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1 | 1 | #!/usr/bin/env python No newline at end of file |
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2 | 2 | No newline at end of file |
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3 | 3 | #---------------------------------------------------------- No newline at end of file |
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4 | 4 | # Original MATLAB code developed by Brian Harding |
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5 | No newline at end of file | |
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5 | # Rewritten in python by Yolian Amaro No newline at end of file | |
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6 | 6 | # Python version 2.7 No newline at end of file |
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7 | 7 | # May 15, 2014 No newline at end of file |
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8 | 8 | # Jicamarca Radio Observatory No newline at end of file |
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9 | 9 | #---------------------------------------------------------- No newline at end of file |
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10 | 10 | |
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11 | No newline at end of file | |
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11 | import math | |
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12 | import numpy as np No newline at end of file | |
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13 | 12 | import matplotlib.pyplot as plt |
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13 | No newline at end of file | |
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14 | from scipy import linalg | |
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14 | No newline at end of file | |
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15 | import time No newline at end of file | |
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16 | 15 | from y_hysell96 import* No newline at end of file |
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17 | 16 | from deb4_basis import * No newline at end of file |
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18 | 17 | from modelf import * No newline at end of file |
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18 | from irls_dn2 import * No newline at end of file | |
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19 | 19 | #from scipy.optimize import fsolve |
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20 | No newline at end of file | |
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20 | from scipy.optimize import root | |
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21 | No newline at end of file | |
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21 | import pywt | |
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22 | No newline at end of file | |
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22 | from irls_dn2 import * | |
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23 | No newline at end of file | |
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23 | No newline at end of file | |
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24 | #------------------------------------------------------------------------------------------------- No newline at end of file | |
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24 | 25 | No newline at end of file |
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25 | 26 | ## Calculate Forward Model No newline at end of file |
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26 | 27 | lambda1 = 6.0 |
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28 | No newline at end of file | |
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27 | k = 2*math.pi/lambda1 | |
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29 | No newline at end of file | |
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28 | ||
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30 | No newline at end of file | |
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29 | ## Calculate Magnetic Declination | |
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30 | ||
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31 | # [~,~,dec] = igrf11magm(350e3, -11-56/60, -76-52/60, 2012); check this | |
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32 | ||
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33 | # or calculate it with the above function No newline at end of file | |
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34 | 31 | dec = -1.24 No newline at end of file |
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35 | 32 | |
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33 | No newline at end of file | |
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36 | # loads rx, ry (Jicamarca antenna positions) #this can be done with numpy.loadtxt() No newline at end of file | |
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34 | antpos = np.loadtxt("antpos.txt", comments="#", delimiter=";", unpack=False) | |
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35 | ||
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36 | ## rx and ry -- for plotting purposes No newline at end of file | |
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37 | 37 | rx = np.array( [[127.5000], [91.5000], [127.5000], [19.5000], [91.5000], [-127.5000], [-55.5000], [-220.8240]] ) No newline at end of file |
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38 | 38 | ry = np.array( [[127.5000], [91.5000], [91.5000], [55.5000], [-19.5000], [-127.5000], [-127.5000], [-322.2940]] ) No newline at end of file |
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39 | 39 | |
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40 | No newline at end of file | |
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40 | antpos = np.array( [[127.5000, 91.5000, 127.5000, 19.5000, 91.5000, -127.5000, -55.5000, -220.8240], | |
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41 | [127.5000, 91.5000, 91.5000, 55.5000, -19.5000, -127.5000, -127.5000, -322.2940]] ) | |
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42 | No newline at end of file | |
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43 | 41 | plt.figure(1) No newline at end of file |
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44 | 42 | plt.plot(rx, ry, 'ro') No newline at end of file |
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45 | 43 | plt.draw() No newline at end of file |
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46 | 44 | |
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45 | No newline at end of file | |
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47 | # Jicamarca is nominally at a 45 degree angle No newline at end of file | |
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48 | 46 | theta = 45 - dec; No newline at end of file |
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49 | 47 | No newline at end of file |
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48 | ## Rotation matrix from antenna coord to magnetic coord (East North) | |
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49 | theta_rad = np.radians(theta) # trig functions take radians as argument | |
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50 | val1 = float( np.cos(theta_rad) ) | |
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51 | val2 = float( np.sin(theta_rad) ) | |
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52 | val3 = float( -1*np.sin(theta_rad)) | |
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53 | val4 = float( np.cos(theta_rad) ) | |
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54 | No newline at end of file | |
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50 | 55 | # Rotation matrix from antenna coord to magnetic coord (East North) |
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56 | No newline at end of file | |
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51 | theta_rad = math.radians(theta) # trig functions take radians as argument | |
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52 | val1 = float( math.cos(theta_rad) ) | |
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53 | val2 = float( math.sin(theta_rad) ) | |
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54 | val3 = float( -1*math.sin(theta_rad)) | |
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55 | val4 = float( math.cos(theta_rad) ) | |
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56 | ||
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57 | # Rotation matrix from antenna coord to magnetic coord (East North) | |
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58 | R = np.array( [[val1, val3], [val2, val4]] ); No newline at end of file | |
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59 | 57 | No newline at end of file |
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60 | 58 | # Rotate antenna positions to magnetic coord. |
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59 | No newline at end of file | |
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61 | AR = np.dot(R.T, antpos); No newline at end of file | |
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62 | 60 | No newline at end of file |
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63 | 61 | # Only take the East component No newline at end of file |
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64 | 62 | r = AR[0,:] |
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63 | No newline at end of file | |
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65 | r.sort() # ROW VECTOR? No newline at end of file | |
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66 | 64 | No newline at end of file |
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67 | 65 | # Truth model (high and low resolution) |
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66 | No newline at end of file | |
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68 | Nt = (1024.0)*(16.0); # number of pixels in truth image: high resolution | |
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67 | No newline at end of file | |
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69 | thbound = 9.0/180*math.pi; # the width of the domain in angle space | |
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68 | No newline at end of file | |
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70 | thetat = np.linspace(-thbound, thbound,Nt) # image domain | |
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69 | No newline at end of file | |
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71 | thetat = np.transpose(thetat) # transpose # FUNCIONA?????????????????????????????? | |
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70 | No newline at end of file | |
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72 | Nr = (256.0); # number of pixels in reconstructed image: low res No newline at end of file | |
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73 | 71 | thetar = np.linspace(-thbound, thbound,Nr) # reconstruction domain |
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72 | No newline at end of file | |
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74 | thetar = np.transpose(thetar) #transpose # FUNCIONA????????????????????????????? | |
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73 | No newline at end of file | |
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75 | ||
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74 | No newline at end of file | |
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76 | # Model for f: Gaussian(s) with amplitudes a, centers mu, widths sig, and | |
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75 | No newline at end of file | |
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77 | # background constant b. No newline at end of file | |
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76 | # Model for f: Gaussian(s) with amplitudes a, centers mu, widths sig, and background constant b. | |
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77 | #------------------------------------------------------------------------------------------------- No newline at end of file | |
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78 | 78 | No newline at end of file |
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79 | 79 | # Triple Gaussian No newline at end of file |
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80 | 80 | # a = np.array([3, 5, 2]); |
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81 | No newline at end of file | |
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81 | # mu = np.array([-5.0/180*math.pi, 2.0/180*math.pi, 7.0/180*math.pi]); | |
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82 | No newline at end of file | |
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82 | # sig = np.array([2.0/180*math.pi, 1.5/180*math.pi, 0.3/180*math.pi]); | |
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83 | No newline at end of file | |
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83 | # b = 0; # background No newline at end of file | |
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84 | 84 | No newline at end of file |
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85 | 85 | # Double Gaussian No newline at end of file |
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86 | 86 | # a = np.array([3, 5]); |
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87 | No newline at end of file | |
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87 | # mu = np.array([-5.0/180*math.pi, 2.0/180*math.pi]); | |
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88 | No newline at end of file | |
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88 | # sig = np.array([2.0/180*math.pi, 1.5/180*math.pi]); | |
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89 | No newline at end of file | |
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89 | # b = 0; # background No newline at end of file | |
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90 | 90 | No newline at end of file |
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91 | 91 | # Single Gaussian |
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92 | No newline at end of file | |
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92 | a = np.array( [3] ); | |
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93 | No newline at end of file | |
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93 | mu = np.array( [-3.0/180*math.pi] ) | |
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94 | No newline at end of file | |
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94 | sig = np.array( [2.0/180*math.pi] ) | |
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95 | No newline at end of file | |
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95 | b = 0; | |
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96 | No newline at end of file | |
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96 | ||
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97 | No newline at end of file | |
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97 | fact = np.zeros(shape=(Nt,1)); | |
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98 | No newline at end of file | |
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98 | factr = np.zeros(shape=(Nr,1)); | |
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99 | No newline at end of file | |
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99 | No newline at end of file | |
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100 | ||
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101 | # DFT Kernels No newline at end of file | |
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100 | 102 | for i in range(0, a.size): No newline at end of file |
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101 | 103 | temp = (-(thetat-mu[i])**2/(sig[i]**2)) No newline at end of file |
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102 | 104 | tempr = (-(thetar-mu[i])**2/(sig[i]**2)) No newline at end of file |
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103 | 105 | for j in range(0, temp.size): |
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106 | No newline at end of file | |
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104 | fact[j] = fact[j] + a[i]*math.exp(temp[j]); No newline at end of file | |
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105 | 107 | for m in range(0, tempr.size): |
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108 | No newline at end of file | |
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106 | factr[m] = factr[m] + a[i]*math.exp(tempr[m]); No newline at end of file | |
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109 | No newline at end of file | |
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107 | 110 | fact = fact + b; No newline at end of file |
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108 | 111 | factr = factr + b; No newline at end of file |
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109 | 112 | |
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113 | No newline at end of file | |
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110 | # # model for f: Square pulse No newline at end of file | |
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114 | # # Model for f: Square pulse | |
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115 | # #------------------------------------------------------------------------------------------------- No newline at end of file | |
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111 | 116 | # for j in range(0, fact.size): |
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117 | No newline at end of file | |
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112 | # if (theta > -5.0/180*math.pi and theta < 2.0/180*math.pi): No newline at end of file | |
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113 | 118 | # fact[j] = 0 No newline at end of file |
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114 | 119 | # else: No newline at end of file |
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115 | 120 | # fact[j] = 1 No newline at end of file |
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116 | 121 | # for k in range(0, factr.size): |
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122 | No newline at end of file | |
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117 | # if (thetar[k] > -5.0/180*math.pi and thetar[k] < 2/180*math.pi): | |
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123 | No newline at end of file | |
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118 | # fact[k] = 0 No newline at end of file | |
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119 | 124 | # else: |
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125 | No newline at end of file | |
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120 | # fact[k] = 1 | |
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126 | No newline at end of file | |
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121 | # | |
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127 | No newline at end of file | |
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122 | # | |
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128 | No newline at end of file | |
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123 | # # model for f: triangle pulse | |
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129 | No newline at end of file | |
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124 | # mu = -1.0/180*math.pi; | |
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130 | No newline at end of file | |
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125 | # sig = 5.0/180*math.pi; No newline at end of file | |
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131 | # sig = 5.0/180*np.pi; No newline at end of file | |
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126 | 132 | # wind1 = theta > mu-sig and theta < mu; No newline at end of file |
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127 | 133 | # wind2 = theta < mu+sig and theta > mu; No newline at end of file |
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128 | 134 | # fact = wind1 * (theta - (mu - sig)); No newline at end of file |
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129 | 135 | # factr = wind1 * (thetar - (mu - sig)); No newline at end of file |
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130 | 136 | # fact = fact + wind2 * (-(theta-(mu+sig))); No newline at end of file |
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131 | 137 | # factr = factr + wind2 * (-(thetar-(mu+sig))); No newline at end of file |
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132 | 138 | No newline at end of file |
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133 | 139 | |
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140 | No newline at end of file | |
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134 | # fact = fact/(sum(fact)[0]*2*thbound/Nt); # normalize to integral(f)==1 No newline at end of file | |
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141 | No newline at end of file | |
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135 | 142 | I = sum(fact)[0]; |
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143 | No newline at end of file | |
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136 | fact = fact/I; # normalize to sum(f)==1 | |
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144 | No newline at end of file | |
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137 | factr = factr/I; # normalize to sum(f)==1 | |
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145 | No newline at end of file | |
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138 | #plt.figure() | |
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146 | No newline at end of file | |
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139 | #plt.plot(thetat,fact,'r'); | |
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140 | #plt.plot(thetar,factr,'k.'); | |
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141 | #xlim([min(thetat) max(thetat)]); | |
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142 | ||
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143 | #x = np.linspace(thetat.min(), thetat.max) ???? | |
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144 | #for i in range(0, thetat.size): No newline at end of file | |
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145 | 147 | plt.figure(2) No newline at end of file |
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146 | 148 | plt.plot(thetat, fact, 'r--') No newline at end of file |
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147 | 149 | plt.plot(thetar, factr, 'ro') No newline at end of file |
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148 | 150 | plt.draw() |
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151 | No newline at end of file | |
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149 | # xlim([min(thetat) max(thetat)]); FALTA ARREGLAR ESTO | |
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152 | No newline at end of file | |
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150 | ||
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153 | No newline at end of file | |
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151 | ||
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152 | ## No newline at end of file | |
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153 | 154 | # Control the type and number of inversions with: No newline at end of file |
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154 | 155 | # SNRdBvec: the SNRs that will be used. No newline at end of file |
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155 | 156 | # NN: the number of trials for each SNR No newline at end of file |
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157 | #------------------------------------------------------------------------------------------------- No newline at end of file | |
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156 | 158 | No newline at end of file |
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157 | 159 | #SNRdBvec = np.linspace(5,20,10); |
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160 | No newline at end of file | |
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158 | SNRdBvec = np.array([15]); | |
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161 | No newline at end of file | |
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159 | NN = 1; # number of trial at each SNR | |
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162 | No newline at end of file | |
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160 | ||
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163 | No newline at end of file | |
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161 | # if using vector arguments should be: (4,SNRdBvec.size,NN) | |
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164 | No newline at end of file | |
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162 | corr = np.zeros(shape=(4,SNRdBvec.size,NN)); # (method, SNR, trial) | |
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165 | No newline at end of file | |
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163 | corrc = np.zeros(shape=(4,SNRdBvec.size,NN)); # (method, SNR, trial) | |
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166 | No newline at end of file | |
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164 | rmse = np.zeros(shape=(4,SNRdBvec.size,NN)); # (method, SNR, trial) | |
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167 | No newline at end of file | |
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165 | ||
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168 | No newline at end of file | |
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166 | for snri in range(0, SNRdBvec.size): # change 1 for SNRdBvec.size when using SNRdBvec as vector | |
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169 | No newline at end of file | |
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167 | for Ni in range(0, NN): No newline at end of file | |
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168 | 170 |
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169 | 171 |
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170 | 172 | No newline at end of file |
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173 | for Ni in range(0, NN): No newline at end of file | |
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171 | 174 | # Calculate cross-correlation matrix (Fourier components of image) No newline at end of file |
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172 | 175 | # This is an inefficient way to do this. No newline at end of file |
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173 | 176 | R = np.zeros(shape=(r.size, r.size), dtype=object); No newline at end of file |
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174 | 177 | No newline at end of file |
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175 | 178 | for i1 in range(0, r.size): No newline at end of file |
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176 | 179 |
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177 | 180 | R[i1,i2] = np.dot(fact.T, np.exp(1j*k*np.dot((r[i1]-r[i2]),np.sin(thetat)))) No newline at end of file |
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178 | 181 | R[i1,i2] = sum(R[i1,i2]) No newline at end of file |
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179 | 182 | No newline at end of file |
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180 | 183 | # Add uncertainty No newline at end of file |
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181 | 184 | # This is an ad-hoc way of adding "noise". It models some combination of No newline at end of file |
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182 | 185 | # receiver noise and finite integration times. We could use a more No newline at end of file |
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183 | 186 | # advanced model (like in Yu et al 2000) in the future. No newline at end of file |
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184 | 187 | No newline at end of file |
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185 | 188 | # This is a way of adding noise while maintaining the No newline at end of file |
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186 | 189 | # positive-semi-definiteness of the matrix. No newline at end of file |
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187 | 190 | No newline at end of file |
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188 | 191 | U = linalg.cholesky(R.astype(complex), lower=False); # U'*U = R No newline at end of file |
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189 | 192 | No newline at end of file |
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190 | 193 | sigma_noise = (np.linalg.norm(U,'fro')/SNR); No newline at end of file |
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191 | 194 | |
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195 | No newline at end of file | |
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192 | temp1 = (-1*np.random.rand(U.shape[0], U.shape[1]) + 0.5) | |
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196 | No newline at end of file | |
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193 | temp2 = 1j*(-1*np.random.rand(U.shape[0], U.shape[1]) + 0.5) | |
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197 | No newline at end of file | |
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194 | temp3 = ((abs(U) > 0).astype(float)) # upper triangle of 1's | |
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198 | No newline at end of file | |
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195 | temp4 = (sigma_noise * (temp1 + temp2))/np.sqrt(2.0) | |
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199 | No newline at end of file | |
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196 | ||
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200 | No newline at end of file | |
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197 | nz = np.multiply(temp4, temp3) | |
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201 | No newline at end of file | |
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198 | ||
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202 | No newline at end of file | |
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199 | #---------------------- Eliminar esto:------------------------------------------ | |
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200 | #nz = ((abs(np.multiply(temp4, temp3)) > 0).astype(int)) | |
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201 | #nz = ((abs(np.dot(temp4, temp3)) > 0).astype(int)) | |
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202 | #nz = np.dot(np.dot(sigma_noise, (temp1 + temp2)/math.sqrt(2), temp3 )); | |
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203 | #nz = np.dot(sigma_noise, (np.dot((np.random.rand(8,8) + j*np.random.rand(8,8))/math.sqrt(2.0) , (abs(U) > 0).astype(int)))); | |
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204 | #-------------------------------------------------------------------------------- No newline at end of file | |
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205 | 203 | No newline at end of file |
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206 | 204 |
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207 | 205 | Rnz = np.dot(Unz.T.conj(),Unz); # the noisy version of R No newline at end of file |
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208 | 206 | plt.figure(3); No newline at end of file |
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209 | 207 |
plt. |
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210 | 208 |
plt.color |
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211 | 209 | |
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210 | No newline at end of file | |
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212 | # Fourier Inversion ################### No newline at end of file | |
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211 | #------------------------------------------------------------------------------------------------- | |
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212 | # Fourier Inversion No newline at end of file | |
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213 | 213 | f_fourier = np.zeros(shape=(Nr,1), dtype=complex); No newline at end of file |
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214 | 214 | No newline at end of file |
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215 | 215 | for i in range(0, thetar.size): No newline at end of file |
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216 | 216 | th = thetar[i]; No newline at end of file |
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217 | 217 | w = np.exp(1j*k*np.dot(r,np.sin(th))); No newline at end of file |
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218 | 218 | No newline at end of file |
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219 | 219 | temp = np.dot(w.T.conj(),U) No newline at end of file |
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220 | 220 | No newline at end of file |
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221 | 221 | f_fourier[i] = np.dot(temp, w); No newline at end of file |
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222 | 222 | |
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223 | No newline at end of file | |
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223 | f_fourier = f_fourier.real; # get rid of numerical imaginary noise | |
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224 | No newline at end of file | |
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224 | ||
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225 | No newline at end of file | |
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225 | #print f_fourier | |
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226 | No newline at end of file | |
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226 | ||
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227 | No newline at end of file | |
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227 | ||
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228 | No newline at end of file | |
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228 | # Capon Inversion ###################### | |
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229 | No newline at end of file | |
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230 | 229 | f_capon = np.zeros(shape=(Nr,1)); No newline at end of file |
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231 | 230 | No newline at end of file |
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232 | 231 | tic_capon = time.time(); No newline at end of file |
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233 | 232 | No newline at end of file |
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234 | 233 | for i in range(0, thetar.size): No newline at end of file |
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235 | 234 | th = thetar[i]; No newline at end of file |
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236 | 235 | w = np.exp(1j*k*np.dot(r,np.sin(th))); No newline at end of file |
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237 | 236 | f_capon[i] = np.divide(1, ( np.dot( w.T.conj(), (linalg.solve(Rnz,w)) ) ).real) No newline at end of file |
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238 | 237 | No newline at end of file |
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239 | 238 | No newline at end of file |
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240 | 239 | toc_capon = time.time() No newline at end of file |
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241 | 240 | No newline at end of file |
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242 | 241 | elapsed_time_capon = toc_capon - tic_capon; No newline at end of file |
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243 | 242 | |
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243 | No newline at end of file | |
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244 | f_capon = f_capon.real; # get rid of numerical imaginary noise | |
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244 | No newline at end of file | |
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245 | ||
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245 | No newline at end of file | |
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246 | # MaxEnt Inversion ##################### | |
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246 | No newline at end of file | |
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247 | ||
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247 | No newline at end of file | |
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248 | # create the appropriate sensing matrix (split into real and imaginary # parts) No newline at end of file | |
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248 | # Create the appropriate sensing matrix (split into real and imaginary # parts) | |
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249 | M = (r.size-1)*(r.size); | |
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250 | Ht = np.zeros(shape=(M,Nt)); # "true" sensing matrix No newline at end of file | |
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249 | 251 | M = (r.size-1)*(r.size); |
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252 | No newline at end of file | |
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250 | Ht = np.zeros(shape=(M,Nt)); # "true" sensing matrix | |
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253 | No newline at end of file | |
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251 | Hr = np.zeros(shape=(M,Nr)); # approximate sensing matrix for reconstruction | |
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254 | No newline at end of file | |
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252 | ||
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255 | No newline at end of file | |
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253 | # need to re-index our measurements from matrix R into vector g No newline at end of file | |
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254 | 256 | g = np.zeros(shape=(M,1)); |
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257 | No newline at end of file | |
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255 | gnz = np.zeros(shape=(M,1)); # noisy version of g | |
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258 | No newline at end of file | |
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256 | ||
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259 | No newline at end of file | |
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257 | # triangular indexing to perform this re-indexing No newline at end of file | |
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258 | 260 | T = np.ones(shape=(r.size,r.size)); No newline at end of file |
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259 | 261 | [i1v,i2v] = np.where(np.triu(T,1) > 0); # converts linear to triangular indexing No newline at end of file |
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260 | 262 | |
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263 | No newline at end of file | |
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261 | # build H No newline at end of file | |
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262 | 264 | for i1 in range(0, r.size): No newline at end of file |
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263 | 265 | for i2 in range(i1+1, r.size): |
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266 | No newline at end of file | |
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264 | idx = np.where(np.logical_and((i1==i1v), (i2==i2v)))[0]; # kind of awkward | |
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267 | No newline at end of file | |
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265 | idx1 = 2*idx; # because index starts at 0 No newline at end of file | |
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266 | 268 | idx2 = 2*idx+1; |
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269 | No newline at end of file | |
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267 | Hr[idx1,:] = np.cos(k*(r[i1]-r[i2])*np.sin(thetar)).T; | |
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270 | No newline at end of file | |
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268 | Hr[idx2,:] = np.sin(k*(r[i1]-r[i2])*np.sin(thetar)).T; | |
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271 | No newline at end of file | |
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269 | Ht[idx1,:] = np.cos(k*(r[i1]-r[i2])*np.sin(thetat)).T*Nr/Nt; | |
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272 | No newline at end of file | |
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270 | Ht[idx2,:] = np.sin(k*(r[i1]-r[i2])*np.sin(thetat)).T*Nr/Nt; | |
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273 | No newline at end of file | |
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271 | g[idx1] = (R[i1,i2]).real*Nr/Nt; # check this again later | |
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274 | No newline at end of file | |
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272 | g[idx2] = (R[i1,i2]).imag*Nr/Nt; # check again No newline at end of file | |
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273 | 275 | gnz[idx1] = (Rnz[i1,i2]).real*Nr/Nt; No newline at end of file |
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274 | 276 | gnz[idx2] = (Rnz[i1,i2]).imag*Nr/Nt; No newline at end of file |
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275 | 277 | |
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278 | No newline at end of file | |
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276 | # inversion | |
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279 | No newline at end of file | |
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277 | F = Nr/Nt; # normalization | |
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280 | No newline at end of file | |
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278 | sigma = 1; # set to 1 because the difference is accounted for in G | |
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281 | No newline at end of file | |
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279 | ||
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282 | No newline at end of file | |
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280 | ##### ADD *10 for consistency with old model, NEED TO VERIFY THIS!!!!? line below | |
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283 | No newline at end of file | |
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281 | G = np.linalg.norm(g-gnz)**2 ; # pretend we know in advance the actual value of chi^2 | |
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284 | No newline at end of file | |
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282 | ||
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283 | tic_maxent = time.time(); | |
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284 | ||
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285 | lambda0 = 1e-5*np.ones(shape=(M,1)); # initial condition (can be set to anything) | |
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286 | ||
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287 | toc_maxent = time.time() | |
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288 | elapsed_time_maxent = toc_maxent - tic_maxent; No newline at end of file | |
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289 | 285 | No newline at end of file |
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290 | 286 | # Whitened solution No newline at end of file |
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291 | 287 | def myfun(lambda1): No newline at end of file |
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292 | 288 | return y_hysell96(lambda1,gnz,sigma,F,G,Hr); No newline at end of file |
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293 | 289 | |
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290 | No newline at end of file | |
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294 | tic_maxEnt = time.time(); | |
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291 | No newline at end of file | |
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295 | ||
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292 | No newline at end of file | |
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296 | #sol1 = fsolve(myfun,lambda0.ravel(), args=(), xtol=1e-14, maxfev=100000); No newline at end of file | |
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297 | 293 | lambda1 = root(myfun,lambda0, method='krylov', tol=1e-14); No newline at end of file |
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298 | 294 | |
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295 | No newline at end of file | |
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299 | #print lambda1 | |
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296 | No newline at end of file | |
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300 | #print lambda1.x | |
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297 | No newline at end of file | |
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301 | No newline at end of file | |
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298 | No newline at end of file | |
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302 | 299 | lambda1 = lambda1.x; No newline at end of file |
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303 | 300 | |
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304 | toc_maxEnt = time.time(); No newline at end of file | |
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305 | 301 | f_maxent = modelf(lambda1, Hr, F); No newline at end of file |
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306 | 302 | ystar = myfun(lambda1); |
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303 | No newline at end of file | |
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307 | Lambda = np.sqrt(sum(lambda1**2.*sigma**2)/(4*G)); No newline at end of file | |
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308 | 304 | ep = np.multiply(-lambda1,sigma**2)/ (2*Lambda); No newline at end of file |
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309 | 305 | es = np.dot(Hr, f_maxent) - gnz; # should be same as ep No newline at end of file |
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310 | 306 | chi2 = np.sum((es/sigma)**2); No newline at end of file |
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311 | 307 | No newline at end of file |
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312 | 308 | |
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309 | No newline at end of file | |
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313 | # --------- CS inversion using Iteratively Reweighted Least Squares (IRLS) ------------- | |
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310 | No newline at end of file | |
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314 | No newline at end of file | |
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311 | No newline at end of file | |
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315 | 312 | # (Use Nr, thetar, gnz, and Hr from MaxEnt above) No newline at end of file |
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316 | 313 | No newline at end of file |
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317 | 314 | Psi = deb4_basis(Nr); No newline at end of file |
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318 | 315 | |
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316 | No newline at end of file | |
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319 | # REMOVE THIS-------------------------------- | |
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317 | No newline at end of file | |
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320 | #wavelet1 = pywt.Wavelet('db4') | |
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318 | No newline at end of file | |
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321 | #Phi, Psi, x = wavelet1.wavefun(level=3) | |
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319 | No newline at end of file | |
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322 | # -------------------------------------------- No newline at end of file | |
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323 | 320 | No newline at end of file |
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324 | 321 | # add "sum to 1" constraint No newline at end of file |
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325 | 322 | H2 = np.concatenate( (Hr, np.ones(shape=(1,Nr))), axis=0 ); |
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323 | No newline at end of file | |
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326 | N_temp = np.array([[Nr/Nt]]); | |
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324 | No newline at end of file | |
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327 | g2 = np.concatenate( (gnz, N_temp), axis=0 ); | |
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325 | No newline at end of file | |
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328 | ||
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326 | No newline at end of file | |
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329 | #H2 = H2.T.conj(); | |
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327 | No newline at end of file | |
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330 | ||
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328 | No newline at end of file | |
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331 | #Psi = Psi.T.conj(); # to align matrices | |
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329 | No newline at end of file | |
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332 | ||
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330 | No newline at end of file | |
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333 | ####print 'H2 shape', H2.shape | |
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331 | No newline at end of file | |
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334 | #####print 'Psi shape', Psi.shape | |
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332 | No newline at end of file | |
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335 | ||
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333 | No newline at end of file | |
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336 | A = np.dot(H2,Psi); | |
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337 | No newline at end of file | |
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338 | 334 | s = irls_dn2(np.dot(H2,Psi),g2,0.5,G); |
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335 | No newline at end of file | |
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339 | # f_cs = Psi*s; | |
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336 | No newline at end of file | |
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340 | # | |
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337 | No newline at end of file | |
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341 | # # plot | |
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338 | No newline at end of file | |
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342 | # plot(thetar,f_cs,'r.-'); | |
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339 | No newline at end of file | |
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343 | # hold on; | |
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340 | No newline at end of file | |
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344 | # plot(thetat,fact,'k-'); | |
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341 | No newline at end of file | |
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345 | # hold off; | |
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342 | No newline at end of file | |
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346 | ||
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343 | No newline at end of file | |
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347 | ||
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344 | No newline at end of file | |
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348 | # # # Scaling and shifting | |
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345 | No newline at end of file | |
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349 | # # # Only necessary for capon solution No newline at end of file | |
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346 | ||
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347 | ||
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348 | #------------------------------------------------------------------------------------------------- | |
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349 | # Scaling and shifting | |
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350 | # (Only necessary for Capon solution) | |
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351 | #------------------------------------------------------------------------------------------------- | |
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352 | f_capon = f_capon/np.max(f_capon)*np.max(fact); | |
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353 | No newline at end of file | |
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350 | 354 | f_capon = f_capon/np.max(f_capon)*np.max(fact); No newline at end of file |
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351 | 355 | No newline at end of file |
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352 | 356 | |
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357 | No newline at end of file | |
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353 | ### analyze stuff ###################### | |
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358 | No newline at end of file | |
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354 | # calculate MSE No newline at end of file | |
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359 | # Calculate MSE | |
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360 | rmse_fourier = np.sqrt(np.mean((f_fourier - factr)**2)); | |
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361 | rmse_capon = np.sqrt(np.mean((f_capon - factr)**2)); No newline at end of file | |
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355 | 362 |
rmse_ |
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356 | 363 |
rmse_c |
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357 | 364 | rmse_maxent = np.sqrt(np.mean((f_maxent - factr)**2)); |
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365 | No newline at end of file | |
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358 | #rmse_cs = np.sqrt(np.mean((f_cs - factr).^2)); No newline at end of file | |
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359 | 366 | No newline at end of file |
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360 | 367 | No newline at end of file |
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361 | 368 |
relrmse_ |
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362 | 369 |
relrmse_c |
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363 | 370 | relrmse_maxent = rmse_maxent / np.linalg.norm(fact); |
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371 | No newline at end of file | |
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364 | #relrmse_cs = rmse_cs / np.norm(fact); | |
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372 | No newline at end of file | |
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365 | ||
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373 | No newline at end of file | |
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366 | # To be able to perform dot product (align matrices) done below within the dot calculations | |
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374 | No newline at end of file | |
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367 | ||
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368 | ||
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369 | #f_fourier = f_fourier.T.conj() | |
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370 | #f_capon = f_capon.T.conj() | |
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371 | #f_maxent = f_maxent.T.conj() | |
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372 | ||
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373 | #factr = factr.T.conj() | |
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374 | ||
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375 | # calculate correlation | |
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376 | No newline at end of file | |
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377 | 375 |
corr_ |
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378 | 376 |
corr_c |
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379 | 377 | corr_maxent = np.dot(f_maxent.T.conj(),factr) / (np.linalg.norm(f_maxent)*np.linalg.norm(factr)); |
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378 | No newline at end of file | |
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380 | #corr_cs = np.dot(f_cs,factr) / (norm(f_cs)*norm(factr)); | |
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379 | No newline at end of file | |
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381 | ||
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380 | No newline at end of file | |
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382 | ||
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381 | No newline at end of file | |
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383 | # calculate centered correlation No newline at end of file | |
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384 | 382 | f0 = factr - np.mean(factr); No newline at end of file |
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385 | 383 | f1 = f_fourier - np.mean(f_fourier); No newline at end of file |
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386 | 384 | No newline at end of file |
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387 | 385 |
corrc_ |
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388 | 386 |
f1 = f_ |
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389 | 387 |
corrc_ |
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390 | 388 |
f1 = f_ |
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391 | 389 |
corrc_ |
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390 | No newline at end of file | |
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392 | #f1 = f_cs - mean(f_cs); | |
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391 | No newline at end of file | |
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393 | #corrc_cs = dot(f0,f1) / (norm(f0)*norm(f1)); | |
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392 | No newline at end of file | |
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394 | ||
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393 | No newline at end of file | |
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395 | ||
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394 | No newline at end of file | |
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396 | ||
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395 | No newline at end of file | |
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397 | # # # plot stuff ######################### No newline at end of file | |
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396 | #---- Capon---- No newline at end of file | |
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398 | 397 | No newline at end of file |
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399 | 398 | #---- Capon---- |
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399 | No newline at end of file | |
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400 | plt.figure(4) | |
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400 | No newline at end of file | |
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401 | plt.subplot(2, 1, 1) | |
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401 | No newline at end of file | |
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402 | plt.plot(180/math.pi*thetar, f_capon, 'r', label='Capon') | |
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402 | No newline at end of file | |
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403 | plt.plot(180/math.pi*thetat,fact, 'k--', label='Truth') No newline at end of file | |
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404 | 403 | plt.ylabel('Power (arbitrary units)') No newline at end of file |
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405 | 404 | plt.legend(loc='upper right') No newline at end of file |
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406 | 405 | No newline at end of file |
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407 | 406 | # formatting y-axis No newline at end of file |
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408 | 407 | locs,labels = plt.yticks() No newline at end of file |
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409 | 408 | plt.yticks(locs, map(lambda x: "%.1f" % x, locs*1e4)) No newline at end of file |
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410 | 409 | plt.text(0.0, 1.01, '1e-4', fontsize=10, transform = plt.gca().transAxes) No newline at end of file |
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411 | 410 | No newline at end of file |
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412 | 411 | No newline at end of file |
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413 | 412 | #---- MaxEnt---- |
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413 | No newline at end of file | |
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414 | plt.subplot(2, 1, 2) | |
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414 | No newline at end of file | |
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415 | plt.plot(180/math.pi*thetar, f_maxent, 'r', label='MaxEnt') | |
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415 | No newline at end of file | |
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416 | plt.plot(180/math.pi*thetat,fact, 'k--', label='Truth') No newline at end of file | |
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417 | 416 | plt.ylabel('Power (arbitrary units)') No newline at end of file |
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418 | 417 | plt.legend(loc='upper right') No newline at end of file |
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419 | 418 | No newline at end of file |
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420 | 419 | # formatting y-axis No newline at end of file |
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421 | 420 | locs,labels = plt.yticks() No newline at end of file |
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422 | 421 | plt.yticks(locs, map(lambda x: "%.1f" % x, locs*1e4)) No newline at end of file |
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423 | 422 | plt.text(0.0, 1.01, '1e-4', fontsize=10, transform = plt.gca().transAxes) No newline at end of file |
|
424 | 423 | |
|
424 | No newline at end of file | |
|
425 | plt.show() No newline at end of file | |
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No newline at end of file | ||
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425 | plt.plot(180/np.pi*thetar, f_cs, 'r', label='CS') | |
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No newline at end of file | ||
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426 | plt.plot(180/np.pi*thetat,fact, 'k--', label='Truth') | |
|
No newline at end of file | ||
|
427 | plt.ylabel('Power (arbitrary units)') | |
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No newline at end of file | ||
|
428 | plt.legend(loc='upper right') | |
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No newline at end of file | ||
|
429 | ||
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No newline at end of file | ||
|
430 | # formatting y-axis | |
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No newline at end of file | ||
|
431 | locs,labels = plt.yticks() | |
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No newline at end of file | ||
|
432 | plt.yticks(locs, map(lambda x: "%.1f" % x, locs*1e4)) | |
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No newline at end of file | ||
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433 | plt.text(0.0, 1.01, '1e-4', fontsize=10, transform = plt.gca().transAxes) | |
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No newline at end of file | ||
|
434 | ||
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No newline at end of file | ||
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435 | No newline at end of file | |
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426 | 436 | No newline at end of file |
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427 | 437 | No newline at end of file |
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428 | 438 | # # PLOT PARA COMPRESSED SENSING No newline at end of file |
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429 | 439 | # # No newline at end of file |
|
430 | 440 |
# # |
|
431 | 441 |
# # plot(180/pi*theta |
|
432 | 442 |
# # hold o |
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433 | 443 |
# # |
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434 | 444 | # # hold off; No newline at end of file |
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435 | 445 | # # ylim([min(f_cs) 1.1*max(fact)]); No newline at end of file |
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436 | 446 | # # # title(sprintf('rel. RMSE: #.2e\tCorr: #.3f Corrc: #.3f', relrmse_cs, corr_cs, corrc_cs)); No newline at end of file |
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437 | 447 | # # # title 'Compressed Sensing - Debauchies Wavelets' No newline at end of file |
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438 | 448 | # # xlabel 'Degrees' No newline at end of file |
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439 | 449 | # # ylabel({'Power';'(arbitrary units)'}) No newline at end of file |
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440 | 450 | # # legend('Comp. Sens.','Truth'); No newline at end of file |
|
441 | 451 | # # No newline at end of file |
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442 | 452 | # # # set(gcf,'Position',[749 143 528 881]); # CSL No newline at end of file |
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443 | 453 | # # # set(gcf,'Position',[885 -21 528 673]); # macbook No newline at end of file |
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444 | 454 | # # pause(0.01); No newline at end of file |
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445 | 455 | No newline at end of file |
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446 | 456 | No newline at end of file |
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447 | 457 | # # Store Results No newline at end of file |
|
448 | 458 |
corr[ |
|
449 | 459 |
corr[ |
|
450 | 460 | corr[2, snri, Ni] = corr_maxent; |
|
461 | No newline at end of file | |
|
451 | #corr[3, snri, Ni] = corr_cs; No newline at end of file | |
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452 | 462 | No newline at end of file |
|
453 | 463 |
rmse[ |
|
454 | 464 |
rmse[ |
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455 | 465 | rmse[2,snri,Ni] = relrmse_maxent; |
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466 | No newline at end of file | |
|
456 | #rmse[3,snri,Ni] = relrmse_cs; No newline at end of file | |
|
457 | 467 | No newline at end of file |
|
458 | 468 |
corrc[ |
|
459 | 469 |
corrc[ |
|
460 | 470 | corrc[2,snri,Ni] = corrc_maxent; |
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471 | No newline at end of file | |
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461 | #corrc[3,snri,Ni] = corrc_cs; No newline at end of file | |
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462 | 472 | No newline at end of file |
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463 | 473 | No newline at end of file |
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464 | 474 |
print 'C |
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465 | 475 | print 'Maxent:\t',elapsed_time_maxent, 'sec'; |
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476 | No newline at end of file | |
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466 | #print 'CS:\t%3.3f sec\n',elapsed_time_cs; No newline at end of file | |
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467 | 477 | No newline at end of file |
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468 | 478 | print (NN*(snri+1) + Ni), '/', (SNRdBvec.size*NN); No newline at end of file |
|
469 | 479 | No newline at end of file |
|
470 | 480 | print corr No newline at end of file |
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471 | 481 | No newline at end of file |
|
482 | ||
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No newline at end of file | ||
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483 | ## Analyze and plot statistics | |
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No newline at end of file | ||
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484 | ||
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No newline at end of file | ||
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485 | metric = corr; # set this to rmse, corr, or corrc | |
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No newline at end of file | ||
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486 | ||
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No newline at end of file | ||
|
487 | # Remove outliers (this part was experimental and wasn't used in the paper) | |
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No newline at end of file | ||
|
488 | # nsig = 3; | |
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No newline at end of file | ||
|
489 | # for i = 1:4 | |
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|
490 | # for snri = 1:length(SNRdBvec) | |
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No newline at end of file | ||
|
491 | # av = mean(met(i,snri,:)); | |
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No newline at end of file | ||
|
492 | # s = std(met(i,snri,:)); | |
|
No newline at end of file | ||
|
493 | # idx = abs(met(i,snri,:) - av) > nsig*s; | |
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No newline at end of file | ||
|
494 | # met(i,snri,idx) = nan; | |
|
No newline at end of file | ||
|
495 | # if sum(idx)>0 | |
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No newline at end of file | ||
|
496 | # fprintf('i=%i, snr=%i, %i/%i pts removed\n',... | |
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No newline at end of file | ||
|
497 | # i,round(SNRdBvec(snri)),sum(idx),length(idx)); | |
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|
498 | # end | |
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No newline at end of file | ||
|
499 | # end | |
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No newline at end of file | ||
|
500 | # end | |
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|
501 | ||
|
No newline at end of file | ||
|
502 | # Avg ignoring NaNs | |
|
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|
503 | def nanmean(data, **args): | |
|
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|
504 | return numpy.ma.filled(numpy.ma.masked_array(data,numpy.isnan(data)).mean(**args), fill_value=numpy.nan) | |
|
No newline at end of file | ||
|
505 | ||
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No newline at end of file | ||
|
506 | # ave = np.zeros(shape=(4)) | |
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|
507 | # | |
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No newline at end of file | ||
|
508 | # ave[0] = nanmean(metric, axis=0); | |
|
No newline at end of file | ||
|
509 | # ave[1] = nanmean(metric, axis=1); | |
|
No newline at end of file | ||
|
510 | # ave[2] = nanmean(metric, axis=2); | |
|
No newline at end of file | ||
|
511 | # ave[3] = nanmean(metric, axis=3); | |
|
No newline at end of file | ||
|
512 | ||
|
No newline at end of file | ||
|
513 | #print ave | |
|
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|
514 | plt.figure(6); | |
|
No newline at end of file | ||
|
515 | f = plt.scatter(SNRdBvec, corr[0], marker='+', color='b', s=60); # Fourier | |
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No newline at end of file | ||
|
516 | c = plt.scatter(SNRdBvec, corr[1], marker='o', color= 'c', s=60); # Capon | |
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No newline at end of file | ||
|
517 | me= plt.scatter(SNRdBvec, corr[2], marker='s', color= 'y', s=60); # MaxEnt | |
|
No newline at end of file | ||
|
518 | cs= plt.scatter(SNRdBvec, corr[3], marker='*', color='r', s=60); # Compressed Sensing | |
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No newline at end of file | ||
|
519 | ||
|
No newline at end of file | ||
|
520 | ||
|
No newline at end of file | ||
|
521 | plt.legend((f,c,me,cs),('Fourier','Capon', 'MaxEnt', 'Comp. Sens.'),scatterpoints=1, loc='upper right') | |
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No newline at end of file | ||
|
522 | plt.xlabel('SNR') | |
|
No newline at end of file | ||
|
523 | plt.ylabel('Correlation with Truth') | |
|
No newline at end of file | ||
|
524 | ||
|
No newline at end of file | ||
|
525 | plt.show() | |
|
No newline at end of file | ||
|
526 | No newline at end of file |
@@ -1,72 +1,76 | |||
|
1 | 1 | ''' No newline at end of file |
|
2 | 2 | Created on May 29, 2014 No newline at end of file |
|
3 | 3 | No newline at end of file |
|
4 | 4 | @author: Yolian Amaro No newline at end of file |
|
5 | 5 | ''' No newline at end of file |
|
6 | 6 | No newline at end of file |
|
7 | 7 | #from sp import multirate No newline at end of file |
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8 | 8 | from cshift import * No newline at end of file |
|
9 | 9 | from multirate import upfirdn No newline at end of file |
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10 | 10 | No newline at end of file |
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11 | 11 | def afb(x, af): No newline at end of file |
|
12 | 12 | No newline at end of file |
|
13 | 13 | # Analysis filter bank No newline at end of file |
|
14 | 14 | # No newline at end of file |
|
15 | 15 | # USAGE: No newline at end of file |
|
16 | 16 | # [lo, hi] = afb(x, af) No newline at end of file |
|
17 | 17 | # INPUT: No newline at end of file |
|
18 | 18 | # x - N-point vector, where No newline at end of file |
|
19 | 19 | # 1) N is even No newline at end of file |
|
20 | 20 | # 2) N >= length(af) No newline at end of file |
|
21 | 21 | # af - analysis filters No newline at end of file |
|
22 | 22 | # af(:, 1) - lowpass filter (even length) No newline at end of file |
|
23 | 23 | # af(:, 2) - highpass filter (even length) No newline at end of file |
|
24 | 24 | # OUTPUT: No newline at end of file |
|
25 | 25 | # lo - Low frequecy output No newline at end of file |
|
26 | 26 | # hi - High frequency output No newline at end of file |
|
27 | 27 | # EXAMPLE: No newline at end of file |
|
28 | 28 | # [af, sf] = farras; No newline at end of file |
|
29 | 29 | # x = rand(1,64); No newline at end of file |
|
30 | 30 | # [lo, hi] = afb(x, af); No newline at end of file |
|
31 | 31 | # y = sfb(lo, hi, sf); No newline at end of file |
|
32 | 32 | # err = x - y; No newline at end of file |
|
33 | 33 | # max(abs(err)) No newline at end of file |
|
34 | 34 | # No newline at end of file |
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35 | 35 | # WAVELET SOFTWARE AT POLYTECHNIC UNIVERSITY, BROOKLYN, NY No newline at end of file |
|
36 | 36 | # http://taco.poly.edu/WaveletSoftware/ No newline at end of file |
|
37 | 37 | No newline at end of file |
|
38 | 38 | N = x.size; No newline at end of file |
|
39 | 39 | L = (af).size/4; #L should be = 5 No newline at end of file |
|
40 | 40 | #print af No newline at end of file |
|
41 | 41 | #print 'L', L No newline at end of file |
|
42 | 42 | x = cshift(x,-(L-1)); No newline at end of file |
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43 | 43 | No newline at end of file |
|
44 | 44 | # print 'afb x', x.shape No newline at end of file |
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45 | 45 | # print 'af[:,0]',af[:,0].shape No newline at end of file |
|
46 | 46 | # print 'af[:,1]',af[:,1].shape No newline at end of file |
|
47 | 47 | # print '-----------------------' No newline at end of file |
|
48 | 48 | No newline at end of file |
|
49 | 49 | # lowpass filter No newline at end of file |
|
50 | 50 | lo = upfirdn(x, af[:,0], 1, 2); No newline at end of file |
|
51 | 51 | No newline at end of file |
|
52 | 52 | |
|
53 | No newline at end of file | |
|
53 | # VERIFY THIS!!!!!!!!!!!! | |
|
No newline at end of file | ||
|
54 | No newline at end of file | |
|
54 | for i in range(0, L): | |
|
No newline at end of file | ||
|
55 | No newline at end of file | |
|
55 | lo[i] = lo[N/2+i] + lo[i]; No newline at end of file | |
|
No newline at end of file | ||
|
56 | ||
|
No newline at end of file | ||
|
57 | lo[0:L-1] = lo[N/2+np.arange(0,L-1)] + lo[0:L-1] No newline at end of file | |
|
56 | 58 | No newline at end of file |
|
57 | 59 | lo = lo[0:N/2]; No newline at end of file |
|
58 | 60 | No newline at end of file |
|
59 | 61 | No newline at end of file |
|
60 | 62 | # highpass filter No newline at end of file |
|
61 | 63 | hi = upfirdn(x, af[:,1], 1, 2); No newline at end of file |
|
62 | 64 | |
|
65 | No newline at end of file | |
|
63 | for j in range(0, L): | |
|
No newline at end of file | ||
|
66 | No newline at end of file | |
|
64 | hi[j] = hi[N/2+j] + hi[j]; No newline at end of file | |
|
No newline at end of file | ||
|
67 | ||
|
No newline at end of file | ||
|
68 | hi[0:L-1] = hi[N/2+np.arange(0,L-1)] + hi[0:L-1] No newline at end of file | |
|
65 | 69 | No newline at end of file |
|
66 | 70 | hi = hi[0:N/2]; No newline at end of file |
|
67 | 71 | No newline at end of file |
|
68 | 72 | # Reshape from 1D to 2D No newline at end of file |
|
69 | 73 | lo = lo.reshape(1, lo.size) No newline at end of file |
|
70 | 74 | hi = hi.reshape(1, hi.size) No newline at end of file |
|
71 | 75 | No newline at end of file |
|
72 | 76 | return lo, hi No newline at end of file |
@@ -1,39 +1,41 | |||
|
1 | 1 | ''' No newline at end of file |
|
2 | 2 | Created on May 26, 2014 No newline at end of file |
|
3 | 3 | No newline at end of file |
|
4 | 4 | @author: Yolian Amaro No newline at end of file |
|
5 | 5 | ''' No newline at end of file |
|
6 | 6 | No newline at end of file |
|
7 | 7 | import numpy as np No newline at end of file |
|
8 | 8 | from FSfarras import * No newline at end of file |
|
9 | 9 | from dualfilt1 import * No newline at end of file |
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10 | 10 | from dualtree import * No newline at end of file |
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11 | 11 | from idualtree import * No newline at end of file |
|
12 | 12 | No newline at end of file |
|
13 | # Debauchie 4 Wavelet No newline at end of file | |
|
13 | 14 | def deb4_basis(N): No newline at end of file |
|
14 | 15 | No newline at end of file |
|
15 | 16 | Psi = np.zeros(shape=(N,2*N+1)); No newline at end of file |
|
16 | 17 | idx = 0; No newline at end of file |
|
17 | 18 | J = 4; No newline at end of file |
|
18 | 19 | [Faf, Fsf] = FSfarras(); No newline at end of file |
|
19 | 20 | [af, sf] = dualfilt1(); No newline at end of file |
|
20 | 21 | No newline at end of file |
|
21 | 22 | # compute transform of zero vector No newline at end of file |
|
22 | 23 | x = np.zeros(shape=(1,N)); No newline at end of file |
|
23 | 24 |
w = dualtree(x, J, Faf, af); |
|
24 | 25 |
|
|
25 | 26 | # Uses both real and imaginary wavelets |
|
27 | No newline at end of file | |
|
26 | for i in range (0, J): | |
|
No newline at end of file | ||
|
28 | No newline at end of file | |
|
27 | for j in range (0, 1): No newline at end of file | |
|
28 | 29 |
|
|
29 | 30 | w[i][j][0,k] = 1; No newline at end of file |
|
30 | 31 | y = idualtree(w, J, Fsf, sf); No newline at end of file |
|
31 | 32 | w[i][j][0,k] = 0; No newline at end of file |
|
32 | 33 |
|
|
33 | 34 | Psi[:,idx] = y.T.conj(); No newline at end of file |
|
34 | 35 |
idx = |
|
35 | 36 | No newline at end of file |
|
36 | 37 | # Add uniform vector (seems to be useful if there's a background No newline at end of file |
|
37 | 38 | Psi[:,2*N] = 1/np.sqrt(N); No newline at end of file |
|
38 | 39 | No newline at end of file |
|
39 | 40 | return Psi No newline at end of file |
|
40 | 41 | L40: rhodecode diff rendering error |
@@ -1,76 +1,76 | |||
|
1 | 1 | ''' No newline at end of file |
|
2 | 2 | Created on May 29, 2014 No newline at end of file |
|
3 | 3 | No newline at end of file |
|
4 | 4 | @author: Yolian Amaro No newline at end of file |
|
5 | 5 | ''' No newline at end of file |
|
6 | 6 | No newline at end of file |
|
7 | 7 | import numpy as np No newline at end of file |
|
8 | 8 | from afb import * No newline at end of file |
|
9 | 9 | No newline at end of file |
|
10 | 10 | def dualtree(x, J, Faf, af): No newline at end of file |
|
11 | 11 | No newline at end of file |
|
12 | 12 | # Dual-tree Complex Discrete Wavelet Transform No newline at end of file |
|
13 | 13 | # No newline at end of file |
|
14 | 14 | # USAGE: No newline at end of file |
|
15 | 15 | # w = dualtree(x, J, Faf, af) No newline at end of file |
|
16 | 16 | # INPUT: No newline at end of file |
|
17 | 17 | # x - N-point vector No newline at end of file |
|
18 | 18 | # 1) N is divisible by 2^J No newline at end of file |
|
19 | 19 | # 2) N >= 2^(J-1)*length(af) No newline at end of file |
|
20 | 20 | # J - number of stages No newline at end of file |
|
21 | 21 | # Faf - filters for the first stage No newline at end of file |
|
22 | 22 | # af - filters for the remaining stages No newline at end of file |
|
23 | 23 | # OUTPUT: No newline at end of file |
|
24 | 24 | # w - DWT coefficients No newline at end of file |
|
25 | 25 | # w{j}{1}, j = 1..J - real part No newline at end of file |
|
26 | 26 | # w{j}{2}, j = 1..J - imaginary part No newline at end of file |
|
27 | 27 | # w{J+1}{d} - lowpass coefficients, d = 1,2 No newline at end of file |
|
28 | 28 | # EXAMPLE: No newline at end of file |
|
29 | 29 | # x = rand(1, 512); No newline at end of file |
|
30 | 30 | # J = 4; No newline at end of file |
|
31 | 31 | # [Faf, Fsf] = FSfarras; No newline at end of file |
|
32 | 32 | # [af, sf] = dualfilt1; No newline at end of file |
|
33 | 33 | # w = dualtree(x, J, Faf, af); No newline at end of file |
|
34 | 34 | # y = idualtree(w, J, Fsf, sf); No newline at end of file |
|
35 | 35 | # err = x - y; No newline at end of file |
|
36 | 36 | # max(abs(err)) No newline at end of file |
|
37 | 37 | # No newline at end of file |
|
38 | 38 | # WAVELET SOFTWARE AT POLYTECHNIC UNIVERSITY, BROOKLYN, NY No newline at end of file |
|
39 | 39 | # http://taco.poly.edu/WaveletSoftware/ No newline at end of file |
|
40 | 40 | No newline at end of file |
|
41 | 41 | # ---------Trees Structure---------------# No newline at end of file |
|
42 | 42 | # w [ 0 1 2 .... J ] # No newline at end of file |
|
43 | 43 | # | | | | # No newline at end of file |
|
44 | 44 | # [0 1] [0 1] [0 1] [0 1] # No newline at end of file |
|
45 | 45 | #----------------------------------------# No newline at end of file |
|
46 | 46 | No newline at end of file |
|
47 | 47 | # normalization |
|
48 | No newline at end of file | |
|
48 | x = x/np.sqrt(2); No newline at end of file | |
|
49 | 49 | No newline at end of file |
|
50 | 50 | No newline at end of file |
|
51 | 51 | w = np.zeros(shape=(J+1), dtype=object) No newline at end of file |
|
52 | 52 | No newline at end of file |
|
53 | 53 | for j in range (0, w.size): No newline at end of file |
|
54 | 54 | w[j] = np.zeros(shape=(J+1), dtype=object) No newline at end of file |
|
55 | 55 | No newline at end of file |
|
56 | 56 | # Tree 1 No newline at end of file |
|
57 | 57 | [x1, w[0][0]] = afb(x, Faf[0,0]); # w{1}{1} No newline at end of file |
|
58 | 58 | No newline at end of file |
|
59 | 59 | No newline at end of file |
|
60 | 60 | for j in range (1,J): No newline at end of file |
|
61 | 61 | [x1,w[j][0]] = afb(x1, af[0,0]); ### or 0,1???? No newline at end of file |
|
62 | 62 | No newline at end of file |
|
63 | 63 | No newline at end of file |
|
64 | 64 | No newline at end of file |
|
65 | 65 | w[J][0] = x1; No newline at end of file |
|
66 | 66 | No newline at end of file |
|
67 | 67 | # Tree 2 No newline at end of file |
|
68 | 68 | [x2,w[0][1]] = afb(x, Faf[0,1]); No newline at end of file |
|
69 | 69 | No newline at end of file |
|
70 | 70 | for j in range (1,J): No newline at end of file |
|
71 | 71 | [x2,w[j][1]] = afb(x2, af[0,1]); No newline at end of file |
|
72 | 72 | No newline at end of file |
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73 | 73 | w[J][1] = x2; No newline at end of file |
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74 | 74 | No newline at end of file |
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75 | 75 | return w No newline at end of file |
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76 | 76 | No newline at end of file |
@@ -1,46 +1,46 | |||
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1 | 1 | ''' No newline at end of file |
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2 | 2 | Created on Jun 5, 2014 No newline at end of file |
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3 | 3 | No newline at end of file |
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4 | 4 | @author: Yolian Amaro No newline at end of file |
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5 | 5 | ''' No newline at end of file |
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6 | 6 | No newline at end of file |
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7 | 7 | from sfb import * No newline at end of file |
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8 | 8 | No newline at end of file |
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9 | 9 | def idualtree(w, J, Fsf, sf): No newline at end of file |
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10 | 10 | No newline at end of file |
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11 | 11 | # Inverse Dual-tree Complex DWT No newline at end of file |
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12 | 12 | # No newline at end of file |
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13 | 13 | # USAGE: No newline at end of file |
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14 | 14 | # y = idualtree(w, J, Fsf, sf) No newline at end of file |
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15 | 15 | # INPUT: No newline at end of file |
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16 | 16 | # w - DWT coefficients No newline at end of file |
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17 | 17 | # J - number of stages No newline at end of file |
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18 | 18 | # Fsf - synthesis filters for the last stage No newline at end of file |
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19 | 19 | # sf - synthesis filters for preceeding stages No newline at end of file |
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20 | 20 | # OUTUT: No newline at end of file |
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21 | 21 | # y - output signal No newline at end of file |
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22 | 22 | # See dualtree No newline at end of file |
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23 | 23 | # No newline at end of file |
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24 | 24 | # WAVELET SOFTWARE AT POLYTECHNIC UNIVERSITY, BROOKLYN, NY No newline at end of file |
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25 | 25 | # http://taco.poly.edu/WaveletSoftware/ No newline at end of file |
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26 | 26 | No newline at end of file |
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27 | 27 | # Tree 1 No newline at end of file |
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28 | 28 | y1 = w[J][0]; No newline at end of file |
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29 | 29 | No newline at end of file |
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30 | 30 | for j in range (J-1, 0, -1): No newline at end of file |
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31 | 31 | y1 = sfb(y1, w[j][0], sf[0,0]); No newline at end of file |
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32 | 32 | No newline at end of file |
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33 | 33 | y1 = sfb(y1, w[0][0], Fsf[0,0]); No newline at end of file |
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34 | 34 | No newline at end of file |
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35 | 35 | # Tree 2 No newline at end of file |
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36 | 36 | y2 = w[J][1]; No newline at end of file |
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37 | 37 | No newline at end of file |
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38 | 38 | for j in range (J-1, 0, -1): No newline at end of file |
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39 | 39 | y2 = sfb(y2, w[j][1], sf[0,1]); No newline at end of file |
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40 | 40 | No newline at end of file |
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41 | 41 | y2 = sfb(y2, w[0][1], Fsf[0,1]); No newline at end of file |
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42 | 42 | No newline at end of file |
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43 | 43 | # normalization |
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44 | No newline at end of file | |
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44 | y = (y1 + y2)/np.sqrt(2); No newline at end of file | |
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45 | 45 | No newline at end of file |
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46 | 46 | return y No newline at end of file |
@@ -1,85 +1,94 | |||
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1 | 1 | ''' No newline at end of file |
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2 | 2 | Created on May 27, 2014 No newline at end of file |
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3 | 3 | No newline at end of file |
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4 | 4 | @author: Yolian Amaro No newline at end of file |
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5 | 5 | ''' No newline at end of file |
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6 | 6 | No newline at end of file |
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7 | 7 | #from scipy.sparse import eye No newline at end of file |
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8 | 8 | from scipy import linalg No newline at end of file |
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9 | 9 | import scipy.sparse as sps No newline at end of file |
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10 | 10 | import numpy as np No newline at end of file |
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11 | from numpy.linalg import norm No newline at end of file | |
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11 | 12 | No newline at end of file |
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12 | 13 | def irls_dn(A,b,p,lambda1): No newline at end of file |
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13 | 14 | No newline at end of file |
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14 | 15 | No newline at end of file |
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15 | 16 | # Minimize lambda*||u||_p + ||A*u-b||_2, 0 < p <= 1 No newline at end of file |
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16 | 17 | # using Iterative Reweighted Least Squares No newline at end of file |
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17 | 18 | # (see http://math.lanl.gov/Research/Publications/Docs/chartrand-2008-iteratively.pdf No newline at end of file |
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18 | 19 | # and http://web.eecs.umich.edu/~aey/sparse/sparse11.pdf) No newline at end of file |
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19 | 20 | No newline at end of file |
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20 | 21 | # Note to self: I found that "warm-starting" didn't really help too much. No newline at end of file |
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21 | 22 | No newline at end of file |
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22 | 23 | [M,N] = A.shape; No newline at end of file |
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23 | 24 | # Initialize and precompute: No newline at end of file |
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24 | 25 | eps = 1e-2; # damping parameter No newline at end of file |
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25 | 26 | No newline at end of file |
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26 | 27 | [Q,R] = linalg.qr(A.T.conj(), mode='economic'); No newline at end of file |
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27 | 28 | No newline at end of file |
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28 | 29 | No newline at end of file |
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29 | 30 | c = linalg.solve(R.T.conj(),b); # will be used later also No newline at end of file |
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30 | 31 | u = np.dot(Q,c); # minimum 2-norm solution No newline at end of file |
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31 | 32 | I = sps.eye(M); No newline at end of file |
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32 | 33 | No newline at end of file |
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34 | # Temporary N x N matrix | |
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35 | temp = np.zeros(shape=(N,N)) | |
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36 | No newline at end of file | |
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33 | 37 | #---------- not needed, defined above-------------- No newline at end of file |
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34 | 38 | # Spacing of floating point numbers No newline at end of file |
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35 | 39 | #eps = np.spacing(1) No newline at end of file |
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36 | 40 | #-------------------------------------------------- No newline at end of file |
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37 | 41 | No newline at end of file |
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38 | 42 | # Loop until damping parameter is small enough No newline at end of file |
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39 | 43 | while (eps > 1e-7): No newline at end of file |
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40 | 44 | epschange = 0; No newline at end of file |
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41 | 45 | # Loop until it's time to change eps |
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46 | No newline at end of file | |
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42 | while (~epschange): No newline at end of file | |
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43 | 47 | # main loop No newline at end of file |
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44 | 48 | # u_n = W*A'*(A*W*A'+ lambda*I)^-1 * b No newline at end of file |
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45 | 49 | # where W = diag(1/w) No newline at end of file |
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46 | 50 | # where w = (u.^2 + eps).^(p/2-1) No newline at end of file |
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47 | 51 | No newline at end of file |
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48 | 52 | # Update |
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53 | No newline at end of file | |
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49 | w = (u**2 + eps)**(1-p/2); No newline at end of file | |
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50 | 54 | |
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55 | No newline at end of file | |
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51 | # Empty temporary N x N matrix | |
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No newline at end of file | ||
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56 | No newline at end of file | |
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52 | temp = np.zeros(shape=(N,N)) No newline at end of file | |
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No newline at end of file | ||
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57 | # # Sparse matrix | |
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58 | # for i in range (0, N): | |
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59 | # for j in range (0,N): | |
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|
60 | # if(i==j): | |
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61 | # temp[i,j] = w[k] | |
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|
62 | # k = k+1 | |
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|
63 | #-------------------------------------------------- No newline at end of file | |
|
53 | 64 | |
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65 | No newline at end of file | |
|
54 | k = 0 | |
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66 | No newline at end of file | |
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55 | # Sparse matrix | |
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56 | for i in range (0, N): | |
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57 | for j in range (0,N): | |
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No newline at end of file | ||
|
58 | if(i==j): | |
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|
59 | temp[i,j] = w[k] | |
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No newline at end of file | ||
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60 | k = k+1 No newline at end of file | |
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61 | 67 | No newline at end of file |
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62 | 68 | # Compressed Sparse Matrix No newline at end of file |
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63 | 69 | W = sps.csr_matrix(temp); #Compressed Sparse Row matrix No newline at end of file |
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64 | 70 | No newline at end of file |
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65 | 71 | No newline at end of file |
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66 | 72 | WAT = W*A.T.conj(); No newline at end of file |
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67 | 73 |
|
|
74 | No newline at end of file | |
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68 | u_new = np.dot(WAT , linalg.solve(np.dot(A,WAT) + np.dot(lambda1,I), b)); No newline at end of file | |
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No newline at end of file | ||
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75 | #print "np.dot(A,WAT)", np.dot(A,WAT).shape | |
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76 | #print "np.dot(lambda1,I)", np.dot(lambda1,I).shape | |
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No newline at end of file | ||
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77 | #print "linalg.solve((np.dot(A,WAT) + np.dot(lambda1,I)), b)", linalg.solve((np.dot(A,WAT) + np.dot(lambda1,I)), b).shape | |
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78 | ||
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No newline at end of file | ||
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79 | u_new = np.dot(WAT , linalg.solve((np.dot(A,WAT) + np.dot(lambda1,I)), b)); No newline at end of file | |
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69 | 80 | No newline at end of file |
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70 | 81 | # See if this subproblem is converging |
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82 | No newline at end of file | |
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71 | delu = np.linalg.norm(u_new-u)/np.linalg.norm(u); No newline at end of file | |
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72 | 83 | epschange = delu < (np.sqrt(eps)/100.0); No newline at end of file |
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73 | 84 | No newline at end of file |
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74 | 85 | # Make update No newline at end of file |
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75 | 86 | u = u_new; No newline at end of file |
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76 | 87 | No newline at end of file |
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77 | 88 | No newline at end of file |
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78 | 89 | eps = eps/10.0; # decrease eps |
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No newline at end of file | ||
|
79 | # Print info | |
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No newline at end of file | ||
|
80 | #print 'eps =',eps; No newline at end of file | |
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81 | 90 | No newline at end of file |
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82 | 91 | return u No newline at end of file |
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83 | 92 | No newline at end of file |
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84 | 93 | No newline at end of file |
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85 | 94 | No newline at end of file |
@@ -1,76 +1,74 | |||
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1 | 1 | ''' No newline at end of file |
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2 | 2 | Created on May 30, 2014 No newline at end of file |
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3 | 3 | No newline at end of file |
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4 | 4 | @author: Yolian Amaro No newline at end of file |
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5 | 5 | ''' No newline at end of file |
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6 | 6 | No newline at end of file |
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7 | 7 | from irls_dn import * No newline at end of file |
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8 | 8 | from scipy.optimize import fsolve No newline at end of file |
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9 | 9 | import numpy as np |
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10 | No newline at end of file | |
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10 | from scipy.optimize import root No newline at end of file | |
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No newline at end of file | ||
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11 | from dogleg import * | |
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No newline at end of file | ||
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12 | from numpy.linalg import norm | |
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No newline at end of file | ||
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13 | ||
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No newline at end of file | ||
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14 | import matplotlib.pyplot as plt No newline at end of file | |
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11 | 15 | No newline at end of file |
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12 | 16 | def irls_dn2(A,b,p,G): No newline at end of file |
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13 | 17 | No newline at end of file |
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14 | 18 | # Minimize ||u||_p subject to ||A*u-b||_2^2 <= G (0 < p <= 1) No newline at end of file |
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15 | 19 | No newline at end of file |
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16 | 20 | # What this function actually does is finds the lambda1 so that the solution No newline at end of file |
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17 | 21 | # to the following problem satisfies ||A*u-b||_2^2 <= G: No newline at end of file |
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18 | 22 | # Minimize lambda1*||u||_p + ||A*u-b||_2 No newline at end of file |
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19 | 23 | No newline at end of file |
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20 | 24 | # Start with a large lambda1, and do a line search until fidelity <= G. No newline at end of file |
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21 | 25 | # (Inversions with large lambda1 are really fast anyway). No newline at end of file |
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22 | 26 | No newline at end of file |
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23 | 27 | # Then spin up fsolve to localize the root even better No newline at end of file |
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24 | 28 | No newline at end of file |
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25 | 29 | # Line Search No newline at end of file |
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26 | 30 | No newline at end of file |
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27 | 31 | alpha = 2.0; # Line search parameter No newline at end of file |
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28 | 32 | lambda1 = 1e5; # What's a reasonable but safe initial guess? No newline at end of file |
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29 | 33 | u = irls_dn(A,b,p,lambda1); |
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34 | No newline at end of file | |
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30 | fid = np.linalg.norm(np.dot(A,u)-b)**2; No newline at end of file | |
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No newline at end of file | ||
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35 | ||
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No newline at end of file | ||
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36 | fid = norm(np.dot(A,u)-b)**2; No newline at end of file | |
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31 | 37 | No newline at end of file |
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32 | 38 | print '----------------------------------\n'; No newline at end of file |
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33 | 39 | No newline at end of file |
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34 | 40 | while (fid >= G): No newline at end of file |
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35 | 41 | lambda1 = lambda1 / alpha; # Balance between speed and accuracy No newline at end of file |
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36 | 42 | u = irls_dn(A,b,p,lambda1); |
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43 | No newline at end of file | |
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37 | fid = np.linalg.norm(np.dot(A,u)-b)**2; No newline at end of file | |
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38 | 44 | print 'lambda = %2e \t' % lambda1, '||A*u-b||^2 = %.1f\n' % fid; No newline at end of file |
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45 | #print u No newline at end of file | |
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39 | 46 | |
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47 | No newline at end of file | |
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40 | # Refinement using fzero No newline at end of file | |
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41 | 48 | lambda0 = np.array([lambda1,lambda1*alpha]); # interval with zero-crossing No newline at end of file |
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42 | 49 | No newline at end of file |
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43 | 50 | def myfun(lambda1): |
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51 | No newline at end of file | |
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44 | print "A = ", A.shape | |
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No newline at end of file | ||
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52 | No newline at end of file | |
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45 | print "b = ", b.shape | |
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53 | No newline at end of file | |
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46 | lambda1 | |
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No newline at end of file | ||
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54 | No newline at end of file | |
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47 | return np.linalg.norm(A*irls_dn(A,b,p,lambda1) - b)**2 - G; No newline at end of file | |
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No newline at end of file | ||
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55 | #return np.linalg.norm(np.dot(A, irls_dn(A,b,p,lambda1)) - b)**2 - G; No newline at end of file | |
|
48 | 56 | |
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No newline at end of file | ||
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49 | #f = lambda lambda1: np.linalg.norm(A*irls_dn(A,b,p,lambda1) - b)**2 - G; NOOOOOO | |
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No newline at end of file | ||
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50 | ||
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No newline at end of file | ||
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51 | ||
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No newline at end of file | ||
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52 | # opts = optimset('fzero'); | |
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No newline at end of file | ||
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53 | # # opts.Display = 'iter'; | |
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No newline at end of file | ||
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54 | # opts.Display = 'none'; | |
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No newline at end of file | ||
|
55 | # opts.TolX = 0.01*lambda1; | |
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No newline at end of file | ||
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56 | ||
|
No newline at end of file | ||
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57 | #sol1 = fsolve(myfun,lambda0.ravel(), args=(), xtol=1e-14, maxfev=100000); No newline at end of file | |
|
58 | 57 | print "tolerancia=", 0.01*lambda1 No newline at end of file |
|
59 | 58 | |
|
59 | No newline at end of file | |
|
60 | #lambda1 = root(myfun,lambda0, method='krylov', tol=0.01*lambda1); No newline at end of file | |
|
No newline at end of file | ||
|
60 | #lambda1 = root(myfun, lambda1, method='krylov', tol=0.01*lambda1); No newline at end of file | |
|
61 | 61 | No newline at end of file |
|
62 | ||
|
No newline at end of file | ||
|
63 | print "lambda0[0]", lambda0[0] No newline at end of file | |
|
62 | 64 | |
|
65 | No newline at end of file | |
|
63 | print "lamda1=", lambda1 | |
|
No newline at end of file | ||
|
64 | print "lambda0=", lambda0 No newline at end of file | |
|
65 | 66 | |
|
67 | No newline at end of file | |
|
66 | lambda1 = fsolve(myfun,lambda0); # FALTA OPTIMIZE ESTO | |
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No newline at end of file | ||
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67 | ||
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No newline at end of file | ||
|
68 | print "A = ", A.shape | |
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No newline at end of file | ||
|
69 | print "b = ", b.shape | |
|
No newline at end of file | ||
|
70 | print "lambda1=", lambda1.shape No newline at end of file | |
|
71 | 68 | No newline at end of file |
|
72 | 69 | u = irls_dn(A,b,p,lambda1); No newline at end of file |
|
73 | 70 | No newline at end of file |
|
74 | 71 | No newline at end of file |
|
75 | 72 | return u; No newline at end of file |
|
76 | 73 | No newline at end of file |
|
77 | 74 |
@@ -1,60 +1,64 | |||
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1 | 1 | ''' No newline at end of file |
|
2 | 2 | Created on Jun 5, 2014 No newline at end of file |
|
3 | 3 | No newline at end of file |
|
4 | 4 | @author: Yolian Amaro No newline at end of file |
|
5 | 5 | ''' No newline at end of file |
|
6 | 6 | No newline at end of file |
|
7 | 7 | from multirate import * No newline at end of file |
|
8 | 8 | import numpy as np No newline at end of file |
|
9 | 9 | from cshift import * No newline at end of file |
|
10 | 10 | No newline at end of file |
|
11 | 11 | def sfb(lo, hi, sf): No newline at end of file |
|
12 | 12 | No newline at end of file |
|
13 | 13 | # Synthesis filter bank No newline at end of file |
|
14 | 14 | # No newline at end of file |
|
15 | 15 | # USAGE: No newline at end of file |
|
16 | 16 | # y = sfb(lo, hi, sf) No newline at end of file |
|
17 | 17 | # INPUT: No newline at end of file |
|
18 | 18 | # lo - low frqeuency input No newline at end of file |
|
19 | 19 | # hi - high frequency input No newline at end of file |
|
20 | 20 | # sf - synthesis filters No newline at end of file |
|
21 | 21 | # sf(:, 1) - lowpass filter (even length) No newline at end of file |
|
22 | 22 | # sf(:, 2) - highpass filter (even length) No newline at end of file |
|
23 | 23 | # OUTPUT: No newline at end of file |
|
24 | 24 | # y - output signal No newline at end of file |
|
25 | 25 | # See also afb No newline at end of file |
|
26 | 26 | # No newline at end of file |
|
27 | 27 | # WAVELET SOFTWARE AT POLYTECHNIC UNIVERSITY, BROOKLYN, NY No newline at end of file |
|
28 | 28 | # http://taco.poly.edu/WaveletSoftware/ No newline at end of file |
|
29 | 29 | No newline at end of file |
|
30 | 30 | N = 2*lo.size; No newline at end of file |
|
31 | 31 | L = sf.size/2; No newline at end of file |
|
32 | 32 | No newline at end of file |
|
33 | 33 | # Need to change format for upfirdn funct: No newline at end of file |
|
34 | 34 | lo = lo.T.conj() No newline at end of file |
|
35 | 35 | lo = lo.reshape(lo.size) No newline at end of file |
|
36 | 36 | No newline at end of file |
|
37 | 37 | #print 'sfb hi', hi No newline at end of file |
|
38 | 38 | No newline at end of file |
|
39 | 39 | # Need to change format for upfirdn funct: No newline at end of file |
|
40 | 40 | hi = hi.T.conj() No newline at end of file |
|
41 | 41 | hi = hi.reshape(hi.size) No newline at end of file |
|
42 | 42 | No newline at end of file |
|
43 | 43 | #hi = hi.reshape(1, hi.size) No newline at end of file |
|
44 | 44 | No newline at end of file |
|
45 | 45 | No newline at end of file |
|
46 | 46 | lo = upfirdn(lo, sf[:,0], 2, 1); No newline at end of file |
|
47 | 47 | hi = upfirdn(hi, sf[:,1], 2, 1); No newline at end of file |
|
48 | ||
|
No newline at end of file | ||
|
49 | lo = lo[0:lo.size-1] | |
|
No newline at end of file | ||
|
50 | hi = hi[0:hi.size-1] | |
|
No newline at end of file | ||
|
51 | No newline at end of file | |
|
48 | 52 | y = lo + hi; |
|
53 | No newline at end of file | |
|
49 | y[0:L-1] = y[0:L-1] + y[N+ np.arange(0,L-1)]; #CHECK IF ARANGE IS CORRECT No newline at end of file | |
|
50 | 54 | y = y[0:N]; No newline at end of file |
|
51 | 55 | No newline at end of file |
|
52 | 56 | #print 'y en sbf\n', y.shape No newline at end of file |
|
53 | 57 | No newline at end of file |
|
54 | 58 | y = y.reshape(1, y.size) No newline at end of file |
|
55 | 59 | #print 'y en sbf\n', y.shape No newline at end of file |
|
56 | 60 | No newline at end of file |
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57 | 61 | y = cshift(y, 1-L/2); No newline at end of file |
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58 | 62 | No newline at end of file |
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59 | 63 | return y; No newline at end of file |
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60 | 64 | No newline at end of file |
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