schain Commit - r1569:c96fc34a400b · Jicamarca Repository

MKFact No Hardcoded

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r1569:c96fc34a400b

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r1569:c96fc34a400b

schainf/mkfact/bfield2.f +2 -2

                   subroutine geobfield(tm,r,theta,phi,br,bt,bp,b)
             c*****evaluate bfield at geocentric coords r,theta,phi
             c     and return components of field in r,theta and phi directions
             c     and magnitude
             c*****theta and phi are in radians, r is in km, b is in gauss
             c ===============================================================
             c
             c   essentially, this is an adaptation of igrfdemo. it interpolates
             c   smoothly between the coefficients from 1945 to 1985.
             c
             c     subroutines:
             c         getshc, interpshc, extrapshc, shval3
             c
             c     igrfdemo is due to:
             c     a. zunde
             c     usgs, ms 964, box 25046 federal center, denver, co  80225
             c
             c ===============================================================
                   character*8 filmod(17)
-                  character*31 fqual
+                  character*9 fqual
                   dimension gh1(220), gh2(220), gha(224), ext(3), dtemod(17)
                   data ext /3*0./
                   data filmod /  'dgrf45', 'dgrf50',
 'dgrf55', 'dgrf60', 'dgrf65',
 'dgrf70', 'dgrf75', 'dgrf80',
 'dgrf85', 'dgrf90', 'dgrf95',
 'dgrf00', 'dgrf05', 'dgrf10',
 'dgrf15', 'igrf20', 'igrf20s'/
-                  data fqual/"/usr/local/lib/faraday/bfmodel/"/
+                  data fqual/"/bfmodel/"/
                   data dtemod / 1945., 1950., 1955., 1960.,
 1965., 1970., 1975., 1980., 1985., 1990., 1995., 2000.,
 2005.,2010.,2015.,2020.,2025./
                   data iu/98/,ndt/17/
             c      data a2/40680925./, b2/40408588./
                   data a2/40680631.6/, b2/40408296.0/ ! updated 2010
             c
                   data rtd/57.29577951/
                   data tmp/0./,lp/0/
                   flat=90. - theta*rtd
                   flon=rtd*phi
             c*****if previous time is not equal to current time
                   if(tm .ne. tmp)then
                      l=0
             C        for i=1,ndt
                      DO  1010  i=1,ndt
             C          exit for if(tm .lt. dtemod(i))
                         if(tm .lt. dtemod(i)) GO TO  1011
                         l=i
             C        end for
 CONTINUE
 CONTINUE
             c       write(*,-)tm,l
                     if(l .eq. 0)then
                        write(*,fmt='(" geobfield: time is before earliest model.")')
                        stop
                     end if
                     if(l .eq. ndt)then
                        l=l-1
                        write(*,fmt='(" geobfield: warning - extrapolating beyond ",
 "last set of coefficients.")')
                     end if
                     if(l .ne. lp)then
             c*********if previous epoch not the same, read in new coefs
             c         write(*,fmt='(" read coefs"))')
             c          write(*,*) fqual//filmod(l)
                        call getshc2 (iu, fqual//filmod(l), nmax1, erad, gh1, ier)
                        if(ier .ne. 0)then
                           write(*,fmt='(" geobfield: read error=",i2," on ",a)')
 ier,filmod(l)
                           stop
                        end if
                        call getshc2 (iu, fqual//filmod(l+1), nmax2, erad, gh2, ier)
                       if(ier .ne. 0)then
                          write(*,fmt='(" geobfield: read error=",i2," on ",a)')
 ier,filmod(l+1)
                          stop
                       end if
                    end if
                    if (l .lt. ndt-1) then
                       call interpshc (tm, dtemod(l), nmax1, gh1, dtemod(l+1),
 nmax2, gh2, nmax, gha)
             c         write(*,fmt='(" interpolate"))')
                    else
                       call extrapshc (tm, dtemod(l), nmax1, gh1, nmax2,
 gh2, nmax, gha)
             c         write(*,fmt='(" extrapolate"))')
                    end if
                   end if
             c      tmp=tm
             c      lp=l
                   call shval3(2,flat,flon,r,erad,a2,b2,nmax,gha,0,ext,x,y,z)
                   br=-z/100000.
                   bp=y/100000.
                   bt=-x/100000.
                   b=sqrt(br**2 + bp**2 + bt**2)
             C      write(*,*)flat,flon,r,erad,a2,b2,nmax,gha,ext
             C      write(*,*)tm,r,theta,phi,br,bt,bp,b
                   return
                   end
             c
                   subroutine convrt(i, gdlat, gdalt, gclat, rkm)
             c     convrt converts between geodetic and geocentric coordinates. the
             c     reference geoid is that adopted by the iau in 1964. a=6378.16,
             c     b=6356.7746, f=1/298.25. the equations for conversion from
             c     geocentric to geodetic are from astron. j., vol 66, 1961, p. 15.
             c          i=1   geodetic to geocentric
             c          i=2   geocentric to geodetic
             c        gdlat   geodetic latitude (degrees)
             c        gdalt   altitude above geoid (km)
             c        gclat   geocentric latitude (degrees)
             c          rkm   geocentric radial distance (km)
             c
             c      data   a/6378.16/,       ab2/1.0067397/,   ep2/.0067397/
             c     update 2010
                   data   a/6378.137/,       ab2/1.0067396/,   ep2/.0067396/
                   data dtr/.0174532925199/
                   if (i .eq. 1) then
             c     .....geodetic to geocentric.....
                      gdl    = dtr*gdlat
                      sinlat = sin(gdl)
                      coslat = cos(gdl)
                      sl2    = sinlat*sinlat
                      cl2    = ab2*coslat
                      cl2    = cl2*cl2
                      sinbet = sinlat/sqrt(sl2+cl2)
                      sb2    = amin1(sinbet*sinbet, 1.)
                      cosbet = sqrt(1. - sb2)
                      rgeoid = a/sqrt(1. + ep2*sb2)
                      x      = rgeoid*cosbet + gdalt*coslat
                      y      = rgeoid*sinbet + gdalt*sinlat
                      rkm    = sqrt(x*x + y*y)
                      gclat  = atan2(y,x)/dtr
                      return
                   else if (i .eq. 2) then
             c     .....geocentric to geodetic.....
                      rer  = rkm/a
                      a2   = ((-1.4127348e-8/rer + .94339131e-8)/rer +
 .33523288e-2)/rer
                      a4   = (((-1.2545063e-10/rer + .11760996e-9)/rer +
 .11238084e-4)/rer - .2814244e-5)/rer
                      a6   = ((54.939685e-9/rer - 28.301730e-9)/rer +
 3.5435979e-9)/rer
                      a8   = (((320./rer - 252.)/rer + 64.)/rer - 5.)
 /rer*0.98008304e-12
                      gcl  = dtr*gclat
                      ccl  = cos(gcl)
                      scl  = sin(gcl)
                      s2cl  = 2.*scl*ccl
                      c2cl  = 2.*ccl*ccl - 1.
                      s4cl  = 2.*s2cl*c2cl
                      c4cl  = 2.*c2cl*c2cl - 1.
                      s8cl  = 2.*s4cl*c4cl
                      s6cl  = s2cl*c4cl + c2cl*s4cl
                      dltcl = s2cl*a2 + s4cl*a4 + s6cl*a6 + s8cl*a8
                      gdlat = gclat + dltcl/dtr
                      gdalt = rkm - a/sqrt(1.+ep2*scl*scl)
                      return
                   end if
                   end
             c
                   subroutine getshc2 (iu, fspec, nmax, erad, gh, ier)
             c ===============================================================
             c
             c      version 1.01
             c
             c      reads spherical harmonic coefficients from the specified
             c      file into an array.
             c
             c      input:
             c          iu    - logical unit number
             c          fspec - file specification
             c
             c      output:
             c          nmax  - maximum degree and order of model
             c          erad  - earth's radius associated with the spherical
             c                harmonic coefficients, in the same units as
             c                elevation
             c          gh    - schmidt quasi-normal internal spherical
             c                harmonic coefficients
             c          ier   - error number: =  0, no error
             c                          = -2, records out of order
             c                               = fortran run-time error number
             c
             c      a. zunde
             c      usgs, ms 964, box 25046 federal center, denver, co  80225
             c
             c ===============================================================
                   character      fspec*(*)
                   dimension      gh(*)
             c ---------------------------------------------------------------
             c      open coefficient file. read past first header record.
             c      read degree and order of model and earth's radius.
             c ---------------------------------------------------------------
                   open (iu, file=fspec, status='old', iostat=ier, err=999 )
                   read (iu, *, iostat=ier, err=999)
                   read (iu, *, iostat=ier, err=999) nmax, erad
             c ---------------------------------------------------------------
             c      read the coefficient file, arranged as follows:
             c
             c                              n     m     g     h
             c                              ----------------------
             c                            /   1     0    gh(1)  -
             c                           /    1     1    gh(2) gh(3)
             c                          /     2     0    gh(4)  -
             c                         /      2     1    gh(5) gh(6)
             c          nmax*(nmax+3)/2     / 2     2    gh(7) gh(8)
             c             records          \ 3     0    gh(9)  -
             c                         \      .     .     .     .
             c                          \     .     .     .     .
             c          nmax*(nmax+2)    \    .     .     .     .
             c          elements in gh    \  nmax  nmax   .     .
             c
             c      n and m are, respectively, the degree and order of the
             c      coefficient.
             c ---------------------------------------------------------------
                   i = 0
             C      for nn = 1, nmax
                   DO  1010  nn = 1, nmax
             C          for mm = 0, nn
                   DO  1020  mm = 0, nn
                         read (iu, *, iostat=ier, err=999) n, m, g, h
             c            write(*,*) n,m,g,h,nn,nmax,mm,ier
                         if (nn .ne. n .or. mm .ne. m) then
                             ier = -2
                             goto 999
                         endif
                         i = i + 1
                         gh(i) = g
                         if (m .ne. 0) then
                             i = i + 1
                             gh(i) = h
                         endif
             C          end for
 CONTINUE
 CONTINUE
             C      end for
 CONTINUE
 CONTINUE
 close (iu)
                   return
                   end
             c
             c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ bfieldsr  ~~~~~~~~~~~~~~~~~~~~~~~~~~~~
             c
                   subroutine interpshc (date, dte1, nmax1, gh1, dte2,
 nmax2, gh2, nmax, gh)
             c ===============================================================
             c
             c      version 1.01
             c
             c      interpolates linearly, in time, between two spherical
             c      harmonic models.
             c
             c      input:
             c          date  - date of resulting model (in decimal year)
             c          dte1  - date of earlier model
             c          nmax1 - maximum degree and order of earlier model
             c          gh1   - schmidt quasi-normal internal spherical
             c                harmonic coefficients of earlier model
             c          dte2  - date of later model
             c          nmax2 - maximum degree and order of later model
             c          gh2   - schmidt quasi-normal internal spherical
             c                harmonic coefficients of later model
             c
             c      output:
             c          gh    - coefficients of resulting model
             c          nmax  - maximum degree and order of resulting model
             c
             c      a. zunde
             c      usgs, ms 964, box 25046 federal center, denver, co  80225
             c
             c ===============================================================
                   dimension      gh1(*), gh2(*), gh(*)
             c ---------------------------------------------------------------
             c      the coefficients (gh) of the resulting model, at date
             c      date, are computed by linearly interpolating between the
             c      coefficients of the earlier model (gh1), at date dte1,
             c      and those of the later model (gh2), at date dte2. if one
             c      model is smaller than the other, the interpolation is
             c      performed with the missing coefficients assumed to be 0.
             c ---------------------------------------------------------------
                   factor = (date - dte1) / (dte2 - dte1)
                   if (nmax1 .eq. nmax2) then
                       k = nmax1 * (nmax1 + 2)
                       nmax = nmax1
                   else if (nmax1 .gt. nmax2) then
                       k = nmax2 * (nmax2 + 2)
                       l = nmax1 * (nmax1 + 2)
             C          for i = k + 1, l
                   DO  1010  i = k + 1, l
                         gh(i) = gh1(i) + factor * (-gh1(i))
             C          end for
 CONTINUE
 CONTINUE
                       nmax = nmax1
                   else
                       k = nmax1 * (nmax1 + 2)
                       l = nmax2 * (nmax2 + 2)
             C          for i = k + 1, l
                   DO  1020  i = k + 1, l
                         gh(i) = factor * gh2(i)
             C          end for
 CONTINUE
 CONTINUE
                       nmax = nmax2
                   endif
             C      for i = 1, k
                   DO  1030  i = 1, k
                       gh(i) = gh1(i) + factor * (gh2(i) - gh1(i))
             C      end for
 CONTINUE
 CONTINUE
                   return
                   end
             c
             c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ bfieldsr  ~~~~~~~~~~~~~~~~~~~~~~~~~~~~
             c
                   subroutine extrapshc (date, dte1, nmax1, gh1, nmax2,
 gh2, nmax, gh)
             c ===============================================================
             c
             c      version 1.01
             c
             c      extrapolates linearly a spherical harmonic model with a
             c      rate-of-change model.
             c
             c      input:
             c          date  - date of resulting model (in decimal year)
             c          dte1  - date of base model
             c          nmax1 - maximum degree and order of base model
             c          gh1   - schmidt quasi-normal internal spherical
             c                harmonic coefficients of base model
             c          nmax2 - maximum degree and order of rate-of-change
             c                model
             c          gh2   - schmidt quasi-normal internal spherical
             c                harmonic coefficients of rate-of-change model
             c
             c      output:
             c          gh    - coefficients of resulting model
             c          nmax  - maximum degree and order of resulting model
             c
             c      a. zunde
             c      usgs, ms 964, box 25046 federal center, denver, co  80225
             c
             c ===============================================================
                   dimension      gh1(*), gh2(*), gh(*)
             c ---------------------------------------------------------------
             c      the coefficients (gh) of the resulting model, at date
             c      date, are computed by linearly extrapolating the coef-
             c      ficients of the base model (gh1), at date dte1, using
             c      those of the rate-of-change model (gh2), at date dte2. if
             c      one model is smaller than the other, the extrapolation is
             c      performed with the missing coefficients assumed to be 0.
             c ---------------------------------------------------------------
                   factor = (date - dte1)
                   if (nmax1 .eq. nmax2) then
                       k = nmax1 * (nmax1 + 2)
                       nmax = nmax1
                   else if (nmax1 .gt. nmax2) then
                       k = nmax2 * (nmax2 + 2)
                       l = nmax1 * (nmax1 + 2)
             C          for i = k + 1, l
                   DO  1010  i = k + 1, l
                         gh(i) = gh1(i)
             C          end for
 CONTINUE
 CONTINUE
                       nmax = nmax1
                   else
                       k = nmax1 * (nmax1 + 2)
                       l = nmax2 * (nmax2 + 2)
             C          for i = k + 1, l
                   DO  1020  i = k + 1, l
                         gh(i) = factor * gh2(i)
             C          end for
 CONTINUE
 CONTINUE
                       nmax = nmax2
                   endif
             C      for i = 1, k
                   DO  1030  i = 1, k
                       gh(i) = gh1(i) + factor * gh2(i)
             C      end for
 CONTINUE
 CONTINUE
                   return
                   end
             c
             c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ bfieldsr  ~~~~~~~~~~~~~~~~~~~~~~~~~~~~
             c
                   subroutine shval3 (igdgc, flat, flon, elev, erad, a2, b2,
 nmax, gh, iext, ext, x, y, z)
             c ================================================================
             c
             c      version 1.01
             c
             c      calculates field components from spherical harmonic (sh)
             c      models.
             c
             c      input:
             c          igdgc - indicates coordinate system used; set equal to
             c                1 if geodetic, 2 if geocentric
             c          flat  - north latitude, in degrees
             c          flon  - east longitude, in degrees
             c          elev  - elevation above mean sea level (igdgc=1), or
             c                radial distance from earth's center (igdgc=2)
             c          erad  - value of earth's radius associated with the sh
             c                coefficients, in same units as elev
             c          a2,b2 - squares of semi-major and semi-minor axes of
             c                the reference spheroid used for transforming
             c                between geodetic and geocentric coordinates or
             c                components
             c          nmax  - maximum degree and order of coefficients
             c          gh    - schmidt quasi-normal internal spherical
             c                harmonic coefficients
             c          iext  - external coefficients flag (= 0 if none)
             c          ext   - the three 1st-degree external coefficients
             c                (not used if iext = 0)
             c
             c      output:
             c          x     -  northward component
             c          y     -  eastward component
             c          z     -  vertically-downward component
             c
             c      based on subroutine "igrf" by d. r. barraclough and
             c      s. r. c. malin, report no. 71/1, institute of geological
             c      sciences, u.k.
             c
             c      norman w. peddie, u.s. geological survey, mail stop 964,
             c      federal center, box 25046, denver, colorado 80225
             c
             c ================================================================
             c      the required sizes of the arrays used in this subroutine
             c      depend on the value of nmax.  the minimum dimensions
             c      needed are indicated in the table below.  (note that this
             c      version is dimensioned for nmax of 14 or less).
             c
             c                                  minimum dimension
             c                              --------------------------
             c  nmax
                   dimension  sl(14), cl(14)
             c (nmax * (nmax + 3)) / 2
                   dimension  p(119), q(119)
             c  nmax * (nmax + 2)
                   dimension  gh(224)
             c  3
                   dimension  ext(3)
             c ================================================================
                   parameter  (dtr = .01745329)
                   r = elev
                   slat = sin (flat * dtr)
                   if (90. - flat .lt. .001) then
             c 300 ft from n. pole
                       aa = 89.999
                   else if (90. + flat .lt. .001) then
             c 300 ft from s. pole
                       aa = -89.999
                   else
                       aa = flat
                   endif
                   clat = cos (aa * dtr)
                   sl(1) = sin (flon * dtr)
                   cl(1) = cos (flon * dtr)
                   x = 0.
                   y = 0.
                   z = 0.
                   sd = 0.
                   cd = 1.
                   n = 0
                   l = 1
                   m = 1
                   npq = (nmax * (nmax + 3)) / 2
                   if (igdgc .eq. 1) then
                       aa = a2 * clat * clat
                       bb = b2 * slat * slat
                       cc = aa + bb
                       dd = sqrt (cc)
                       r = sqrt (elev * (elev + 2. * dd)
 + (a2 * aa + b2 * bb) / cc)
                       cd = (elev + dd) / r
                       sd = (a2 - b2) / dd * slat * clat / r
                       aa = slat
                       slat = slat * cd - clat * sd
                       clat = clat * cd + aa * sd
                   endif
                   ratio = erad / r
                   aa = sqrt (3.)
                   p(1) = 2. * slat
                   p(2) = 2. * clat
                   p(3) = 4.5 * slat * slat - 1.5
                   p(4) = 3. * aa * clat * slat
                   q(1) = -clat
                   q(2) = slat
                   q(3) = -3. * clat * slat
                   q(4) = aa * (slat * slat - clat * clat)
             C      for k = 1, npq
                   DO  1010  k = 1, npq
                       if (n .lt. m) then
                         m = 0
                         n = n + 1
                         rr = ratio**(n + 2)
                         fn = n
                       endif
                       fm = m
                       if (k .ge. 5) then
                         if (m .eq. n) then
                             aa = sqrt (1. - .5 / fm)
                             j = k - n - 1
                             p(k) = (1. + 1. / fm) * aa * clat * p(j)
                             q(k) = aa * (clat * q(j) + slat / fm * p(j))
                             sl(m) = sl(m-1) * cl(1) + cl(m-1) * sl(1)
                             cl(m) = cl(m-1) * cl(1) - sl(m-1) * sl(1)
                         else
                             aa = sqrt (fn * fn - fm * fm)
                             bb = sqrt ((fn - 1.)**2 - fm * fm) / aa
                             cc = (2. * fn - 1.) / aa
                             i = k - n
                             j = k - 2 * n + 1
                             p(k) = (fn + 1.) * (cc * slat / fn * p(i) - bb
 / (fn - 1.) * p(j))
                             q(k) = cc * (slat * q(i) - clat / fn * p(i))
 - bb * q(j)
                         endif
                       endif
                       aa = rr * gh(l)
                       if (m .eq. 0) then
                         x = x + aa * q(k)
                         z = z - aa * p(k)
                         l = l + 1
                       else
                         bb = rr * gh(l+1)
                         cc = aa * cl(m) + bb * sl(m)
                         x = x + cc * q(k)
                         z = z - cc * p(k)
                         if (clat .gt. 0.) then
                             y = y + (aa * sl(m) - bb * cl(m)) * fm * p(k)
 / ((fn + 1.) * clat)
                         else
                             y = y + (aa * sl(m) - bb * cl(m)) * q(k)
 * slat
                         endif
                         l = l + 2
                       endif
                       m = m + 1
             C      end for
 CONTINUE
 CONTINUE
                   if (iext .ne. 0) then
                       aa = ext(2) * cl(1) + ext(3) * sl(1)
                       x = x - ext(1) * clat + aa * slat
                       y = y + ext(2) * sl(1) - ext(3) * cl(1)
                       z = z + ext(1) * slat + aa * clat
                   endif
                   aa = x
                   x = x * cd + z * sd
                   z = z * cd - aa * sd
                   return
                   end
             c
             c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ bfieldsr  ~~~~~~~~~~~~~~~~~~~~~~~~~~~~
             c
                   subroutine dihf (x, y, z, d, i, h, f)
             c ===============================================================
             c
             c      version 1.01
             c
             c      computes the geomagnetic elements d, i, h, and f from
             c      x, y, and z.
             c
             c      input:
             c          x   - northward component
             c          y   - eastward component
             c          z   - vertically-downward component
             c
             c      output:
             c          d   - declination
             c          i   - inclination
             c          h   - horizontal intensity
             c          f   - total intensity
             c
             c      a. zunde
             c      usgs, ms 964, box 25046 federal center, denver, co  80225
             c
             c ===============================================================
                   real            i
                   parameter     ( sn = 0.0001 )
             c ---------------------------------------------------------------
             c      if d and i cannot be determined, set equal to 999.0.
             c ---------------------------------------------------------------
                   h2 = x*x + y*y
                   h = sqrt (h2)
                   f = sqrt (h2 + z*z)
                   if (f .lt. sn) then
                       d = 999.
                       i = 999.
                   else
                       i = atan2 (z, h)
                       if (h .lt. sn) then
                         d = 999.
                       else
                         hpx = h + x
                         if (hpx .lt. sn) then
                             d = 180.
                         else
                             d = 2. * atan2 (y, hpx)
                         endif
                       endif
                   endif
                   return
                   end

setup.py +14 0

             # Copyright (c) 2012-2020 Jicamarca Radio Observatory
             # All rights reserved.
             #
             # Distributed under the terms of the BSD 3-clause license.
             """schainpy is an open source library to read, write and process radar data
             Signal Chain is a radar data processing library wich includes modules to read,
             and write different files formats, besides modules to process and visualize the
             data.
             """
             import os
             from setuptools import setup, Extension
             from setuptools.command.build_ext import build_ext as _build_ext
             from schainpy import __version__
             DOCLINES = __doc__.split("\n")
             class build_ext(_build_ext):
                 def finalize_options(self):
                     _build_ext.finalize_options(self)
                     # Prevent numpy from thinking it is still in its setup process:
                     __builtins__.__NUMPY_SETUP__ = False
                     import numpy
                     self.include_dirs.append(numpy.get_include())
             setup(
                 name = "schainpy",
                 version = __version__,
                 description = DOCLINES[0],
                 long_description = "\n".join(DOCLINES[2:]),
                 url = "https://github.com/JRO-Peru/schainpy",
                 author = "Jicamarca Radio Observatory",
                 author_email = "jro-developers@jro.igp.gob.pe",
                 license="BSD-3-Clause",
                 classifiers=[
                     "Development Status :: 4 - Beta",
                     "Environment :: Console",
                     "Intended Audience :: Science/Research",
                     "License :: OSI Approved :: BSD License",
                     "Operating System :: MacOS :: MacOS X",
                     "Operating System :: POSIX :: Linux",
                     "Programming Language :: Python :: 2",
                     "Programming Language :: Python :: 2.7",
                     "Programming Language :: Python :: 3",
                     "Programming Language :: Python :: 3.5",
                     "Programming Language :: Python :: 3.6",
                     "Programming Language :: Python :: 3.7",
                     "Programming Language :: Python :: 3.8",
                     "Topic :: Scientific/Engineering",
                 ],
                 packages = {
                     'schainpy',
                     'schainpy.model',
                     'schainpy.model.data',
                     'schainpy.model.graphics',
                     'schainpy.model.io',
                     'schainpy.model.proc',
                     'schainpy.model.utils',
                     'schainpy.utils',
                     'schainpy.gui',
                     'schainpy.cli',
                     },
                 package_data = {'': ['schain.conf.template'],
                                 'schainpy.files': ['*.oga']
                                 },
                 include_package_data = False,
                 scripts = ['schainpy/gui/schainGUI'],
                 entry_points = {
                     'console_scripts': [
                         'schain = schainpy.cli.cli:main',
                         ],
                     },
                 cmdclass = {'build_ext': build_ext},
                 ext_modules=[
                     Extension("schainpy.model.data._noise", ["schainc/_noise.c"]),
                     Extension("schainpy.model.data._HS_algorithm", ["schainc/_HS_algorithm.c"]),
                     ],
                 setup_requires = ["numpy"],
                 install_requires = [
                     "scipy",
                     "h5py",
                     "matplotlib",
                     "pyzmq",
                     "fuzzywuzzy",
                     "click",
                     ],
             )
             from numpy.distutils.core import Extension, setup
             setup(name='schainpy',
                 ext_modules = [
                     Extension("schainpy.model.proc.mkfact_short_2020_2",
                         sources=[
                             "schainf/mkfact/mkfact_short_2020_2.pyf",
                             "schainf/mkfact/lmdif1.f",
                             "schainf/mkfact/mkfact.f",
                             "schainf/mkfact/r1mach.f",
+                            "schainf/mkfact/bfield2.f"])
+                            ]
+                            )
+            '''
+            setup(name='schainpy',
+                ext_modules = [
+                    Extension("schainpy.model.proc.mkfact_short_2020_2",
+                        sources=[
+                            "schainf/mkfact/mkfact_short_2020_2.pyf",
+                            "schainf/mkfact/lmdif1.f",
+                            "schainf/mkfact/mkfact.f",
+                            "schainf/mkfact/r1mach.f",
                             "schainf/mkfact/bfield2.f"]),
                     Extension("schainpy.model.proc.full_profile_profile",
                         sources=[
                             "schainf/full_profile/full_profile_profile.pyf",
                             "schainf/full_profile/full_profile_profile.f",
                             "schainf/full_profile/fitacf.f",
                             "schainf/full_profile/r1mach.f",
                             "schainf/full_profile/lmdif1.f",
                             "schainf/full_profile/lagp.f",
                             "schainf/full_profile/reader.c",
                             "schainf/full_profile/cbesi.f",
                             "schainf/full_profile/i1mach.f",
                             "schainf/full_profile/zeta.f",
                             "schainf/full_profile/qc25f.f",
                             "schainf/full_profile/qwgtf.f",
                             "schainf/full_profile/qcheb.f",
                             "schainf/full_profile/sgtsl.f",
                             "schainf/full_profile/qk15w.f",
                             "schainf/full_profile/complex.c",
                             "schainf/full_profile/cbinu.f",
                             "schainf/full_profile/cseri.f",
                             "schainf/full_profile/cwrsk.f",
                             "schainf/full_profile/crati.f",
                             "schainf/full_profile/casyi.f",
                             "schainf/full_profile/cbuni.f",
                             "schainf/full_profile/cuni2.f",
                             "schainf/full_profile/gamln.f",
                             "schainf/full_profile/cuchk.f",
                             "schainf/full_profile/cbknu.f",
                             "schainf/full_profile/cshch.f",
                             "schainf/full_profile/ckscl.f",
                             "schainf/full_profile/cuoik.f",
                             "schainf/full_profile/cunik.f",
                             "schainf/full_profile/cuni1.f",
                             "schainf/full_profile/cairy.f",
                             "schainf/full_profile/cmlri.f",
                             "schainf/full_profile/cunhj.f",
                             "schainf/full_profile/cacai.f",
                             "schainf/full_profile/csisl.f",
                             "schainf/full_profile/caxpy.f",
                             "schainf/full_profile/cs1s2.f",
                             "schainf/full_profile/scabs1.f",
                             "schainf/full_profile/cdotu.f",
                             "schainf/full_profile/rs.f",
                             "schainf/full_profile/sppfa.f",
                             "schainf/full_profile/sdot.f",
                             "schainf/full_profile/tred2.f",
                             "schainf/full_profile/tql2.f",
                             "schainf/full_profile/sppdi.f",
                             "schainf/full_profile/saxpy.f",
                             "schainf/full_profile/sscal.f",
                             "schainf/full_profile/pythag.f",
                             "schainf/full_profile/tql1.f",
                             "schainf/full_profile/tred1.f"]),
                     Extension("schainpy.model.proc.fitacf_acf2",
                         sources = [
                             "schainf/acf2/fitacf_acf2.pyf",
                             "schainf/acf2/full_profile_profile.f",
                             "schainf/acf2/fitacf.f",
                             "schainf/acf2/r1mach.f",
                             "schainf/acf2/lmdif1.f",
                             "schainf/acf2/lagp.f",
                             "schainf/acf2/reader.c",
                             "schainf/acf2/cbesi.f",
                             "schainf/acf2/i1mach.f",
                             "schainf/acf2/zeta.f",
                             "schainf/acf2/qc25f.f",
                             "schainf/acf2/qwgtf.f",
                             "schainf/acf2/qcheb.f",
                             "schainf/acf2/sgtsl.f",
                             "schainf/acf2/qk15w.f",
                             "schainf/acf2/complex.c",
                             "schainf/acf2/cbinu.f",
                             "schainf/acf2/cseri.f",
                             "schainf/acf2/cwrsk.f",
                             "schainf/acf2/crati.f",
                             "schainf/acf2/casyi.f",
                             "schainf/acf2/cbuni.f",
                             "schainf/acf2/cuni2.f",
                             "schainf/acf2/gamln.f",
                             "schainf/acf2/cuchk.f",
                             "schainf/acf2/cbknu.f",
                             "schainf/acf2/cshch.f",
                             "schainf/acf2/ckscl.f",
                             "schainf/acf2/cuoik.f",
                             "schainf/acf2/cunik.f",
                             "schainf/acf2/cuni1.f",
                             "schainf/acf2/cairy.f",
                             "schainf/acf2/cmlri.f",
                             "schainf/acf2/cunhj.f",
                             "schainf/acf2/cacai.f",
                             "schainf/acf2/csisl.f",
                             "schainf/acf2/caxpy.f",
                             "schainf/acf2/cs1s2.f",
                             "schainf/acf2/scabs1.f",
                             "schainf/acf2/cdotu.f",
                             "schainf/acf2/rs.f",
                             "schainf/acf2/sppfa.f",
                             "schainf/acf2/sdot.f",
                             "schainf/acf2/tred2.f",
                             "schainf/acf2/tql2.f",
                             "schainf/acf2/sppdi.f",
                             "schainf/acf2/saxpy.f",
                             "schainf/acf2/sscal.f",
                             "schainf/acf2/pythag.f",
                             "schainf/acf2/tql1.f",
                             "schainf/acf2/tred1.f"])
                             ]
                             )
+            '''

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