = spc / spc_norm_max |
|
371 | 387 |
pnoise = pnoise #/ spc_norm_max |
|
372 | 388 |
############################################# |
|
373 | ||
|
389 | ||
|
374 | 390 |
fatspectra=1.0 |
|
375 | ||
|
391 | ||
|
376 | 392 |
wnoise = noise_ #/ spc_norm_max |
|
377 | 393 |
#wnoise,stdv,i_max,index =enoise(spc,num_intg) #noise estimate using Hildebrand Sekhon, only wnoise is used |
|
378 |
#if wnoise>1.1*pnoise: # to be tested later |
|
|
394 | #if wnoise>1.1*pnoise: # to be tested later | |
|
379 | 395 |
# wnoise=pnoise |
|
380 |
noisebl=wnoise*0.9; |
|
|
396 | noisebl=wnoise*0.9; | |
|
381 | 397 |
noisebh=wnoise*1.1 |
|
382 | 398 |
spc=spc-wnoise |
|
383 | ||
|
399 | ||
|
384 | 400 |
minx=numpy.argmin(spc) |
|
385 |
#spcs=spc.copy() |
|
|
401 | #spcs=spc.copy() | |
|
386 | 402 |
spcs=numpy.roll(spc,-minx) |
|
387 | 403 |
cum=numpy.cumsum(spcs) |
|
388 | 404 |
tot_noise=wnoise * self.Num_Bin #64; |
|
389 | ||
|
405 | ||
|
390 | 406 |
snr = sum(spcs)/tot_noise |
|
391 | 407 |
snrdB=10.*numpy.log10(snr) |
|
392 | ||
|
408 | ||
|
393 | 409 |
if snrdB < SNRlimit : |
|
394 | 410 |
snr = numpy.NaN |
|
395 | 411 |
SPC_ch1[:,ht] = 0#numpy.NaN |
|
396 | 412 |
SPC_ch1[:,ht] = 0#numpy.NaN |
|
397 | 413 |
SPCparam = (SPC_ch1,SPC_ch2) |
|
398 | 414 |
continue |
|
399 | ||
|
400 | ||
|
415 | ||
|
416 | ||
|
401 | 417 |
#if snrdB<-18 or numpy.isnan(snrdB) or num_intg<4: |
|
402 | 418 |
# return [None,]*4,[None,]*4,None,snrdB,None,None,[None,]*5,[None,]*9,None |
|
403 | ||
|
404 |
cummax=max(cum); |
|
|
419 | ||
|
420 | cummax=max(cum); | |
|
405 | 421 |
epsi=0.08*fatspectra # cumsum to narrow down the energy region |
|
406 |
cumlo=cummax*epsi; |
|
|
422 | cumlo=cummax*epsi; | |
|
407 | 423 |
cumhi=cummax*(1-epsi) |
|
408 | 424 |
powerindex=numpy.array(numpy.where(numpy.logical_and(cum>cumlo, cum<cumhi))[0]) |
|
409 | ||
|
410 | ||
|
425 | ||
|
426 | ||
|
411 | 427 |
if len(powerindex) < 1:# case for powerindex 0 |
|
412 | 428 |
continue |
|
413 | 429 |
powerlo=powerindex[0] |
|
414 | 430 |
powerhi=powerindex[-1] |
|
415 | 431 |
powerwidth=powerhi-powerlo |
|
416 | ||
|
432 | ||
|
417 | 433 |
firstpeak=powerlo+powerwidth/10.# first gaussian energy location |
|
418 | 434 |
secondpeak=powerhi-powerwidth/10.#second gaussian energy location |
|
419 | 435 |
midpeak=(firstpeak+secondpeak)/2. |
|
420 | 436 |
firstamp=spcs[int(firstpeak)] |
|
421 | 437 |
secondamp=spcs[int(secondpeak)] |
|
422 | 438 |
midamp=spcs[int(midpeak)] |
|
423 | ||
|
439 | ||
|
424 | 440 |
x=numpy.arange( self.Num_Bin ) |
|
425 | 441 |
y_data=spc+wnoise |
|
426 | ||
|
442 | ||
|
427 | 443 |
''' single Gaussian ''' |
|
428 | 444 |
shift0=numpy.mod(midpeak+minx, self.Num_Bin ) |
|
429 | 445 |
width0=powerwidth/4.#Initialization entire power of spectrum divided by 4 |
@@ -432,10 +448,10 class GaussianFit(Operation): | |||
|
432 | 448 |
state0=[shift0,width0,amplitude0,power0,wnoise] |
|
433 | 449 |
bnds=(( 0,(self.Num_Bin-1) ),(1,powerwidth),(0,None),(0.5,3.),(noisebl,noisebh)) |
|
434 | 450 |
lsq1=fmin_l_bfgs_b(self.misfit1,state0,args=(y_data,x,num_intg),bounds=bnds,approx_grad=True) |
|
435 | ||
|
436 | chiSq1=lsq1[1]; | |
|
437 | 451 | |
|
438 |
|
|
|
452 | chiSq1=lsq1[1]; | |
|
453 | ||
|
454 | ||
|
439 | 455 |
if fatspectra<1.0 and powerwidth<4: |
|
440 | 456 |
choice=0 |
|
441 | 457 |
Amplitude0=lsq1[0][2] |
@@ -449,31 +465,31 class GaussianFit(Operation): | |||
|
449 | 465 |
noise=lsq1[0][4] |
|
450 | 466 |
#return (numpy.array([shift0,width0,Amplitude0,p0]), |
|
451 | 467 |
# numpy.array([shift1,width1,Amplitude1,p1]),noise,snrdB,chiSq1,6.,sigmas1,[None,]*9,choice) |
|
452 | ||
|
468 | ||
|
453 | 469 |
''' two gaussians ''' |
|
454 | 470 |
#shift0=numpy.mod(firstpeak+minx,64); shift1=numpy.mod(secondpeak+minx,64) |
|
455 |
shift0=numpy.mod(firstpeak+minx, self.Num_Bin ); |
|
|
471 | shift0=numpy.mod(firstpeak+minx, self.Num_Bin ); | |
|
456 | 472 |
shift1=numpy.mod(secondpeak+minx, self.Num_Bin ) |
|
457 |
width0=powerwidth/6.; |
|
|
473 | width0=powerwidth/6.; | |
|
458 | 474 |
width1=width0 |
|
459 |
power0=2.; |
|
|
475 | power0=2.; | |
|
460 | 476 |
power1=power0 |
|
461 |
amplitude0=firstamp; |
|
|
477 | amplitude0=firstamp; | |
|
462 | 478 |
amplitude1=secondamp |
|
463 | 479 |
state0=[shift0,width0,amplitude0,power0,shift1,width1,amplitude1,power1,wnoise] |
|
464 | 480 |
#bnds=((0,63),(1,powerwidth/2.),(0,None),(0.5,3.),(0,63),(1,powerwidth/2.),(0,None),(0.5,3.),(noisebl,noisebh)) |
|
465 | 481 |
bnds=(( 0,(self.Num_Bin-1) ),(1,powerwidth/2.),(0,None),(0.5,3.),( 0,(self.Num_Bin-1)),(1,powerwidth/2.),(0,None),(0.5,3.),(noisebl,noisebh)) |
|
466 | 482 |
#bnds=(( 0,(self.Num_Bin-1) ),(1,powerwidth/2.),(0,None),(0.5,3.),( 0,(self.Num_Bin-1)),(1,powerwidth/2.),(0,None),(0.5,3.),(0.1,0.5)) |
|
467 | ||
|
483 | ||
|
468 | 484 |
lsq2 = fmin_l_bfgs_b( self.misfit2 , state0 , args=(y_data,x,num_intg) , bounds=bnds , approx_grad=True ) |
|
469 | ||
|
470 | ||
|
471 |
chiSq2=lsq2[1]; |
|
|
472 | ||
|
473 | ||
|
474 | ||
|
485 | ||
|
486 | ||
|
487 | chiSq2=lsq2[1]; | |
|
488 | ||
|
489 | ||
|
490 | ||
|
475 | 491 |
oneG=(chiSq1<5 and chiSq1/chiSq2<2.0) and (abs(lsq2[0][0]-lsq2[0][4])<(lsq2[0][1]+lsq2[0][5])/3. or abs(lsq2[0][0]-lsq2[0][4])<10) |
|
476 | ||
|
492 | ||
|
477 | 493 |
if snrdB>-12: # when SNR is strong pick the peak with least shift (LOS velocity) error |
|
478 | 494 |
if oneG: |
|
479 | 495 |
choice=0 |
@@ -481,10 +497,10 class GaussianFit(Operation): | |||
|
481 | 497 |
w1=lsq2[0][1]; w2=lsq2[0][5] |
|
482 | 498 |
a1=lsq2[0][2]; a2=lsq2[0][6] |
|
483 | 499 |
p1=lsq2[0][3]; p2=lsq2[0][7] |
|
484 |
s1=(2**(1+1./p1))*scipy.special.gamma(1./p1)/p1; |
|
|
500 | s1=(2**(1+1./p1))*scipy.special.gamma(1./p1)/p1; | |
|
485 | 501 |
s2=(2**(1+1./p2))*scipy.special.gamma(1./p2)/p2; |
|
486 | 502 |
gp1=a1*w1*s1; gp2=a2*w2*s2 # power content of each ggaussian with proper p scaling |
|
487 | ||
|
503 | ||
|
488 | 504 |
if gp1>gp2: |
|
489 | 505 |
if a1>0.7*a2: |
|
490 | 506 |
choice=1 |
@@ -499,157 +515,157 class GaussianFit(Operation): | |||
|
499 | 515 |
choice=numpy.argmax([a1,a2])+1 |
|
500 | 516 |
#else: |
|
501 | 517 |
#choice=argmin([std2a,std2b])+1 |
|
502 | ||
|
518 | ||
|
503 | 519 |
else: # with low SNR go to the most energetic peak |
|
504 | 520 |
choice=numpy.argmax([lsq1[0][2]*lsq1[0][1],lsq2[0][2]*lsq2[0][1],lsq2[0][6]*lsq2[0][5]]) |
|
505 | ||
|
506 | ||
|
507 |
shift0=lsq2[0][0]; |
|
|
521 | ||
|
522 | ||
|
523 | shift0=lsq2[0][0]; | |
|
508 | 524 |
vel0=Vrange[0] + shift0*(Vrange[1]-Vrange[0]) |
|
509 |
shift1=lsq2[0][4]; |
|
|
525 | shift1=lsq2[0][4]; | |
|
510 | 526 |
vel1=Vrange[0] + shift1*(Vrange[1]-Vrange[0]) |
|
511 | ||
|
527 | ||
|
512 | 528 |
max_vel = 1.0 |
|
513 | ||
|
529 | ||
|
514 | 530 |
#first peak will be 0, second peak will be 1 |
|
515 | 531 |
if vel0 > -1.0 and vel0 < max_vel : #first peak is in the correct range |
|
516 | 532 |
shift0=lsq2[0][0] |
|
517 | 533 |
width0=lsq2[0][1] |
|
518 | 534 |
Amplitude0=lsq2[0][2] |
|
519 | 535 |
p0=lsq2[0][3] |
|
520 | ||
|
536 | ||
|
521 | 537 |
shift1=lsq2[0][4] |
|
522 | 538 |
width1=lsq2[0][5] |
|
523 | 539 |
Amplitude1=lsq2[0][6] |
|
524 | 540 |
p1=lsq2[0][7] |
|
525 |
noise=lsq2[0][8] |
|
|
541 | noise=lsq2[0][8] | |
|
526 | 542 |
else: |
|
527 | 543 |
shift1=lsq2[0][0] |
|
528 | 544 |
width1=lsq2[0][1] |
|
529 | 545 |
Amplitude1=lsq2[0][2] |
|
530 | 546 |
p1=lsq2[0][3] |
|
531 | ||
|
547 | ||
|
532 | 548 |
shift0=lsq2[0][4] |
|
533 | 549 |
width0=lsq2[0][5] |
|
534 | 550 |
Amplitude0=lsq2[0][6] |
|
535 |
p0=lsq2[0][7] |
|
|
536 |
noise=lsq2[0][8] |
|
|
537 | ||
|
551 | p0=lsq2[0][7] | |
|
552 | noise=lsq2[0][8] | |
|
553 | ||
|
538 | 554 |
if Amplitude0<0.05: # in case the peak is noise |
|
539 |
shift0,width0,Amplitude0,p0 = [0,0,0,0]#4*[numpy.NaN] |
|
|
555 | shift0,width0,Amplitude0,p0 = [0,0,0,0]#4*[numpy.NaN] | |
|
540 | 556 |
if Amplitude1<0.05: |
|
541 |
shift1,width1,Amplitude1,p1 = [0,0,0,0]#4*[numpy.NaN] |
|
|
542 | ||
|
543 | ||
|
557 | shift1,width1,Amplitude1,p1 = [0,0,0,0]#4*[numpy.NaN] | |
|
558 | ||
|
559 | ||
|
544 | 560 |
SPC_ch1[:,ht] = noise + Amplitude0*numpy.exp(-0.5*(abs(x-shift0))/width0)**p0 |
|
545 | 561 |
SPC_ch2[:,ht] = noise + Amplitude1*numpy.exp(-0.5*(abs(x-shift1))/width1)**p1 |
|
546 | 562 |
SPCparam = (SPC_ch1,SPC_ch2) |
|
547 | ||
|
548 | ||
|
563 | ||
|
564 | ||
|
549 | 565 |
return GauSPC |
|
550 | ||
|
566 | ||
|
551 | 567 |
def y_model1(self,x,state): |
|
552 | 568 |
shift0,width0,amplitude0,power0,noise=state |
|
553 | 569 |
model0=amplitude0*numpy.exp(-0.5*abs((x-shift0)/width0)**power0) |
|
554 | ||
|
570 | ||
|
555 | 571 |
model0u=amplitude0*numpy.exp(-0.5*abs((x-shift0- self.Num_Bin )/width0)**power0) |
|
556 | ||
|
572 | ||
|
557 | 573 |
model0d=amplitude0*numpy.exp(-0.5*abs((x-shift0+ self.Num_Bin )/width0)**power0) |
|
558 | 574 |
return model0+model0u+model0d+noise |
|
559 | ||
|
560 |
def y_model2(self,x,state): #Equation for two generalized Gaussians with Nyquist |
|
|
575 | ||
|
576 | def y_model2(self,x,state): #Equation for two generalized Gaussians with Nyquist | |
|
561 | 577 |
shift0,width0,amplitude0,power0,shift1,width1,amplitude1,power1,noise=state |
|
562 | 578 |
model0=amplitude0*numpy.exp(-0.5*abs((x-shift0)/width0)**power0) |
|
563 | ||
|
579 | ||
|
564 | 580 |
model0u=amplitude0*numpy.exp(-0.5*abs((x-shift0- self.Num_Bin )/width0)**power0) |
|
565 | ||
|
581 | ||
|
566 | 582 |
model0d=amplitude0*numpy.exp(-0.5*abs((x-shift0+ self.Num_Bin )/width0)**power0) |
|
567 | 583 |
model1=amplitude1*numpy.exp(-0.5*abs((x-shift1)/width1)**power1) |
|
568 | ||
|
584 | ||
|
569 | 585 |
model1u=amplitude1*numpy.exp(-0.5*abs((x-shift1- self.Num_Bin )/width1)**power1) |
|
570 | ||
|
586 | ||
|
571 | 587 |
model1d=amplitude1*numpy.exp(-0.5*abs((x-shift1+ self.Num_Bin )/width1)**power1) |
|
572 | 588 |
return model0+model0u+model0d+model1+model1u+model1d+noise |
|
573 | ||
|
574 |
def misfit1(self,state,y_data,x,num_intg): # This function compares how close real data is with the model data, the close it is, the better it is. |
|
|
589 | ||
|
590 | def misfit1(self,state,y_data,x,num_intg): # This function compares how close real data is with the model data, the close it is, the better it is. | |
|
575 | 591 | |
|
576 | 592 |
return num_intg*sum((numpy.log(y_data)-numpy.log(self.y_model1(x,state)))**2)#/(64-5.) # /(64-5.) can be commented |
|
577 | ||
|
593 | ||
|
578 | 594 |
def misfit2(self,state,y_data,x,num_intg): |
|
579 | 595 |
return num_intg*sum((numpy.log(y_data)-numpy.log(self.y_model2(x,state)))**2)#/(64-9.) |
|
580 | ||
|
581 | ||
|
596 | ||
|
597 | ||
|
582 | 598 | |
|
583 | 599 |
class PrecipitationProc(Operation): |
|
584 | ||
|
600 | ||
|
585 | 601 |
''' |
|
586 | 602 |
Operator that estimates Reflectivity factor (Z), and estimates rainfall Rate (R) |
|
587 | ||
|
588 |
Input: |
|
|
603 | ||
|
604 | Input: | |
|
589 | 605 |
self.dataOut.data_pre : SelfSpectra |
|
590 | ||
|
591 |
Output: |
|
|
592 | ||
|
593 |
self.dataOut.data_output : Reflectivity factor, rainfall Rate |
|
|
594 | ||
|
595 | ||
|
596 |
Parameters affected: |
|
|
606 | ||
|
607 | Output: | |
|
608 | ||
|
609 | self.dataOut.data_output : Reflectivity factor, rainfall Rate | |
|
610 | ||
|
611 | ||
|
612 | Parameters affected: | |
|
597 | 613 |
''' |
|
598 | ||
|
614 | ||
|
599 | 615 |
def __init__(self): |
|
600 | 616 |
Operation.__init__(self) |
|
601 | 617 |
self.i=0 |
|
602 | ||
|
603 | ||
|
618 | ||
|
619 | ||
|
604 | 620 |
def gaus(self,xSamples,Amp,Mu,Sigma): |
|
605 | 621 |
return ( Amp / ((2*numpy.pi)**0.5 * Sigma) ) * numpy.exp( -( xSamples - Mu )**2 / ( 2 * (Sigma**2) )) |
|
606 | ||
|
607 | ||
|
608 | ||
|
622 | ||
|
623 | ||
|
624 | ||
|
609 | 625 |
def Moments(self, ySamples, xSamples): |
|
610 | 626 |
Pot = numpy.nansum( ySamples ) # Potencia, momento 0 |
|
611 | 627 |
yNorm = ySamples / Pot |
|
612 | ||
|
628 | ||
|
613 | 629 |
Vr = numpy.nansum( yNorm * xSamples ) # Velocidad radial, mu, corrimiento doppler, primer momento |
|
614 |
Sigma2 = abs(numpy.nansum( yNorm * ( xSamples - Vr )**2 )) # Segundo Momento |
|
|
630 | Sigma2 = abs(numpy.nansum( yNorm * ( xSamples - Vr )**2 )) # Segundo Momento | |
|
615 | 631 |
Desv = Sigma2**0.5 # Desv. Estandar, Ancho espectral |
|
616 | ||
|
617 |
return numpy.array([Pot, Vr, Desv]) |
|
|
618 | ||
|
619 |
def run(self, dataOut, radar=None, Pt=5000, Gt=295.1209, Gr=70.7945, Lambda=0.6741, aL=2.5118, |
|
|
632 | ||
|
633 | return numpy.array([Pot, Vr, Desv]) | |
|
634 | ||
|
635 | def run(self, dataOut, radar=None, Pt=5000, Gt=295.1209, Gr=70.7945, Lambda=0.6741, aL=2.5118, | |
|
620 | 636 |
tauW=4e-06, ThetaT=0.1656317, ThetaR=0.36774087, Km = 0.93, Altitude=3350): |
|
621 | ||
|
622 | ||
|
637 | ||
|
638 | ||
|
623 | 639 |
Velrange = dataOut.spcparam_range[2] |
|
624 | 640 |
FrecRange = dataOut.spcparam_range[0] |
|
625 | ||
|
641 | ||
|
626 | 642 |
dV= Velrange[1]-Velrange[0] |
|
627 | 643 |
dF= FrecRange[1]-FrecRange[0] |
|
628 | ||
|
644 | ||
|
629 | 645 |
if radar == "MIRA35C" : |
|
630 | ||
|
646 | ||
|
631 | 647 |
self.spc = dataOut.data_pre[0].copy() |
|
632 | 648 |
self.Num_Hei = self.spc.shape[2] |
|
633 | 649 |
self.Num_Bin = self.spc.shape[1] |
|
634 | 650 |
self.Num_Chn = self.spc.shape[0] |
|
635 | 651 |
Ze = self.dBZeMODE2(dataOut) |
|
636 | ||
|
652 | ||
|
637 | 653 |
else: |
|
638 | ||
|
654 | ||
|
639 | 655 |
self.spc = dataOut.SPCparam[1].copy() #dataOut.data_pre[0].copy() # |
|
640 | ||
|
656 | ||
|
641 | 657 |
"""NOTA SE DEBE REMOVER EL RANGO DEL PULSO TX""" |
|
642 | ||
|
643 |
self.spc[:,:,0:7]= numpy.NaN |
|
|
644 | ||
|
658 | ||
|
659 | self.spc[:,:,0:7]= numpy.NaN | |
|
660 | ||
|
645 | 661 |
"""##########################################""" |
|
646 | ||
|
662 | ||
|
647 | 663 |
self.Num_Hei = self.spc.shape[2] |
|
648 | 664 |
self.Num_Bin = self.spc.shape[1] |
|
649 | 665 |
self.Num_Chn = self.spc.shape[0] |
|
650 | ||
|
666 | ||
|
651 | 667 |
''' Se obtiene la constante del RADAR ''' |
|
652 | ||
|
668 | ||
|
653 | 669 |
self.Pt = Pt |
|
654 | 670 |
self.Gt = Gt |
|
655 | 671 |
self.Gr = Gr |
@@ -658,30 +674,30 class PrecipitationProc(Operation): | |||
|
658 | 674 |
self.tauW = tauW |
|
659 | 675 |
self.ThetaT = ThetaT |
|
660 | 676 |
self.ThetaR = ThetaR |
|
661 | ||
|
677 | ||
|
662 | 678 |
Numerator = ( (4*numpy.pi)**3 * aL**2 * 16 * numpy.log(2) ) |
|
663 | 679 |
Denominator = ( Pt * Gt * Gr * Lambda**2 * SPEED_OF_LIGHT * tauW * numpy.pi * ThetaT * ThetaR) |
|
664 | 680 |
RadarConstant = 10e-26 * Numerator / Denominator # |
|
665 | ||
|
681 | ||
|
666 | 682 |
''' ============================= ''' |
|
667 | ||
|
668 |
self.spc[0] = (self.spc[0]-dataOut.noise[0]) |
|
|
669 |
self.spc[1] = (self.spc[1]-dataOut.noise[1]) |
|
|
670 |
self.spc[2] = (self.spc[2]-dataOut.noise[2]) |
|
|
671 | ||
|
683 | ||
|
684 | self.spc[0] = (self.spc[0]-dataOut.noise[0]) | |
|
685 | self.spc[1] = (self.spc[1]-dataOut.noise[1]) | |
|
686 | self.spc[2] = (self.spc[2]-dataOut.noise[2]) | |
|
687 | ||
|
672 | 688 |
self.spc[ numpy.where(self.spc < 0)] = 0 |
|
673 | ||
|
674 |
SPCmean = (numpy.mean(self.spc,0) - numpy.mean(dataOut.noise)) |
|
|
689 | ||
|
690 | SPCmean = (numpy.mean(self.spc,0) - numpy.mean(dataOut.noise)) | |
|
675 | 691 |
SPCmean[ numpy.where(SPCmean < 0)] = 0 |
|
676 | ||
|
692 | ||
|
677 | 693 |
ETAn = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
|
678 | 694 |
ETAv = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
|
679 | 695 |
ETAd = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
|
680 | ||
|
696 | ||
|
681 | 697 |
Pr = SPCmean[:,:] |
|
682 | ||
|
698 | ||
|
683 | 699 |
VelMeteoro = numpy.mean(SPCmean,axis=0) |
|
684 | ||
|
700 | ||
|
685 | 701 |
D_range = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
|
686 | 702 |
SIGMA = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
|
687 | 703 |
N_dist = numpy.zeros([self.Num_Bin,self.Num_Hei]) |
@@ -690,102 +706,102 class PrecipitationProc(Operation): | |||
|
690 | 706 |
Z = numpy.zeros(self.Num_Hei) |
|
691 | 707 |
Ze = numpy.zeros(self.Num_Hei) |
|
692 | 708 |
RR = numpy.zeros(self.Num_Hei) |
|
693 | ||
|
709 | ||
|
694 | 710 |
Range = dataOut.heightList*1000. |
|
695 | ||
|
711 | ||
|
696 | 712 |
for R in range(self.Num_Hei): |
|
697 | ||
|
713 | ||
|
698 | 714 |
h = Range[R] + Altitude #Range from ground to radar pulse altitude |
|
699 | 715 |
del_V[R] = 1 + 3.68 * 10**-5 * h + 1.71 * 10**-9 * h**2 #Density change correction for velocity |
|
700 | ||
|
716 | ||
|
701 | 717 |
D_range[:,R] = numpy.log( (9.65 - (Velrange[0:self.Num_Bin] / del_V[R])) / 10.3 ) / -0.6 #Diameter range [m]x10**-3 |
|
702 | ||
|
718 | ||
|
703 | 719 |
'''NOTA: ETA(n) dn = ETA(f) df |
|
704 | ||
|
720 | ||
|
705 | 721 |
dn = 1 Diferencial de muestreo |
|
706 | 722 |
df = ETA(n) / ETA(f) |
|
707 | ||
|
723 | ||
|
708 | 724 |
''' |
|
709 | ||
|
725 | ||
|
710 | 726 |
ETAn[:,R] = RadarConstant * Pr[:,R] * (Range[R] )**2 #Reflectivity (ETA) |
|
711 | ||
|
727 | ||
|
712 | 728 |
ETAv[:,R]=ETAn[:,R]/dV |
|
713 | ||
|
729 | ||
|
714 | 730 |
ETAd[:,R]=ETAv[:,R]*6.18*exp(-0.6*D_range[:,R]) |
|
715 | ||
|
731 | ||
|
716 | 732 |
SIGMA[:,R] = Km * (D_range[:,R] * 1e-3 )**6 * numpy.pi**5 / Lambda**4 #Equivalent Section of drops (sigma) |
|
717 | ||
|
718 |
N_dist[:,R] = ETAn[:,R] / SIGMA[:,R] |
|
|
719 | ||
|
733 | ||
|
734 | N_dist[:,R] = ETAn[:,R] / SIGMA[:,R] | |
|
735 | ||
|
720 | 736 |
DMoments = self.Moments(Pr[:,R], Velrange[0:self.Num_Bin]) |
|
721 | ||
|
737 | ||
|
722 | 738 |
try: |
|
723 | 739 |
popt01,pcov = curve_fit(self.gaus, Velrange[0:self.Num_Bin] , Pr[:,R] , p0=DMoments) |
|
724 |
except: |
|
|
740 | except: | |
|
725 | 741 |
popt01=numpy.zeros(3) |
|
726 | 742 |
popt01[1]= DMoments[1] |
|
727 | ||
|
743 | ||
|
728 | 744 |
if popt01[1]<0 or popt01[1]>20: |
|
729 | 745 |
popt01[1]=numpy.NaN |
|
730 | ||
|
731 | ||
|
746 | ||
|
747 | ||
|
732 | 748 |
V_mean[R]=popt01[1] |
|
733 | ||
|
749 | ||
|
734 | 750 |
Z[R] = numpy.nansum( N_dist[:,R] * (D_range[:,R])**6 )#*10**-18 |
|
735 | ||
|
751 | ||
|
736 | 752 |
RR[R] = 0.0006*numpy.pi * numpy.nansum( D_range[:,R]**3 * N_dist[:,R] * Velrange[0:self.Num_Bin] ) #Rainfall rate |
|
737 | ||
|
753 | ||
|
738 | 754 |
Ze[R] = (numpy.nansum( ETAn[:,R]) * Lambda**4) / ( 10**-18*numpy.pi**5 * Km) |
|
739 | ||
|
740 | ||
|
741 | ||
|
755 | ||
|
756 | ||
|
757 | ||
|
742 | 758 |
RR2 = (Z/200)**(1/1.6) |
|
743 | 759 |
dBRR = 10*numpy.log10(RR) |
|
744 | 760 |
dBRR2 = 10*numpy.log10(RR2) |
|
745 | ||
|
761 | ||
|
746 | 762 |
dBZe = 10*numpy.log10(Ze) |
|
747 | 763 |
dBZ = 10*numpy.log10(Z) |
|
748 | ||
|
764 | ||
|
749 | 765 |
dataOut.data_output = RR[8] |
|
750 | 766 |
dataOut.data_param = numpy.ones([3,self.Num_Hei]) |
|
751 | 767 |
dataOut.channelList = [0,1,2] |
|
752 | ||
|
768 | ||
|
753 | 769 |
dataOut.data_param[0]=dBZ |
|
754 | 770 |
dataOut.data_param[1]=V_mean |
|
755 | 771 |
dataOut.data_param[2]=RR |
|
756 | 772 | |
|
757 | 773 |
return dataOut |
|
758 | ||
|
774 | ||
|
759 | 775 |
def dBZeMODE2(self, dataOut): # Processing for MIRA35C |
|
760 | ||
|
776 | ||
|
761 | 777 |
NPW = dataOut.NPW |
|
762 | 778 |
COFA = dataOut.COFA |
|
763 | ||
|
779 | ||
|
764 | 780 |
SNR = numpy.array([self.spc[0,:,:] / NPW[0]]) #, self.spc[1,:,:] / NPW[1]]) |
|
765 | 781 |
RadarConst = dataOut.RadarConst |
|
766 | 782 |
#frequency = 34.85*10**9 |
|
767 | ||
|
783 | ||
|
768 | 784 |
ETA = numpy.zeros(([self.Num_Chn ,self.Num_Hei])) |
|
769 | 785 |
data_output = numpy.ones([self.Num_Chn , self.Num_Hei])*numpy.NaN |
|
770 | ||
|
786 | ||
|
771 | 787 |
ETA = numpy.sum(SNR,1) |
|
772 | ||
|
788 | ||
|
773 | 789 |
ETA = numpy.where(ETA is not 0. , ETA, numpy.NaN) |
|
774 | ||
|
790 | ||
|
775 | 791 |
Ze = numpy.ones([self.Num_Chn, self.Num_Hei] ) |
|
776 | ||
|
792 | ||
|
777 | 793 |
for r in range(self.Num_Hei): |
|
778 | ||
|
794 | ||
|
779 | 795 |
Ze[0,r] = ( ETA[0,r] ) * COFA[0,r][0] * RadarConst * ((r/5000.)**2) |
|
780 | 796 |
#Ze[1,r] = ( ETA[1,r] ) * COFA[1,r][0] * RadarConst * ((r/5000.)**2) |
|
781 | ||
|
797 | ||
|
782 | 798 |
return Ze |
|
783 | ||
|
799 | ||
|
784 | 800 |
# def GetRadarConstant(self): |
|
785 | # | |
|
786 |
# """ |
|
|
801 | # | |
|
802 | # """ | |
|
787 | 803 |
# Constants: |
|
788 | # | |
|
804 | # | |
|
789 | 805 |
# Pt: Transmission Power dB 5kW 5000 |
|
790 | 806 |
# Gt: Transmission Gain dB 24.7 dB 295.1209 |
|
791 | 807 |
# Gr: Reception Gain dB 18.5 dB 70.7945 |
@@ -794,55 +810,55 class PrecipitationProc(Operation): | |||
|
794 | 810 |
# tauW: Width of transmission pulse s 4us 4e-6 |
|
795 | 811 |
# ThetaT: Transmission antenna bean angle rad 0.1656317 rad 0.1656317 |
|
796 | 812 |
# ThetaR: Reception antenna beam angle rad 0.36774087 rad 0.36774087 |
|
797 | # | |
|
813 | # | |
|
798 | 814 |
# """ |
|
799 | # | |
|
815 | # | |
|
800 | 816 |
# Numerator = ( (4*numpy.pi)**3 * aL**2 * 16 * numpy.log(2) ) |
|
801 | 817 |
# Denominator = ( Pt * Gt * Gr * Lambda**2 * SPEED_OF_LIGHT * TauW * numpy.pi * ThetaT * TheraR) |
|
802 | 818 |
# RadarConstant = Numerator / Denominator |
|
803 | # | |
|
819 | # | |
|
804 | 820 |
# return RadarConstant |
|
805 | ||
|
806 | ||
|
807 | ||
|
808 |
class FullSpectralAnalysis(Operation): |
|
|
809 | ||
|
821 | ||
|
822 | ||
|
823 | ||
|
824 | class FullSpectralAnalysis(Operation): | |
|
825 | ||
|
810 | 826 |
""" |
|
811 | 827 |
Function that implements Full Spectral Analysis technique. |
|
812 | ||
|
813 |
Input: |
|
|
828 | ||
|
829 | Input: | |
|
814 | 830 |
self.dataOut.data_pre : SelfSpectra and CrossSpectra data |
|
815 | 831 |
self.dataOut.groupList : Pairlist of channels |
|
816 | 832 |
self.dataOut.ChanDist : Physical distance between receivers |
|
817 | ||
|
818 | ||
|
819 |
Output: |
|
|
820 | ||
|
821 |
self.dataOut.data_output : Zonal wind, Meridional wind and Vertical wind |
|
|
822 | ||
|
823 | ||
|
833 | ||
|
834 | ||
|
835 | Output: | |
|
836 | ||
|
837 | self.dataOut.data_output : Zonal wind, Meridional wind and Vertical wind | |
|
838 | ||
|
839 | ||
|
824 | 840 |
Parameters affected: Winds, height range, SNR |
|
825 | ||
|
841 | ||
|
826 | 842 |
""" |
|
827 | 843 |
def run(self, dataOut, Xi01=None, Xi02=None, Xi12=None, Eta01=None, Eta02=None, Eta12=None, SNRlimit=7, minheight=None, maxheight=None): |
|
828 | ||
|
829 |
self.indice=int(numpy.random.rand()*1000) |
|
|
830 | ||
|
844 | ||
|
845 | self.indice=int(numpy.random.rand()*1000) | |
|
846 | ||
|
831 | 847 |
spc = dataOut.data_pre[0].copy() |
|
832 | 848 |
cspc = dataOut.data_pre[1] |
|
833 | ||
|
849 | ||
|
834 | 850 |
"""Erick: NOTE THE RANGE OF THE PULSE TX MUST BE REMOVED""" |
|
835 | 851 | |
|
836 | 852 |
SNRspc = spc.copy() |
|
837 | 853 |
SNRspc[:,:,0:7]= numpy.NaN |
|
838 | ||
|
854 | ||
|
839 | 855 |
"""##########################################""" |
|
840 | ||
|
841 | ||
|
856 | ||
|
857 | ||
|
842 | 858 |
nChannel = spc.shape[0] |
|
843 | 859 |
nProfiles = spc.shape[1] |
|
844 | 860 |
nHeights = spc.shape[2] |
|
845 | ||
|
861 | ||
|
846 | 862 |
# first_height = 0.75 #km (ref: data header 20170822) |
|
847 | 863 |
# resolution_height = 0.075 #km |
|
848 | 864 |
''' |
@@ -866,37 +882,37 class FullSpectralAnalysis(Operation): | |||
|
866 | 882 |
ChanDist = dataOut.ChanDist |
|
867 | 883 |
else: |
|
868 | 884 |
ChanDist = numpy.array([[Xi01, Eta01],[Xi02,Eta02],[Xi12,Eta12]]) |
|
869 | ||
|
885 | ||
|
870 | 886 |
FrecRange = dataOut.spc_range[0] |
|
871 | ||
|
887 | ||
|
872 | 888 |
data_SNR=numpy.zeros([nProfiles]) |
|
873 | 889 |
noise = dataOut.noise |
|
874 | ||
|
890 | ||
|
875 | 891 |
dataOut.data_SNR = (numpy.mean(SNRspc,axis=1)- noise[0]) / noise[0] |
|
876 | ||
|
892 | ||
|
877 | 893 |
dataOut.data_SNR[numpy.where( dataOut.data_SNR <0 )] = 1e-20 |
|
878 | ||
|
879 | ||
|
894 | ||
|
895 | ||
|
880 | 896 |
data_output=numpy.ones([spc.shape[0],spc.shape[2]])*numpy.NaN |
|
881 | ||
|
897 | ||
|
882 | 898 |
velocityX=[] |
|
883 | 899 |
velocityY=[] |
|
884 |
velocityV=[] |
|
|
885 | ||
|
900 | velocityV=[] | |
|
901 | ||
|
886 | 902 |
dbSNR = 10*numpy.log10(dataOut.data_SNR) |
|
887 | 903 |
dbSNR = numpy.average(dbSNR,0) |
|
888 | ||
|
904 | ||
|
889 | 905 |
'''***********************************************WIND ESTIMATION**************************************''' |
|
890 | ||
|
906 | ||
|
891 | 907 |
for Height in range(nHeights): |
|
892 | ||
|
893 |
if Height >= range_min and Height < range_max: |
|
|
894 |
# error_code unused, yet maybe useful for future analysis. |
|
|
908 | ||
|
909 | if Height >= range_min and Height < range_max: | |
|
910 | # error_code unused, yet maybe useful for future analysis. | |
|
895 | 911 |
[Vzon,Vmer,Vver, error_code] = self.WindEstimation(spc[:,:,Height], cspc[:,:,Height], pairsList, ChanDist, Height, noise, dataOut.spc_range, dbSNR[Height], SNRlimit) |
|
896 | 912 |
else: |
|
897 | 913 |
Vzon,Vmer,Vver = 0., 0., numpy.NaN |
|
898 | ||
|
899 | ||
|
914 | ||
|
915 | ||
|
900 | 916 |
if abs(Vzon) < 100. and abs(Vzon) > 0. and abs(Vmer) < 100. and abs(Vmer) > 0.: |
|
901 | 917 |
velocityX=numpy.append(velocityX, Vzon) |
|
902 | 918 |
velocityY=numpy.append(velocityY, -Vmer) |
@@ -904,33 +920,33 class FullSpectralAnalysis(Operation): | |||
|
904 | 920 |
else: |
|
905 | 921 |
velocityX=numpy.append(velocityX, numpy.NaN) |
|
906 | 922 |
velocityY=numpy.append(velocityY, numpy.NaN) |
|
907 | ||
|
923 | ||
|
908 | 924 |
if dbSNR[Height] > SNRlimit: |
|
909 | 925 |
velocityV=numpy.append(velocityV, -Vver) # reason for this minus sign -> convention? (taken from Ericks version) |
|
910 | 926 |
else: |
|
911 | 927 |
velocityV=numpy.append(velocityV, numpy.NaN) |
|
912 | ||
|
913 | ||
|
928 | ||
|
929 | ||
|
914 | 930 |
'''Change the numpy.array (velocityX) sign when trying to process BLTR data (Erick)''' |
|
915 |
data_output[0] = numpy.array(velocityX) |
|
|
916 |
data_output[1] = numpy.array(velocityY) |
|
|
931 | data_output[0] = numpy.array(velocityX) | |
|
932 | data_output[1] = numpy.array(velocityY) | |
|
917 | 933 |
data_output[2] = velocityV |
|
918 | ||
|
919 | ||
|
934 | ||
|
935 | ||
|
920 | 936 |
dataOut.data_output = data_output |
|
921 | ||
|
937 | ||
|
922 | 938 |
return dataOut |
|
923 | ||
|
939 | ||
|
924 | 940 | |
|
925 | 941 |
def moving_average(self,x, N=2): |
|
926 | 942 |
""" convolution for smoothenig data. note that last N-1 values are convolution with zeroes """ |
|
927 | 943 |
return numpy.convolve(x, numpy.ones((N,))/N)[(N-1):] |
|
928 | ||
|
944 | ||
|
929 | 945 |
def gaus(self,xSamples,Amp,Mu,Sigma): |
|
930 | 946 |
return ( Amp / ((2*numpy.pi)**0.5 * Sigma) ) * numpy.exp( -( xSamples - Mu )**2 / ( 2 * (Sigma**2) )) |
|
931 | ||
|
947 | ||
|
932 | 948 |
def Moments(self, ySamples, xSamples): |
|
933 |
'''*** |
|
|
949 | '''*** | |
|
934 | 950 |
Variables corresponding to moments of distribution. |
|
935 | 951 |
Also used as initial coefficients for curve_fit. |
|
936 | 952 |
Vr was corrected. Only a velocity when x is velocity, of course. |
@@ -939,9 +955,9 class FullSpectralAnalysis(Operation): | |||
|
939 | 955 |
yNorm = ySamples / Pot |
|
940 | 956 |
x_range = (numpy.max(xSamples)-numpy.min(xSamples)) |
|
941 | 957 |
Vr = numpy.nansum( yNorm * xSamples )*x_range/len(xSamples) # Velocidad radial, mu, corrimiento doppler, primer momento |
|
942 |
Sigma2 = abs(numpy.nansum( yNorm * ( xSamples - Vr )**2 )) # Segundo Momento |
|
|
958 | Sigma2 = abs(numpy.nansum( yNorm * ( xSamples - Vr )**2 )) # Segundo Momento | |
|
943 | 959 |
Desv = Sigma2**0.5 # Desv. Estandar, Ancho espectral |
|
944 | ||
|
960 | ||
|
945 | 961 |
return numpy.array([Pot, Vr, Desv]) |
|
946 | 962 | |
|
947 | 963 |
def StopWindEstimation(self, error_code): |
@@ -954,7 +970,7 class FullSpectralAnalysis(Operation): | |||
|
954 | 970 |
return Vzon, Vmer, Vver, error_code |
|
955 | 971 | |
|
956 | 972 |
def AntiAliasing(self, interval, maxstep): |
|
957 |
""" |
|
|
973 | """ | |
|
958 | 974 |
function to prevent errors from aliased values when computing phaseslope |
|
959 | 975 |
""" |
|
960 | 976 |
antialiased = numpy.zeros(len(interval))*0.0 |
@@ -964,8 +980,8 class FullSpectralAnalysis(Operation): | |||
|
964 | 980 | |
|
965 | 981 |
for i in range(1,len(antialiased)): |
|
966 | 982 | |
|
967 |
step = interval[i] - interval[i-1] |
|
|
968 | ||
|
983 | step = interval[i] - interval[i-1] | |
|
984 | ||
|
969 | 985 |
if step > maxstep: |
|
970 | 986 |
copyinterval -= 2*numpy.pi |
|
971 | 987 |
antialiased[i] = copyinterval[i] |
@@ -973,7 +989,7 class FullSpectralAnalysis(Operation): | |||
|
973 | 989 |
elif step < maxstep*(-1): |
|
974 | 990 |
copyinterval += 2*numpy.pi |
|
975 | 991 |
antialiased[i] = copyinterval[i] |
|
976 | ||
|
992 | ||
|
977 | 993 |
else: |
|
978 | 994 |
antialiased[i] = copyinterval[i].copy() |
|
979 | 995 | |
@@ -1003,27 +1019,27 class FullSpectralAnalysis(Operation): | |||
|
1003 | 1019 |
3 : SNR to low or velocity to high -> prec. e.g. |
|
1004 | 1020 |
4 : at least one Gaussian of cspc exceeds widthlimit |
|
1005 | 1021 |
5 : zero out of three cspc Gaussian fits converged |
|
1006 |
6 : phase slope fit could not be found |
|
|
1022 | 6 : phase slope fit could not be found | |
|
1007 | 1023 |
7 : arrays used to fit phase have different length |
|
1008 | 1024 |
8 : frequency range is either too short (len <= 5) or very long (> 30% of cspc) |
|
1009 | 1025 | |
|
1010 | 1026 |
""" |
|
1011 | 1027 | |
|
1012 | 1028 |
error_code = 0 |
|
1013 | ||
|
1029 | ||
|
1014 | 1030 | |
|
1015 | 1031 |
SPC_Samples = numpy.ones([spc.shape[0],spc.shape[1]]) # for normalized spc values for one height |
|
1016 | 1032 |
phase = numpy.ones([spc.shape[0],spc.shape[1]]) # phase between channels |
|
1017 | 1033 |
CSPC_Samples = numpy.ones([spc.shape[0],spc.shape[1]],dtype=numpy.complex_) # for normalized cspc values |
|
1018 | 1034 |
PhaseSlope = numpy.zeros(spc.shape[0]) # slope of the phases, channelwise |
|
1019 | 1035 |
PhaseInter = numpy.ones(spc.shape[0]) # intercept to the slope of the phases, channelwise |
|
1020 |
xFrec = AbbsisaRange[0][0:spc.shape[1]] # frequency range |
|
|
1036 | xFrec = AbbsisaRange[0][0:spc.shape[1]] # frequency range | |
|
1021 | 1037 |
xVel = AbbsisaRange[2][0:spc.shape[1]] # velocity range |
|
1022 | 1038 |
SPCav = numpy.average(spc, axis=0)-numpy.average(noise) # spc[0]-noise[0] |
|
1023 | ||
|
1039 | ||
|
1024 | 1040 |
SPCmoments_vel = self.Moments(SPCav, xVel ) # SPCmoments_vel[1] corresponds to vertical velocity and is used to determine if signal corresponds to wind (if .. <3) |
|
1025 | 1041 |
CSPCmoments = [] |
|
1026 | ||
|
1042 | ||
|
1027 | 1043 | |
|
1028 | 1044 |
'''Getting Eij and Nij''' |
|
1029 | 1045 | |
@@ -1038,13 +1054,13 class FullSpectralAnalysis(Operation): | |||
|
1038 | 1054 |
spc_norm = spc.copy() # need copy() because untouched spc is needed for normalization of cspc below |
|
1039 | 1055 |
spc_norm = numpy.where(numpy.isfinite(spc_norm), spc_norm, numpy.NAN) |
|
1040 | 1056 | |
|
1041 |
for i in range(spc.shape[0]): |
|
|
1042 | ||
|
1057 | for i in range(spc.shape[0]): | |
|
1058 | ||
|
1043 | 1059 |
spc_sub = spc_norm[i,:] - noise[i] # spc not smoothed here or in previous version. |
|
1044 | 1060 | |
|
1045 | 1061 |
Factor_Norm = 2*numpy.max(xFrec) / numpy.count_nonzero(~numpy.isnan(spc_sub)) # usually = Freq range / nfft |
|
1046 |
normalized_spc = spc_sub / (numpy.nansum(numpy.abs(spc_sub)) * Factor_Norm) |
|
|
1047 | ||
|
1062 | normalized_spc = spc_sub / (numpy.nansum(numpy.abs(spc_sub)) * Factor_Norm) | |
|
1063 | ||
|
1048 | 1064 |
xSamples = xFrec # the frequency range is taken |
|
1049 | 1065 |
SPC_Samples[i] = normalized_spc # Normalized SPC values are taken |
|
1050 | 1066 | |
@@ -1055,49 +1071,49 class FullSpectralAnalysis(Operation): | |||
|
1055 | 1071 |
only for estimation of width. for normalization of cross spectra, you need initial, |
|
1056 | 1072 |
unnormalized self-spectra With noise. |
|
1057 | 1073 | |
|
1058 |
Technically, you don't even need to normalize the self-spectra, as you only need the |
|
|
1074 | Technically, you don't even need to normalize the self-spectra, as you only need the | |
|
1059 | 1075 |
width of the peak. However, it was left this way. Note that the normalization has a flaw: |
|
1060 | 1076 |
due to subtraction of the noise, some values are below zero. Raw "spc" values should be |
|
1061 | 1077 |
>= 0, as it is the modulus squared of the signals (complex * it's conjugate) |
|
1062 | 1078 |
""" |
|
1063 | 1079 | |
|
1064 |
SPCMean = numpy.average(SPC_Samples, axis=0) |
|
|
1065 | ||
|
1080 | SPCMean = numpy.average(SPC_Samples, axis=0) | |
|
1081 | ||
|
1066 | 1082 |
popt = [1e-10,0,1e-10] |
|
1067 | 1083 |
SPCMoments = self.Moments(SPCMean, xSamples) |
|
1068 | 1084 | |
|
1069 |
if dbSNR > SNRlimit and numpy.abs(SPCmoments_vel[1]) < 3: |
|
|
1085 | if dbSNR > SNRlimit and numpy.abs(SPCmoments_vel[1]) < 3: | |
|
1070 | 1086 |
try: |
|
1071 | 1087 |
popt,pcov = curve_fit(self.gaus,xSamples,SPCMean,p0=SPCMoments)#, bounds=(-numpy.inf, [numpy.inf, numpy.inf, 10])). Setting bounds does not make the code faster but only keeps the fit from finding the minimum. |
|
1072 | 1088 |
if popt[2] > widthlimit: # CONDITION |
|
1073 | 1089 |
return self.StopWindEstimation(error_code = 1) |
|
1074 | 1090 | |
|
1075 | 1091 |
FitGauss = self.gaus(xSamples,*popt) |
|
1076 | ||
|
1092 | ||
|
1077 | 1093 |
except :#RuntimeError: |
|
1078 | 1094 |
return self.StopWindEstimation(error_code = 2) |
|
1079 | 1095 | |
|
1080 | 1096 |
else: |
|
1081 | 1097 |
return self.StopWindEstimation(error_code = 3) |
|
1082 | ||
|
1098 | ||
|
1083 | 1099 | |
|
1084 | 1100 | |
|
1085 | 1101 |
'''***************************** CSPC Normalization ************************* |
|
1086 | 1102 |
new section: |
|
1087 | 1103 |
The Spc spectra are used to normalize the crossspectra. Peaks from precipitation |
|
1088 |
influence the norm which is not desired. First, a range is identified where the |
|
|
1089 |
wind peak is estimated -> sum_wind is sum of those frequencies. Next, the area |
|
|
1090 |
around it gets cut off and values replaced by mean determined by the boundary |
|
|
1104 | influence the norm which is not desired. First, a range is identified where the | |
|
1105 | wind peak is estimated -> sum_wind is sum of those frequencies. Next, the area | |
|
1106 | around it gets cut off and values replaced by mean determined by the boundary | |
|
1091 | 1107 |
data -> sum_noise (spc is not normalized here, thats why the noise is important) |
|
1092 | 1108 | |
|
1093 | 1109 |
The sums are then added and multiplied by range/datapoints, because you need |
|
1094 | 1110 |
an integral and not a sum for normalization. |
|
1095 | ||
|
1096 |
A norm is found according to Briggs 92. |
|
|
1111 | ||
|
1112 | A norm is found according to Briggs 92. | |
|
1097 | 1113 |
''' |
|
1098 | 1114 | |
|
1099 | 1115 |
radarWavelength = 0.6741 # meters |
|
1100 |
count_limit_freq = numpy.abs(popt[1]) + widthlimit # Hz, m/s can be also used if velocity is desired abscissa. |
|
|
1116 | count_limit_freq = numpy.abs(popt[1]) + widthlimit # Hz, m/s can be also used if velocity is desired abscissa. | |
|
1101 | 1117 |
# count_limit_freq = numpy.max(xFrec) |
|
1102 | 1118 | |
|
1103 | 1119 |
channel_integrals = numpy.zeros(3) |
@@ -1108,11 +1124,11 class FullSpectralAnalysis(Operation): | |||
|
1108 | 1124 |
sum over all frequencies in the range around zero Hz @ math.ceil(N_freq/2) |
|
1109 | 1125 |
''' |
|
1110 | 1126 |
N_freq = numpy.count_nonzero(~numpy.isnan(spc[i,:])) |
|
1111 |
count_limit_int = int(math.ceil( count_limit_freq / numpy.max(xFrec) * (N_freq / 2) )) # gives integer point |
|
|
1127 | count_limit_int = int(math.ceil( count_limit_freq / numpy.max(xFrec) * (N_freq / 2) )) # gives integer point | |
|
1112 | 1128 |
sum_wind = numpy.nansum( spc[i, (math.ceil(N_freq/2) - count_limit_int) : (math.ceil(N_freq / 2) + count_limit_int)] ) #N_freq/2 is where frequency (velocity) is zero, i.e. middle of spectrum. |
|
1113 | 1129 |
sum_noise = (numpy.mean(spc[i, :4]) + numpy.mean(spc[i, -6:-2]))/2.0 * (N_freq - 2*count_limit_int) |
|
1114 | 1130 |
channel_integrals[i] = (sum_noise + sum_wind) * (2*numpy.max(xFrec) / N_freq) |
|
1115 | ||
|
1131 | ||
|
1116 | 1132 | |
|
1117 | 1133 |
cross_integrals_peak = numpy.zeros(3) |
|
1118 | 1134 |
# cross_integrals_totalrange = numpy.zeros(3) |
@@ -1125,45 +1141,45 class FullSpectralAnalysis(Operation): | |||
|
1125 | 1141 |
chan_index1 = pairsList[i][1] |
|
1126 | 1142 | |
|
1127 | 1143 |
cross_integrals_peak[i] = channel_integrals[chan_index0]*channel_integrals[chan_index1] |
|
1128 |
normalized_cspc = cspc_norm / numpy.sqrt(cross_integrals_peak[i]) |
|
|
1144 | normalized_cspc = cspc_norm / numpy.sqrt(cross_integrals_peak[i]) | |
|
1129 | 1145 |
CSPC_Samples[i] = normalized_cspc |
|
1130 | 1146 | |
|
1131 | 1147 |
''' Finding cross integrals without subtracting any peaks:''' |
|
1132 | 1148 |
# FactorNorm0 = 2*numpy.max(xFrec) / numpy.count_nonzero(~numpy.isnan(spc[chan_index0,:])) |
|
1133 | 1149 |
# FactorNorm1 = 2*numpy.max(xFrec) / numpy.count_nonzero(~numpy.isnan(spc[chan_index1,:])) |
|
1134 |
# cross_integrals_totalrange[i] = (numpy.nansum(spc[chan_index0,:])) * FactorNorm0 * (numpy.nansum(spc[chan_index1,:])) * FactorNorm1 |
|
|
1135 |
# normalized_cspc = cspc_norm / numpy.sqrt(cross_integrals_totalrange[i]) |
|
|
1150 | # cross_integrals_totalrange[i] = (numpy.nansum(spc[chan_index0,:])) * FactorNorm0 * (numpy.nansum(spc[chan_index1,:])) * FactorNorm1 | |
|
1151 | # normalized_cspc = cspc_norm / numpy.sqrt(cross_integrals_totalrange[i]) | |
|
1136 | 1152 |
# CSPC_Samples[i] = normalized_cspc |
|
1137 | ||
|
1138 | ||
|
1153 | ||
|
1154 | ||
|
1139 | 1155 |
phase[i] = numpy.arctan2(CSPC_Samples[i].imag, CSPC_Samples[i].real) |
|
1140 | 1156 | |
|
1141 | 1157 | |
|
1142 | 1158 |
CSPCmoments = numpy.vstack([self.Moments(numpy.abs(CSPC_Samples[0]), xSamples), |
|
1143 | 1159 |
self.Moments(numpy.abs(CSPC_Samples[1]), xSamples), |
|
1144 | 1160 |
self.Moments(numpy.abs(CSPC_Samples[2]), xSamples)]) |
|
1145 | ||
|
1161 | ||
|
1146 | 1162 | |
|
1147 | 1163 |
'''***Sorting out NaN entries***''' |
|
1148 | 1164 |
CSPCMask01 = numpy.abs(CSPC_Samples[0]) |
|
1149 | 1165 |
CSPCMask02 = numpy.abs(CSPC_Samples[1]) |
|
1150 | 1166 |
CSPCMask12 = numpy.abs(CSPC_Samples[2]) |
|
1151 | ||
|
1167 | ||
|
1152 | 1168 |
mask01 = ~numpy.isnan(CSPCMask01) |
|
1153 | 1169 |
mask02 = ~numpy.isnan(CSPCMask02) |
|
1154 | 1170 |
mask12 = ~numpy.isnan(CSPCMask12) |
|
1155 | ||
|
1171 | ||
|
1156 | 1172 |
CSPCMask01 = CSPCMask01[mask01] |
|
1157 | 1173 |
CSPCMask02 = CSPCMask02[mask02] |
|
1158 | 1174 |
CSPCMask12 = CSPCMask12[mask12] |
|
1159 | 1175 | |
|
1160 | ||
|
1161 |
popt01, popt02, popt12 = [1e-10,1e-10,1e-10], [1e-10,1e-10,1e-10] ,[1e-10,1e-10,1e-10] |
|
|
1176 | ||
|
1177 | popt01, popt02, popt12 = [1e-10,1e-10,1e-10], [1e-10,1e-10,1e-10] ,[1e-10,1e-10,1e-10] | |
|
1162 | 1178 |
FitGauss01, FitGauss02, FitGauss12 = numpy.empty(len(xSamples))*0, numpy.empty(len(xSamples))*0, numpy.empty(len(xSamples))*0 |
|
1163 | ||
|
1179 | ||
|
1164 | 1180 |
'''*******************************FIT GAUSS CSPC************************************''' |
|
1165 | 1181 | |
|
1166 |
try: |
|
|
1182 | try: | |
|
1167 | 1183 |
popt01,pcov = curve_fit(self.gaus,xSamples[mask01],numpy.abs(CSPCMask01),p0=CSPCmoments[0]) |
|
1168 | 1184 |
if popt01[2] > widthlimit: # CONDITION |
|
1169 | 1185 |
return self.StopWindEstimation(error_code = 4) |
@@ -1186,53 +1202,53 class FullSpectralAnalysis(Operation): | |||
|
1186 | 1202 | |
|
1187 | 1203 |
'''************* Getting Fij ***************''' |
|
1188 | 1204 | |
|
1189 | ||
|
1190 |
#Punto en Eje X de la Gaussiana donde se encuentra el centro -- x-axis point of the gaussian where the center is located |
|
|
1191 |
# -> PointGauCenter |
|
|
1192 |
GaussCenter = popt[1] |
|
|
1205 | ||
|
1206 | #Punto en Eje X de la Gaussiana donde se encuentra el centro -- x-axis point of the gaussian where the center is located | |
|
1207 | # -> PointGauCenter | |
|
1208 | GaussCenter = popt[1] | |
|
1193 | 1209 |
ClosestCenter = xSamples[numpy.abs(xSamples-GaussCenter).argmin()] |
|
1194 | 1210 |
PointGauCenter = numpy.where(xSamples==ClosestCenter)[0][0] |
|
1195 | ||
|
1211 | ||
|
1196 | 1212 |
#Punto e^-1 hubicado en la Gaussiana -- point where e^-1 is located in the gaussian |
|
1197 | 1213 |
PeMinus1 = numpy.max(FitGauss) * numpy.exp(-1) |
|
1198 | 1214 |
FijClosest = FitGauss[numpy.abs(FitGauss-PeMinus1).argmin()] # El punto mas cercano a "Peminus1" dentro de "FitGauss" |
|
1199 | 1215 |
PointFij = numpy.where(FitGauss==FijClosest)[0][0] |
|
1200 | 1216 | |
|
1201 | 1217 |
Fij = numpy.abs(xSamples[PointFij] - xSamples[PointGauCenter]) |
|
1202 | ||
|
1218 | ||
|
1203 | 1219 |
'''********** Taking frequency ranges from mean SPCs **********''' |
|
1204 | ||
|
1220 | ||
|
1205 | 1221 |
#GaussCenter = popt[1] #Primer momento 01 |
|
1206 | 1222 |
GauWidth = popt[2] * 3/2 #Ancho de banda de Gau01 -- Bandwidth of Gau01 TODO why *3/2? |
|
1207 | 1223 |
Range = numpy.empty(2) |
|
1208 | 1224 |
Range[0] = GaussCenter - GauWidth |
|
1209 |
Range[1] = GaussCenter + GauWidth |
|
|
1225 | Range[1] = GaussCenter + GauWidth | |
|
1210 | 1226 |
#Punto en Eje X de la Gaussiana donde se encuentra ancho de banda (min:max) -- Point in x-axis where the bandwidth is located (min:max) |
|
1211 | 1227 |
ClosRangeMin = xSamples[numpy.abs(xSamples-Range[0]).argmin()] |
|
1212 | 1228 |
ClosRangeMax = xSamples[numpy.abs(xSamples-Range[1]).argmin()] |
|
1213 | ||
|
1229 | ||
|
1214 | 1230 |
PointRangeMin = numpy.where(xSamples==ClosRangeMin)[0][0] |
|
1215 | 1231 |
PointRangeMax = numpy.where(xSamples==ClosRangeMax)[0][0] |
|
1216 | ||
|
1232 | ||
|
1217 | 1233 |
Range = numpy.array([ PointRangeMin, PointRangeMax ]) |
|
1218 | ||
|
1234 | ||
|
1219 | 1235 |
FrecRange = xFrec[ Range[0] : Range[1] ] |
|
1220 | 1236 | |
|
1221 | ||
|
1222 |
'''************************** Getting Phase Slope ***************************''' |
|
|
1223 | ||
|
1224 |
for i in range(1,3): # Changed to only compute two |
|
|
1225 | ||
|
1237 | ||
|
1238 | '''************************** Getting Phase Slope ***************************''' | |
|
1239 | ||
|
1240 | for i in range(1,3): # Changed to only compute two | |
|
1241 | ||
|
1226 | 1242 |
if len(FrecRange) > 5 and len(FrecRange) < spc.shape[1] * 0.3: |
|
1227 | 1243 |
# PhaseRange=self.moving_average(phase[i,Range[0]:Range[1]],N=1) #used before to smooth phase with N=3 |
|
1228 | 1244 |
PhaseRange = phase[i,Range[0]:Range[1]].copy() |
|
1229 | ||
|
1245 | ||
|
1230 | 1246 |
mask = ~numpy.isnan(FrecRange) & ~numpy.isnan(PhaseRange) |
|
1231 | ||
|
1247 | ||
|
1232 | 1248 | |
|
1233 | 1249 |
if len(FrecRange) == len(PhaseRange): |
|
1234 | ||
|
1235 |
try: |
|
|
1250 | ||
|
1251 | try: | |
|
1236 | 1252 |
slope, intercept, _, _, _ = stats.linregress(FrecRange[mask], self.AntiAliasing(PhaseRange[mask], 4.5)) |
|
1237 | 1253 |
PhaseSlope[i] = slope |
|
1238 | 1254 |
PhaseInter[i] = intercept |
@@ -1242,49 +1258,49 class FullSpectralAnalysis(Operation): | |||
|
1242 | 1258 | |
|
1243 | 1259 |
else: |
|
1244 | 1260 |
return self.StopWindEstimation(error_code = 7) |
|
1245 | ||
|
1261 | ||
|
1246 | 1262 |
else: |
|
1247 | 1263 |
return self.StopWindEstimation(error_code = 8) |
|
1248 | ||
|
1249 | ||
|
1250 | ||
|
1264 | ||
|
1265 | ||
|
1266 | ||
|
1251 | 1267 |
'''*** Constants A-H correspond to the convention as in Briggs and Vincent 1992 ***''' |
|
1252 | 1268 | |
|
1253 | 1269 |
'''Getting constant C''' |
|
1254 | 1270 |
cC=(Fij*numpy.pi)**2 |
|
1255 | ||
|
1271 | ||
|
1256 | 1272 |
'''****** Getting constants F and G ******''' |
|
1257 | 1273 |
MijEijNij = numpy.array([[Xi02,Eta02], [Xi12,Eta12]]) |
|
1258 | 1274 |
MijResult0 = (-PhaseSlope[1] * cC) / (2*numpy.pi) |
|
1259 |
MijResult1 = (-PhaseSlope[2] * cC) / (2*numpy.pi) |
|
|
1275 | MijResult1 = (-PhaseSlope[2] * cC) / (2*numpy.pi) | |
|
1260 | 1276 |
MijResults = numpy.array([MijResult0,MijResult1]) |
|
1261 |
(cF,cG) = numpy.linalg.solve(MijEijNij, MijResults) |
|
|
1262 | ||
|
1277 | (cF,cG) = numpy.linalg.solve(MijEijNij, MijResults) | |
|
1278 | ||
|
1263 | 1279 |
'''****** Getting constants A, B and H ******''' |
|
1264 |
W01 = numpy.nanmax( FitGauss01 ) |
|
|
1265 |
W02 = numpy.nanmax( FitGauss02 ) |
|
|
1266 |
W12 = numpy.nanmax( FitGauss12 ) |
|
|
1267 | ||
|
1280 | W01 = numpy.nanmax( FitGauss01 ) | |
|
1281 | W02 = numpy.nanmax( FitGauss02 ) | |
|
1282 | W12 = numpy.nanmax( FitGauss12 ) | |
|
1283 | ||
|
1268 | 1284 |
WijResult0 = ((cF * Xi01 + cG * Eta01)**2)/cC - numpy.log(W01 / numpy.sqrt(numpy.pi / cC)) |
|
1269 | 1285 |
WijResult1 = ((cF * Xi02 + cG * Eta02)**2)/cC - numpy.log(W02 / numpy.sqrt(numpy.pi / cC)) |
|
1270 | 1286 |
WijResult2 = ((cF * Xi12 + cG * Eta12)**2)/cC - numpy.log(W12 / numpy.sqrt(numpy.pi / cC)) |
|
1271 | ||
|
1287 | ||
|
1272 | 1288 |
WijResults = numpy.array([WijResult0, WijResult1, WijResult2]) |
|
1273 | ||
|
1274 |
WijEijNij = numpy.array([ [Xi01**2, Eta01**2, 2*Xi01*Eta01] , [Xi02**2, Eta02**2, 2*Xi02*Eta02] , [Xi12**2, Eta12**2, 2*Xi12*Eta12] ]) |
|
|
1289 | ||
|
1290 | WijEijNij = numpy.array([ [Xi01**2, Eta01**2, 2*Xi01*Eta01] , [Xi02**2, Eta02**2, 2*Xi02*Eta02] , [Xi12**2, Eta12**2, 2*Xi12*Eta12] ]) | |
|
1275 | 1291 |
(cA,cB,cH) = numpy.linalg.solve(WijEijNij, WijResults) |
|
1276 | ||
|
1292 | ||
|
1277 | 1293 |
VxVy = numpy.array([[cA,cH],[cH,cB]]) |
|
1278 | 1294 |
VxVyResults = numpy.array([-cF,-cG]) |
|
1279 | 1295 |
(Vx,Vy) = numpy.linalg.solve(VxVy, VxVyResults) |
|
1280 | ||
|
1296 | ||
|
1281 | 1297 |
Vzon = Vy |
|
1282 | 1298 |
Vmer = Vx |
|
1283 | ||
|
1299 | ||
|
1284 | 1300 |
# Vmag=numpy.sqrt(Vzon**2+Vmer**2) # unused |
|
1285 | 1301 |
# Vang=numpy.arctan2(Vmer,Vzon) # unused |
|
1286 | 1302 | |
|
1287 | ||
|
1303 | ||
|
1288 | 1304 |
''' using frequency as abscissa. Due to three channels, the offzenith angle is zero |
|
1289 | 1305 |
and Vrad equal to Vver. formula taken from Briggs 92, figure 4. |
|
1290 | 1306 |
''' |
@@ -1295,40 +1311,40 class FullSpectralAnalysis(Operation): | |||
|
1295 | 1311 | |
|
1296 | 1312 |
error_code = 0 |
|
1297 | 1313 | |
|
1298 |
return Vzon, Vmer, Vver, error_code |
|
|
1314 | return Vzon, Vmer, Vver, error_code | |
|
1299 | 1315 | |
|
1300 | 1316 | |
|
1301 | 1317 |
class SpectralMoments(Operation): |
|
1302 | ||
|
1318 | ||
|
1303 | 1319 |
''' |
|
1304 | 1320 |
Function SpectralMoments() |
|
1305 | ||
|
1321 | ||
|
1306 | 1322 |
Calculates moments (power, mean, standard deviation) and SNR of the signal |
|
1307 | ||
|
1323 | ||
|
1308 | 1324 |
Type of dataIn: Spectra |
|
1309 | ||
|
1325 | ||
|
1310 | 1326 |
Configuration Parameters: |
|
1311 | ||
|
1327 | ||
|
1312 | 1328 |
dirCosx : Cosine director in X axis |
|
1313 | 1329 |
dirCosy : Cosine director in Y axis |
|
1314 | ||
|
1330 | ||
|
1315 | 1331 |
elevation : |
|
1316 | 1332 |
azimuth : |
|
1317 | ||
|
1333 | ||
|
1318 | 1334 |
Input: |
|
1319 |
channelList : simple channel list to select e.g. [2,3,7] |
|
|
1335 | channelList : simple channel list to select e.g. [2,3,7] | |
|
1320 | 1336 |
self.dataOut.data_pre : Spectral data |
|
1321 | 1337 |
self.dataOut.abscissaList : List of frequencies |
|
1322 | 1338 |
self.dataOut.noise : Noise level per channel |
|
1323 | ||
|
1339 | ||
|
1324 | 1340 |
Affected: |
|
1325 | 1341 |
self.dataOut.moments : Parameters per channel |
|
1326 | 1342 |
self.dataOut.data_SNR : SNR per channel |
|
1327 | ||
|
1343 | ||
|
1328 | 1344 |
''' |
|
1329 | ||
|
1345 | ||
|
1330 | 1346 |
def run(self, dataOut): |
|
1331 | ||
|
1347 | ||
|
1332 | 1348 |
data = dataOut.data_pre[0] |
|
1333 | 1349 |
absc = dataOut.abscissaList[:-1] |
|
1334 | 1350 |
noise = dataOut.noise |
@@ -1337,7 +1353,7 class SpectralMoments(Operation): | |||
|
1337 | 1353 | |
|
1338 | 1354 |
for ind in range(nChannel): |
|
1339 | 1355 |
data_param[ind,:,:] = self.__calculateMoments( data[ind,:,:] , absc , noise[ind] ) |
|
1340 | ||
|
1356 | ||
|
1341 | 1357 |
dataOut.moments = data_param[:,1:,:] |
|
1342 | 1358 |
dataOut.data_SNR = data_param[:,0] |
|
1343 | 1359 |
dataOut.data_POW = data_param[:,1] |
@@ -1345,12 +1361,12 class SpectralMoments(Operation): | |||
|
1345 | 1361 |
dataOut.data_WIDTH = data_param[:,3] |
|
1346 | 1362 | |
|
1347 | 1363 |
return dataOut |
|
1348 | ||
|
1349 |
def __calculateMoments(self, oldspec, oldfreq, n0, |
|
|
1364 | ||
|
1365 | def __calculateMoments(self, oldspec, oldfreq, n0, | |
|
1350 | 1366 |
nicoh = None, graph = None, smooth = None, type1 = None, fwindow = None, snrth = None, dc = None, aliasing = None, oldfd = None, wwauto = None): |
|
1351 | ||
|
1367 | ||
|
1352 | 1368 |
if (nicoh is None): nicoh = 1 |
|
1353 |
if (graph is None): graph = 0 |
|
|
1369 | if (graph is None): graph = 0 | |
|
1354 | 1370 |
if (smooth is None): smooth = 0 |
|
1355 | 1371 |
elif (self.smooth < 3): smooth = 0 |
|
1356 | 1372 | |
@@ -1361,102 +1377,102 class SpectralMoments(Operation): | |||
|
1361 | 1377 |
if (aliasing is None): aliasing = 0 |
|
1362 | 1378 |
if (oldfd is None): oldfd = 0 |
|
1363 | 1379 |
if (wwauto is None): wwauto = 0 |
|
1364 | ||
|
1380 | ||
|
1365 | 1381 |
if (n0 < 1.e-20): n0 = 1.e-20 |
|
1366 | ||
|
1382 | ||
|
1367 | 1383 |
freq = oldfreq |
|
1368 | 1384 |
vec_power = numpy.zeros(oldspec.shape[1]) |
|
1369 | 1385 |
vec_fd = numpy.zeros(oldspec.shape[1]) |
|
1370 | 1386 |
vec_w = numpy.zeros(oldspec.shape[1]) |
|
1371 | 1387 |
vec_snr = numpy.zeros(oldspec.shape[1]) |
|
1372 | ||
|
1388 | ||
|
1373 | 1389 |
# oldspec = numpy.ma.masked_invalid(oldspec) |
|
1374 | ||
|
1390 | ||
|
1375 | 1391 |
for ind in range(oldspec.shape[1]): |
|
1376 | ||
|
1392 | ||
|
1377 | 1393 |
spec = oldspec[:,ind] |
|
1378 | 1394 |
aux = spec*fwindow |
|
1379 | 1395 |
max_spec = aux.max() |
|
1380 | 1396 |
m = aux.tolist().index(max_spec) |
|
1381 | ||
|
1382 |
#Smooth |
|
|
1397 | ||
|
1398 | #Smooth | |
|
1383 | 1399 |
if (smooth == 0): |
|
1384 | 1400 |
spec2 = spec |
|
1385 | 1401 |
else: |
|
1386 | 1402 |
spec2 = scipy.ndimage.filters.uniform_filter1d(spec,size=smooth) |
|
1387 | ||
|
1403 | ||
|
1388 | 1404 |
# Calculo de Momentos |
|
1389 | 1405 |
bb = spec2[numpy.arange(m,spec2.size)] |
|
1390 | 1406 |
bb = (bb<n0).nonzero() |
|
1391 | 1407 |
bb = bb[0] |
|
1392 | ||
|
1408 | ||
|
1393 | 1409 |
ss = spec2[numpy.arange(0,m + 1)] |
|
1394 | 1410 |
ss = (ss<n0).nonzero() |
|
1395 | 1411 |
ss = ss[0] |
|
1396 | ||
|
1412 | ||
|
1397 | 1413 |
if (bb.size == 0): |
|
1398 | 1414 |
bb0 = spec.size - 1 - m |
|
1399 |
else: |
|
|
1415 | else: | |
|
1400 | 1416 |
bb0 = bb[0] - 1 |
|
1401 | 1417 |
if (bb0 < 0): |
|
1402 | 1418 |
bb0 = 0 |
|
1403 | ||
|
1419 | ||
|
1404 | 1420 |
if (ss.size == 0): |
|
1405 | 1421 |
ss1 = 1 |
|
1406 | 1422 |
else: |
|
1407 | 1423 |
ss1 = max(ss) + 1 |
|
1408 | ||
|
1424 | ||
|
1409 | 1425 |
if (ss1 > m): |
|
1410 | 1426 |
ss1 = m |
|
1411 | ||
|
1412 |
valid = numpy.arange(int(m + bb0 - ss1 + 1)) + ss1 |
|
|
1413 | ||
|
1427 | ||
|
1428 | valid = numpy.arange(int(m + bb0 - ss1 + 1)) + ss1 | |
|
1429 | ||
|
1414 | 1430 |
power = ((spec2[valid] - n0) * fwindow[valid]).sum() |
|
1415 | 1431 |
fd = ((spec2[valid]- n0)*freq[valid] * fwindow[valid]).sum() / power |
|
1416 | 1432 |
w = numpy.sqrt(((spec2[valid] - n0)*fwindow[valid]*(freq[valid]- fd)**2).sum() / power) |
|
1417 | 1433 |
snr = (spec2.mean()-n0)/n0 |
|
1418 |
if (snr < 1.e-20) : |
|
|
1434 | if (snr < 1.e-20) : | |
|
1419 | 1435 |
snr = 1.e-20 |
|
1420 | ||
|
1436 | ||
|
1421 | 1437 |
vec_power[ind] = power |
|
1422 | 1438 |
vec_fd[ind] = fd |
|
1423 | 1439 |
vec_w[ind] = w |
|
1424 | 1440 |
vec_snr[ind] = snr |
|
1425 | 1441 | |
|
1426 | 1442 |
return numpy.vstack((vec_snr, vec_power, vec_fd, vec_w)) |
|
1427 | ||
|
1443 | ||
|
1428 | 1444 |
#------------------ Get SA Parameters -------------------------- |
|
1429 | ||
|
1445 | ||
|
1430 | 1446 |
def GetSAParameters(self): |
|
1431 | 1447 |
#SA en frecuencia |
|
1432 | 1448 |
pairslist = self.dataOut.groupList |
|
1433 | 1449 |
num_pairs = len(pairslist) |
|
1434 | ||
|
1450 | ||
|
1435 | 1451 |
vel = self.dataOut.abscissaList |
|
1436 | 1452 |
spectra = self.dataOut.data_pre |
|
1437 | 1453 |
cspectra = self.dataIn.data_cspc |
|
1438 |
delta_v = vel[1] - vel[0] |
|
|
1439 | ||
|
1454 | delta_v = vel[1] - vel[0] | |
|
1455 | ||
|
1440 | 1456 |
#Calculating the power spectrum |
|
1441 | 1457 |
spc_pow = numpy.sum(spectra, 3)*delta_v |
|
1442 | 1458 |
#Normalizing Spectra |
|
1443 | 1459 |
norm_spectra = spectra/spc_pow |
|
1444 | 1460 |
#Calculating the norm_spectra at peak |
|
1445 |
max_spectra = numpy.max(norm_spectra, 3) |
|
|
1446 | ||
|
1461 | max_spectra = numpy.max(norm_spectra, 3) | |
|
1462 | ||
|
1447 | 1463 |
#Normalizing Cross Spectra |
|
1448 | 1464 |
norm_cspectra = numpy.zeros(cspectra.shape) |
|
1449 | ||
|
1465 | ||
|
1450 | 1466 |
for i in range(num_chan): |
|
1451 | 1467 |
norm_cspectra[i,:,:] = cspectra[i,:,:]/numpy.sqrt(spc_pow[pairslist[i][0],:]*spc_pow[pairslist[i][1],:]) |
|
1452 | ||
|
1468 | ||
|
1453 | 1469 |
max_cspectra = numpy.max(norm_cspectra,2) |
|
1454 | 1470 |
max_cspectra_index = numpy.argmax(norm_cspectra, 2) |
|
1455 | ||
|
1471 | ||
|
1456 | 1472 |
for i in range(num_pairs): |
|
1457 | 1473 |
cspc_par[i,:,:] = __calculateMoments(norm_cspectra) |
|
1458 | 1474 |
#------------------- Get Lags ---------------------------------- |
|
1459 | ||
|
1475 | ||
|
1460 | 1476 |
class SALags(Operation): |
|
1461 | 1477 |
''' |
|
1462 | 1478 |
Function GetMoments() |
@@ -1469,19 +1485,19 class SALags(Operation): | |||
|
1469 | 1485 |
self.dataOut.data_SNR |
|
1470 | 1486 |
self.dataOut.groupList |
|
1471 | 1487 |
self.dataOut.nChannels |
|
1472 | ||
|
1488 | ||
|
1473 | 1489 |
Affected: |
|
1474 | 1490 |
self.dataOut.data_param |
|
1475 | ||
|
1491 | ||
|
1476 | 1492 |
''' |
|
1477 |
def run(self, dataOut): |
|
|
1493 | def run(self, dataOut): | |
|
1478 | 1494 |
data_acf = dataOut.data_pre[0] |
|
1479 | 1495 |
data_ccf = dataOut.data_pre[1] |
|
1480 | 1496 |
normFactor_acf = dataOut.normFactor[0] |
|
1481 | 1497 |
normFactor_ccf = dataOut.normFactor[1] |
|
1482 | 1498 |
pairs_acf = dataOut.groupList[0] |
|
1483 | 1499 |
pairs_ccf = dataOut.groupList[1] |
|
1484 | ||
|
1500 | ||
|
1485 | 1501 |
nHeights = dataOut.nHeights |
|
1486 | 1502 |
absc = dataOut.abscissaList |
|
1487 | 1503 |
noise = dataOut.noise |
@@ -1492,97 +1508,97 class SALags(Operation): | |||
|
1492 | 1508 | |
|
1493 | 1509 |
for l in range(len(pairs_acf)): |
|
1494 | 1510 |
data_acf[l,:,:] = data_acf[l,:,:]/normFactor_acf[l,:] |
|
1495 | ||
|
1511 | ||
|
1496 | 1512 |
for l in range(len(pairs_ccf)): |
|
1497 | 1513 |
data_ccf[l,:,:] = data_ccf[l,:,:]/normFactor_ccf[l,:] |
|
1498 | ||
|
1514 | ||
|
1499 | 1515 |
dataOut.data_param = numpy.zeros((len(pairs_ccf)*2 + 1, nHeights)) |
|
1500 | 1516 |
dataOut.data_param[:-1,:] = self.__calculateTaus(data_acf, data_ccf, absc) |
|
1501 | 1517 |
dataOut.data_param[-1,:] = self.__calculateLag1Phase(data_acf, absc) |
|
1502 | 1518 |
return |
|
1503 | ||
|
1519 | ||
|
1504 | 1520 |
# def __getPairsAutoCorr(self, pairsList, nChannels): |
|
1505 | # | |
|
1521 | # | |
|
1506 | 1522 |
# pairsAutoCorr = numpy.zeros(nChannels, dtype = 'int')*numpy.nan |
|
1507 | # | |
|
1508 |
# for l in range(len(pairsList)): |
|
|
1523 | # | |
|
1524 | # for l in range(len(pairsList)): | |
|
1509 | 1525 |
# firstChannel = pairsList[l][0] |
|
1510 | 1526 |
# secondChannel = pairsList[l][1] |
|
1511 | # | |
|
1512 |
# #Obteniendo pares de Autocorrelacion |
|
|
1527 | # | |
|
1528 | # #Obteniendo pares de Autocorrelacion | |
|
1513 | 1529 |
# if firstChannel == secondChannel: |
|
1514 | 1530 |
# pairsAutoCorr[firstChannel] = int(l) |
|
1515 | # | |
|
1531 | # | |
|
1516 | 1532 |
# pairsAutoCorr = pairsAutoCorr.astype(int) |
|
1517 | # | |
|
1533 | # | |
|
1518 | 1534 |
# pairsCrossCorr = range(len(pairsList)) |
|
1519 | 1535 |
# pairsCrossCorr = numpy.delete(pairsCrossCorr,pairsAutoCorr) |
|
1520 | # | |
|
1536 | # | |
|
1521 | 1537 |
# return pairsAutoCorr, pairsCrossCorr |
|
1522 | ||
|
1538 | ||
|
1523 | 1539 |
def __calculateTaus(self, data_acf, data_ccf, lagRange): |
|
1524 | ||
|
1540 | ||
|
1525 | 1541 |
lag0 = data_acf.shape[1]/2 |
|
1526 | 1542 |
#Funcion de Autocorrelacion |
|
1527 | 1543 |
mean_acf = stats.nanmean(data_acf, axis = 0) |
|
1528 | ||
|
1544 | ||
|
1529 | 1545 |
#Obtencion Indice de TauCross |
|
1530 | 1546 |
ind_ccf = data_ccf.argmax(axis = 1) |
|
1531 | 1547 |
#Obtencion Indice de TauAuto |
|
1532 | 1548 |
ind_acf = numpy.zeros(ind_ccf.shape,dtype = 'int') |
|
1533 | 1549 |
ccf_lag0 = data_ccf[:,lag0,:] |
|
1534 | ||
|
1550 | ||
|
1535 | 1551 |
for i in range(ccf_lag0.shape[0]): |
|
1536 | 1552 |
ind_acf[i,:] = numpy.abs(mean_acf - ccf_lag0[i,:]).argmin(axis = 0) |
|
1537 | ||
|
1553 | ||
|
1538 | 1554 |
#Obtencion de TauCross y TauAuto |
|
1539 | 1555 |
tau_ccf = lagRange[ind_ccf] |
|
1540 | 1556 |
tau_acf = lagRange[ind_acf] |
|
1541 | ||
|
1557 | ||
|
1542 | 1558 |
Nan1, Nan2 = numpy.where(tau_ccf == lagRange[0]) |
|
1543 | ||
|
1559 | ||
|
1544 | 1560 |
tau_ccf[Nan1,Nan2] = numpy.nan |
|
1545 | 1561 |
tau_acf[Nan1,Nan2] = numpy.nan |
|
1546 | 1562 |
tau = numpy.vstack((tau_ccf,tau_acf)) |
|
1547 | ||
|
1563 | ||
|
1548 | 1564 |
return tau |
|
1549 | ||
|
1565 | ||
|
1550 | 1566 |
def __calculateLag1Phase(self, data, lagTRange): |
|
1551 | 1567 |
data1 = stats.nanmean(data, axis = 0) |
|
1552 | 1568 |
lag1 = numpy.where(lagTRange == 0)[0][0] + 1 |
|
1553 | 1569 | |
|
1554 | 1570 |
phase = numpy.angle(data1[lag1,:]) |
|
1555 | ||
|
1571 | ||
|
1556 | 1572 |
return phase |
|
1557 | ||
|
1573 | ||
|
1558 | 1574 |
class SpectralFitting(Operation): |
|
1559 | 1575 |
''' |
|
1560 | 1576 |
Function GetMoments() |
|
1561 | ||
|
1577 | ||
|
1562 | 1578 |
Input: |
|
1563 | 1579 |
Output: |
|
1564 | 1580 |
Variables modified: |
|
1565 | 1581 |
''' |
|
1566 | ||
|
1567 |
def run(self, dataOut, getSNR = True, path=None, file=None, groupList=None): |
|
|
1568 | ||
|
1569 | ||
|
1582 | ||
|
1583 | def run(self, dataOut, getSNR = True, path=None, file=None, groupList=None): | |
|
1584 | ||
|
1585 | ||
|
1570 | 1586 |
if path != None: |
|
1571 | 1587 |
sys.path.append(path) |
|
1572 | 1588 |
self.dataOut.library = importlib.import_module(file) |
|
1573 | ||
|
1589 | ||
|
1574 | 1590 |
#To be inserted as a parameter |
|
1575 | 1591 |
groupArray = numpy.array(groupList) |
|
1576 |
# groupArray = numpy.array([[0,1],[2,3]]) |
|
|
1592 | # groupArray = numpy.array([[0,1],[2,3]]) | |
|
1577 | 1593 |
self.dataOut.groupList = groupArray |
|
1578 | ||
|
1594 | ||
|
1579 | 1595 |
nGroups = groupArray.shape[0] |
|
1580 | 1596 |
nChannels = self.dataIn.nChannels |
|
1581 | 1597 |
nHeights=self.dataIn.heightList.size |
|
1582 | ||
|
1598 | ||
|
1583 | 1599 |
#Parameters Array |
|
1584 | 1600 |
self.dataOut.data_param = None |
|
1585 | ||
|
1601 | ||
|
1586 | 1602 |
#Set constants |
|
1587 | 1603 |
constants = self.dataOut.library.setConstants(self.dataIn) |
|
1588 | 1604 |
self.dataOut.constants = constants |
@@ -1591,24 +1607,24 class SpectralFitting(Operation): | |||
|
1591 | 1607 |
ippSeconds = self.dataIn.ippSeconds |
|
1592 | 1608 |
K = self.dataIn.nIncohInt |
|
1593 | 1609 |
pairsArray = numpy.array(self.dataIn.pairsList) |
|
1594 | ||
|
1610 | ||
|
1595 | 1611 |
#List of possible combinations |
|
1596 | 1612 |
listComb = itertools.combinations(numpy.arange(groupArray.shape[1]),2) |
|
1597 | 1613 |
indCross = numpy.zeros(len(list(listComb)), dtype = 'int') |
|
1598 | ||
|
1614 | ||
|
1599 | 1615 |
if getSNR: |
|
1600 | 1616 |
listChannels = groupArray.reshape((groupArray.size)) |
|
1601 | 1617 |
listChannels.sort() |
|
1602 | 1618 |
noise = self.dataIn.getNoise() |
|
1603 | 1619 |
self.dataOut.data_SNR = self.__getSNR(self.dataIn.data_spc[listChannels,:,:], noise[listChannels]) |
|
1604 | ||
|
1605 |
for i in range(nGroups): |
|
|
1620 | ||
|
1621 | for i in range(nGroups): | |
|
1606 | 1622 |
coord = groupArray[i,:] |
|
1607 | ||
|
1623 | ||
|
1608 | 1624 |
#Input data array |
|
1609 | 1625 |
data = self.dataIn.data_spc[coord,:,:]/(M*N) |
|
1610 | 1626 |
data = data.reshape((data.shape[0]*data.shape[1],data.shape[2])) |
|
1611 | ||
|
1627 | ||
|
1612 | 1628 |
#Cross Spectra data array for Covariance Matrixes |
|
1613 | 1629 |
ind = 0 |
|
1614 | 1630 |
for pairs in listComb: |
@@ -1617,9 +1633,9 class SpectralFitting(Operation): | |||
|
1617 | 1633 |
ind += 1 |
|
1618 | 1634 |
dataCross = self.dataIn.data_cspc[indCross,:,:]/(M*N) |
|
1619 | 1635 |
dataCross = dataCross**2/K |
|
1620 | ||
|
1636 | ||
|
1621 | 1637 |
for h in range(nHeights): |
|
1622 | ||
|
1638 | ||
|
1623 | 1639 |
#Input |
|
1624 | 1640 |
d = data[:,h] |
|
1625 | 1641 | |
@@ -1628,7 +1644,7 class SpectralFitting(Operation): | |||
|
1628 | 1644 |
ind = 0 |
|
1629 | 1645 |
for pairs in listComb: |
|
1630 | 1646 |
#Coordinates in Covariance Matrix |
|
1631 |
x = pairs[0] |
|
|
1647 | x = pairs[0] | |
|
1632 | 1648 |
y = pairs[1] |
|
1633 | 1649 |
#Channel Index |
|
1634 | 1650 |
S12 = dataCross[ind,:,h] |
@@ -1642,15 +1658,15 class SpectralFitting(Operation): | |||
|
1642 | 1658 |
LT=L.T |
|
1643 | 1659 | |
|
1644 | 1660 |
dp = numpy.dot(LT,d) |
|
1645 | ||
|
1661 | ||
|
1646 | 1662 |
#Initial values |
|
1647 | 1663 |
data_spc = self.dataIn.data_spc[coord,:,h] |
|
1648 | ||
|
1664 | ||
|
1649 | 1665 |
if (h>0)and(error1[3]<5): |
|
1650 | 1666 |
p0 = self.dataOut.data_param[i,:,h-1] |
|
1651 | 1667 |
else: |
|
1652 | 1668 |
p0 = numpy.array(self.dataOut.library.initialValuesFunction(data_spc, constants, i)) |
|
1653 | ||
|
1669 | ||
|
1654 | 1670 |
try: |
|
1655 | 1671 |
#Least Squares |
|
1656 | 1672 |
minp,covp,infodict,mesg,ier = optimize.leastsq(self.__residFunction,p0,args=(dp,LT,constants),full_output=True) |
@@ -1663,30 +1679,30 class SpectralFitting(Operation): | |||
|
1663 | 1679 |
minp = p0*numpy.nan |
|
1664 | 1680 |
error0 = numpy.nan |
|
1665 | 1681 |
error1 = p0*numpy.nan |
|
1666 | ||
|
1682 | ||
|
1667 | 1683 |
#Save |
|
1668 | 1684 |
if self.dataOut.data_param is None: |
|
1669 | 1685 |
self.dataOut.data_param = numpy.zeros((nGroups, p0.size, nHeights))*numpy.nan |
|
1670 | 1686 |
self.dataOut.data_error = numpy.zeros((nGroups, p0.size + 1, nHeights))*numpy.nan |
|
1671 | ||
|
1687 | ||
|
1672 | 1688 |
self.dataOut.data_error[i,:,h] = numpy.hstack((error0,error1)) |
|
1673 | 1689 |
self.dataOut.data_param[i,:,h] = minp |
|
1674 | 1690 |
return |
|
1675 | ||
|
1691 | ||
|
1676 | 1692 |
def __residFunction(self, p, dp, LT, constants): |
|
1677 | 1693 | |
|
1678 | 1694 |
fm = self.dataOut.library.modelFunction(p, constants) |
|
1679 | 1695 |
fmp=numpy.dot(LT,fm) |
|
1680 | ||
|
1696 | ||
|
1681 | 1697 |
return dp-fmp |
|
1682 | 1698 | |
|
1683 | 1699 |
def __getSNR(self, z, noise): |
|
1684 | ||
|
1700 | ||
|
1685 | 1701 |
avg = numpy.average(z, axis=1) |
|
1686 | 1702 |
SNR = (avg.T-noise)/noise |
|
1687 | 1703 |
SNR = SNR.T |
|
1688 | 1704 |
return SNR |
|
1689 | ||
|
1705 | ||
|
1690 | 1706 |
def __chisq(p,chindex,hindex): |
|
1691 | 1707 |
#similar to Resid but calculates CHI**2 |
|
1692 | 1708 |
[LT,d,fm]=setupLTdfm(p,chindex,hindex) |
@@ -1694,53 +1710,53 class SpectralFitting(Operation): | |||
|
1694 | 1710 |
fmp=numpy.dot(LT,fm) |
|
1695 | 1711 |
chisq=numpy.dot((dp-fmp).T,(dp-fmp)) |
|
1696 | 1712 |
return chisq |
|
1697 | ||
|
1713 | ||
|
1698 | 1714 |
class WindProfiler(Operation): |
|
1699 | ||
|
1715 | ||
|
1700 | 1716 |
__isConfig = False |
|
1701 | ||
|
1717 | ||
|
1702 | 1718 |
__initime = None |
|
1703 | 1719 |
__lastdatatime = None |
|
1704 | 1720 |
__integrationtime = None |
|
1705 | ||
|
1721 | ||
|
1706 | 1722 |
__buffer = None |
|
1707 | ||
|
1723 | ||
|
1708 | 1724 |
__dataReady = False |
|
1709 | ||
|
1725 | ||
|
1710 | 1726 |
__firstdata = None |
|
1711 | ||
|
1727 | ||
|
1712 | 1728 |
n = None |
|
1713 | ||
|
1714 |
def __init__(self): |
|
|
1729 | ||
|
1730 | def __init__(self): | |
|
1715 | 1731 |
Operation.__init__(self) |
|
1716 | ||
|
1732 | ||
|
1717 | 1733 |
def __calculateCosDir(self, elev, azim): |
|
1718 | 1734 |
zen = (90 - elev)*numpy.pi/180 |
|
1719 | 1735 |
azim = azim*numpy.pi/180 |
|
1720 |
cosDirX = numpy.sqrt((1-numpy.cos(zen)**2)/((1+numpy.tan(azim)**2))) |
|
|
1736 | cosDirX = numpy.sqrt((1-numpy.cos(zen)**2)/((1+numpy.tan(azim)**2))) | |
|
1721 | 1737 |
cosDirY = numpy.sqrt(1-numpy.cos(zen)**2-cosDirX**2) |
|
1722 | ||
|
1738 | ||
|
1723 | 1739 |
signX = numpy.sign(numpy.cos(azim)) |
|
1724 | 1740 |
signY = numpy.sign(numpy.sin(azim)) |
|
1725 | ||
|
1741 | ||
|
1726 | 1742 |
cosDirX = numpy.copysign(cosDirX, signX) |
|
1727 | 1743 |
cosDirY = numpy.copysign(cosDirY, signY) |
|
1728 | 1744 |
return cosDirX, cosDirY |
|
1729 | ||
|
1745 | ||
|
1730 | 1746 |
def __calculateAngles(self, theta_x, theta_y, azimuth): |
|
1731 | ||
|
1747 | ||
|
1732 | 1748 |
dir_cosw = numpy.sqrt(1-theta_x**2-theta_y**2) |
|
1733 | 1749 |
zenith_arr = numpy.arccos(dir_cosw) |
|
1734 | 1750 |
azimuth_arr = numpy.arctan2(theta_x,theta_y) + azimuth*math.pi/180 |
|
1735 | ||
|
1751 | ||
|
1736 | 1752 |
dir_cosu = numpy.sin(azimuth_arr)*numpy.sin(zenith_arr) |
|
1737 | 1753 |
dir_cosv = numpy.cos(azimuth_arr)*numpy.sin(zenith_arr) |
|
1738 | ||
|
1754 | ||
|
1739 | 1755 |
return azimuth_arr, zenith_arr, dir_cosu, dir_cosv, dir_cosw |
|
1740 | 1756 | |
|
1741 | 1757 |
def __calculateMatA(self, dir_cosu, dir_cosv, dir_cosw, horOnly): |
|
1742 | ||
|
1743 | # | |
|
1758 | ||
|
1759 | # | |
|
1744 | 1760 |
if horOnly: |
|
1745 | 1761 |
A = numpy.c_[dir_cosu,dir_cosv] |
|
1746 | 1762 |
else: |
@@ -1754,37 +1770,37 class WindProfiler(Operation): | |||
|
1754 | 1770 |
listPhi = phi.tolist() |
|
1755 | 1771 |
maxid = listPhi.index(max(listPhi)) |
|
1756 | 1772 |
minid = listPhi.index(min(listPhi)) |
|
1757 | ||
|
1758 |
rango = list(range(len(phi))) |
|
|
1773 | ||
|
1774 | rango = list(range(len(phi))) | |
|
1759 | 1775 |
# rango = numpy.delete(rango,maxid) |
|
1760 | ||
|
1776 | ||
|
1761 | 1777 |
heiRang1 = heiRang*math.cos(phi[maxid]) |
|
1762 | 1778 |
heiRangAux = heiRang*math.cos(phi[minid]) |
|
1763 | 1779 |
indOut = (heiRang1 < heiRangAux[0]).nonzero() |
|
1764 | 1780 |
heiRang1 = numpy.delete(heiRang1,indOut) |
|
1765 | ||
|
1781 | ||
|
1766 | 1782 |
velRadial1 = numpy.zeros([len(phi),len(heiRang1)]) |
|
1767 | 1783 |
SNR1 = numpy.zeros([len(phi),len(heiRang1)]) |
|
1768 | ||
|
1784 | ||
|
1769 | 1785 |
for i in rango: |
|
1770 | 1786 |
x = heiRang*math.cos(phi[i]) |
|
1771 | 1787 |
y1 = velRadial[i,:] |
|
1772 | 1788 |
f1 = interpolate.interp1d(x,y1,kind = 'cubic') |
|
1773 | ||
|
1789 | ||
|
1774 | 1790 |
x1 = heiRang1 |
|
1775 | 1791 |
y11 = f1(x1) |
|
1776 | ||
|
1792 | ||
|
1777 | 1793 |
y2 = SNR[i,:] |
|
1778 | 1794 |
f2 = interpolate.interp1d(x,y2,kind = 'cubic') |
|
1779 | 1795 |
y21 = f2(x1) |
|
1780 | ||
|
1796 | ||
|
1781 | 1797 |
velRadial1[i,:] = y11 |
|
1782 | 1798 |
SNR1[i,:] = y21 |
|
1783 | ||
|
1799 | ||
|
1784 | 1800 |
return heiRang1, velRadial1, SNR1 |
|
1785 | 1801 | |
|
1786 | 1802 |
def __calculateVelUVW(self, A, velRadial): |
|
1787 | ||
|
1803 | ||
|
1788 | 1804 |
#Operacion Matricial |
|
1789 | 1805 |
# velUVW = numpy.zeros((velRadial.shape[1],3)) |
|
1790 | 1806 |
# for ind in range(velRadial.shape[1]): |
@@ -1792,27 +1808,27 class WindProfiler(Operation): | |||
|
1792 | 1808 |
# velUVW = velUVW.transpose() |
|
1793 | 1809 |
velUVW = numpy.zeros((A.shape[0],velRadial.shape[1])) |
|
1794 | 1810 |
velUVW[:,:] = numpy.dot(A,velRadial) |
|
1795 | ||
|
1796 | ||
|
1811 | ||
|
1812 | ||
|
1797 | 1813 |
return velUVW |
|
1798 | ||
|
1814 | ||
|
1799 | 1815 |
# def techniqueDBS(self, velRadial0, dirCosx, disrCosy, azimuth, correct, horizontalOnly, heiRang, SNR0): |
|
1800 | ||
|
1816 | ||
|
1801 | 1817 |
def techniqueDBS(self, kwargs): |
|
1802 | 1818 |
""" |
|
1803 | 1819 |
Function that implements Doppler Beam Swinging (DBS) technique. |
|
1804 | ||
|
1820 | ||
|
1805 | 1821 |
Input: Radial velocities, Direction cosines (x and y) of the Beam, Antenna azimuth, |
|
1806 | 1822 |
Direction correction (if necessary), Ranges and SNR |
|
1807 | ||
|
1823 | ||
|
1808 | 1824 |
Output: Winds estimation (Zonal, Meridional and Vertical) |
|
1809 | ||
|
1825 | ||
|
1810 | 1826 |
Parameters affected: Winds, height range, SNR |
|
1811 | 1827 |
""" |
|
1812 | 1828 |
velRadial0 = kwargs['velRadial'] |
|
1813 | 1829 |
heiRang = kwargs['heightList'] |
|
1814 | 1830 |
SNR0 = kwargs['SNR'] |
|
1815 | ||
|
1831 | ||
|
1816 | 1832 |
if 'dirCosx' in kwargs and 'dirCosy' in kwargs: |
|
1817 | 1833 |
theta_x = numpy.array(kwargs['dirCosx']) |
|
1818 | 1834 |
theta_y = numpy.array(kwargs['dirCosy']) |
@@ -1820,7 +1836,7 class WindProfiler(Operation): | |||
|
1820 | 1836 |
elev = numpy.array(kwargs['elevation']) |
|
1821 | 1837 |
azim = numpy.array(kwargs['azimuth']) |
|
1822 | 1838 |
theta_x, theta_y = self.__calculateCosDir(elev, azim) |
|
1823 |
azimuth = kwargs['correctAzimuth'] |
|
|
1839 | azimuth = kwargs['correctAzimuth'] | |
|
1824 | 1840 |
if 'horizontalOnly' in kwargs: |
|
1825 | 1841 |
horizontalOnly = kwargs['horizontalOnly'] |
|
1826 | 1842 |
else: horizontalOnly = False |
@@ -1835,22 +1851,22 class WindProfiler(Operation): | |||
|
1835 | 1851 |
param = param[arrayChannel,:,:] |
|
1836 | 1852 |
theta_x = theta_x[arrayChannel] |
|
1837 | 1853 |
theta_y = theta_y[arrayChannel] |
|
1838 | ||
|
1839 |
azimuth_arr, zenith_arr, dir_cosu, dir_cosv, dir_cosw = self.__calculateAngles(theta_x, theta_y, azimuth) |
|
|
1840 |
heiRang1, velRadial1, SNR1 = self.__correctValues(heiRang, zenith_arr, correctFactor*velRadial0, SNR0) |
|
|
1854 | ||
|
1855 | azimuth_arr, zenith_arr, dir_cosu, dir_cosv, dir_cosw = self.__calculateAngles(theta_x, theta_y, azimuth) | |
|
1856 | heiRang1, velRadial1, SNR1 = self.__correctValues(heiRang, zenith_arr, correctFactor*velRadial0, SNR0) | |
|
1841 | 1857 |
A = self.__calculateMatA(dir_cosu, dir_cosv, dir_cosw, horizontalOnly) |
|
1842 | ||
|
1858 | ||
|
1843 | 1859 |
#Calculo de Componentes de la velocidad con DBS |
|
1844 | 1860 |
winds = self.__calculateVelUVW(A,velRadial1) |
|
1845 | ||
|
1861 | ||
|
1846 | 1862 |
return winds, heiRang1, SNR1 |
|
1847 | ||
|
1863 | ||
|
1848 | 1864 |
def __calculateDistance(self, posx, posy, pairs_ccf, azimuth = None): |
|
1849 | ||
|
1865 | ||
|
1850 | 1866 |
nPairs = len(pairs_ccf) |
|
1851 | 1867 |
posx = numpy.asarray(posx) |
|
1852 | 1868 |
posy = numpy.asarray(posy) |
|
1853 | ||
|
1869 | ||
|
1854 | 1870 |
#Rotacion Inversa para alinear con el azimuth |
|
1855 | 1871 |
if azimuth!= None: |
|
1856 | 1872 |
azimuth = azimuth*math.pi/180 |
@@ -1859,126 +1875,126 class WindProfiler(Operation): | |||
|
1859 | 1875 |
else: |
|
1860 | 1876 |
posx1 = posx |
|
1861 | 1877 |
posy1 = posy |
|
1862 | ||
|
1878 | ||
|
1863 | 1879 |
#Calculo de Distancias |
|
1864 | 1880 |
distx = numpy.zeros(nPairs) |
|
1865 | 1881 |
disty = numpy.zeros(nPairs) |
|
1866 | 1882 |
dist = numpy.zeros(nPairs) |
|
1867 | 1883 |
ang = numpy.zeros(nPairs) |
|
1868 | ||
|
1884 | ||
|
1869 | 1885 |
for i in range(nPairs): |
|
1870 | 1886 |
distx[i] = posx1[pairs_ccf[i][1]] - posx1[pairs_ccf[i][0]] |
|
1871 |
disty[i] = posy1[pairs_ccf[i][1]] - posy1[pairs_ccf[i][0]] |
|
|
1887 | disty[i] = posy1[pairs_ccf[i][1]] - posy1[pairs_ccf[i][0]] | |
|
1872 | 1888 |
dist[i] = numpy.sqrt(distx[i]**2 + disty[i]**2) |
|
1873 | 1889 |
ang[i] = numpy.arctan2(disty[i],distx[i]) |
|
1874 | ||
|
1890 | ||
|
1875 | 1891 |
return distx, disty, dist, ang |
|
1876 |
#Calculo de Matrices |
|
|
1892 | #Calculo de Matrices | |
|
1877 | 1893 |
# nPairs = len(pairs) |
|
1878 | 1894 |
# ang1 = numpy.zeros((nPairs, 2, 1)) |
|
1879 | 1895 |
# dist1 = numpy.zeros((nPairs, 2, 1)) |
|
1880 | # | |
|
1896 | # | |
|
1881 | 1897 |
# for j in range(nPairs): |
|
1882 | 1898 |
# dist1[j,0,0] = dist[pairs[j][0]] |
|
1883 | 1899 |
# dist1[j,1,0] = dist[pairs[j][1]] |
|
1884 | 1900 |
# ang1[j,0,0] = ang[pairs[j][0]] |
|
1885 | 1901 |
# ang1[j,1,0] = ang[pairs[j][1]] |
|
1886 | # | |
|
1902 | # | |
|
1887 | 1903 |
# return distx,disty, dist1,ang1 |
|
1888 | 1904 | |
|
1889 | ||
|
1905 | ||
|
1890 | 1906 |
def __calculateVelVer(self, phase, lagTRange, _lambda): |
|
1891 | 1907 | |
|
1892 | 1908 |
Ts = lagTRange[1] - lagTRange[0] |
|
1893 | 1909 |
velW = -_lambda*phase/(4*math.pi*Ts) |
|
1894 | ||
|
1910 | ||
|
1895 | 1911 |
return velW |
|
1896 | ||
|
1912 | ||
|
1897 | 1913 |
def __calculateVelHorDir(self, dist, tau1, tau2, ang): |
|
1898 | 1914 |
nPairs = tau1.shape[0] |
|
1899 | 1915 |
nHeights = tau1.shape[1] |
|
1900 |
vel = numpy.zeros((nPairs,3,nHeights)) |
|
|
1916 | vel = numpy.zeros((nPairs,3,nHeights)) | |
|
1901 | 1917 |
dist1 = numpy.reshape(dist, (dist.size,1)) |
|
1902 | ||
|
1918 | ||
|
1903 | 1919 |
angCos = numpy.cos(ang) |
|
1904 | 1920 |
angSin = numpy.sin(ang) |
|
1905 | ||
|
1906 |
vel0 = dist1*tau1/(2*tau2**2) |
|
|
1921 | ||
|
1922 | vel0 = dist1*tau1/(2*tau2**2) | |
|
1907 | 1923 |
vel[:,0,:] = (vel0*angCos).sum(axis = 1) |
|
1908 | 1924 |
vel[:,1,:] = (vel0*angSin).sum(axis = 1) |
|
1909 | ||
|
1925 | ||
|
1910 | 1926 |
ind = numpy.where(numpy.isinf(vel)) |
|
1911 | 1927 |
vel[ind] = numpy.nan |
|
1912 | ||
|
1928 | ||
|
1913 | 1929 |
return vel |
|
1914 | ||
|
1930 | ||
|
1915 | 1931 |
# def __getPairsAutoCorr(self, pairsList, nChannels): |
|
1916 | # | |
|
1932 | # | |
|
1917 | 1933 |
# pairsAutoCorr = numpy.zeros(nChannels, dtype = 'int')*numpy.nan |
|
1918 | # | |
|
1919 |
# for l in range(len(pairsList)): |
|
|
1934 | # | |
|
1935 | # for l in range(len(pairsList)): | |
|
1920 | 1936 |
# firstChannel = pairsList[l][0] |
|
1921 | 1937 |
# secondChannel = pairsList[l][1] |
|
1922 | # | |
|
1923 |
# #Obteniendo pares de Autocorrelacion |
|
|
1938 | # | |
|
1939 | # #Obteniendo pares de Autocorrelacion | |
|
1924 | 1940 |
# if firstChannel == secondChannel: |
|
1925 | 1941 |
# pairsAutoCorr[firstChannel] = int(l) |
|
1926 | # | |
|
1942 | # | |
|
1927 | 1943 |
# pairsAutoCorr = pairsAutoCorr.astype(int) |
|
1928 | # | |
|
1944 | # | |
|
1929 | 1945 |
# pairsCrossCorr = range(len(pairsList)) |
|
1930 | 1946 |
# pairsCrossCorr = numpy.delete(pairsCrossCorr,pairsAutoCorr) |
|
1931 | # | |
|
1947 | # | |
|
1932 | 1948 |
# return pairsAutoCorr, pairsCrossCorr |
|
1933 | ||
|
1949 | ||
|
1934 | 1950 |
# def techniqueSA(self, pairsSelected, pairsList, nChannels, tau, azimuth, _lambda, position_x, position_y, lagTRange, correctFactor): |
|
1935 | 1951 |
def techniqueSA(self, kwargs): |
|
1936 | ||
|
1937 |
""" |
|
|
1952 | ||
|
1953 | """ | |
|
1938 | 1954 |
Function that implements Spaced Antenna (SA) technique. |
|
1939 | ||
|
1955 | ||
|
1940 | 1956 |
Input: Radial velocities, Direction cosines (x and y) of the Beam, Antenna azimuth, |
|
1941 | 1957 |
Direction correction (if necessary), Ranges and SNR |
|
1942 | ||
|
1958 | ||
|
1943 | 1959 |
Output: Winds estimation (Zonal, Meridional and Vertical) |
|
1944 | ||
|
1960 | ||
|
1945 | 1961 |
Parameters affected: Winds |
|
1946 | 1962 |
""" |
|
1947 | 1963 |
position_x = kwargs['positionX'] |
|
1948 | 1964 |
position_y = kwargs['positionY'] |
|
1949 | 1965 |
azimuth = kwargs['azimuth'] |
|
1950 | ||
|
1966 | ||
|
1951 | 1967 |
if 'correctFactor' in kwargs: |
|
1952 | 1968 |
correctFactor = kwargs['correctFactor'] |
|
1953 | 1969 |
else: |
|
1954 | 1970 |
correctFactor = 1 |
|
1955 | ||
|
1971 | ||
|
1956 | 1972 |
groupList = kwargs['groupList'] |
|
1957 | 1973 |
pairs_ccf = groupList[1] |
|
1958 | 1974 |
tau = kwargs['tau'] |
|
1959 | 1975 |
_lambda = kwargs['_lambda'] |
|
1960 | ||
|
1976 | ||
|
1961 | 1977 |
#Cross Correlation pairs obtained |
|
1962 | 1978 |
# pairsAutoCorr, pairsCrossCorr = self.__getPairsAutoCorr(pairssList, nChannels) |
|
1963 | 1979 |
# pairsArray = numpy.array(pairsList)[pairsCrossCorr] |
|
1964 | 1980 |
# pairsSelArray = numpy.array(pairsSelected) |
|
1965 | 1981 |
# pairs = [] |
|
1966 | # | |
|
1982 | # | |
|
1967 | 1983 |
# #Wind estimation pairs obtained |
|
1968 | 1984 |
# for i in range(pairsSelArray.shape[0]/2): |
|
1969 | 1985 |
# ind1 = numpy.where(numpy.all(pairsArray == pairsSelArray[2*i], axis = 1))[0][0] |
|
1970 | 1986 |
# ind2 = numpy.where(numpy.all(pairsArray == pairsSelArray[2*i + 1], axis = 1))[0][0] |
|
1971 | 1987 |
# pairs.append((ind1,ind2)) |
|
1972 | ||
|
1988 | ||
|
1973 | 1989 |
indtau = tau.shape[0]/2 |
|
1974 | 1990 |
tau1 = tau[:indtau,:] |
|
1975 | 1991 |
tau2 = tau[indtau:-1,:] |
|
1976 | 1992 |
# tau1 = tau1[pairs,:] |
|
1977 | 1993 |
# tau2 = tau2[pairs,:] |
|
1978 | 1994 |
phase1 = tau[-1,:] |
|
1979 | ||
|
1995 | ||
|
1980 | 1996 |
#--------------------------------------------------------------------- |
|
1981 |
#Metodo Directo |
|
|
1997 | #Metodo Directo | |
|
1982 | 1998 |
distx, disty, dist, ang = self.__calculateDistance(position_x, position_y, pairs_ccf,azimuth) |
|
1983 | 1999 |
winds = self.__calculateVelHorDir(dist, tau1, tau2, ang) |
|
1984 | 2000 |
winds = stats.nanmean(winds, axis=0) |
@@ -1994,97 +2010,97 class WindProfiler(Operation): | |||
|
1994 | 2010 |
winds[2,:] = self.__calculateVelVer(phase1, lagTRange, _lambda) |
|
1995 | 2011 |
winds = correctFactor*winds |
|
1996 | 2012 |
return winds |
|
1997 | ||
|
2013 | ||
|
1998 | 2014 |
def __checkTime(self, currentTime, paramInterval, outputInterval): |
|
1999 | ||
|
2015 | ||
|
2000 | 2016 |
dataTime = currentTime + paramInterval |
|
2001 | 2017 |
deltaTime = dataTime - self.__initime |
|
2002 | ||
|
2018 | ||
|
2003 | 2019 |
if deltaTime >= outputInterval or deltaTime < 0: |
|
2004 | 2020 |
self.__dataReady = True |
|
2005 |
return |
|
|
2006 | ||
|
2021 | return | |
|
2022 | ||
|
2007 | 2023 |
def techniqueMeteors(self, arrayMeteor, meteorThresh, heightMin, heightMax): |
|
2008 | 2024 |
''' |
|
2009 | 2025 |
Function that implements winds estimation technique with detected meteors. |
|
2010 | ||
|
2026 | ||
|
2011 | 2027 |
Input: Detected meteors, Minimum meteor quantity to wind estimation |
|
2012 | ||
|
2028 | ||
|
2013 | 2029 |
Output: Winds estimation (Zonal and Meridional) |
|
2014 | ||
|
2030 | ||
|
2015 | 2031 |
Parameters affected: Winds |
|
2016 |
''' |
|
|
2032 | ''' | |
|
2017 | 2033 |
#Settings |
|
2018 | 2034 |
nInt = (heightMax - heightMin)/2 |
|
2019 | 2035 |
nInt = int(nInt) |
|
2020 |
winds = numpy.zeros((2,nInt))*numpy.nan |
|
|
2021 | ||
|
2036 | winds = numpy.zeros((2,nInt))*numpy.nan | |
|
2037 | ||
|
2022 | 2038 |
#Filter errors |
|
2023 | 2039 |
error = numpy.where(arrayMeteor[:,-1] == 0)[0] |
|
2024 | 2040 |
finalMeteor = arrayMeteor[error,:] |
|
2025 | ||
|
2041 | ||
|
2026 | 2042 |
#Meteor Histogram |
|
2027 | 2043 |
finalHeights = finalMeteor[:,2] |
|
2028 | 2044 |
hist = numpy.histogram(finalHeights, bins = nInt, range = (heightMin,heightMax)) |
|
2029 | 2045 |
nMeteorsPerI = hist[0] |
|
2030 | 2046 |
heightPerI = hist[1] |
|
2031 | ||
|
2047 | ||
|
2032 | 2048 |
#Sort of meteors |
|
2033 | 2049 |
indSort = finalHeights.argsort() |
|
2034 | 2050 |
finalMeteor2 = finalMeteor[indSort,:] |
|
2035 | ||
|
2051 | ||
|
2036 | 2052 |
# Calculating winds |
|
2037 | 2053 |
ind1 = 0 |
|
2038 |
ind2 = 0 |
|
|
2039 | ||
|
2054 | ind2 = 0 | |
|
2055 | ||
|
2040 | 2056 |
for i in range(nInt): |
|
2041 | 2057 |
nMet = nMeteorsPerI[i] |
|
2042 | 2058 |
ind1 = ind2 |
|
2043 | 2059 |
ind2 = ind1 + nMet |
|
2044 | ||
|
2060 | ||
|
2045 | 2061 |
meteorAux = finalMeteor2[ind1:ind2,:] |
|
2046 | ||
|
2062 | ||
|
2047 | 2063 |
if meteorAux.shape[0] >= meteorThresh: |
|
2048 | 2064 |
vel = meteorAux[:, 6] |
|
2049 | 2065 |
zen = meteorAux[:, 4]*numpy.pi/180 |
|
2050 | 2066 |
azim = meteorAux[:, 3]*numpy.pi/180 |
|
2051 | ||
|
2067 | ||
|
2052 | 2068 |
n = numpy.cos(zen) |
|
2053 | 2069 |
# m = (1 - n**2)/(1 - numpy.tan(azim)**2) |
|
2054 | 2070 |
# l = m*numpy.tan(azim) |
|
2055 | 2071 |
l = numpy.sin(zen)*numpy.sin(azim) |
|
2056 | 2072 |
m = numpy.sin(zen)*numpy.cos(azim) |
|
2057 | ||
|
2073 | ||
|
2058 | 2074 |
A = numpy.vstack((l, m)).transpose() |
|
2059 | 2075 |
A1 = numpy.dot(numpy.linalg.inv( numpy.dot(A.transpose(),A) ),A.transpose()) |
|
2060 | 2076 |
windsAux = numpy.dot(A1, vel) |
|
2061 | ||
|
2077 | ||
|
2062 | 2078 |
winds[0,i] = windsAux[0] |
|
2063 | 2079 |
winds[1,i] = windsAux[1] |
|
2064 | ||
|
2080 | ||
|
2065 | 2081 |
return winds, heightPerI[:-1] |
|
2066 | ||
|
2082 | ||
|
2067 | 2083 |
def techniqueNSM_SA(self, **kwargs): |
|
2068 | 2084 |
metArray = kwargs['metArray'] |
|
2069 | 2085 |
heightList = kwargs['heightList'] |
|
2070 | 2086 |
timeList = kwargs['timeList'] |
|
2071 | ||
|
2087 | ||
|
2072 | 2088 |
rx_location = kwargs['rx_location'] |
|
2073 | 2089 |
groupList = kwargs['groupList'] |
|
2074 | 2090 |
azimuth = kwargs['azimuth'] |
|
2075 | 2091 |
dfactor = kwargs['dfactor'] |
|
2076 | 2092 |
k = kwargs['k'] |
|
2077 | ||
|
2093 | ||
|
2078 | 2094 |
azimuth1, dist = self.__calculateAzimuth1(rx_location, groupList, azimuth) |
|
2079 | 2095 |
d = dist*dfactor |
|
2080 | 2096 |
#Phase calculation |
|
2081 | 2097 |
metArray1 = self.__getPhaseSlope(metArray, heightList, timeList) |
|
2082 | ||
|
2098 | ||
|
2083 | 2099 |
metArray1[:,-2] = metArray1[:,-2]*metArray1[:,2]*1000/(k*d[metArray1[:,1].astype(int)]) #angles into velocities |
|
2084 | ||
|
2100 | ||
|
2085 | 2101 |
velEst = numpy.zeros((heightList.size,2))*numpy.nan |
|
2086 | 2102 |
azimuth1 = azimuth1*numpy.pi/180 |
|
2087 | ||
|
2103 | ||
|
2088 | 2104 |
for i in range(heightList.size): |
|
2089 | 2105 |
h = heightList[i] |
|
2090 | 2106 |
indH = numpy.where((metArray1[:,2] == h)&(numpy.abs(metArray1[:,-2]) < 100))[0] |
@@ -2097,71 +2113,71 class WindProfiler(Operation): | |||
|
2097 | 2113 |
A = numpy.asmatrix(A) |
|
2098 | 2114 |
A1 = numpy.linalg.pinv(A.transpose()*A)*A.transpose() |
|
2099 | 2115 |
velHor = numpy.dot(A1,velAux) |
|
2100 | ||
|
2116 | ||
|
2101 | 2117 |
velEst[i,:] = numpy.squeeze(velHor) |
|
2102 | 2118 |
return velEst |
|
2103 | ||
|
2119 | ||
|
2104 | 2120 |
def __getPhaseSlope(self, metArray, heightList, timeList): |
|
2105 | 2121 |
meteorList = [] |
|
2106 | 2122 |
#utctime sec1 height SNR velRad ph0 ph1 ph2 coh0 coh1 coh2 |
|
2107 | 2123 |
#Putting back together the meteor matrix |
|
2108 | 2124 |
utctime = metArray[:,0] |
|
2109 | 2125 |
uniqueTime = numpy.unique(utctime) |
|
2110 | ||
|
2126 | ||
|
2111 | 2127 |
phaseDerThresh = 0.5 |
|
2112 | 2128 |
ippSeconds = timeList[1] - timeList[0] |
|
2113 | 2129 |
sec = numpy.where(timeList>1)[0][0] |
|
2114 | 2130 |
nPairs = metArray.shape[1] - 6 |
|
2115 | 2131 |
nHeights = len(heightList) |
|
2116 | ||
|
2132 | ||
|
2117 | 2133 |
for t in uniqueTime: |
|
2118 | 2134 |
metArray1 = metArray[utctime==t,:] |
|
2119 | 2135 |
# phaseDerThresh = numpy.pi/4 #reducir Phase thresh |
|
2120 | 2136 |
tmet = metArray1[:,1].astype(int) |
|
2121 | 2137 |
hmet = metArray1[:,2].astype(int) |
|
2122 | ||
|
2138 | ||
|
2123 | 2139 |
metPhase = numpy.zeros((nPairs, heightList.size, timeList.size - 1)) |
|
2124 | 2140 |
metPhase[:,:] = numpy.nan |
|
2125 | 2141 |
metPhase[:,hmet,tmet] = metArray1[:,6:].T |
|
2126 | ||
|
2142 | ||
|
2127 | 2143 |
#Delete short trails |
|
2128 | 2144 |
metBool = ~numpy.isnan(metPhase[0,:,:]) |
|
2129 | 2145 |
heightVect = numpy.sum(metBool, axis = 1) |
|
2130 | 2146 |
metBool[heightVect<sec,:] = False |
|
2131 | 2147 |
metPhase[:,heightVect<sec,:] = numpy.nan |
|
2132 | ||
|
2148 | ||
|
2133 | 2149 |
#Derivative |
|
2134 | 2150 |
metDer = numpy.abs(metPhase[:,:,1:] - metPhase[:,:,:-1]) |
|
2135 | 2151 |
phDerAux = numpy.dstack((numpy.full((nPairs,nHeights,1), False, dtype=bool),metDer > phaseDerThresh)) |
|
2136 | 2152 |
metPhase[phDerAux] = numpy.nan |
|
2137 | ||
|
2153 | ||
|
2138 | 2154 |
#--------------------------METEOR DETECTION ----------------------------------------- |
|
2139 | 2155 |
indMet = numpy.where(numpy.any(metBool,axis=1))[0] |
|
2140 | ||
|
2156 | ||
|
2141 | 2157 |
for p in numpy.arange(nPairs): |
|
2142 | 2158 |
phase = metPhase[p,:,:] |
|
2143 | 2159 |
phDer = metDer[p,:,:] |
|
2144 | ||
|
2160 | ||
|
2145 | 2161 |
for h in indMet: |
|
2146 | 2162 |
height = heightList[h] |
|
2147 | 2163 |
phase1 = phase[h,:] #82 |
|
2148 | 2164 |
phDer1 = phDer[h,:] |
|
2149 | ||
|
2165 | ||
|
2150 | 2166 |
phase1[~numpy.isnan(phase1)] = numpy.unwrap(phase1[~numpy.isnan(phase1)]) #Unwrap |
|
2151 | ||
|
2167 | ||
|
2152 | 2168 |
indValid = numpy.where(~numpy.isnan(phase1))[0] |
|
2153 | 2169 |
initMet = indValid[0] |
|
2154 | 2170 |
endMet = 0 |
|
2155 | ||
|
2171 | ||
|
2156 | 2172 |
for i in range(len(indValid)-1): |
|
2157 | ||
|
2173 | ||
|
2158 | 2174 |
#Time difference |
|
2159 | 2175 |
inow = indValid[i] |
|
2160 | 2176 |
inext = indValid[i+1] |
|
2161 | 2177 |
idiff = inext - inow |
|
2162 | 2178 |
#Phase difference |
|
2163 |
phDiff = numpy.abs(phase1[inext] - phase1[inow]) |
|
|
2164 | ||
|
2179 | phDiff = numpy.abs(phase1[inext] - phase1[inow]) | |
|
2180 | ||
|
2165 | 2181 |
if idiff>sec or phDiff>numpy.pi/4 or inext==indValid[-1]: #End of Meteor |
|
2166 | 2182 |
sizeTrail = inow - initMet + 1 |
|
2167 | 2183 |
if sizeTrail>3*sec: #Too short meteors |
@@ -2177,43 +2193,43 class WindProfiler(Operation): | |||
|
2177 | 2193 |
vel = slope#*height*1000/(k*d) |
|
2178 | 2194 |
estAux = numpy.array([utctime,p,height, vel, rsq]) |
|
2179 | 2195 |
meteorList.append(estAux) |
|
2180 |
initMet = inext |
|
|
2196 | initMet = inext | |
|
2181 | 2197 |
metArray2 = numpy.array(meteorList) |
|
2182 | ||
|
2198 | ||
|
2183 | 2199 |
return metArray2 |
|
2184 | ||
|
2200 | ||
|
2185 | 2201 |
def __calculateAzimuth1(self, rx_location, pairslist, azimuth0): |
|
2186 | ||
|
2202 | ||
|
2187 | 2203 |
azimuth1 = numpy.zeros(len(pairslist)) |
|
2188 | 2204 |
dist = numpy.zeros(len(pairslist)) |
|
2189 | ||
|
2205 | ||
|
2190 | 2206 |
for i in range(len(rx_location)): |
|
2191 | 2207 |
ch0 = pairslist[i][0] |
|
2192 | 2208 |
ch1 = pairslist[i][1] |
|
2193 | ||
|
2209 | ||
|
2194 | 2210 |
diffX = rx_location[ch0][0] - rx_location[ch1][0] |
|
2195 | 2211 |
diffY = rx_location[ch0][1] - rx_location[ch1][1] |
|
2196 | 2212 |
azimuth1[i] = numpy.arctan2(diffY,diffX)*180/numpy.pi |
|
2197 | 2213 |
dist[i] = numpy.sqrt(diffX**2 + diffY**2) |
|
2198 | ||
|
2214 | ||
|
2199 | 2215 |
azimuth1 -= azimuth0 |
|
2200 | 2216 |
return azimuth1, dist |
|
2201 | ||
|
2217 | ||
|
2202 | 2218 |
def techniqueNSM_DBS(self, **kwargs): |
|
2203 | 2219 |
metArray = kwargs['metArray'] |
|
2204 | 2220 |
heightList = kwargs['heightList'] |
|
2205 |
timeList = kwargs['timeList'] |
|
|
2221 | timeList = kwargs['timeList'] | |
|
2206 | 2222 |
azimuth = kwargs['azimuth'] |
|
2207 | 2223 |
theta_x = numpy.array(kwargs['theta_x']) |
|
2208 | 2224 |
theta_y = numpy.array(kwargs['theta_y']) |
|
2209 | ||
|
2225 | ||
|
2210 | 2226 |
utctime = metArray[:,0] |
|
2211 | 2227 |
cmet = metArray[:,1].astype(int) |
|
2212 | 2228 |
hmet = metArray[:,3].astype(int) |
|
2213 | 2229 |
SNRmet = metArray[:,4] |
|
2214 | 2230 |
vmet = metArray[:,5] |
|
2215 | 2231 |
spcmet = metArray[:,6] |
|
2216 | ||
|
2232 | ||
|
2217 | 2233 |
nChan = numpy.max(cmet) + 1 |
|
2218 | 2234 |
nHeights = len(heightList) |
|
2219 | 2235 | |
@@ -2229,20 +2245,20 class WindProfiler(Operation): | |||
|
2229 | 2245 | |
|
2230 | 2246 |
thisH = (h1met>=hmin) & (h1met<hmax) & (cmet!=2) & (SNRmet>8) & (vmet<50) & (spcmet<10) |
|
2231 | 2247 |
indthisH = numpy.where(thisH) |
|
2232 | ||
|
2248 | ||
|
2233 | 2249 |
if numpy.size(indthisH) > 3: |
|
2234 | ||
|
2250 | ||
|
2235 | 2251 |
vel_aux = vmet[thisH] |
|
2236 | 2252 |
chan_aux = cmet[thisH] |
|
2237 | 2253 |
cosu_aux = dir_cosu[chan_aux] |
|
2238 | 2254 |
cosv_aux = dir_cosv[chan_aux] |
|
2239 | 2255 |
cosw_aux = dir_cosw[chan_aux] |
|
2240 | ||
|
2241 |
nch = numpy.size(numpy.unique(chan_aux)) |
|
|
2256 | ||
|
2257 | nch = numpy.size(numpy.unique(chan_aux)) | |
|
2242 | 2258 |
if nch > 1: |
|
2243 | 2259 |
A = self.__calculateMatA(cosu_aux, cosv_aux, cosw_aux, True) |
|
2244 | 2260 |
velEst[i,:] = numpy.dot(A,vel_aux) |
|
2245 | ||
|
2261 | ||
|
2246 | 2262 |
return velEst |
|
2247 | 2263 | |
|
2248 | 2264 |
def run(self, dataOut, technique, nHours=1, hmin=70, hmax=110, **kwargs): |
@@ -2253,39 +2269,39 class WindProfiler(Operation): | |||
|
2253 | 2269 |
# noise = dataOut.noise |
|
2254 | 2270 |
heightList = dataOut.heightList |
|
2255 | 2271 |
SNR = dataOut.data_SNR |
|
2256 | ||
|
2272 | ||
|
2257 | 2273 |
if technique == 'DBS': |
|
2258 | ||
|
2259 |
kwargs['velRadial'] = param[:,1,:] #Radial velocity |
|
|
2274 | ||
|
2275 | kwargs['velRadial'] = param[:,1,:] #Radial velocity | |
|
2260 | 2276 |
kwargs['heightList'] = heightList |
|
2261 | 2277 |
kwargs['SNR'] = SNR |
|
2262 | ||
|
2278 | ||
|
2263 | 2279 |
dataOut.data_output, dataOut.heightList, dataOut.data_SNR = self.techniqueDBS(kwargs) #DBS Function |
|
2264 | 2280 |
dataOut.utctimeInit = dataOut.utctime |
|
2265 | 2281 |
dataOut.outputInterval = dataOut.paramInterval |
|
2266 | ||
|
2282 | ||
|
2267 | 2283 |
elif technique == 'SA': |
|
2268 | ||
|
2284 | ||
|
2269 | 2285 |
#Parameters |
|
2270 | 2286 |
# position_x = kwargs['positionX'] |
|
2271 | 2287 |
# position_y = kwargs['positionY'] |
|
2272 | 2288 |
# azimuth = kwargs['azimuth'] |
|
2273 | # | |
|
2289 | # | |
|
2274 | 2290 |
# if kwargs.has_key('crosspairsList'): |
|
2275 | 2291 |
# pairs = kwargs['crosspairsList'] |
|
2276 | 2292 |
# else: |
|
2277 |
# pairs = None |
|
|
2278 | # | |
|
2293 | # pairs = None | |
|
2294 | # | |
|
2279 | 2295 |
# if kwargs.has_key('correctFactor'): |
|
2280 | 2296 |
# correctFactor = kwargs['correctFactor'] |
|
2281 | 2297 |
# else: |
|
2282 | 2298 |
# correctFactor = 1 |
|
2283 | ||
|
2299 | ||
|
2284 | 2300 |
# tau = dataOut.data_param |
|
2285 | 2301 |
# _lambda = dataOut.C/dataOut.frequency |
|
2286 | 2302 |
# pairsList = dataOut.groupList |
|
2287 | 2303 |
# nChannels = dataOut.nChannels |
|
2288 | ||
|
2304 | ||
|
2289 | 2305 |
kwargs['groupList'] = dataOut.groupList |
|
2290 | 2306 |
kwargs['tau'] = dataOut.data_param |
|
2291 | 2307 |
kwargs['_lambda'] = dataOut.C/dataOut.frequency |
@@ -2293,30 +2309,30 class WindProfiler(Operation): | |||
|
2293 | 2309 |
dataOut.data_output = self.techniqueSA(kwargs) |
|
2294 | 2310 |
dataOut.utctimeInit = dataOut.utctime |
|
2295 | 2311 |
dataOut.outputInterval = dataOut.timeInterval |
|
2296 | ||
|
2297 |
elif technique == 'Meteors': |
|
|
2312 | ||
|
2313 | elif technique == 'Meteors': | |
|
2298 | 2314 |
dataOut.flagNoData = True |
|
2299 | 2315 |
self.__dataReady = False |
|
2300 | ||
|
2316 | ||
|
2301 | 2317 |
if 'nHours' in kwargs: |
|
2302 | 2318 |
nHours = kwargs['nHours'] |
|
2303 |
else: |
|
|
2319 | else: | |
|
2304 | 2320 |
nHours = 1 |
|
2305 | ||
|
2321 | ||
|
2306 | 2322 |
if 'meteorsPerBin' in kwargs: |
|
2307 | 2323 |
meteorThresh = kwargs['meteorsPerBin'] |
|
2308 | 2324 |
else: |
|
2309 | 2325 |
meteorThresh = 6 |
|
2310 | ||
|
2326 | ||
|
2311 | 2327 |
if 'hmin' in kwargs: |
|
2312 | 2328 |
hmin = kwargs['hmin'] |
|
2313 | 2329 |
else: hmin = 70 |
|
2314 | 2330 |
if 'hmax' in kwargs: |
|
2315 | 2331 |
hmax = kwargs['hmax'] |
|
2316 | 2332 |
else: hmax = 110 |
|
2317 | ||
|
2333 | ||
|
2318 | 2334 |
dataOut.outputInterval = nHours*3600 |
|
2319 | ||
|
2335 | ||
|
2320 | 2336 |
if self.__isConfig == False: |
|
2321 | 2337 |
# self.__initime = dataOut.datatime.replace(minute = 0, second = 0, microsecond = 03) |
|
2322 | 2338 |
#Get Initial LTC time |
@@ -2324,29 +2340,29 class WindProfiler(Operation): | |||
|
2324 | 2340 |
self.__initime = (self.__initime.replace(minute = 0, second = 0, microsecond = 0) - datetime.datetime(1970, 1, 1)).total_seconds() |
|
2325 | 2341 | |
|
2326 | 2342 |
self.__isConfig = True |
|
2327 | ||
|
2343 | ||
|
2328 | 2344 |
if self.__buffer is None: |
|
2329 | 2345 |
self.__buffer = dataOut.data_param |
|
2330 | 2346 |
self.__firstdata = copy.copy(dataOut) |
|
2331 | 2347 | |
|
2332 | 2348 |
else: |
|
2333 | 2349 |
self.__buffer = numpy.vstack((self.__buffer, dataOut.data_param)) |
|
2334 | ||
|
2350 | ||
|
2335 | 2351 |
self.__checkTime(dataOut.utctime, dataOut.paramInterval, dataOut.outputInterval) #Check if the buffer is ready |
|
2336 | ||
|
2352 | ||
|
2337 | 2353 |
if self.__dataReady: |
|
2338 | 2354 |
dataOut.utctimeInit = self.__initime |
|
2339 | ||
|
2355 | ||
|
2340 | 2356 |
self.__initime += dataOut.outputInterval #to erase time offset |
|
2341 | ||
|
2357 | ||
|
2342 | 2358 |
dataOut.data_output, dataOut.heightList = self.techniqueMeteors(self.__buffer, meteorThresh, hmin, hmax) |
|
2343 | 2359 |
dataOut.flagNoData = False |
|
2344 | 2360 |
self.__buffer = None |
|
2345 | ||
|
2361 | ||
|
2346 | 2362 |
elif technique == 'Meteors1': |
|
2347 | 2363 |
dataOut.flagNoData = True |
|
2348 | 2364 |
self.__dataReady = False |
|
2349 | ||
|
2365 | ||
|
2350 | 2366 |
if 'nMins' in kwargs: |
|
2351 | 2367 |
nMins = kwargs['nMins'] |
|
2352 | 2368 |
else: nMins = 20 |
@@ -2361,7 +2377,7 class WindProfiler(Operation): | |||
|
2361 | 2377 |
if 'mode' in kwargs: |
|
2362 | 2378 |
mode = kwargs['mode'] |
|
2363 | 2379 |
if 'theta_x' in kwargs: |
|
2364 |
theta_x = kwargs['theta_x'] |
|
|
2380 | theta_x = kwargs['theta_x'] | |
|
2365 | 2381 |
if 'theta_y' in kwargs: |
|
2366 | 2382 |
theta_y = kwargs['theta_y'] |
|
2367 | 2383 |
else: mode = 'SA' |
@@ -2374,10 +2390,10 class WindProfiler(Operation): | |||
|
2374 | 2390 |
freq = 50e6 |
|
2375 | 2391 |
lamb = C/freq |
|
2376 | 2392 |
k = 2*numpy.pi/lamb |
|
2377 | ||
|
2393 | ||
|
2378 | 2394 |
timeList = dataOut.abscissaList |
|
2379 | 2395 |
heightList = dataOut.heightList |
|
2380 | ||
|
2396 | ||
|
2381 | 2397 |
if self.__isConfig == False: |
|
2382 | 2398 |
dataOut.outputInterval = nMins*60 |
|
2383 | 2399 |
# self.__initime = dataOut.datatime.replace(minute = 0, second = 0, microsecond = 03) |
@@ -2388,20 +2404,20 class WindProfiler(Operation): | |||
|
2388 | 2404 |
self.__initime = (initime.replace(minute = minuteNew, second = 0, microsecond = 0) - datetime.datetime(1970, 1, 1)).total_seconds() |
|
2389 | 2405 | |
|
2390 | 2406 |
self.__isConfig = True |
|
2391 | ||
|
2407 | ||
|
2392 | 2408 |
if self.__buffer is None: |
|
2393 | 2409 |
self.__buffer = dataOut.data_param |
|
2394 | 2410 |
self.__firstdata = copy.copy(dataOut) |
|
2395 | 2411 | |
|
2396 | 2412 |
else: |
|
2397 | 2413 |
self.__buffer = numpy.vstack((self.__buffer, dataOut.data_param)) |
|
2398 | ||
|
2414 | ||
|
2399 | 2415 |
self.__checkTime(dataOut.utctime, dataOut.paramInterval, dataOut.outputInterval) #Check if the buffer is ready |
|
2400 | ||
|
2416 | ||
|
2401 | 2417 |
if self.__dataReady: |
|
2402 | 2418 |
dataOut.utctimeInit = self.__initime |
|
2403 | 2419 |
self.__initime += dataOut.outputInterval #to erase time offset |
|
2404 | ||
|
2420 | ||
|
2405 | 2421 |
metArray = self.__buffer |
|
2406 | 2422 |
if mode == 'SA': |
|
2407 | 2423 |
dataOut.data_output = self.techniqueNSM_SA(rx_location=rx_location, groupList=groupList, azimuth=azimuth, dfactor=dfactor, k=k,metArray=metArray, heightList=heightList,timeList=timeList) |
@@ -2412,71 +2428,71 class WindProfiler(Operation): | |||
|
2412 | 2428 |
self.__buffer = None |
|
2413 | 2429 | |
|
2414 | 2430 |
return |
|
2415 | ||
|
2431 | ||
|
2416 | 2432 |
class EWDriftsEstimation(Operation): |
|
2417 | ||
|
2418 |
def __init__(self): |
|
|
2419 |
Operation.__init__(self) |
|
|
2420 | ||
|
2433 | ||
|
2434 | def __init__(self): | |
|
2435 | Operation.__init__(self) | |
|
2436 | ||
|
2421 | 2437 |
def __correctValues(self, heiRang, phi, velRadial, SNR): |
|
2422 | 2438 |
listPhi = phi.tolist() |
|
2423 | 2439 |
maxid = listPhi.index(max(listPhi)) |
|
2424 | 2440 |
minid = listPhi.index(min(listPhi)) |
|
2425 | ||
|
2426 |
rango = list(range(len(phi))) |
|
|
2441 | ||
|
2442 | rango = list(range(len(phi))) | |
|
2427 | 2443 |
# rango = numpy.delete(rango,maxid) |
|
2428 | ||
|
2444 | ||
|
2429 | 2445 |
heiRang1 = heiRang*math.cos(phi[maxid]) |
|
2430 | 2446 |
heiRangAux = heiRang*math.cos(phi[minid]) |
|
2431 | 2447 |
indOut = (heiRang1 < heiRangAux[0]).nonzero() |
|
2432 | 2448 |
heiRang1 = numpy.delete(heiRang1,indOut) |
|
2433 | ||
|
2449 | ||
|
2434 | 2450 |
velRadial1 = numpy.zeros([len(phi),len(heiRang1)]) |
|
2435 | 2451 |
SNR1 = numpy.zeros([len(phi),len(heiRang1)]) |
|
2436 | ||
|
2452 | ||
|
2437 | 2453 |
for i in rango: |
|
2438 | 2454 |
x = heiRang*math.cos(phi[i]) |
|
2439 | 2455 |
y1 = velRadial[i,:] |
|
2440 | 2456 |
f1 = interpolate.interp1d(x,y1,kind = 'cubic') |
|
2441 | ||
|
2457 | ||
|
2442 | 2458 |
x1 = heiRang1 |
|
2443 | 2459 |
y11 = f1(x1) |
|
2444 | ||
|
2460 | ||
|
2445 | 2461 |
y2 = SNR[i,:] |
|
2446 | 2462 |
f2 = interpolate.interp1d(x,y2,kind = 'cubic') |
|
2447 | 2463 |
y21 = f2(x1) |
|
2448 | ||
|
2464 | ||
|
2449 | 2465 |
velRadial1[i,:] = y11 |
|
2450 | 2466 |
SNR1[i,:] = y21 |
|
2451 | ||
|
2467 | ||
|
2452 | 2468 |
return heiRang1, velRadial1, SNR1 |
|
2453 | 2469 | |
|
2454 | 2470 |
def run(self, dataOut, zenith, zenithCorrection): |
|
2455 | 2471 |
heiRang = dataOut.heightList |
|
2456 | 2472 |
velRadial = dataOut.data_param[:,3,:] |
|
2457 | 2473 |
SNR = dataOut.data_SNR |
|
2458 | ||
|
2474 | ||
|
2459 | 2475 |
zenith = numpy.array(zenith) |
|
2460 |
zenith -= zenithCorrection |
|
|
2476 | zenith -= zenithCorrection | |
|
2461 | 2477 |
zenith *= numpy.pi/180 |
|
2462 | ||
|
2478 | ||
|
2463 | 2479 |
heiRang1, velRadial1, SNR1 = self.__correctValues(heiRang, numpy.abs(zenith), velRadial, SNR) |
|
2464 | ||
|
2480 | ||
|
2465 | 2481 |
alp = zenith[0] |
|
2466 | 2482 |
bet = zenith[1] |
|
2467 | ||
|
2483 | ||
|
2468 | 2484 |
w_w = velRadial1[0,:] |
|
2469 | 2485 |
w_e = velRadial1[1,:] |
|
2470 | ||
|
2471 |
w = (w_w*numpy.sin(bet) - w_e*numpy.sin(alp))/(numpy.cos(alp)*numpy.sin(bet) - numpy.cos(bet)*numpy.sin(alp)) |
|
|
2472 |
u = (w_w*numpy.cos(bet) - w_e*numpy.cos(alp))/(numpy.sin(alp)*numpy.cos(bet) - numpy.sin(bet)*numpy.cos(alp)) |
|
|
2473 | ||
|
2486 | ||
|
2487 | w = (w_w*numpy.sin(bet) - w_e*numpy.sin(alp))/(numpy.cos(alp)*numpy.sin(bet) - numpy.cos(bet)*numpy.sin(alp)) | |
|
2488 | u = (w_w*numpy.cos(bet) - w_e*numpy.cos(alp))/(numpy.sin(alp)*numpy.cos(bet) - numpy.sin(bet)*numpy.cos(alp)) | |
|
2489 | ||
|
2474 | 2490 |
winds = numpy.vstack((u,w)) |
|
2475 | ||
|
2491 | ||
|
2476 | 2492 |
dataOut.heightList = heiRang1 |
|
2477 | 2493 |
dataOut.data_output = winds |
|
2478 | 2494 |
dataOut.data_SNR = SNR1 |
|
2479 | ||
|
2495 | ||
|
2480 | 2496 |
dataOut.utctimeInit = dataOut.utctime |
|
2481 | 2497 |
dataOut.outputInterval = dataOut.timeInterval |
|
2482 | 2498 |
return |
@@ -2489,11 +2505,11 class NonSpecularMeteorDetection(Operation): | |||
|
2489 | 2505 |
data_acf = dataOut.data_pre[0] |
|
2490 | 2506 |
data_ccf = dataOut.data_pre[1] |
|
2491 | 2507 |
pairsList = dataOut.groupList[1] |
|
2492 | ||
|
2508 | ||
|
2493 | 2509 |
lamb = dataOut.C/dataOut.frequency |
|
2494 | 2510 |
tSamp = dataOut.ippSeconds*dataOut.nCohInt |
|
2495 | 2511 |
paramInterval = dataOut.paramInterval |
|
2496 | ||
|
2512 | ||
|
2497 | 2513 |
nChannels = data_acf.shape[0] |
|
2498 | 2514 |
nLags = data_acf.shape[1] |
|
2499 | 2515 |
nProfiles = data_acf.shape[2] |
@@ -2503,7 +2519,7 class NonSpecularMeteorDetection(Operation): | |||
|
2503 | 2519 |
heightList = dataOut.heightList |
|
2504 | 2520 |
ippSeconds = dataOut.ippSeconds*dataOut.nCohInt*dataOut.nAvg |
|
2505 | 2521 |
utctime = dataOut.utctime |
|
2506 | ||
|
2522 | ||
|
2507 | 2523 |
dataOut.abscissaList = numpy.arange(0,paramInterval+ippSeconds,ippSeconds) |
|
2508 | 2524 | |
|
2509 | 2525 |
#------------------------ SNR -------------------------------------- |
@@ -2515,7 +2531,7 class NonSpecularMeteorDetection(Operation): | |||
|
2515 | 2531 |
SNR[i] = (power[i]-noise[i])/noise[i] |
|
2516 | 2532 |
SNRm = numpy.nanmean(SNR, axis = 0) |
|
2517 | 2533 |
SNRdB = 10*numpy.log10(SNR) |
|
2518 | ||
|
2534 | ||
|
2519 | 2535 |
if mode == 'SA': |
|
2520 | 2536 |
dataOut.groupList = dataOut.groupList[1] |
|
2521 | 2537 |
nPairs = data_ccf.shape[0] |
@@ -2523,22 +2539,22 class NonSpecularMeteorDetection(Operation): | |||
|
2523 | 2539 |
phase = numpy.zeros(data_ccf[:,0,:,:].shape) |
|
2524 | 2540 |
# phase1 = numpy.copy(phase) |
|
2525 | 2541 |
coh1 = numpy.zeros(data_ccf[:,0,:,:].shape) |
|
2526 | ||
|
2542 | ||
|
2527 | 2543 |
for p in range(nPairs): |
|
2528 | 2544 |
ch0 = pairsList[p][0] |
|
2529 | 2545 |
ch1 = pairsList[p][1] |
|
2530 | 2546 |
ccf = data_ccf[p,0,:,:]/numpy.sqrt(data_acf[ch0,0,:,:]*data_acf[ch1,0,:,:]) |
|
2531 |
phase[p,:,:] = ndimage.median_filter(numpy.angle(ccf), size = (5,1)) #median filter |
|
|
2532 |
# phase1[p,:,:] = numpy.angle(ccf) #median filter |
|
|
2533 |
coh1[p,:,:] = ndimage.median_filter(numpy.abs(ccf), 5) #median filter |
|
|
2534 |
# coh1[p,:,:] = numpy.abs(ccf) #median filter |
|
|
2547 | phase[p,:,:] = ndimage.median_filter(numpy.angle(ccf), size = (5,1)) #median filter | |
|
2548 | # phase1[p,:,:] = numpy.angle(ccf) #median filter | |
|
2549 | coh1[p,:,:] = ndimage.median_filter(numpy.abs(ccf), 5) #median filter | |
|
2550 | # coh1[p,:,:] = numpy.abs(ccf) #median filter | |
|
2535 | 2551 |
coh = numpy.nanmax(coh1, axis = 0) |
|
2536 | 2552 |
# struc = numpy.ones((5,1)) |
|
2537 | 2553 |
# coh = ndimage.morphology.grey_dilation(coh, size=(10,1)) |
|
2538 | 2554 |
#---------------------- Radial Velocity ---------------------------- |
|
2539 | 2555 |
phaseAux = numpy.mean(numpy.angle(data_acf[:,1,:,:]), axis = 0) |
|
2540 | 2556 |
velRad = phaseAux*lamb/(4*numpy.pi*tSamp) |
|
2541 | ||
|
2557 | ||
|
2542 | 2558 |
if allData: |
|
2543 | 2559 |
boolMetFin = ~numpy.isnan(SNRm) |
|
2544 | 2560 |
# coh[:-1,:] = numpy.nanmean(numpy.abs(phase[:,1:,:] - phase[:,:-1,:]),axis=0) |
@@ -2546,31 +2562,31 class NonSpecularMeteorDetection(Operation): | |||
|
2546 | 2562 |
#------------------------ Meteor mask --------------------------------- |
|
2547 | 2563 |
# #SNR mask |
|
2548 | 2564 |
# boolMet = (SNRdB>SNRthresh)#|(~numpy.isnan(SNRdB)) |
|
2549 | # | |
|
2565 | # | |
|
2550 | 2566 |
# #Erase small objects |
|
2551 |
# boolMet1 = self.__erase_small(boolMet, 2*sec, 5) |
|
|
2552 | # | |
|
2567 | # boolMet1 = self.__erase_small(boolMet, 2*sec, 5) | |
|
2568 | # | |
|
2553 | 2569 |
# auxEEJ = numpy.sum(boolMet1,axis=0) |
|
2554 | 2570 |
# indOver = auxEEJ>nProfiles*0.8 #Use this later |
|
2555 | 2571 |
# indEEJ = numpy.where(indOver)[0] |
|
2556 | 2572 |
# indNEEJ = numpy.where(~indOver)[0] |
|
2557 | # | |
|
2573 | # | |
|
2558 | 2574 |
# boolMetFin = boolMet1 |
|
2559 | # | |
|
2575 | # | |
|
2560 | 2576 |
# if indEEJ.size > 0: |
|
2561 |
# boolMet1[:,indEEJ] = False #Erase heights with EEJ |
|
|
2562 | # | |
|
2577 | # boolMet1[:,indEEJ] = False #Erase heights with EEJ | |
|
2578 | # | |
|
2563 | 2579 |
# boolMet2 = coh > cohThresh |
|
2564 | 2580 |
# boolMet2 = self.__erase_small(boolMet2, 2*sec,5) |
|
2565 | # | |
|
2581 | # | |
|
2566 | 2582 |
# #Final Meteor mask |
|
2567 | 2583 |
# boolMetFin = boolMet1|boolMet2 |
|
2568 | ||
|
2584 | ||
|
2569 | 2585 |
#Coherence mask |
|
2570 | 2586 |
boolMet1 = coh > 0.75 |
|
2571 | 2587 |
struc = numpy.ones((30,1)) |
|
2572 | 2588 |
boolMet1 = ndimage.morphology.binary_dilation(boolMet1, structure=struc) |
|
2573 | ||
|
2589 | ||
|
2574 | 2590 |
#Derivative mask |
|
2575 | 2591 |
derPhase = numpy.nanmean(numpy.abs(phase[:,1:,:] - phase[:,:-1,:]),axis=0) |
|
2576 | 2592 |
boolMet2 = derPhase < 0.2 |
@@ -2587,7 +2603,7 class NonSpecularMeteorDetection(Operation): | |||
|
2587 | 2603 | |
|
2588 | 2604 |
tmet = coordMet[0] |
|
2589 | 2605 |
hmet = coordMet[1] |
|
2590 | ||
|
2606 | ||
|
2591 | 2607 |
data_param = numpy.zeros((tmet.size, 6 + nPairs)) |
|
2592 | 2608 |
data_param[:,0] = utctime |
|
2593 | 2609 |
data_param[:,1] = tmet |
@@ -2596,7 +2612,7 class NonSpecularMeteorDetection(Operation): | |||
|
2596 | 2612 |
data_param[:,4] = velRad[tmet,hmet] |
|
2597 | 2613 |
data_param[:,5] = coh[tmet,hmet] |
|
2598 | 2614 |
data_param[:,6:] = phase[:,tmet,hmet].T |
|
2599 | ||
|
2615 | ||
|
2600 | 2616 |
elif mode == 'DBS': |
|
2601 | 2617 |
dataOut.groupList = numpy.arange(nChannels) |
|
2602 | 2618 | |
@@ -2604,7 +2620,7 class NonSpecularMeteorDetection(Operation): | |||
|
2604 | 2620 |
phase = numpy.angle(data_acf[:,1,:,:]) |
|
2605 | 2621 |
# phase = ndimage.median_filter(numpy.angle(data_acf[:,1,:,:]), size = (1,5,1)) |
|
2606 | 2622 |
velRad = phase*lamb/(4*numpy.pi*tSamp) |
|
2607 | ||
|
2623 | ||
|
2608 | 2624 |
#Spectral width |
|
2609 | 2625 |
# acf1 = ndimage.median_filter(numpy.abs(data_acf[:,1,:,:]), size = (1,5,1)) |
|
2610 | 2626 |
# acf2 = ndimage.median_filter(numpy.abs(data_acf[:,2,:,:]), size = (1,5,1)) |
@@ -2619,24 +2635,24 class NonSpecularMeteorDetection(Operation): | |||
|
2619 | 2635 |
#SNR |
|
2620 | 2636 |
boolMet1 = (SNRdB>SNRthresh) #SNR mask |
|
2621 | 2637 |
boolMet1 = ndimage.median_filter(boolMet1, size=(1,5,5)) |
|
2622 | ||
|
2638 | ||
|
2623 | 2639 |
#Radial velocity |
|
2624 | 2640 |
boolMet2 = numpy.abs(velRad) < 20 |
|
2625 | 2641 |
boolMet2 = ndimage.median_filter(boolMet2, (1,5,5)) |
|
2626 | ||
|
2642 | ||
|
2627 | 2643 |
#Spectral Width |
|
2628 | 2644 |
boolMet3 = spcWidth < 30 |
|
2629 | 2645 |
boolMet3 = ndimage.median_filter(boolMet3, (1,5,5)) |
|
2630 | 2646 |
# boolMetFin = self.__erase_small(boolMet1, 10,5) |
|
2631 | 2647 |
boolMetFin = boolMet1&boolMet2&boolMet3 |
|
2632 | ||
|
2648 | ||
|
2633 | 2649 |
#Creating data_param |
|
2634 | 2650 |
coordMet = numpy.where(boolMetFin) |
|
2635 | 2651 | |
|
2636 | 2652 |
cmet = coordMet[0] |
|
2637 | 2653 |
tmet = coordMet[1] |
|
2638 | 2654 |
hmet = coordMet[2] |
|
2639 | ||
|
2655 | ||
|
2640 | 2656 |
data_param = numpy.zeros((tmet.size, 7)) |
|
2641 | 2657 |
data_param[:,0] = utctime |
|
2642 | 2658 |
data_param[:,1] = cmet |
@@ -2645,7 +2661,7 class NonSpecularMeteorDetection(Operation): | |||
|
2645 | 2661 |
data_param[:,4] = SNR[cmet,tmet,hmet].T |
|
2646 | 2662 |
data_param[:,5] = velRad[cmet,tmet,hmet].T |
|
2647 | 2663 |
data_param[:,6] = spcWidth[cmet,tmet,hmet].T |
|
2648 | ||
|
2664 | ||
|
2649 | 2665 |
# self.dataOut.data_param = data_int |
|
2650 | 2666 |
if len(data_param) == 0: |
|
2651 | 2667 |
dataOut.flagNoData = True |
@@ -2655,21 +2671,21 class NonSpecularMeteorDetection(Operation): | |||
|
2655 | 2671 |
def __erase_small(self, binArray, threshX, threshY): |
|
2656 | 2672 |
labarray, numfeat = ndimage.measurements.label(binArray) |
|
2657 | 2673 |
binArray1 = numpy.copy(binArray) |
|
2658 | ||
|
2674 | ||
|
2659 | 2675 |
for i in range(1,numfeat + 1): |
|
2660 | 2676 |
auxBin = (labarray==i) |
|
2661 | 2677 |
auxSize = auxBin.sum() |
|
2662 | ||
|
2678 | ||
|
2663 | 2679 |
x,y = numpy.where(auxBin) |
|
2664 | 2680 |
widthX = x.max() - x.min() |
|
2665 | 2681 |
widthY = y.max() - y.min() |
|
2666 | ||
|
2682 | ||
|
2667 | 2683 |
#width X: 3 seg -> 12.5*3 |
|
2668 |
#width Y: |
|
|
2669 | ||
|
2684 | #width Y: | |
|
2685 | ||
|
2670 | 2686 |
if (auxSize < 50) or (widthX < threshX) or (widthY < threshY): |
|
2671 | 2687 |
binArray1[auxBin] = False |
|
2672 | ||
|
2688 | ||
|
2673 | 2689 |
return binArray1 |
|
2674 | 2690 | |
|
2675 | 2691 |
#--------------- Specular Meteor ---------------- |
@@ -2679,36 +2695,36 class SMDetection(Operation): | |||
|
2679 | 2695 |
Function DetectMeteors() |
|
2680 | 2696 |
Project developed with paper: |
|
2681 | 2697 |
HOLDSWORTH ET AL. 2004 |
|
2682 | ||
|
2698 | ||
|
2683 | 2699 |
Input: |
|
2684 | 2700 |
self.dataOut.data_pre |
|
2685 | ||
|
2701 | ||
|
2686 | 2702 |
centerReceiverIndex: From the channels, which is the center receiver |
|
2687 | ||
|
2703 | ||
|
2688 | 2704 |
hei_ref: Height reference for the Beacon signal extraction |
|
2689 | 2705 |
tauindex: |
|
2690 | 2706 |
predefinedPhaseShifts: Predefined phase offset for the voltge signals |
|
2691 | ||
|
2707 | ||
|
2692 | 2708 |
cohDetection: Whether to user Coherent detection or not |
|
2693 | 2709 |
cohDet_timeStep: Coherent Detection calculation time step |
|
2694 | 2710 |
cohDet_thresh: Coherent Detection phase threshold to correct phases |
|
2695 | ||
|
2711 | ||
|
2696 | 2712 |
noise_timeStep: Noise calculation time step |
|
2697 | 2713 |
noise_multiple: Noise multiple to define signal threshold |
|
2698 | ||
|
2714 | ||
|
2699 | 2715 |
multDet_timeLimit: Multiple Detection Removal time limit in seconds |
|
2700 | 2716 |
multDet_rangeLimit: Multiple Detection Removal range limit in km |
|
2701 | ||
|
2717 | ||
|
2702 | 2718 |
phaseThresh: Maximum phase difference between receiver to be consider a meteor |
|
2703 |
SNRThresh: Minimum SNR threshold of the meteor signal to be consider a meteor |
|
|
2704 | ||
|
2719 | SNRThresh: Minimum SNR threshold of the meteor signal to be consider a meteor | |
|
2720 | ||
|
2705 | 2721 |
hmin: Minimum Height of the meteor to use it in the further wind estimations |
|
2706 | 2722 |
hmax: Maximum Height of the meteor to use it in the further wind estimations |
|
2707 | 2723 |
azimuth: Azimuth angle correction |
|
2708 | ||
|
2724 | ||
|
2709 | 2725 |
Affected: |
|
2710 | 2726 |
self.dataOut.data_param |
|
2711 | ||
|
2727 | ||
|
2712 | 2728 |
Rejection Criteria (Errors): |
|
2713 | 2729 |
0: No error; analysis OK |
|
2714 | 2730 |
1: SNR < SNR threshold |
@@ -2727,9 +2743,9 class SMDetection(Operation): | |||
|
2727 | 2743 |
14: height ambiguous echo: more then one possible height within 70 to 110 km |
|
2728 | 2744 |
15: radial drift velocity or projected horizontal velocity exceeds 200 m/s |
|
2729 | 2745 |
16: oscilatory echo, indicating event most likely not an underdense echo |
|
2730 | ||
|
2746 | ||
|
2731 | 2747 |
17: phase difference in meteor Reestimation |
|
2732 | ||
|
2748 | ||
|
2733 | 2749 |
Data Storage: |
|
2734 | 2750 |
Meteors for Wind Estimation (8): |
|
2735 | 2751 |
Utc Time | Range Height |
@@ -2737,19 +2753,19 class SMDetection(Operation): | |||
|
2737 | 2753 |
VelRad errorVelRad |
|
2738 | 2754 |
Phase0 Phase1 Phase2 Phase3 |
|
2739 | 2755 |
TypeError |
|
2740 | ||
|
2741 |
''' |
|
|
2742 | ||
|
2756 | ||
|
2757 | ''' | |
|
2758 | ||
|
2743 | 2759 |
def run(self, dataOut, hei_ref = None, tauindex = 0, |
|
2744 | 2760 |
phaseOffsets = None, |
|
2745 |
cohDetection = False, cohDet_timeStep = 1, cohDet_thresh = 25, |
|
|
2761 | cohDetection = False, cohDet_timeStep = 1, cohDet_thresh = 25, | |
|
2746 | 2762 |
noise_timeStep = 4, noise_multiple = 4, |
|
2747 | 2763 |
multDet_timeLimit = 1, multDet_rangeLimit = 3, |
|
2748 | 2764 |
phaseThresh = 20, SNRThresh = 5, |
|
2749 | 2765 |
hmin = 50, hmax=150, azimuth = 0, |
|
2750 | 2766 |
channelPositions = None) : |
|
2751 | ||
|
2752 | ||
|
2767 | ||
|
2768 | ||
|
2753 | 2769 |
#Getting Pairslist |
|
2754 | 2770 |
if channelPositions is None: |
|
2755 | 2771 |
# channelPositions = [(2.5,0), (0,2.5), (0,0), (0,4.5), (-2,0)] #T |
@@ -2759,53 +2775,53 class SMDetection(Operation): | |||
|
2759 | 2775 |
heiRang = dataOut.getHeiRange() |
|
2760 | 2776 |
#Get Beacon signal - No Beacon signal anymore |
|
2761 | 2777 |
# newheis = numpy.where(self.dataOut.heightList>self.dataOut.radarControllerHeaderObj.Taus[tauindex]) |
|
2762 | # | |
|
2778 | # | |
|
2763 | 2779 |
# if hei_ref != None: |
|
2764 | 2780 |
# newheis = numpy.where(self.dataOut.heightList>hei_ref) |
|
2765 | # | |
|
2766 | ||
|
2767 | ||
|
2781 | # | |
|
2782 | ||
|
2783 | ||
|
2768 | 2784 |
#****************REMOVING HARDWARE PHASE DIFFERENCES*************** |
|
2769 | 2785 |
# see if the user put in pre defined phase shifts |
|
2770 | 2786 |
voltsPShift = dataOut.data_pre.copy() |
|
2771 | ||
|
2787 | ||
|
2772 | 2788 |
# if predefinedPhaseShifts != None: |
|
2773 | 2789 |
# hardwarePhaseShifts = numpy.array(predefinedPhaseShifts)*numpy.pi/180 |
|
2774 | # | |
|
2790 | # | |
|
2775 | 2791 |
# # elif beaconPhaseShifts: |
|
2776 | 2792 |
# # #get hardware phase shifts using beacon signal |
|
2777 | 2793 |
# # hardwarePhaseShifts = self.__getHardwarePhaseDiff(self.dataOut.data_pre, pairslist, newheis, 10) |
|
2778 | 2794 |
# # hardwarePhaseShifts = numpy.insert(hardwarePhaseShifts,centerReceiverIndex,0) |
|
2779 | # | |
|
2795 | # | |
|
2780 | 2796 |
# else: |
|
2781 |
# hardwarePhaseShifts = numpy.zeros(5) |
|
|
2782 | # | |
|
2797 | # hardwarePhaseShifts = numpy.zeros(5) | |
|
2798 | # | |
|
2783 | 2799 |
# voltsPShift = numpy.zeros((self.dataOut.data_pre.shape[0],self.dataOut.data_pre.shape[1],self.dataOut.data_pre.shape[2]), dtype = 'complex') |
|
2784 | 2800 |
# for i in range(self.dataOut.data_pre.shape[0]): |
|
2785 | 2801 |
# voltsPShift[i,:,:] = self.__shiftPhase(self.dataOut.data_pre[i,:,:], hardwarePhaseShifts[i]) |
|
2786 | 2802 | |
|
2787 | 2803 |
#******************END OF REMOVING HARDWARE PHASE DIFFERENCES********* |
|
2788 | ||
|
2804 | ||
|
2789 | 2805 |
#Remove DC |
|
2790 | 2806 |
voltsDC = numpy.mean(voltsPShift,1) |
|
2791 | 2807 |
voltsDC = numpy.mean(voltsDC,1) |
|
2792 | 2808 |
for i in range(voltsDC.shape[0]): |
|
2793 | 2809 |
voltsPShift[i] = voltsPShift[i] - voltsDC[i] |
|
2794 | ||
|
2795 |
#Don't considerate last heights, theyre used to calculate Hardware Phase Shift |
|
|
2810 | ||
|
2811 | #Don't considerate last heights, theyre used to calculate Hardware Phase Shift | |
|
2796 | 2812 |
# voltsPShift = voltsPShift[:,:,:newheis[0][0]] |
|
2797 | ||
|
2813 | ||
|
2798 | 2814 |
#************ FIND POWER OF DATA W/COH OR NON COH DETECTION (3.4) ********** |
|
2799 | 2815 |
#Coherent Detection |
|
2800 | 2816 |
if cohDetection: |
|
2801 | 2817 |
#use coherent detection to get the net power |
|
2802 | 2818 |
cohDet_thresh = cohDet_thresh*numpy.pi/180 |
|
2803 | 2819 |
voltsPShift = self.__coherentDetection(voltsPShift, cohDet_timeStep, dataOut.timeInterval, pairslist0, cohDet_thresh) |
|
2804 | ||
|
2820 | ||
|
2805 | 2821 |
#Non-coherent detection! |
|
2806 | 2822 |
powerNet = numpy.nansum(numpy.abs(voltsPShift[:,:,:])**2,0) |
|
2807 | 2823 |
#********** END OF COH/NON-COH POWER CALCULATION********************** |
|
2808 | ||
|
2824 | ||
|
2809 | 2825 |
#********** FIND THE NOISE LEVEL AND POSSIBLE METEORS **************** |
|
2810 | 2826 |
#Get noise |
|
2811 | 2827 |
noise, noise1 = self.__getNoise(powerNet, noise_timeStep, dataOut.timeInterval) |
@@ -2815,7 +2831,7 class SMDetection(Operation): | |||
|
2815 | 2831 |
#Meteor echoes detection |
|
2816 | 2832 |
listMeteors = self.__findMeteors(powerNet, signalThresh) |
|
2817 | 2833 |
#******* END OF NOISE LEVEL AND POSSIBLE METEORS CACULATION ********** |
|
2818 | ||
|
2834 | ||
|
2819 | 2835 |
#************** REMOVE MULTIPLE DETECTIONS (3.5) *************************** |
|
2820 | 2836 |
#Parameters |
|
2821 | 2837 |
heiRange = dataOut.getHeiRange() |
@@ -2825,7 +2841,7 class SMDetection(Operation): | |||
|
2825 | 2841 |
#Multiple detection removals |
|
2826 | 2842 |
listMeteors1 = self.__removeMultipleDetections(listMeteors, rangeLimit, timeLimit) |
|
2827 | 2843 |
#************ END OF REMOVE MULTIPLE DETECTIONS ********************** |
|
2828 | ||
|
2844 | ||
|
2829 | 2845 |
#********************* METEOR REESTIMATION (3.7, 3.8, 3.9, 3.10) ******************** |
|
2830 | 2846 |
#Parameters |
|
2831 | 2847 |
phaseThresh = phaseThresh*numpy.pi/180 |
@@ -2836,40 +2852,40 class SMDetection(Operation): | |||
|
2836 | 2852 |
#Estimation of decay times (Errors N 7, 8, 11) |
|
2837 | 2853 |
listMeteors3 = self.__estimateDecayTime(listMeteors2, listMeteorsPower, dataOut.timeInterval, dataOut.frequency) |
|
2838 | 2854 |
#******************* END OF METEOR REESTIMATION ******************* |
|
2839 | ||
|
2855 | ||
|
2840 | 2856 |
#********************* METEOR PARAMETERS CALCULATION (3.11, 3.12, 3.13) ************************** |
|
2841 | 2857 |
#Calculating Radial Velocity (Error N 15) |
|
2842 | 2858 |
radialStdThresh = 10 |
|
2843 |
listMeteors4 = self.__getRadialVelocity(listMeteors3, listMeteorsVolts, radialStdThresh, pairslist0, dataOut.timeInterval) |
|
|
2859 | listMeteors4 = self.__getRadialVelocity(listMeteors3, listMeteorsVolts, radialStdThresh, pairslist0, dataOut.timeInterval) | |
|
2844 | 2860 | |
|
2845 | 2861 |
if len(listMeteors4) > 0: |
|
2846 | 2862 |
#Setting New Array |
|
2847 | 2863 |
date = dataOut.utctime |
|
2848 | 2864 |
arrayParameters = self.__setNewArrays(listMeteors4, date, heiRang) |
|
2849 | ||
|
2865 | ||
|
2850 | 2866 |
#Correcting phase offset |
|
2851 | 2867 |
if phaseOffsets != None: |
|
2852 | 2868 |
phaseOffsets = numpy.array(phaseOffsets)*numpy.pi/180 |
|
2853 | 2869 |
arrayParameters[:,8:12] = numpy.unwrap(arrayParameters[:,8:12] + phaseOffsets) |
|
2854 | ||
|
2870 | ||
|
2855 | 2871 |
#Second Pairslist |
|
2856 | 2872 |
pairsList = [] |
|
2857 | 2873 |
pairx = (0,1) |
|
2858 | 2874 |
pairy = (2,3) |
|
2859 | 2875 |
pairsList.append(pairx) |
|
2860 | 2876 |
pairsList.append(pairy) |
|
2861 | ||
|
2877 | ||
|
2862 | 2878 |
jph = numpy.array([0,0,0,0]) |
|
2863 | 2879 |
h = (hmin,hmax) |
|
2864 | 2880 |
arrayParameters = meteorOps.getMeteorParams(arrayParameters, azimuth, h, pairsList, distances, jph) |
|
2865 | ||
|
2881 | ||
|
2866 | 2882 |
# #Calculate AOA (Error N 3, 4) |
|
2867 | 2883 |
# #JONES ET AL. 1998 |
|
2868 | 2884 |
# error = arrayParameters[:,-1] |
|
2869 | 2885 |
# AOAthresh = numpy.pi/8 |
|
2870 | 2886 |
# phases = -arrayParameters[:,9:13] |
|
2871 | 2887 |
# arrayParameters[:,4:7], arrayParameters[:,-1] = meteorOps.getAOA(phases, pairsList, error, AOAthresh, azimuth) |
|
2872 | # | |
|
2888 | # | |
|
2873 | 2889 |
# #Calculate Heights (Error N 13 and 14) |
|
2874 | 2890 |
# error = arrayParameters[:,-1] |
|
2875 | 2891 |
# Ranges = arrayParameters[:,2] |
@@ -2877,73 +2893,73 class SMDetection(Operation): | |||
|
2877 | 2893 |
# arrayParameters[:,3], arrayParameters[:,-1] = meteorOps.getHeights(Ranges, zenith, error, hmin, hmax) |
|
2878 | 2894 |
# error = arrayParameters[:,-1] |
|
2879 | 2895 |
#********************* END OF PARAMETERS CALCULATION ************************** |
|
2880 | ||
|
2881 |
#***************************+ PASS DATA TO NEXT STEP ********************** |
|
|
2896 | ||
|
2897 | #***************************+ PASS DATA TO NEXT STEP ********************** | |
|
2882 | 2898 |
# arrayFinal = arrayParameters.reshape((1,arrayParameters.shape[0],arrayParameters.shape[1])) |
|
2883 | 2899 |
dataOut.data_param = arrayParameters |
|
2884 | ||
|
2900 | ||
|
2885 | 2901 |
if arrayParameters is None: |
|
2886 | 2902 |
dataOut.flagNoData = True |
|
2887 | 2903 |
else: |
|
2888 | 2904 |
dataOut.flagNoData = True |
|
2889 | ||
|
2905 | ||
|
2890 | 2906 |
return |
|
2891 | ||
|
2907 | ||
|
2892 | 2908 |
def __getHardwarePhaseDiff(self, voltage0, pairslist, newheis, n): |
|
2893 | ||
|
2909 | ||
|
2894 | 2910 |
minIndex = min(newheis[0]) |
|
2895 | 2911 |
maxIndex = max(newheis[0]) |
|
2896 | ||
|
2912 | ||
|
2897 | 2913 |
voltage = voltage0[:,:,minIndex:maxIndex+1] |
|
2898 | 2914 |
nLength = voltage.shape[1]/n |
|
2899 | 2915 |
nMin = 0 |
|
2900 | 2916 |
nMax = 0 |
|
2901 | 2917 |
phaseOffset = numpy.zeros((len(pairslist),n)) |
|
2902 | ||
|
2918 | ||
|
2903 | 2919 |
for i in range(n): |
|
2904 | 2920 |
nMax += nLength |
|
2905 | 2921 |
phaseCCF = -numpy.angle(self.__calculateCCF(voltage[:,nMin:nMax,:], pairslist, [0])) |
|
2906 | 2922 |
phaseCCF = numpy.mean(phaseCCF, axis = 2) |
|
2907 |
phaseOffset[:,i] = phaseCCF.transpose() |
|
|
2923 | phaseOffset[:,i] = phaseCCF.transpose() | |
|
2908 | 2924 |
nMin = nMax |
|
2909 | 2925 |
# phaseDiff, phaseArrival = self.estimatePhaseDifference(voltage, pairslist) |
|
2910 | ||
|
2926 | ||
|
2911 | 2927 |
#Remove Outliers |
|
2912 | 2928 |
factor = 2 |
|
2913 | 2929 |
wt = phaseOffset - signal.medfilt(phaseOffset,(1,5)) |
|
2914 | 2930 |
dw = numpy.std(wt,axis = 1) |
|
2915 | 2931 |
dw = dw.reshape((dw.size,1)) |
|
2916 |
ind = numpy.where(numpy.logical_or(wt>dw*factor,wt<-dw*factor)) |
|
|
2932 | ind = numpy.where(numpy.logical_or(wt>dw*factor,wt<-dw*factor)) | |
|
2917 | 2933 |
phaseOffset[ind] = numpy.nan |
|
2918 |
phaseOffset = stats.nanmean(phaseOffset, axis=1) |
|
|
2919 | ||
|
2934 | phaseOffset = stats.nanmean(phaseOffset, axis=1) | |
|
2935 | ||
|
2920 | 2936 |
return phaseOffset |
|
2921 | ||
|
2937 | ||
|
2922 | 2938 |
def __shiftPhase(self, data, phaseShift): |
|
2923 | 2939 |
#this will shift the phase of a complex number |
|
2924 |
dataShifted = numpy.abs(data) * numpy.exp((numpy.angle(data)+phaseShift)*1j) |
|
|
2940 | dataShifted = numpy.abs(data) * numpy.exp((numpy.angle(data)+phaseShift)*1j) | |
|
2925 | 2941 |
return dataShifted |
|
2926 | ||
|
2942 | ||
|
2927 | 2943 |
def __estimatePhaseDifference(self, array, pairslist): |
|
2928 | 2944 |
nChannel = array.shape[0] |
|
2929 | 2945 |
nHeights = array.shape[2] |
|
2930 | 2946 |
numPairs = len(pairslist) |
|
2931 | 2947 |
# phaseCCF = numpy.zeros((nChannel, 5, nHeights)) |
|
2932 | 2948 |
phaseCCF = numpy.angle(self.__calculateCCF(array, pairslist, [-2,-1,0,1,2])) |
|
2933 | ||
|
2949 | ||
|
2934 | 2950 |
#Correct phases |
|
2935 | 2951 |
derPhaseCCF = phaseCCF[:,1:,:] - phaseCCF[:,0:-1,:] |
|
2936 | 2952 |
indDer = numpy.where(numpy.abs(derPhaseCCF) > numpy.pi) |
|
2937 | ||
|
2938 |
if indDer[0].shape[0] > 0: |
|
|
2953 | ||
|
2954 | if indDer[0].shape[0] > 0: | |
|
2939 | 2955 |
for i in range(indDer[0].shape[0]): |
|
2940 | 2956 |
signo = -numpy.sign(derPhaseCCF[indDer[0][i],indDer[1][i],indDer[2][i]]) |
|
2941 | 2957 |
phaseCCF[indDer[0][i],indDer[1][i]+1:,:] += signo*2*numpy.pi |
|
2942 | ||
|
2958 | ||
|
2943 | 2959 |
# for j in range(numSides): |
|
2944 | 2960 |
# phaseCCFAux = self.calculateCCF(arrayCenter, arraySides[j,:,:], [-2,1,0,1,2]) |
|
2945 | 2961 |
# phaseCCF[j,:,:] = numpy.angle(phaseCCFAux) |
|
2946 | # | |
|
2962 | # | |
|
2947 | 2963 |
#Linear |
|
2948 | 2964 |
phaseInt = numpy.zeros((numPairs,1)) |
|
2949 | 2965 |
angAllCCF = phaseCCF[:,[0,1,3,4],0] |
@@ -2953,16 +2969,16 class SMDetection(Operation): | |||
|
2953 | 2969 |
#Phase Differences |
|
2954 | 2970 |
phaseDiff = phaseInt - phaseCCF[:,2,:] |
|
2955 | 2971 |
phaseArrival = phaseInt.reshape(phaseInt.size) |
|
2956 | ||
|
2972 | ||
|
2957 | 2973 |
#Dealias |
|
2958 | 2974 |
phaseArrival = numpy.angle(numpy.exp(1j*phaseArrival)) |
|
2959 | 2975 |
# indAlias = numpy.where(phaseArrival > numpy.pi) |
|
2960 | 2976 |
# phaseArrival[indAlias] -= 2*numpy.pi |
|
2961 | 2977 |
# indAlias = numpy.where(phaseArrival < -numpy.pi) |
|
2962 | 2978 |
# phaseArrival[indAlias] += 2*numpy.pi |
|
2963 | ||
|
2979 | ||
|
2964 | 2980 |
return phaseDiff, phaseArrival |
|
2965 | ||
|
2981 | ||
|
2966 | 2982 |
def __coherentDetection(self, volts, timeSegment, timeInterval, pairslist, thresh): |
|
2967 | 2983 |
#this function will run the coherent detection used in Holdworth et al. 2004 and return the net power |
|
2968 | 2984 |
#find the phase shifts of each channel over 1 second intervals |
@@ -2972,25 +2988,25 class SMDetection(Operation): | |||
|
2972 | 2988 |
numHeights = volts.shape[2] |
|
2973 | 2989 |
nChannel = volts.shape[0] |
|
2974 | 2990 |
voltsCohDet = volts.copy() |
|
2975 | ||
|
2991 | ||
|
2976 | 2992 |
pairsarray = numpy.array(pairslist) |
|
2977 | 2993 |
indSides = pairsarray[:,1] |
|
2978 | 2994 |
# indSides = numpy.array(range(nChannel)) |
|
2979 | 2995 |
# indSides = numpy.delete(indSides, indCenter) |
|
2980 | # | |
|
2996 | # | |
|
2981 | 2997 |
# listCenter = numpy.array_split(volts[indCenter,:,:], numBlocks, 0) |
|
2982 | 2998 |
listBlocks = numpy.array_split(volts, numBlocks, 1) |
|
2983 | ||
|
2999 | ||
|
2984 | 3000 |
startInd = 0 |
|
2985 | 3001 |
endInd = 0 |
|
2986 | ||
|
3002 | ||
|
2987 | 3003 |
for i in range(numBlocks): |
|
2988 | 3004 |
startInd = endInd |
|
2989 |
endInd = endInd + listBlocks[i].shape[1] |
|
|
2990 | ||
|
3005 | endInd = endInd + listBlocks[i].shape[1] | |
|
3006 | ||
|
2991 | 3007 |
arrayBlock = listBlocks[i] |
|
2992 | 3008 |
# arrayBlockCenter = listCenter[i] |
|
2993 | ||
|
3009 | ||
|
2994 | 3010 |
#Estimate the Phase Difference |
|
2995 | 3011 |
phaseDiff, aux = self.__estimatePhaseDifference(arrayBlock, pairslist) |
|
2996 | 3012 |
#Phase Difference RMS |
@@ -3002,21 +3018,21 class SMDetection(Operation): | |||
|
3002 | 3018 |
for j in range(indSides.size): |
|
3003 | 3019 |
arrayBlock[indSides[j],:,indPhase] = self.__shiftPhase(arrayBlock[indSides[j],:,indPhase], phaseDiff[j,indPhase].transpose()) |
|
3004 | 3020 |
voltsCohDet[:,startInd:endInd,:] = arrayBlock |
|
3005 | ||
|
3021 | ||
|
3006 | 3022 |
return voltsCohDet |
|
3007 | ||
|
3023 | ||
|
3008 | 3024 |
def __calculateCCF(self, volts, pairslist ,laglist): |
|
3009 | ||
|
3025 | ||
|
3010 | 3026 |
nHeights = volts.shape[2] |
|
3011 |
nPoints = volts.shape[1] |
|
|
3027 | nPoints = volts.shape[1] | |
|
3012 | 3028 |
voltsCCF = numpy.zeros((len(pairslist), len(laglist), nHeights),dtype = 'complex') |
|
3013 | ||
|
3029 | ||
|
3014 | 3030 |
for i in range(len(pairslist)): |
|
3015 | 3031 |
volts1 = volts[pairslist[i][0]] |
|
3016 |
volts2 = volts[pairslist[i][1]] |
|
|
3017 | ||
|
3032 | volts2 = volts[pairslist[i][1]] | |
|
3033 | ||
|
3018 | 3034 |
for t in range(len(laglist)): |
|
3019 |
idxT = laglist[t] |
|
|
3035 | idxT = laglist[t] | |
|
3020 | 3036 |
if idxT >= 0: |
|
3021 | 3037 |
vStacked = numpy.vstack((volts2[idxT:,:], |
|
3022 | 3038 |
numpy.zeros((idxT, nHeights),dtype='complex'))) |
@@ -3024,10 +3040,10 class SMDetection(Operation): | |||
|
3024 | 3040 |
vStacked = numpy.vstack((numpy.zeros((-idxT, nHeights),dtype='complex'), |
|
3025 | 3041 |
volts2[:(nPoints + idxT),:])) |
|
3026 | 3042 |
voltsCCF[i,t,:] = numpy.sum((numpy.conjugate(volts1)*vStacked),axis=0) |
|
3027 | ||
|
3043 | ||
|
3028 | 3044 |
vStacked = None |
|
3029 | 3045 |
return voltsCCF |
|
3030 | ||
|
3046 | ||
|
3031 | 3047 |
def __getNoise(self, power, timeSegment, timeInterval): |
|
3032 | 3048 |
numProfPerBlock = numpy.ceil(timeSegment/timeInterval) |
|
3033 | 3049 |
numBlocks = int(power.shape[0]/numProfPerBlock) |
@@ -3036,100 +3052,100 class SMDetection(Operation): | |||
|
3036 | 3052 |
listPower = numpy.array_split(power, numBlocks, 0) |
|
3037 | 3053 |
noise = numpy.zeros((power.shape[0], power.shape[1])) |
|
3038 | 3054 |
noise1 = numpy.zeros((power.shape[0], power.shape[1])) |
|
3039 | ||
|
3055 | ||
|
3040 | 3056 |
startInd = 0 |
|
3041 | 3057 |
endInd = 0 |
|
3042 | ||
|
3058 | ||
|
3043 | 3059 |
for i in range(numBlocks): #split por canal |
|
3044 | 3060 |
startInd = endInd |
|
3045 |
endInd = endInd + listPower[i].shape[0] |
|
|
3046 | ||
|
3061 | endInd = endInd + listPower[i].shape[0] | |
|
3062 | ||
|
3047 | 3063 |
arrayBlock = listPower[i] |
|
3048 | 3064 |
noiseAux = numpy.mean(arrayBlock, 0) |
|
3049 | 3065 |
# noiseAux = numpy.median(noiseAux) |
|
3050 | 3066 |
# noiseAux = numpy.mean(arrayBlock) |
|
3051 |
noise[startInd:endInd,:] = noise[startInd:endInd,:] + noiseAux |
|
|
3052 | ||
|
3067 | noise[startInd:endInd,:] = noise[startInd:endInd,:] + noiseAux | |
|
3068 | ||
|
3053 | 3069 |
noiseAux1 = numpy.mean(arrayBlock) |
|
3054 |
noise1[startInd:endInd,:] = noise1[startInd:endInd,:] + noiseAux1 |
|
|
3055 | ||
|
3070 | noise1[startInd:endInd,:] = noise1[startInd:endInd,:] + noiseAux1 | |
|
3071 | ||
|
3056 | 3072 |
return noise, noise1 |
|
3057 | ||
|
3073 | ||
|
3058 | 3074 |
def __findMeteors(self, power, thresh): |
|
3059 | 3075 |
nProf = power.shape[0] |
|
3060 | 3076 |
nHeights = power.shape[1] |
|
3061 | 3077 |
listMeteors = [] |
|
3062 | ||
|
3078 | ||
|
3063 | 3079 |
for i in range(nHeights): |
|
3064 | 3080 |
powerAux = power[:,i] |
|
3065 | 3081 |
threshAux = thresh[:,i] |
|
3066 | ||
|
3082 | ||
|
3067 | 3083 |
indUPthresh = numpy.where(powerAux > threshAux)[0] |
|
3068 | 3084 |
indDNthresh = numpy.where(powerAux <= threshAux)[0] |
|
3069 | ||
|
3085 | ||
|
3070 | 3086 |
j = 0 |
|
3071 | ||
|
3087 | ||
|
3072 | 3088 |
while (j < indUPthresh.size - 2): |
|
3073 | 3089 |
if (indUPthresh[j + 2] == indUPthresh[j] + 2): |
|
3074 | 3090 |
indDNAux = numpy.where(indDNthresh > indUPthresh[j]) |
|
3075 | 3091 |
indDNthresh = indDNthresh[indDNAux] |
|
3076 | ||
|
3092 | ||
|
3077 | 3093 |
if (indDNthresh.size > 0): |
|
3078 | 3094 |
indEnd = indDNthresh[0] - 1 |
|
3079 | 3095 |
indInit = indUPthresh[j] |
|
3080 | ||
|
3096 | ||
|
3081 | 3097 |
meteor = powerAux[indInit:indEnd + 1] |
|
3082 | 3098 |
indPeak = meteor.argmax() + indInit |
|
3083 | 3099 |
FLA = sum(numpy.conj(meteor)*numpy.hstack((meteor[1:],0))) |
|
3084 | ||
|
3100 | ||
|
3085 | 3101 |
listMeteors.append(numpy.array([i,indInit,indPeak,indEnd,FLA])) #CHEQUEAR!!!!! |
|
3086 | 3102 |
j = numpy.where(indUPthresh == indEnd)[0] + 1 |
|
3087 | 3103 |
else: j+=1 |
|
3088 | 3104 |
else: j+=1 |
|
3089 | ||
|
3105 | ||
|
3090 | 3106 |
return listMeteors |
|
3091 | ||
|
3107 | ||
|
3092 | 3108 |
def __removeMultipleDetections(self,listMeteors, rangeLimit, timeLimit): |
|
3093 | ||
|
3094 |
arrayMeteors = numpy.asarray(listMeteors) |
|
|
3109 | ||
|
3110 | arrayMeteors = numpy.asarray(listMeteors) | |
|
3095 | 3111 |
listMeteors1 = [] |
|
3096 | ||
|
3112 | ||
|
3097 | 3113 |
while arrayMeteors.shape[0] > 0: |
|
3098 | 3114 |
FLAs = arrayMeteors[:,4] |
|
3099 | 3115 |
maxFLA = FLAs.argmax() |
|
3100 | 3116 |
listMeteors1.append(arrayMeteors[maxFLA,:]) |
|
3101 | ||
|
3117 | ||
|
3102 | 3118 |
MeteorInitTime = arrayMeteors[maxFLA,1] |
|
3103 | 3119 |
MeteorEndTime = arrayMeteors[maxFLA,3] |
|
3104 | 3120 |
MeteorHeight = arrayMeteors[maxFLA,0] |
|
3105 | ||
|
3121 | ||
|
3106 | 3122 |
#Check neighborhood |
|
3107 | 3123 |
maxHeightIndex = MeteorHeight + rangeLimit |
|
3108 | 3124 |
minHeightIndex = MeteorHeight - rangeLimit |
|
3109 | 3125 |
minTimeIndex = MeteorInitTime - timeLimit |
|
3110 | 3126 |
maxTimeIndex = MeteorEndTime + timeLimit |
|
3111 | ||
|
3127 | ||
|
3112 | 3128 |
#Check Heights |
|
3113 | 3129 |
indHeight = numpy.logical_and(arrayMeteors[:,0] >= minHeightIndex, arrayMeteors[:,0] <= maxHeightIndex) |
|
3114 | 3130 |
indTime = numpy.logical_and(arrayMeteors[:,3] >= minTimeIndex, arrayMeteors[:,1] <= maxTimeIndex) |
|
3115 | 3131 |
indBoth = numpy.where(numpy.logical_and(indTime,indHeight)) |
|
3116 | ||
|
3132 | ||
|
3117 | 3133 |
arrayMeteors = numpy.delete(arrayMeteors, indBoth, axis = 0) |
|
3118 | ||
|
3134 | ||
|
3119 | 3135 |
return listMeteors1 |
|
3120 | ||
|
3136 | ||
|
3121 | 3137 |
def __meteorReestimation(self, listMeteors, volts, pairslist, thresh, noise, timeInterval,frequency): |
|
3122 | 3138 |
numHeights = volts.shape[2] |
|
3123 | 3139 |
nChannel = volts.shape[0] |
|
3124 | ||
|
3140 | ||
|
3125 | 3141 |
thresholdPhase = thresh[0] |
|
3126 | 3142 |
thresholdNoise = thresh[1] |
|
3127 | 3143 |
thresholdDB = float(thresh[2]) |
|
3128 | ||
|
3144 | ||
|
3129 | 3145 |
thresholdDB1 = 10**(thresholdDB/10) |
|
3130 | 3146 |
pairsarray = numpy.array(pairslist) |
|
3131 | 3147 |
indSides = pairsarray[:,1] |
|
3132 | ||
|
3148 | ||
|
3133 | 3149 |
pairslist1 = list(pairslist) |
|
3134 | 3150 |
pairslist1.append((0,1)) |
|
3135 | 3151 |
pairslist1.append((3,4)) |
@@ -3138,31 +3154,31 class SMDetection(Operation): | |||
|
3138 | 3154 |
listPowerSeries = [] |
|
3139 | 3155 |
listVoltageSeries = [] |
|
3140 | 3156 |
#volts has the war data |
|
3141 | ||
|
3157 | ||
|
3142 | 3158 |
if frequency == 30e6: |
|
3143 | 3159 |
timeLag = 45*10**-3 |
|
3144 | 3160 |
else: |
|
3145 | 3161 |
timeLag = 15*10**-3 |
|
3146 | 3162 |
lag = numpy.ceil(timeLag/timeInterval) |
|
3147 | ||
|
3163 | ||
|
3148 | 3164 |
for i in range(len(listMeteors)): |
|
3149 | ||
|
3165 | ||
|
3150 | 3166 |
###################### 3.6 - 3.7 PARAMETERS REESTIMATION ######################### |
|
3151 | 3167 |
meteorAux = numpy.zeros(16) |
|
3152 | ||
|
3168 | ||
|
3153 | 3169 |
#Loading meteor Data (mHeight, mStart, mPeak, mEnd) |
|
3154 | 3170 |
mHeight = listMeteors[i][0] |
|
3155 | 3171 |
mStart = listMeteors[i][1] |
|
3156 | 3172 |
mPeak = listMeteors[i][2] |
|
3157 | 3173 |
mEnd = listMeteors[i][3] |
|
3158 | ||
|
3174 | ||
|
3159 | 3175 |
#get the volt data between the start and end times of the meteor |
|
3160 | 3176 |
meteorVolts = volts[:,mStart:mEnd+1,mHeight] |
|
3161 | 3177 |
meteorVolts = meteorVolts.reshape(meteorVolts.shape[0], meteorVolts.shape[1], 1) |
|
3162 | ||
|
3178 | ||
|
3163 | 3179 |
#3.6. Phase Difference estimation |
|
3164 | 3180 |
phaseDiff, aux = self.__estimatePhaseDifference(meteorVolts, pairslist) |
|
3165 | ||
|
3181 | ||
|
3166 | 3182 |
#3.7. Phase difference removal & meteor start, peak and end times reestimated |
|
3167 | 3183 |
#meteorVolts0.- all Channels, all Profiles |
|
3168 | 3184 |
meteorVolts0 = volts[:,:,mHeight] |
@@ -3170,15 +3186,15 class SMDetection(Operation): | |||
|
3170 | 3186 |
meteorNoise = noise[:,mHeight] |
|
3171 | 3187 |
meteorVolts0[indSides,:] = self.__shiftPhase(meteorVolts0[indSides,:], phaseDiff) #Phase Shifting |
|
3172 | 3188 |
powerNet0 = numpy.nansum(numpy.abs(meteorVolts0)**2, axis = 0) #Power |
|
3173 | ||
|
3189 | ||
|
3174 | 3190 |
#Times reestimation |
|
3175 | 3191 |
mStart1 = numpy.where(powerNet0[:mPeak] < meteorThresh[:mPeak])[0] |
|
3176 | 3192 |
if mStart1.size > 0: |
|
3177 | 3193 |
mStart1 = mStart1[-1] + 1 |
|
3178 | ||
|
3179 |
else: |
|
|
3194 | ||
|
3195 | else: | |
|
3180 | 3196 |
mStart1 = mPeak |
|
3181 | ||
|
3197 | ||
|
3182 | 3198 |
mEnd1 = numpy.where(powerNet0[mPeak:] < meteorThresh[mPeak:])[0][0] + mPeak - 1 |
|
3183 | 3199 |
mEndDecayTime1 = numpy.where(powerNet0[mPeak:] < meteorNoise[mPeak:])[0] |
|
3184 | 3200 |
if mEndDecayTime1.size == 0: |
@@ -3186,7 +3202,7 class SMDetection(Operation): | |||
|
3186 | 3202 |
else: |
|
3187 | 3203 |
mEndDecayTime1 = mEndDecayTime1[0] + mPeak - 1 |
|
3188 | 3204 |
# mPeak1 = meteorVolts0[mStart1:mEnd1 + 1].argmax() |
|
3189 | ||
|
3205 | ||
|
3190 | 3206 |
#meteorVolts1.- all Channels, from start to end |
|
3191 | 3207 |
meteorVolts1 = meteorVolts0[:,mStart1:mEnd1 + 1] |
|
3192 | 3208 |
meteorVolts2 = meteorVolts0[:,mPeak + lag:mEnd1 + 1] |
@@ -3195,17 +3211,17 class SMDetection(Operation): | |||
|
3195 | 3211 |
meteorVolts1 = meteorVolts1.reshape(meteorVolts1.shape[0], meteorVolts1.shape[1], 1) |
|
3196 | 3212 |
meteorVolts2 = meteorVolts2.reshape(meteorVolts2.shape[0], meteorVolts2.shape[1], 1) |
|
3197 | 3213 |
##################### END PARAMETERS REESTIMATION ######################### |
|
3198 | ||
|
3214 | ||
|
3199 | 3215 |
##################### 3.8 PHASE DIFFERENCE REESTIMATION ######################## |
|
3200 | 3216 |
# if mEnd1 - mStart1 > 4: #Error Number 6: echo less than 5 samples long; too short for analysis |
|
3201 |
if meteorVolts2.shape[1] > 0: |
|
|
3217 | if meteorVolts2.shape[1] > 0: | |
|
3202 | 3218 |
#Phase Difference re-estimation |
|
3203 | 3219 |
phaseDiff1, phaseDiffint = self.__estimatePhaseDifference(meteorVolts2, pairslist1) #Phase Difference Estimation |
|
3204 | 3220 |
# phaseDiff1, phaseDiffint = self.estimatePhaseDifference(meteorVolts2, pairslist) |
|
3205 | 3221 |
meteorVolts2 = meteorVolts2.reshape(meteorVolts2.shape[0], meteorVolts2.shape[1]) |
|
3206 | 3222 |
phaseDiff11 = numpy.reshape(phaseDiff1, (phaseDiff1.shape[0],1)) |
|
3207 | 3223 |
meteorVolts2[indSides,:] = self.__shiftPhase(meteorVolts2[indSides,:], phaseDiff11[0:4]) #Phase Shifting |
|
3208 | ||
|
3224 | ||
|
3209 | 3225 |
#Phase Difference RMS |
|
3210 | 3226 |
phaseRMS1 = numpy.sqrt(numpy.mean(numpy.square(phaseDiff1))) |
|
3211 | 3227 |
powerNet1 = numpy.nansum(numpy.abs(meteorVolts1[:,:])**2,0) |
@@ -3220,27 +3236,27 class SMDetection(Operation): | |||
|
3220 | 3236 |
#Vectorize |
|
3221 | 3237 |
meteorAux[0:7] = [mHeight, mStart1, mPeak1, mEnd1, mPeakPower1, mSNR1, phaseRMS1] |
|
3222 | 3238 |
meteorAux[7:11] = phaseDiffint[0:4] |
|
3223 | ||
|
3239 | ||
|
3224 | 3240 |
#Rejection Criterions |
|
3225 | 3241 |
if phaseRMS1 > thresholdPhase: #Error Number 17: Phase variation |
|
3226 | 3242 |
meteorAux[-1] = 17 |
|
3227 | 3243 |
elif mSNR1 < thresholdDB1: #Error Number 1: SNR < threshold dB |
|
3228 | 3244 |
meteorAux[-1] = 1 |
|
3229 | ||
|
3230 | ||
|
3231 |
else: |
|
|
3245 | ||
|
3246 | ||
|
3247 | else: | |
|
3232 | 3248 |
meteorAux[0:4] = [mHeight, mStart, mPeak, mEnd] |
|
3233 | 3249 |
meteorAux[-1] = 6 #Error Number 6: echo less than 5 samples long; too short for analysis |
|
3234 | 3250 |
PowerSeries = 0 |
|
3235 | ||
|
3251 | ||
|
3236 | 3252 |
listMeteors1.append(meteorAux) |
|
3237 | 3253 |
listPowerSeries.append(PowerSeries) |
|
3238 | 3254 |
listVoltageSeries.append(meteorVolts1) |
|
3239 | ||
|
3240 |
return listMeteors1, listPowerSeries, listVoltageSeries |
|
|
3241 | ||
|
3255 | ||
|
3256 | return listMeteors1, listPowerSeries, listVoltageSeries | |
|
3257 | ||
|
3242 | 3258 |
def __estimateDecayTime(self, listMeteors, listPower, timeInterval, frequency): |
|
3243 | ||
|
3259 | ||
|
3244 | 3260 |
threshError = 10 |
|
3245 | 3261 |
#Depending if it is 30 or 50 MHz |
|
3246 | 3262 |
if frequency == 30e6: |
@@ -3248,22 +3264,22 class SMDetection(Operation): | |||
|
3248 | 3264 |
else: |
|
3249 | 3265 |
timeLag = 15*10**-3 |
|
3250 | 3266 |
lag = numpy.ceil(timeLag/timeInterval) |
|
3251 | ||
|
3267 | ||
|
3252 | 3268 |
listMeteors1 = [] |
|
3253 | ||
|
3269 | ||
|
3254 | 3270 |
for i in range(len(listMeteors)): |
|
3255 | 3271 |
meteorPower = listPower[i] |
|
3256 | 3272 |
meteorAux = listMeteors[i] |
|
3257 | ||
|
3273 | ||
|
3258 | 3274 |
if meteorAux[-1] == 0: |
|
3259 | 3275 | |
|
3260 |
try: |
|
|
3276 | try: | |
|
3261 | 3277 |
indmax = meteorPower.argmax() |
|
3262 | 3278 |
indlag = indmax + lag |
|
3263 | ||
|
3279 | ||
|
3264 | 3280 |
y = meteorPower[indlag:] |
|
3265 | 3281 |
x = numpy.arange(0, y.size)*timeLag |
|
3266 | ||
|
3282 | ||
|
3267 | 3283 |
#first guess |
|
3268 | 3284 |
a = y[0] |
|
3269 | 3285 |
tau = timeLag |
@@ -3272,26 +3288,26 class SMDetection(Operation): | |||
|
3272 | 3288 |
y1 = self.__exponential_function(x, *popt) |
|
3273 | 3289 |
#error estimation |
|
3274 | 3290 |
error = sum((y - y1)**2)/(numpy.var(y)*(y.size - popt.size)) |
|
3275 | ||
|
3291 | ||
|
3276 | 3292 |
decayTime = popt[1] |
|
3277 | 3293 |
riseTime = indmax*timeInterval |
|
3278 | 3294 |
meteorAux[11:13] = [decayTime, error] |
|
3279 | ||
|
3295 | ||
|
3280 | 3296 |
#Table items 7, 8 and 11 |
|
3281 | 3297 |
if (riseTime > 0.3): #Number 7: Echo rise exceeds 0.3s |
|
3282 |
meteorAux[-1] = 7 |
|
|
3298 | meteorAux[-1] = 7 | |
|
3283 | 3299 |
elif (decayTime < 2*riseTime) : #Number 8: Echo decay time less than than twice rise time |
|
3284 | 3300 |
meteorAux[-1] = 8 |
|
3285 | 3301 |
if (error > threshError): #Number 11: Poor fit to amplitude for estimation of decay time |
|
3286 |
meteorAux[-1] = 11 |
|
|
3287 | ||
|
3288 | ||
|
3302 | meteorAux[-1] = 11 | |
|
3303 | ||
|
3304 | ||
|
3289 | 3305 |
except: |
|
3290 |
meteorAux[-1] = 11 |
|
|
3291 | ||
|
3292 | ||
|
3306 | meteorAux[-1] = 11 | |
|
3307 | ||
|
3308 | ||
|
3293 | 3309 |
listMeteors1.append(meteorAux) |
|
3294 | ||
|
3310 | ||
|
3295 | 3311 |
return listMeteors1 |
|
3296 | 3312 | |
|
3297 | 3313 |
#Exponential Function |
@@ -3299,9 +3315,9 class SMDetection(Operation): | |||
|
3299 | 3315 |
def __exponential_function(self, x, a, tau): |
|
3300 | 3316 |
y = a*numpy.exp(-x/tau) |
|
3301 | 3317 |
return y |
|
3302 | ||
|
3318 | ||
|
3303 | 3319 |
def __getRadialVelocity(self, listMeteors, listVolts, radialStdThresh, pairslist, timeInterval): |
|
3304 | ||
|
3320 | ||
|
3305 | 3321 |
pairslist1 = list(pairslist) |
|
3306 | 3322 |
pairslist1.append((0,1)) |
|
3307 | 3323 |
pairslist1.append((3,4)) |
@@ -3311,33 +3327,33 class SMDetection(Operation): | |||
|
3311 | 3327 |
c = 3e8 |
|
3312 | 3328 |
lag = numpy.ceil(timeLag/timeInterval) |
|
3313 | 3329 |
freq = 30e6 |
|
3314 | ||
|
3330 | ||
|
3315 | 3331 |
listMeteors1 = [] |
|
3316 | ||
|
3332 | ||
|
3317 | 3333 |
for i in range(len(listMeteors)): |
|
3318 | 3334 |
meteorAux = listMeteors[i] |
|
3319 | 3335 |
if meteorAux[-1] == 0: |
|
3320 | 3336 |
mStart = listMeteors[i][1] |
|
3321 |
mPeak = listMeteors[i][2] |
|
|
3337 | mPeak = listMeteors[i][2] | |
|
3322 | 3338 |
mLag = mPeak - mStart + lag |
|
3323 | ||
|
3339 | ||
|
3324 | 3340 |
#get the volt data between the start and end times of the meteor |
|
3325 | 3341 |
meteorVolts = listVolts[i] |
|
3326 | 3342 |
meteorVolts = meteorVolts.reshape(meteorVolts.shape[0], meteorVolts.shape[1], 1) |
|
3327 | 3343 | |
|
3328 | 3344 |
#Get CCF |
|
3329 | 3345 |
allCCFs = self.__calculateCCF(meteorVolts, pairslist1, [-2,-1,0,1,2]) |
|
3330 | ||
|
3346 | ||
|
3331 | 3347 |
#Method 2 |
|
3332 | 3348 |
slopes = numpy.zeros(numPairs) |
|
3333 | 3349 |
time = numpy.array([-2,-1,1,2])*timeInterval |
|
3334 | 3350 |
angAllCCF = numpy.angle(allCCFs[:,[0,1,3,4],0]) |
|
3335 | ||
|
3351 | ||
|
3336 | 3352 |
#Correct phases |
|
3337 | 3353 |
derPhaseCCF = angAllCCF[:,1:] - angAllCCF[:,0:-1] |
|
3338 | 3354 |
indDer = numpy.where(numpy.abs(derPhaseCCF) > numpy.pi) |
|
3339 | ||
|
3340 |
if indDer[0].shape[0] > 0: |
|
|
3355 | ||
|
3356 | if indDer[0].shape[0] > 0: | |
|
3341 | 3357 |
for i in range(indDer[0].shape[0]): |
|
3342 | 3358 |
signo = -numpy.sign(derPhaseCCF[indDer[0][i],indDer[1][i]]) |
|
3343 | 3359 |
angAllCCF[indDer[0][i],indDer[1][i]+1:] += signo*2*numpy.pi |
@@ -3346,51 +3362,51 class SMDetection(Operation): | |||
|
3346 | 3362 |
for j in range(numPairs): |
|
3347 | 3363 |
fit = stats.linregress(time, angAllCCF[j,:]) |
|
3348 | 3364 |
slopes[j] = fit[0] |
|
3349 | ||
|
3365 | ||
|
3350 | 3366 |
#Remove Outlier |
|
3351 | 3367 |
# indOut = numpy.argmax(numpy.abs(slopes - numpy.mean(slopes))) |
|
3352 | 3368 |
# slopes = numpy.delete(slopes,indOut) |
|
3353 | 3369 |
# indOut = numpy.argmax(numpy.abs(slopes - numpy.mean(slopes))) |
|
3354 | 3370 |
# slopes = numpy.delete(slopes,indOut) |
|
3355 | ||
|
3371 | ||
|
3356 | 3372 |
radialVelocity = -numpy.mean(slopes)*(0.25/numpy.pi)*(c/freq) |
|
3357 | 3373 |
radialError = numpy.std(slopes)*(0.25/numpy.pi)*(c/freq) |
|
3358 | 3374 |
meteorAux[-2] = radialError |
|
3359 | 3375 |
meteorAux[-3] = radialVelocity |
|
3360 | ||
|
3376 | ||
|
3361 | 3377 |
#Setting Error |
|
3362 | 3378 |
#Number 15: Radial Drift velocity or projected horizontal velocity exceeds 200 m/s |
|
3363 |
if numpy.abs(radialVelocity) > 200: |
|
|
3379 | if numpy.abs(radialVelocity) > 200: | |
|
3364 | 3380 |
meteorAux[-1] = 15 |
|
3365 | 3381 |
#Number 12: Poor fit to CCF variation for estimation of radial drift velocity |
|
3366 | 3382 |
elif radialError > radialStdThresh: |
|
3367 | 3383 |
meteorAux[-1] = 12 |
|
3368 | ||
|
3384 | ||
|
3369 | 3385 |
listMeteors1.append(meteorAux) |
|
3370 | 3386 |
return listMeteors1 |
|
3371 | ||
|
3387 | ||
|
3372 | 3388 |
def __setNewArrays(self, listMeteors, date, heiRang): |
|
3373 | ||
|
3389 | ||
|
3374 | 3390 |
#New arrays |
|
3375 | 3391 |
arrayMeteors = numpy.array(listMeteors) |
|
3376 | 3392 |
arrayParameters = numpy.zeros((len(listMeteors), 13)) |
|
3377 | ||
|
3393 | ||
|
3378 | 3394 |
#Date inclusion |
|
3379 | 3395 |
# date = re.findall(r'\((.*?)\)', date) |
|
3380 | 3396 |
# date = date[0].split(',') |
|
3381 | 3397 |
# date = map(int, date) |
|
3382 | # | |
|
3398 | # | |
|
3383 | 3399 |
# if len(date)<6: |
|
3384 | 3400 |
# date.append(0) |
|
3385 | # | |
|
3401 | # | |
|
3386 | 3402 |
# date = [date[0]*10000 + date[1]*100 + date[2], date[3]*10000 + date[4]*100 + date[5]] |
|
3387 | 3403 |
# arrayDate = numpy.tile(date, (len(listMeteors), 1)) |
|
3388 | 3404 |
arrayDate = numpy.tile(date, (len(listMeteors))) |
|
3389 | ||
|
3405 | ||
|
3390 | 3406 |
#Meteor array |
|
3391 | 3407 |
# arrayMeteors[:,0] = heiRang[arrayMeteors[:,0].astype(int)] |
|
3392 | 3408 |
# arrayMeteors = numpy.hstack((arrayDate, arrayMeteors)) |
|
3393 | ||
|
3409 | ||
|
3394 | 3410 |
#Parameters Array |
|
3395 | 3411 |
arrayParameters[:,0] = arrayDate #Date |
|
3396 | 3412 |
arrayParameters[:,1] = heiRang[arrayMeteors[:,0].astype(int)] #Range |
@@ -3398,13 +3414,13 class SMDetection(Operation): | |||
|
3398 | 3414 |
arrayParameters[:,8:12] = arrayMeteors[:,7:11] #Phases |
|
3399 | 3415 |
arrayParameters[:,-1] = arrayMeteors[:,-1] #Error |
|
3400 | 3416 | |
|
3401 | ||
|
3417 | ||
|
3402 | 3418 |
return arrayParameters |
|
3403 | ||
|
3419 | ||
|
3404 | 3420 |
class CorrectSMPhases(Operation): |
|
3405 | ||
|
3421 | ||
|
3406 | 3422 |
def run(self, dataOut, phaseOffsets, hmin = 50, hmax = 150, azimuth = 45, channelPositions = None): |
|
3407 | ||
|
3423 | ||
|
3408 | 3424 |
arrayParameters = dataOut.data_param |
|
3409 | 3425 |
pairsList = [] |
|
3410 | 3426 |
pairx = (0,1) |
@@ -3412,49 +3428,49 class CorrectSMPhases(Operation): | |||
|
3412 | 3428 |
pairsList.append(pairx) |
|
3413 | 3429 |
pairsList.append(pairy) |
|
3414 | 3430 |
jph = numpy.zeros(4) |
|
3415 | ||
|
3431 | ||
|
3416 | 3432 |
phaseOffsets = numpy.array(phaseOffsets)*numpy.pi/180 |
|
3417 | 3433 |
# arrayParameters[:,8:12] = numpy.unwrap(arrayParameters[:,8:12] + phaseOffsets) |
|
3418 | 3434 |
arrayParameters[:,8:12] = numpy.angle(numpy.exp(1j*(arrayParameters[:,8:12] + phaseOffsets))) |
|
3419 | ||
|
3435 | ||
|
3420 | 3436 |
meteorOps = SMOperations() |
|
3421 | 3437 |
if channelPositions is None: |
|
3422 | 3438 |
# channelPositions = [(2.5,0), (0,2.5), (0,0), (0,4.5), (-2,0)] #T |
|
3423 | 3439 |
channelPositions = [(4.5,2), (2,4.5), (2,2), (2,0), (0,2)] #Estrella |
|
3424 | ||
|
3440 | ||
|
3425 | 3441 |
pairslist0, distances = meteorOps.getPhasePairs(channelPositions) |
|
3426 | 3442 |
h = (hmin,hmax) |
|
3427 | ||
|
3443 | ||
|
3428 | 3444 |
arrayParameters = meteorOps.getMeteorParams(arrayParameters, azimuth, h, pairsList, distances, jph) |
|
3429 | ||
|
3445 | ||
|
3430 | 3446 |
dataOut.data_param = arrayParameters |
|
3431 | 3447 |
return |
|
3432 | 3448 | |
|
3433 | 3449 |
class SMPhaseCalibration(Operation): |
|
3434 | ||
|
3450 | ||
|
3435 | 3451 |
__buffer = None |
|
3436 | 3452 | |
|
3437 | 3453 |
__initime = None |
|
3438 | 3454 | |
|
3439 | 3455 |
__dataReady = False |
|
3440 | ||
|
3456 | ||
|
3441 | 3457 |
__isConfig = False |
|
3442 | ||
|
3458 | ||
|
3443 | 3459 |
def __checkTime(self, currentTime, initTime, paramInterval, outputInterval): |
|
3444 | ||
|
3460 | ||
|
3445 | 3461 |
dataTime = currentTime + paramInterval |
|
3446 | 3462 |
deltaTime = dataTime - initTime |
|
3447 | ||
|
3463 | ||
|
3448 | 3464 |
if deltaTime >= outputInterval or deltaTime < 0: |
|
3449 | 3465 |
return True |
|
3450 | ||
|
3466 | ||
|
3451 | 3467 |
return False |
|
3452 | ||
|
3468 | ||
|
3453 | 3469 |
def __getGammas(self, pairs, d, phases): |
|
3454 | 3470 |
gammas = numpy.zeros(2) |
|
3455 | ||
|
3471 | ||
|
3456 | 3472 |
for i in range(len(pairs)): |
|
3457 | ||
|
3473 | ||
|
3458 | 3474 |
pairi = pairs[i] |
|
3459 | 3475 | |
|
3460 | 3476 |
phip3 = phases[:,pairi[0]] |
@@ -3468,7 +3484,7 class SMPhaseCalibration(Operation): | |||
|
3468 | 3484 |
jgamma = numpy.angle(numpy.exp(1j*jgamma)) |
|
3469 | 3485 |
# jgamma[jgamma>numpy.pi] -= 2*numpy.pi |
|
3470 | 3486 |
# jgamma[jgamma<-numpy.pi] += 2*numpy.pi |
|
3471 | ||
|
3487 | ||
|
3472 | 3488 |
#Revised distribution |
|
3473 | 3489 |
jgammaArray = numpy.hstack((jgamma,jgamma+0.5*numpy.pi,jgamma-0.5*numpy.pi)) |
|
3474 | 3490 | |
@@ -3477,39 +3493,39 class SMPhaseCalibration(Operation): | |||
|
3477 | 3493 |
rmin = -0.5*numpy.pi |
|
3478 | 3494 |
rmax = 0.5*numpy.pi |
|
3479 | 3495 |
phaseHisto = numpy.histogram(jgammaArray, bins=nBins, range=(rmin,rmax)) |
|
3480 | ||
|
3496 | ||
|
3481 | 3497 |
meteorsY = phaseHisto[0] |
|
3482 | 3498 |
phasesX = phaseHisto[1][:-1] |
|
3483 | 3499 |
width = phasesX[1] - phasesX[0] |
|
3484 | 3500 |
phasesX += width/2 |
|
3485 | ||
|
3501 | ||
|
3486 | 3502 |
#Gaussian aproximation |
|
3487 | 3503 |
bpeak = meteorsY.argmax() |
|
3488 | 3504 |
peak = meteorsY.max() |
|
3489 | 3505 |
jmin = bpeak - 5 |
|
3490 | 3506 |
jmax = bpeak + 5 + 1 |
|
3491 | ||
|
3507 | ||
|
3492 | 3508 |
if jmin<0: |
|
3493 | 3509 |
jmin = 0 |
|
3494 | 3510 |
jmax = 6 |
|
3495 | 3511 |
elif jmax > meteorsY.size: |
|
3496 | 3512 |
jmin = meteorsY.size - 6 |
|
3497 | 3513 |
jmax = meteorsY.size |
|
3498 | ||
|
3514 | ||
|
3499 | 3515 |
x0 = numpy.array([peak,bpeak,50]) |
|
3500 | 3516 |
coeff = optimize.leastsq(self.__residualFunction, x0, args=(meteorsY[jmin:jmax], phasesX[jmin:jmax])) |
|
3501 | ||
|
3517 | ||
|
3502 | 3518 |
#Gammas |
|
3503 | 3519 |
gammas[i] = coeff[0][1] |
|
3504 | ||
|
3520 | ||
|
3505 | 3521 |
return gammas |
|
3506 | ||
|
3522 | ||
|
3507 | 3523 |
def __residualFunction(self, coeffs, y, t): |
|
3508 | ||
|
3524 | ||
|
3509 | 3525 |
return y - self.__gauss_function(t, coeffs) |
|
3510 | 3526 | |
|
3511 | 3527 |
def __gauss_function(self, t, coeffs): |
|
3512 | ||
|
3528 | ||
|
3513 | 3529 |
return coeffs[0]*numpy.exp(-0.5*((t - coeffs[1]) / coeffs[2])**2) |
|
3514 | 3530 | |
|
3515 | 3531 |
def __getPhases(self, azimuth, h, pairsList, d, gammas, meteorsArray): |
@@ -3530,16 +3546,16 class SMPhaseCalibration(Operation): | |||
|
3530 | 3546 |
max_xangle = range_angle[iz]/2 + center_xangle |
|
3531 | 3547 |
min_yangle = -range_angle[iz]/2 + center_yangle |
|
3532 | 3548 |
max_yangle = range_angle[iz]/2 + center_yangle |
|
3533 | ||
|
3549 | ||
|
3534 | 3550 |
inc_x = (max_xangle-min_xangle)/nstepsx |
|
3535 | 3551 |
inc_y = (max_yangle-min_yangle)/nstepsy |
|
3536 | ||
|
3552 | ||
|
3537 | 3553 |
alpha_y = numpy.arange(nstepsy)*inc_y + min_yangle |
|
3538 | 3554 |
alpha_x = numpy.arange(nstepsx)*inc_x + min_xangle |
|
3539 | 3555 |
penalty = numpy.zeros((nstepsx,nstepsy)) |
|
3540 | 3556 |
jph_array = numpy.zeros((nchan,nstepsx,nstepsy)) |
|
3541 | 3557 |
jph = numpy.zeros(nchan) |
|
3542 | ||
|
3558 | ||
|
3543 | 3559 |
# Iterations looking for the offset |
|
3544 | 3560 |
for iy in range(int(nstepsy)): |
|
3545 | 3561 |
for ix in range(int(nstepsx)): |
@@ -3547,46 +3563,46 class SMPhaseCalibration(Operation): | |||
|
3547 | 3563 |
d2 = d[pairsList[1][1]] |
|
3548 | 3564 |
d5 = d[pairsList[0][0]] |
|
3549 | 3565 |
d4 = d[pairsList[0][1]] |
|
3550 | ||
|
3566 | ||
|
3551 | 3567 |
alp2 = alpha_y[iy] #gamma 1 |
|
3552 |
alp4 = alpha_x[ix] #gamma 0 |
|
|
3553 | ||
|
3568 | alp4 = alpha_x[ix] #gamma 0 | |
|
3569 | ||
|
3554 | 3570 |
alp3 = -alp2*d3/d2 - gammas[1] |
|
3555 | 3571 |
alp5 = -alp4*d5/d4 - gammas[0] |
|
3556 | 3572 |
# jph[pairy[1]] = alpha_y[iy] |
|
3557 |
# jph[pairy[0]] = -gammas[1] - alpha_y[iy]*d[pairy[1]]/d[pairy[0]] |
|
|
3558 | ||
|
3573 | # jph[pairy[0]] = -gammas[1] - alpha_y[iy]*d[pairy[1]]/d[pairy[0]] | |
|
3574 | ||
|
3559 | 3575 |
# jph[pairx[1]] = alpha_x[ix] |
|
3560 | 3576 |
# jph[pairx[0]] = -gammas[0] - alpha_x[ix]*d[pairx[1]]/d[pairx[0]] |
|
3561 | 3577 |
jph[pairsList[0][1]] = alp4 |
|
3562 | 3578 |
jph[pairsList[0][0]] = alp5 |
|
3563 | 3579 |
jph[pairsList[1][0]] = alp3 |
|
3564 |
jph[pairsList[1][1]] = alp2 |
|
|
3580 | jph[pairsList[1][1]] = alp2 | |
|
3565 | 3581 |
jph_array[:,ix,iy] = jph |
|
3566 | 3582 |
# d = [2.0,2.5,2.5,2.0] |
|
3567 |
#falta chequear si va a leer bien los meteoros |
|
|
3583 | #falta chequear si va a leer bien los meteoros | |
|
3568 | 3584 |
meteorsArray1 = meteorOps.getMeteorParams(meteorsArray, azimuth, h, pairsList, d, jph) |
|
3569 | 3585 |
error = meteorsArray1[:,-1] |
|
3570 | 3586 |
ind1 = numpy.where(error==0)[0] |
|
3571 | 3587 |
penalty[ix,iy] = ind1.size |
|
3572 | ||
|
3588 | ||
|
3573 | 3589 |
i,j = numpy.unravel_index(penalty.argmax(), penalty.shape) |
|
3574 | 3590 |
phOffset = jph_array[:,i,j] |
|
3575 | ||
|
3591 | ||
|
3576 | 3592 |
center_xangle = phOffset[pairx[1]] |
|
3577 | 3593 |
center_yangle = phOffset[pairy[1]] |
|
3578 | ||
|
3594 | ||
|
3579 | 3595 |
phOffset = numpy.angle(numpy.exp(1j*jph_array[:,i,j])) |
|
3580 |
phOffset = phOffset*180/numpy.pi |
|
|
3596 | phOffset = phOffset*180/numpy.pi | |
|
3581 | 3597 |
return phOffset |
|
3582 | ||
|
3583 | ||
|
3598 | ||
|
3599 | ||
|
3584 | 3600 |
def run(self, dataOut, hmin, hmax, channelPositions=None, nHours = 1): |
|
3585 | ||
|
3601 | ||
|
3586 | 3602 |
dataOut.flagNoData = True |
|
3587 |
self.__dataReady = False |
|
|
3603 | self.__dataReady = False | |
|
3588 | 3604 |
dataOut.outputInterval = nHours*3600 |
|
3589 | ||
|
3605 | ||
|
3590 | 3606 |
if self.__isConfig == False: |
|
3591 | 3607 |
# self.__initime = dataOut.datatime.replace(minute = 0, second = 0, microsecond = 03) |
|
3592 | 3608 |
#Get Initial LTC time |
@@ -3594,19 +3610,19 class SMPhaseCalibration(Operation): | |||
|
3594 | 3610 |
self.__initime = (self.__initime.replace(minute = 0, second = 0, microsecond = 0) - datetime.datetime(1970, 1, 1)).total_seconds() |
|
3595 | 3611 | |
|
3596 | 3612 |
self.__isConfig = True |
|
3597 | ||
|
3613 | ||
|
3598 | 3614 |
if self.__buffer is None: |
|
3599 | 3615 |
self.__buffer = dataOut.data_param.copy() |
|
3600 | 3616 | |
|
3601 | 3617 |
else: |
|
3602 | 3618 |
self.__buffer = numpy.vstack((self.__buffer, dataOut.data_param)) |
|
3603 | ||
|
3619 | ||
|
3604 | 3620 |
self.__dataReady = self.__checkTime(dataOut.utctime, self.__initime, dataOut.paramInterval, dataOut.outputInterval) #Check if the buffer is ready |
|
3605 | ||
|
3621 | ||
|
3606 | 3622 |
if self.__dataReady: |
|
3607 | 3623 |
dataOut.utctimeInit = self.__initime |
|
3608 | 3624 |
self.__initime += dataOut.outputInterval #to erase time offset |
|
3609 | ||
|
3625 | ||
|
3610 | 3626 |
freq = dataOut.frequency |
|
3611 | 3627 |
c = dataOut.C #m/s |
|
3612 | 3628 |
lamb = c/freq |
@@ -3628,13 +3644,13 class SMPhaseCalibration(Operation): | |||
|
3628 | 3644 |
pairs.append((1,0)) |
|
3629 | 3645 |
else: |
|
3630 | 3646 |
pairs.append((0,1)) |
|
3631 | ||
|
3647 | ||
|
3632 | 3648 |
if distances[3] > distances[2]: |
|
3633 | 3649 |
pairs.append((3,2)) |
|
3634 | 3650 |
else: |
|
3635 | 3651 |
pairs.append((2,3)) |
|
3636 | 3652 |
# distances1 = [-distances[0]*lamb, distances[1]*lamb, -distances[2]*lamb, distances[3]*lamb] |
|
3637 | ||
|
3653 | ||
|
3638 | 3654 |
meteorsArray = self.__buffer |
|
3639 | 3655 |
error = meteorsArray[:,-1] |
|
3640 | 3656 |
boolError = (error==0)|(error==3)|(error==4)|(error==13)|(error==14) |
@@ -3642,7 +3658,7 class SMPhaseCalibration(Operation): | |||
|
3642 | 3658 |
meteorsArray = meteorsArray[ind1,:] |
|
3643 | 3659 |
meteorsArray[:,-1] = 0 |
|
3644 | 3660 |
phases = meteorsArray[:,8:12] |
|
3645 | ||
|
3661 | ||
|
3646 | 3662 |
#Calculate Gammas |
|
3647 | 3663 |
gammas = self.__getGammas(pairs, distances, phases) |
|
3648 | 3664 |
# gammas = numpy.array([-21.70409463,45.76935864])*numpy.pi/180 |
@@ -3652,22 +3668,22 class SMPhaseCalibration(Operation): | |||
|
3652 | 3668 |
dataOut.data_output = -phasesOff |
|
3653 | 3669 |
dataOut.flagNoData = False |
|
3654 | 3670 |
self.__buffer = None |
|
3655 | ||
|
3656 | ||
|
3671 | ||
|
3672 | ||
|
3657 | 3673 |
return |
|
3658 | ||
|
3674 | ||
|
3659 | 3675 |
class SMOperations(): |
|
3660 | ||
|
3676 | ||
|
3661 | 3677 |
def __init__(self): |
|
3662 | ||
|
3678 | ||
|
3663 | 3679 |
return |
|
3664 | ||
|
3680 | ||
|
3665 | 3681 |
def getMeteorParams(self, arrayParameters0, azimuth, h, pairsList, distances, jph): |
|
3666 | ||
|
3682 | ||
|
3667 | 3683 |
arrayParameters = arrayParameters0.copy() |
|
3668 | 3684 |
hmin = h[0] |
|
3669 | 3685 |
hmax = h[1] |
|
3670 | ||
|
3686 | ||
|
3671 | 3687 |
#Calculate AOA (Error N 3, 4) |
|
3672 | 3688 |
#JONES ET AL. 1998 |
|
3673 | 3689 |
AOAthresh = numpy.pi/8 |
@@ -3675,72 +3691,72 class SMOperations(): | |||
|
3675 | 3691 |
phases = -arrayParameters[:,8:12] + jph |
|
3676 | 3692 |
# phases = numpy.unwrap(phases) |
|
3677 | 3693 |
arrayParameters[:,3:6], arrayParameters[:,-1] = self.__getAOA(phases, pairsList, distances, error, AOAthresh, azimuth) |
|
3678 | ||
|
3694 | ||
|
3679 | 3695 |
#Calculate Heights (Error N 13 and 14) |
|
3680 | 3696 |
error = arrayParameters[:,-1] |
|
3681 | 3697 |
Ranges = arrayParameters[:,1] |
|
3682 | 3698 |
zenith = arrayParameters[:,4] |
|
3683 | 3699 |
arrayParameters[:,2], arrayParameters[:,-1] = self.__getHeights(Ranges, zenith, error, hmin, hmax) |
|
3684 | ||
|
3700 | ||
|
3685 | 3701 |
#----------------------- Get Final data ------------------------------------ |
|
3686 | 3702 |
# error = arrayParameters[:,-1] |
|
3687 | 3703 |
# ind1 = numpy.where(error==0)[0] |
|
3688 | 3704 |
# arrayParameters = arrayParameters[ind1,:] |
|
3689 | ||
|
3705 | ||
|
3690 | 3706 |
return arrayParameters |
|
3691 | ||
|
3707 | ||
|
3692 | 3708 |
def __getAOA(self, phases, pairsList, directions, error, AOAthresh, azimuth): |
|
3693 | ||
|
3709 | ||
|
3694 | 3710 |
arrayAOA = numpy.zeros((phases.shape[0],3)) |
|
3695 | 3711 |
cosdir0, cosdir = self.__getDirectionCosines(phases, pairsList,directions) |
|
3696 | ||
|
3712 | ||
|
3697 | 3713 |
arrayAOA[:,:2] = self.__calculateAOA(cosdir, azimuth) |
|
3698 | 3714 |
cosDirError = numpy.sum(numpy.abs(cosdir0 - cosdir), axis = 1) |
|
3699 | 3715 |
arrayAOA[:,2] = cosDirError |
|
3700 | ||
|
3716 | ||
|
3701 | 3717 |
azimuthAngle = arrayAOA[:,0] |
|
3702 | 3718 |
zenithAngle = arrayAOA[:,1] |
|
3703 | ||
|
3719 | ||
|
3704 | 3720 |
#Setting Error |
|
3705 | 3721 |
indError = numpy.where(numpy.logical_or(error == 3, error == 4))[0] |
|
3706 | 3722 |
error[indError] = 0 |
|
3707 | 3723 |
#Number 3: AOA not fesible |
|
3708 | 3724 |
indInvalid = numpy.where(numpy.logical_and((numpy.logical_or(numpy.isnan(zenithAngle), numpy.isnan(azimuthAngle))),error == 0))[0] |
|
3709 |
error[indInvalid] = 3 |
|
|
3725 | error[indInvalid] = 3 | |
|
3710 | 3726 |
#Number 4: Large difference in AOAs obtained from different antenna baselines |
|
3711 | 3727 |
indInvalid = numpy.where(numpy.logical_and(cosDirError > AOAthresh,error == 0))[0] |
|
3712 |
error[indInvalid] = 4 |
|
|
3728 | error[indInvalid] = 4 | |
|
3713 | 3729 |
return arrayAOA, error |
|
3714 | ||
|
3730 | ||
|
3715 | 3731 |
def __getDirectionCosines(self, arrayPhase, pairsList, distances): |
|
3716 | ||
|
3732 | ||
|
3717 | 3733 |
#Initializing some variables |
|
3718 | 3734 |
ang_aux = numpy.array([-8,-7,-6,-5,-4,-3,-2,-1,0,1,2,3,4,5,6,7,8])*2*numpy.pi |
|
3719 | 3735 |
ang_aux = ang_aux.reshape(1,ang_aux.size) |
|
3720 | ||
|
3736 | ||
|
3721 | 3737 |
cosdir = numpy.zeros((arrayPhase.shape[0],2)) |
|
3722 | 3738 |
cosdir0 = numpy.zeros((arrayPhase.shape[0],2)) |
|
3723 | ||
|
3724 | ||
|
3739 | ||
|
3740 | ||
|
3725 | 3741 |
for i in range(2): |
|
3726 | 3742 |
ph0 = arrayPhase[:,pairsList[i][0]] |
|
3727 | 3743 |
ph1 = arrayPhase[:,pairsList[i][1]] |
|
3728 | 3744 |
d0 = distances[pairsList[i][0]] |
|
3729 | 3745 |
d1 = distances[pairsList[i][1]] |
|
3730 | ||
|
3731 |
ph0_aux = ph0 + ph1 |
|
|
3746 | ||
|
3747 | ph0_aux = ph0 + ph1 | |
|
3732 | 3748 |
ph0_aux = numpy.angle(numpy.exp(1j*ph0_aux)) |
|
3733 | 3749 |
# ph0_aux[ph0_aux > numpy.pi] -= 2*numpy.pi |
|
3734 |
# ph0_aux[ph0_aux < -numpy.pi] += 2*numpy.pi |
|
|
3750 | # ph0_aux[ph0_aux < -numpy.pi] += 2*numpy.pi | |
|
3735 | 3751 |
#First Estimation |
|
3736 | 3752 |
cosdir0[:,i] = (ph0_aux)/(2*numpy.pi*(d0 - d1)) |
|
3737 | ||
|
3753 | ||
|
3738 | 3754 |
#Most-Accurate Second Estimation |
|
3739 | 3755 |
phi1_aux = ph0 - ph1 |
|
3740 | 3756 |
phi1_aux = phi1_aux.reshape(phi1_aux.size,1) |
|
3741 | 3757 |
#Direction Cosine 1 |
|
3742 | 3758 |
cosdir1 = (phi1_aux + ang_aux)/(2*numpy.pi*(d0 + d1)) |
|
3743 | ||
|
3759 | ||
|
3744 | 3760 |
#Searching the correct Direction Cosine |
|
3745 | 3761 |
cosdir0_aux = cosdir0[:,i] |
|
3746 | 3762 |
cosdir0_aux = cosdir0_aux.reshape(cosdir0_aux.size,1) |
@@ -3749,59 +3765,59 class SMOperations(): | |||
|
3749 | 3765 |
indcos = cosDiff.argmin(axis = 1) |
|
3750 | 3766 |
#Saving Value obtained |
|
3751 | 3767 |
cosdir[:,i] = cosdir1[numpy.arange(len(indcos)),indcos] |
|
3752 | ||
|
3768 | ||
|
3753 | 3769 |
return cosdir0, cosdir |
|
3754 | ||
|
3770 | ||
|
3755 | 3771 |
def __calculateAOA(self, cosdir, azimuth): |
|
3756 | 3772 |
cosdirX = cosdir[:,0] |
|
3757 | 3773 |
cosdirY = cosdir[:,1] |
|
3758 | ||
|
3774 | ||
|
3759 | 3775 |
zenithAngle = numpy.arccos(numpy.sqrt(1 - cosdirX**2 - cosdirY**2))*180/numpy.pi |
|
3760 | 3776 |
azimuthAngle = numpy.arctan2(cosdirX,cosdirY)*180/numpy.pi + azimuth#0 deg north, 90 deg east |
|
3761 | 3777 |
angles = numpy.vstack((azimuthAngle, zenithAngle)).transpose() |
|
3762 | ||
|
3778 | ||
|
3763 | 3779 |
return angles |
|
3764 | ||
|
3780 | ||
|
3765 | 3781 |
def __getHeights(self, Ranges, zenith, error, minHeight, maxHeight): |
|
3766 | ||
|
3782 | ||
|
3767 | 3783 |
Ramb = 375 #Ramb = c/(2*PRF) |
|
3768 | 3784 |
Re = 6371 #Earth Radius |
|
3769 | 3785 |
heights = numpy.zeros(Ranges.shape) |
|
3770 | ||
|
3786 | ||
|
3771 | 3787 |
R_aux = numpy.array([0,1,2])*Ramb |
|
3772 | 3788 |
R_aux = R_aux.reshape(1,R_aux.size) |
|
3773 | 3789 | |
|
3774 | 3790 |
Ranges = Ranges.reshape(Ranges.size,1) |
|
3775 | ||
|
3791 | ||
|
3776 | 3792 |
Ri = Ranges + R_aux |
|
3777 | 3793 |
hi = numpy.sqrt(Re**2 + Ri**2 + (2*Re*numpy.cos(zenith*numpy.pi/180)*Ri.transpose()).transpose()) - Re |
|
3778 | ||
|
3794 | ||
|
3779 | 3795 |
#Check if there is a height between 70 and 110 km |
|
3780 | 3796 |
h_bool = numpy.sum(numpy.logical_and(hi > minHeight, hi < maxHeight), axis = 1) |
|
3781 | 3797 |
ind_h = numpy.where(h_bool == 1)[0] |
|
3782 | ||
|
3798 | ||
|
3783 | 3799 |
hCorr = hi[ind_h, :] |
|
3784 | 3800 |
ind_hCorr = numpy.where(numpy.logical_and(hi > minHeight, hi < maxHeight)) |
|
3785 | ||
|
3801 | ||
|
3786 | 3802 |
hCorr = hi[ind_hCorr][:len(ind_h)] |
|
3787 | 3803 |
heights[ind_h] = hCorr |
|
3788 | ||
|
3804 | ||
|
3789 | 3805 |
#Setting Error |
|
3790 | 3806 |
#Number 13: Height unresolvable echo: not valid height within 70 to 110 km |
|
3791 |
#Number 14: Height ambiguous echo: more than one possible height within 70 to 110 km |
|
|
3807 | #Number 14: Height ambiguous echo: more than one possible height within 70 to 110 km | |
|
3792 | 3808 |
indError = numpy.where(numpy.logical_or(error == 13, error == 14))[0] |
|
3793 | 3809 |
error[indError] = 0 |
|
3794 |
indInvalid2 = numpy.where(numpy.logical_and(h_bool > 1, error == 0))[0] |
|
|
3810 | indInvalid2 = numpy.where(numpy.logical_and(h_bool > 1, error == 0))[0] | |
|
3795 | 3811 |
error[indInvalid2] = 14 |
|
3796 | 3812 |
indInvalid1 = numpy.where(numpy.logical_and(h_bool == 0, error == 0))[0] |
|
3797 |
error[indInvalid1] = 13 |
|
|
3798 | ||
|
3813 | error[indInvalid1] = 13 | |
|
3814 | ||
|
3799 | 3815 |
return heights, error |
|
3800 | ||
|
3816 | ||
|
3801 | 3817 |
def getPhasePairs(self, channelPositions): |
|
3802 | 3818 |
chanPos = numpy.array(channelPositions) |
|
3803 | 3819 |
listOper = list(itertools.combinations(list(range(5)),2)) |
|
3804 | ||
|
3820 | ||
|
3805 | 3821 |
distances = numpy.zeros(4) |
|
3806 | 3822 |
axisX = [] |
|
3807 | 3823 |
axisY = [] |
@@ -3809,15 +3825,15 class SMOperations(): | |||
|
3809 | 3825 |
distY = numpy.zeros(3) |
|
3810 | 3826 |
ix = 0 |
|
3811 | 3827 |
iy = 0 |
|
3812 | ||
|
3828 | ||
|
3813 | 3829 |
pairX = numpy.zeros((2,2)) |
|
3814 | 3830 |
pairY = numpy.zeros((2,2)) |
|
3815 | ||
|
3831 | ||
|
3816 | 3832 |
for i in range(len(listOper)): |
|
3817 | 3833 |
pairi = listOper[i] |
|
3818 | ||
|
3834 | ||
|
3819 | 3835 |
posDif = numpy.abs(chanPos[pairi[0],:] - chanPos[pairi[1],:]) |
|
3820 | ||
|
3836 | ||
|
3821 | 3837 |
if posDif[0] == 0: |
|
3822 | 3838 |
axisY.append(pairi) |
|
3823 | 3839 |
distY[iy] = posDif[1] |
@@ -3826,7 +3842,7 class SMOperations(): | |||
|
3826 | 3842 |
axisX.append(pairi) |
|
3827 | 3843 |
distX[ix] = posDif[0] |
|
3828 | 3844 |
ix += 1 |
|
3829 | ||
|
3845 | ||
|
3830 | 3846 |
for i in range(2): |
|
3831 | 3847 |
if i==0: |
|
3832 | 3848 |
dist0 = distX |
@@ -3834,7 +3850,7 class SMOperations(): | |||
|
3834 | 3850 |
else: |
|
3835 | 3851 |
dist0 = distY |
|
3836 | 3852 |
axis0 = axisY |
|
3837 | ||
|
3853 | ||
|
3838 | 3854 |
side = numpy.argsort(dist0)[:-1] |
|
3839 | 3855 |
axis0 = numpy.array(axis0)[side,:] |
|
3840 | 3856 |
chanC = int(numpy.intersect1d(axis0[0,:], axis0[1,:])[0]) |
@@ -3842,7 +3858,7 class SMOperations(): | |||
|
3842 | 3858 |
side = axis1[axis1 != chanC] |
|
3843 | 3859 |
diff1 = chanPos[chanC,i] - chanPos[side[0],i] |
|
3844 | 3860 |
diff2 = chanPos[chanC,i] - chanPos[side[1],i] |
|
3845 |
if diff1<0: |
|
|
3861 | if diff1<0: | |
|
3846 | 3862 |
chan2 = side[0] |
|
3847 | 3863 |
d2 = numpy.abs(diff1) |
|
3848 | 3864 |
chan1 = side[1] |
@@ -3852,7 +3868,7 class SMOperations(): | |||
|
3852 | 3868 |
d2 = numpy.abs(diff2) |
|
3853 | 3869 |
chan1 = side[0] |
|
3854 | 3870 |
d1 = numpy.abs(diff1) |
|
3855 | ||
|
3871 | ||
|
3856 | 3872 |
if i==0: |
|
3857 | 3873 |
chanCX = chanC |
|
3858 | 3874 |
chan1X = chan1 |
@@ -3864,10 +3880,10 class SMOperations(): | |||
|
3864 | 3880 |
chan2Y = chan2 |
|
3865 | 3881 |
distances[2:4] = numpy.array([d1,d2]) |
|
3866 | 3882 |
# axisXsides = numpy.reshape(axisX[ix,:],4) |
|
3867 | # | |
|
3883 | # | |
|
3868 | 3884 |
# channelCentX = int(numpy.intersect1d(pairX[0,:], pairX[1,:])[0]) |
|
3869 | 3885 |
# channelCentY = int(numpy.intersect1d(pairY[0,:], pairY[1,:])[0]) |
|
3870 | # | |
|
3886 | # | |
|
3871 | 3887 |
# ind25X = numpy.where(pairX[0,:] != channelCentX)[0][0] |
|
3872 | 3888 |
# ind20X = numpy.where(pairX[1,:] != channelCentX)[0][0] |
|
3873 | 3889 |
# channel25X = int(pairX[0,ind25X]) |
@@ -3876,59 +3892,59 class SMOperations(): | |||
|
3876 | 3892 |
# ind20Y = numpy.where(pairY[1,:] != channelCentY)[0][0] |
|
3877 | 3893 |
# channel25Y = int(pairY[0,ind25Y]) |
|
3878 | 3894 |
# channel20Y = int(pairY[1,ind20Y]) |
|
3879 | ||
|
3895 | ||
|
3880 | 3896 |
# pairslist = [(channelCentX, channel25X),(channelCentX, channel20X),(channelCentY,channel25Y),(channelCentY, channel20Y)] |
|
3881 |
pairslist = [(chanCX, chan1X),(chanCX, chan2X),(chanCY,chan1Y),(chanCY, chan2Y)] |
|
|
3882 | ||
|
3897 | pairslist = [(chanCX, chan1X),(chanCX, chan2X),(chanCY,chan1Y),(chanCY, chan2Y)] | |
|
3898 | ||
|
3883 | 3899 |
return pairslist, distances |
|
3884 | 3900 |
# def __getAOA(self, phases, pairsList, error, AOAthresh, azimuth): |
|
3885 | # | |
|
3901 | # | |
|
3886 | 3902 |
# arrayAOA = numpy.zeros((phases.shape[0],3)) |
|
3887 | 3903 |
# cosdir0, cosdir = self.__getDirectionCosines(phases, pairsList) |
|
3888 | # | |
|
3904 | # | |
|
3889 | 3905 |
# arrayAOA[:,:2] = self.__calculateAOA(cosdir, azimuth) |
|
3890 | 3906 |
# cosDirError = numpy.sum(numpy.abs(cosdir0 - cosdir), axis = 1) |
|
3891 | 3907 |
# arrayAOA[:,2] = cosDirError |
|
3892 | # | |
|
3908 | # | |
|
3893 | 3909 |
# azimuthAngle = arrayAOA[:,0] |
|
3894 | 3910 |
# zenithAngle = arrayAOA[:,1] |
|
3895 | # | |
|
3911 | # | |
|
3896 | 3912 |
# #Setting Error |
|
3897 | 3913 |
# #Number 3: AOA not fesible |
|
3898 | 3914 |
# indInvalid = numpy.where(numpy.logical_and((numpy.logical_or(numpy.isnan(zenithAngle), numpy.isnan(azimuthAngle))),error == 0))[0] |
|
3899 |
# error[indInvalid] = 3 |
|
|
3915 | # error[indInvalid] = 3 | |
|
3900 | 3916 |
# #Number 4: Large difference in AOAs obtained from different antenna baselines |
|
3901 | 3917 |
# indInvalid = numpy.where(numpy.logical_and(cosDirError > AOAthresh,error == 0))[0] |
|
3902 |
# error[indInvalid] = 4 |
|
|
3918 | # error[indInvalid] = 4 | |
|
3903 | 3919 |
# return arrayAOA, error |
|
3904 | # | |
|
3920 | # | |
|
3905 | 3921 |
# def __getDirectionCosines(self, arrayPhase, pairsList): |
|
3906 | # | |
|
3922 | # | |
|
3907 | 3923 |
# #Initializing some variables |
|
3908 | 3924 |
# ang_aux = numpy.array([-8,-7,-6,-5,-4,-3,-2,-1,0,1,2,3,4,5,6,7,8])*2*numpy.pi |
|
3909 | 3925 |
# ang_aux = ang_aux.reshape(1,ang_aux.size) |
|
3910 | # | |
|
3926 | # | |
|
3911 | 3927 |
# cosdir = numpy.zeros((arrayPhase.shape[0],2)) |
|
3912 | 3928 |
# cosdir0 = numpy.zeros((arrayPhase.shape[0],2)) |
|
3913 | # | |
|
3914 | # | |
|
3929 | # | |
|
3930 | # | |
|
3915 | 3931 |
# for i in range(2): |
|
3916 | 3932 |
# #First Estimation |
|
3917 | 3933 |
# phi0_aux = arrayPhase[:,pairsList[i][0]] + arrayPhase[:,pairsList[i][1]] |
|
3918 | 3934 |
# #Dealias |
|
3919 | 3935 |
# indcsi = numpy.where(phi0_aux > numpy.pi) |
|
3920 |
# phi0_aux[indcsi] -= 2*numpy.pi |
|
|
3936 | # phi0_aux[indcsi] -= 2*numpy.pi | |
|
3921 | 3937 |
# indcsi = numpy.where(phi0_aux < -numpy.pi) |
|
3922 |
# phi0_aux[indcsi] += 2*numpy.pi |
|
|
3938 | # phi0_aux[indcsi] += 2*numpy.pi | |
|
3923 | 3939 |
# #Direction Cosine 0 |
|
3924 | 3940 |
# cosdir0[:,i] = -(phi0_aux)/(2*numpy.pi*0.5) |
|
3925 | # | |
|
3941 | # | |
|
3926 | 3942 |
# #Most-Accurate Second Estimation |
|
3927 | 3943 |
# phi1_aux = arrayPhase[:,pairsList[i][0]] - arrayPhase[:,pairsList[i][1]] |
|
3928 | 3944 |
# phi1_aux = phi1_aux.reshape(phi1_aux.size,1) |
|
3929 | 3945 |
# #Direction Cosine 1 |
|
3930 | 3946 |
# cosdir1 = -(phi1_aux + ang_aux)/(2*numpy.pi*4.5) |
|
3931 | # | |
|
3947 | # | |
|
3932 | 3948 |
# #Searching the correct Direction Cosine |
|
3933 | 3949 |
# cosdir0_aux = cosdir0[:,i] |
|
3934 | 3950 |
# cosdir0_aux = cosdir0_aux.reshape(cosdir0_aux.size,1) |
@@ -3937,51 +3953,50 class SMOperations(): | |||
|
3937 | 3953 |
# indcos = cosDiff.argmin(axis = 1) |
|
3938 | 3954 |
# #Saving Value obtained |
|
3939 | 3955 |
# cosdir[:,i] = cosdir1[numpy.arange(len(indcos)),indcos] |
|
3940 | # | |
|
3956 | # | |
|
3941 | 3957 |
# return cosdir0, cosdir |
|
3942 | # | |
|
3958 | # | |
|
3943 | 3959 |
# def __calculateAOA(self, cosdir, azimuth): |
|
3944 | 3960 |
# cosdirX = cosdir[:,0] |
|
3945 | 3961 |
# cosdirY = cosdir[:,1] |
|
3946 | # | |
|
3962 | # | |
|
3947 | 3963 |
# zenithAngle = numpy.arccos(numpy.sqrt(1 - cosdirX**2 - cosdirY**2))*180/numpy.pi |
|
3948 | 3964 |
# azimuthAngle = numpy.arctan2(cosdirX,cosdirY)*180/numpy.pi + azimuth #0 deg north, 90 deg east |
|
3949 | 3965 |
# angles = numpy.vstack((azimuthAngle, zenithAngle)).transpose() |
|
3950 | # | |
|
3966 | # | |
|
3951 | 3967 |
# return angles |
|
3952 | # | |
|
3968 | # | |
|
3953 | 3969 |
# def __getHeights(self, Ranges, zenith, error, minHeight, maxHeight): |
|
3954 | # | |
|
3970 | # | |
|
3955 | 3971 |
# Ramb = 375 #Ramb = c/(2*PRF) |
|
3956 | 3972 |
# Re = 6371 #Earth Radius |
|
3957 | 3973 |
# heights = numpy.zeros(Ranges.shape) |
|
3958 | # | |
|
3974 | # | |
|
3959 | 3975 |
# R_aux = numpy.array([0,1,2])*Ramb |
|
3960 | 3976 |
# R_aux = R_aux.reshape(1,R_aux.size) |
|
3961 | # | |
|
3977 | # | |
|
3962 | 3978 |
# Ranges = Ranges.reshape(Ranges.size,1) |
|
3963 | # | |
|
3979 | # | |
|
3964 | 3980 |
# Ri = Ranges + R_aux |
|
3965 | 3981 |
# hi = numpy.sqrt(Re**2 + Ri**2 + (2*Re*numpy.cos(zenith*numpy.pi/180)*Ri.transpose()).transpose()) - Re |
|
3966 | # | |
|
3982 | # | |
|
3967 | 3983 |
# #Check if there is a height between 70 and 110 km |
|
3968 | 3984 |
# h_bool = numpy.sum(numpy.logical_and(hi > minHeight, hi < maxHeight), axis = 1) |
|
3969 | 3985 |
# ind_h = numpy.where(h_bool == 1)[0] |
|
3970 | # | |
|
3986 | # | |
|
3971 | 3987 |
# hCorr = hi[ind_h, :] |
|
3972 | 3988 |
# ind_hCorr = numpy.where(numpy.logical_and(hi > minHeight, hi < maxHeight)) |
|
3973 | # | |
|
3974 |
# hCorr = hi[ind_hCorr] |
|
|
3989 | # | |
|
3990 | # hCorr = hi[ind_hCorr] | |
|
3975 | 3991 |
# heights[ind_h] = hCorr |
|
3976 | # | |
|
3992 | # | |
|
3977 | 3993 |
# #Setting Error |
|
3978 | 3994 |
# #Number 13: Height unresolvable echo: not valid height within 70 to 110 km |
|
3979 |
# #Number 14: Height ambiguous echo: more than one possible height within 70 to 110 km |
|
|
3980 | # | |
|
3981 |
# indInvalid2 = numpy.where(numpy.logical_and(h_bool > 1, error == 0))[0] |
|
|
3995 | # #Number 14: Height ambiguous echo: more than one possible height within 70 to 110 km | |
|
3996 | # | |
|
3997 | # indInvalid2 = numpy.where(numpy.logical_and(h_bool > 1, error == 0))[0] | |
|
3982 | 3998 |
# error[indInvalid2] = 14 |
|
3983 | 3999 |
# indInvalid1 = numpy.where(numpy.logical_and(h_bool == 0, error == 0))[0] |
|
3984 |
# error[indInvalid1] = 13 |
|
|
3985 | # | |
|
3986 |
# return heights, error |
|
|
3987 | No newline at end of file | |
|
4000 | # error[indInvalid1] = 13 | |
|
4001 | # | |
|
4002 | # return heights, error |
@@ -2,7 +2,8 import sys | |||
|
2 | 2 | import numpy,math |
|
3 | 3 | from scipy import interpolate |
|
4 | 4 | from schainpy.model.proc.jroproc_base import ProcessingUnit, Operation, MPDecorator |
|
5 | from schainpy.model.data.jrodata import Voltage | |
|
5 | from schainpy.model.data.jrodata import Voltage,hildebrand_sekhon | |
|
6 | from schainpy.model.data import _noise | |
|
6 | 7 | from schainpy.utils import log |
|
7 | 8 | from time import time |
|
8 | 9 | |
@@ -1338,9 +1339,6 class PulsePairVoltage(Operation): | |||
|
1338 | 1339 | n, |
|
1339 | 1340 | dataOut.nHeights), |
|
1340 | 1341 | dtype='complex') |
|
1341 | #self.noise = numpy.zeros([self.__nch,self.__nHeis]) | |
|
1342 | #for i in range(self.__nch): | |
|
1343 | # self.noise[i]=dataOut.getNoise(channel=i) | |
|
1344 | 1342 | |
|
1345 | 1343 | def putData(self,data): |
|
1346 | 1344 | ''' |
@@ -1355,95 +1353,118 class PulsePairVoltage(Operation): | |||
|
1355 | 1353 | Return the PULSEPAIR and the profiles used in the operation |
|
1356 | 1354 | Affected : self.__profileIndex |
|
1357 | 1355 | ''' |
|
1356 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Remove DCΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1358 | 1357 | if self.removeDC==True: |
|
1359 | 1358 | mean = numpy.mean(self.__buffer,1) |
|
1360 | 1359 | tmp = mean.reshape(self.__nch,1,self.__nHeis) |
|
1361 | 1360 | dc= numpy.tile(tmp,[1,self.__nProf,1]) |
|
1362 | 1361 | self.__buffer = self.__buffer - dc |
|
1362 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Calculo de Potencia Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1363 | pair0 = self.__buffer*numpy.conj(self.__buffer) | |
|
1364 | pair0 = pair0.real | |
|
1365 | lag_0 = numpy.sum(pair0,1) | |
|
1366 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Calculo de Ruido x canalΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1367 | self.noise = numpy.zeros(self.__nch) | |
|
1368 | for i in range(self.__nch): | |
|
1369 | daux = numpy.sort(pair0[i,:,:],axis= None) | |
|
1370 | self.noise[i]=hildebrand_sekhon( daux ,self.nCohInt) | |
|
1371 | ||
|
1372 | self.noise = self.noise.reshape(self.__nch,1) | |
|
1373 | self.noise = numpy.tile(self.noise,[1,self.__nHeis]) | |
|
1374 | noise_buffer = self.noise.reshape(self.__nch,1,self.__nHeis) | |
|
1375 | noise_buffer = numpy.tile(noise_buffer,[1,self.__nProf,1]) | |
|
1376 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Potencia recibida= P , Potencia senal = S , Ruido= NΒ·Β· | |
|
1377 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· P= S+N ,P=lag_0/N Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1378 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Power Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1379 | data_power = lag_0/(self.n*self.nCohInt) | |
|
1380 | #------------------ Senal Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1381 | data_intensity = pair0 - noise_buffer | |
|
1382 | data_intensity = numpy.sum(data_intensity,axis=1)*(self.n*self.nCohInt)#*self.nCohInt) | |
|
1383 | #data_intensity = (lag_0-self.noise*self.n)*(self.n*self.nCohInt) | |
|
1384 | for i in range(self.__nch): | |
|
1385 | for j in range(self.__nHeis): | |
|
1386 | if data_intensity[i][j] < 0: | |
|
1387 | data_intensity[i][j] = numpy.min(numpy.absolute(data_intensity[i][j])) | |
|
1363 | 1388 | |
|
1364 | lag_0 = numpy.sum(self.__buffer*numpy.conj(self.__buffer),1) | |
|
1365 | data_intensity = lag_0/(self.n*self.nCohInt)#*self.nCohInt) | |
|
1366 | ||
|
1389 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Calculo de Frecuencia y Velocidad dopplerΒ·Β·Β·Β·Β·Β·Β·Β· | |
|
1367 | 1390 | pair1 = self.__buffer[:,:-1,:]*numpy.conjugate(self.__buffer[:,1:,:]) |
|
1368 | 1391 | lag_1 = numpy.sum(pair1,1) |
|
1369 | #angle = numpy.angle(numpy.sum(pair1,1))*180/(math.pi) | |
|
1370 | data_velocity = (-1.0*self.lambda_/(4*math.pi*self.ippSec))*numpy.angle(lag_1)#self.ippSec*self.nCohInt | |
|
1392 | data_freq = (-1/(2.0*math.pi*self.ippSec*self.nCohInt))*numpy.angle(lag_1) | |
|
1393 | data_velocity = (self.lambda_/2.0)*data_freq | |
|
1371 | 1394 | |
|
1372 | self.noise = numpy.zeros([self.__nch,self.__nHeis]) | |
|
1373 | for i in range(self.__nch): | |
|
1374 | self.noise[i]=dataOut.getNoise(channel=i) | |
|
1395 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Potencia promedio estimada de la SenalΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1396 | lag_0 = lag_0/self.n | |
|
1397 | S = lag_0-self.noise | |
|
1375 | 1398 | |
|
1376 | lag_0 = lag_0.real/(self.n) | |
|
1399 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Frecuencia Doppler promedio Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1377 | 1400 | lag_1 = lag_1/(self.n-1) |
|
1378 | 1401 | R1 = numpy.abs(lag_1) |
|
1379 | S = (lag_0-self.noise) | |
|
1380 | 1402 | |
|
1403 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Calculo del SNRΒ·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1381 | 1404 | data_snrPP = S/self.noise |
|
1382 | data_snrPP = numpy.where(data_snrPP<0,1,data_snrPP) | |
|
1405 | for i in range(self.__nch): | |
|
1406 | for j in range(self.__nHeis): | |
|
1407 | if data_snrPP[i][j] < 1.e-20: | |
|
1408 | data_snrPP[i][j] = 1.e-20 | |
|
1383 | 1409 | |
|
1410 | #Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· Calculo del ancho espectral Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β·Β· | |
|
1384 | 1411 | L = S/R1 |
|
1385 | 1412 | L = numpy.where(L<0,1,L) |
|
1386 | 1413 | L = numpy.log(L) |
|
1387 | ||
|
1388 | 1414 | tmp = numpy.sqrt(numpy.absolute(L)) |
|
1389 | ||
|
1390 | data_specwidth = (self.lambda_/(2*math.sqrt(2)*math.pi*self.ippSec))*tmp*numpy.sign(L) | |
|
1391 | #data_specwidth = (self.lambda_/(2*math.sqrt(2)*math.pi*self.ippSec))*k | |
|
1415 | data_specwidth = (self.lambda_/(2*math.sqrt(2)*math.pi*self.ippSec*self.nCohInt))*tmp*numpy.sign(L) | |
|
1392 | 1416 | n = self.__profIndex |
|
1393 | 1417 | |
|
1394 | 1418 | self.__buffer = numpy.zeros((self.__nch, self.__nProf,self.__nHeis), dtype='complex') |
|
1395 | 1419 | self.__profIndex = 0 |
|
1396 | return data_intensity,data_velocity,data_snrPP,data_specwidth,n | |
|
1420 | return data_power,data_intensity,data_velocity,data_snrPP,data_specwidth,n | |
|
1397 | 1421 | |
|
1398 | 1422 | def pulsePairbyProfiles(self,dataOut): |
|
1399 | 1423 | |
|
1400 | 1424 | self.__dataReady = False |
|
1425 | data_power = None | |
|
1401 | 1426 | data_intensity = None |
|
1402 | 1427 | data_velocity = None |
|
1403 | 1428 | data_specwidth = None |
|
1404 | 1429 | data_snrPP = None |
|
1405 | 1430 | self.putData(data=dataOut.data) |
|
1406 | 1431 | if self.__profIndex == self.n: |
|
1407 | #self.noise = numpy.zeros([self.__nch,self.__nHeis]) | |
|
1408 | #for i in range(self.__nch): | |
|
1409 | # self.noise[i]=data.getNoise(channel=i) | |
|
1410 | #print(self.noise.shape) | |
|
1411 | data_intensity, data_velocity,data_snrPP,data_specwidth, n = self.pushData(dataOut=dataOut) | |
|
1432 | data_power,data_intensity, data_velocity,data_snrPP,data_specwidth, n = self.pushData(dataOut=dataOut) | |
|
1412 | 1433 | self.__dataReady = True |
|
1413 | 1434 | |
|
1414 | return data_intensity, data_velocity,data_snrPP,data_specwidth | |
|
1435 | return data_power, data_intensity, data_velocity, data_snrPP, data_specwidth | |
|
1415 | 1436 | |
|
1416 | 1437 | def pulsePairOp(self, dataOut, datatime= None): |
|
1417 | 1438 | |
|
1418 | 1439 | if self.__initime == None: |
|
1419 | 1440 | self.__initime = datatime |
|
1420 | #print("hola") | |
|
1421 | data_intensity, data_velocity,data_snrPP,data_specwidth = self.pulsePairbyProfiles(dataOut) | |
|
1441 | data_power, data_intensity, data_velocity, data_snrPP, data_specwidth = self.pulsePairbyProfiles(dataOut) | |
|
1422 | 1442 | self.__lastdatatime = datatime |
|
1423 | 1443 | |
|
1424 |
if data_ |
|
|
1425 | return None, None,None,None,None | |
|
1444 | if data_power is None: | |
|
1445 | return None, None, None,None,None,None | |
|
1426 | 1446 | |
|
1427 | 1447 | avgdatatime = self.__initime |
|
1428 | 1448 | deltatime = datatime - self.__lastdatatime |
|
1429 | 1449 | self.__initime = datatime |
|
1430 | 1450 | |
|
1431 | return data_intensity, data_velocity,data_snrPP,data_specwidth,avgdatatime | |
|
1451 | return data_power, data_intensity, data_velocity, data_snrPP, data_specwidth, avgdatatime | |
|
1432 | 1452 | |
|
1433 | 1453 | def run(self, dataOut,n = None,removeDC= False, overlapping= False,**kwargs): |
|
1434 | 1454 | |
|
1435 | 1455 | if not self.isConfig: |
|
1436 | 1456 | self.setup(dataOut = dataOut, n = n , removeDC=removeDC , **kwargs) |
|
1437 | 1457 | self.isConfig = True |
|
1438 | data_intensity, data_velocity,data_snrPP,data_specwidth, avgdatatime = self.pulsePairOp(dataOut, dataOut.utctime) | |
|
1458 | data_power, data_intensity, data_velocity,data_snrPP,data_specwidth, avgdatatime = self.pulsePairOp(dataOut, dataOut.utctime) | |
|
1439 | 1459 | dataOut.flagNoData = True |
|
1440 | 1460 | |
|
1441 | 1461 | if self.__dataReady: |
|
1442 | 1462 | dataOut.nCohInt *= self.n |
|
1443 |
dataOut.data |
|
|
1444 |
dataOut.data |
|
|
1445 |
dataOut.data |
|
|
1446 |
dataOut.data |
|
|
1463 | dataOut.dataPP_POW = data_intensity # S | |
|
1464 | dataOut.dataPP_POWER = data_power # P | |
|
1465 | dataOut.dataPP_DOP = data_velocity | |
|
1466 | dataOut.dataPP_SNR = data_snrPP | |
|
1467 | dataOut.dataPP_WIDTH = data_specwidth | |
|
1447 | 1468 | dataOut.PRFbyAngle = self.n #numero de PRF*cada angulo rotado que equivale a un tiempo. |
|
1448 | 1469 | dataOut.utctime = avgdatatime |
|
1449 | 1470 | dataOut.flagNoData = False |
@@ -2,8 +2,11 import os,sys | |||
|
2 | 2 | import datetime |
|
3 | 3 | import time |
|
4 | 4 | from schainpy.controller import Project |
|
5 | path = '/home/alex/Downloads/NEW_WR2/spc16removeDC' | |
|
6 | figpath = path | |
|
5 | #path = '/home/alex/Downloads/NEW_WR2/spc16removeDC' | |
|
6 | #figpath = path | |
|
7 | ||
|
8 | path = '/home/alex/Downloads/test_rawdata' | |
|
9 | figpath = '/home/alex/Downloads/hdf5_testPP' | |
|
7 | 10 | desc = "Simulator Test" |
|
8 | 11 | |
|
9 | 12 | controllerObj = Project() |
@@ -25,25 +28,49 readUnitConfObj = controllerObj.addReadUnit(datatype='SimulatorReader', | |||
|
25 | 28 | delay=0, |
|
26 | 29 | online=0, |
|
27 | 30 | walk=0, |
|
28 |
|
|
|
29 | ||
|
30 | opObj11 = readUnitConfObj.addOperation(name='printInfo') | |
|
31 | profilesPerBlock=625, | |
|
32 | dataBlocksPerFile=100)#,#nTotalReadFiles=2) | |
|
31 | 33 | |
|
34 | ''' | |
|
35 | readUnitConfObj = controllerObj.addReadUnit(datatype='VoltageReader', | |
|
36 | path=path, | |
|
37 | startDate="2020/01/01", #"2020/01/01",#today, | |
|
38 | endDate= "2020/12/01", #"2020/12/30",#today, | |
|
39 | startTime='00:00:00', | |
|
40 | endTime='23:59:59', | |
|
41 | delay=0, | |
|
42 | #set=0, | |
|
43 | online=0, | |
|
44 | walk=1) | |
|
45 | ''' | |
|
46 | #opObj11 = readUnitConfObj.addOperation(name='printInfo') | |
|
32 | 47 | procUnitConfObjA = controllerObj.addProcUnit(datatype='VoltageProc', inputId=readUnitConfObj.getId()) |
|
33 | 48 | #opObj11 = procUnitConfObjA.addOperation(name='CohInt', optype='other') |
|
34 |
#opObj11.addParameter(name='n', value=' |
|
|
49 | #opObj11.addParameter(name='n', value='4', format='int') | |
|
35 | 50 | |
|
36 | 51 | #opObj10 = procUnitConfObjA.addOperation(name='selectChannels') |
|
37 | 52 | #opObj10.addParameter(name='channelList', value=[0]) |
|
38 | 53 | opObj11 = procUnitConfObjA.addOperation(name='PulsePairVoltage', optype='other') |
|
39 |
opObj11.addParameter(name='n', value=' |
|
|
54 | opObj11.addParameter(name='n', value='625', format='int')#10 | |
|
40 | 55 | opObj11.addParameter(name='removeDC', value=1, format='int') |
|
41 | 56 | |
|
42 | 57 | #opObj11 = procUnitConfObjA.addOperation(name='PulsepairPowerPlot', optype='other') |
|
58 | #opObj11 = procUnitConfObjA.addOperation(name='PulsepairSignalPlot', optype='other') | |
|
43 | 59 | |
|
44 | opObj11 = procUnitConfObjA.addOperation(name='PulsepairVelocityPlot', optype='other') | |
|
60 | ||
|
61 | #opObj11 = procUnitConfObjA.addOperation(name='PulsepairVelocityPlot', optype='other') | |
|
45 | 62 | #opObj11.addParameter(name='xmax', value=8) |
|
46 | 63 | |
|
47 | opObj11 = procUnitConfObjA.addOperation(name='PulsepairSpecwidthPlot', optype='other') | |
|
64 | #opObj11 = procUnitConfObjA.addOperation(name='PulsepairSpecwidthPlot', optype='other') | |
|
65 | ||
|
66 | procUnitConfObjB= controllerObj.addProcUnit(datatype='ParametersProc',inputId=procUnitConfObjA.getId()) | |
|
67 | ||
|
68 | ||
|
69 | opObj10 = procUnitConfObjB.addOperation(name='ParameterWriter') | |
|
70 | opObj10.addParameter(name='path',value=figpath) | |
|
71 | #opObj10.addParameter(name='mode',value=0) | |
|
72 | opObj10.addParameter(name='blocksPerFile',value='100',format='int') | |
|
73 | opObj10.addParameter(name='metadataList',value='utctimeInit,timeInterval',format='list') | |
|
74 | opObj10.addParameter(name='dataList',value='dataPP_POW,dataPP_DOP,dataPP_SNR,dataPP_WIDTH')#,format='list' | |
|
48 | 75 | |
|
49 | 76 | controllerObj.start() |
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