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assemble.c
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/* $Id$
*
* (C) 2003-2007, Friedrich Woeger <woeger@kis.uni-freiburg.de>,
* Kiepenheuer-Institut für Sonnenphysik, Freiburg (Breisgau), Germany
* All rights reserved.
*
* Redistribution and use in source and binary forms, with or without
* modification, are permitted provided that the following conditions are
* met:
*
* * Redistributions of source code must retain the above copyright
* notice, this list of conditions and the following disclaimer.
* * Redistributions in binary form must reproduce the above copyright
* notice, this list of conditions and the following disclaimer in
* the documentation and/or other materials provided with the
* distribution.
* * Neither the name of the Kiepenheuer-Institut nor the
* names of its contributors may be used to endorse or promote
* products derived from this software without specific prior
* written permission.
*
* THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
* "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
* LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
* FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
* COPYRIGHT OWNER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
* INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
* BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
* LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
* CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
* LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
* ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
* POSSIBILITY OF SUCH DAMAGE.
*/
/* =====================================================================
**
** core speckle routines
**
** =====================================================================
**
** uses: fftw3 library:
** http://www.fftw.org
**
** Library for fast fourier transform
**
** =====================================================================
**
** Author: F. Woeger
** Kiepenheuer-Institut fuer Sonnenphysik
** Freiburg, Germany
**
** Written 17. 06. 2003
**
** =====================================================================
*/
#include "speckle_core.h"
/* =====================================================================
**
** Reassemble the Image
** This is basically putting together the phases and amplitudes.
** Then a retransformation FFT is performed.
**
** =====================================================================
*/
void assemble(int nx, int ny, float *amp, float *phs, float *rec, maininfo info)
{
float *mask = ellmask(nx, ny, NULL, info.tc.max_rad, info.tc.max_rad);
static int INIT = 0;
static long N;
static fftw_complex *in;
static fftw_complex *out;
fftw_plan fft;
long i, j;
long r1, r2, r3;
if (INIT == 0) {
N = nx * ny;
in = fftw_malloc(N * sizeof(fftw_complex));
out = fftw_malloc(N * sizeof(fftw_complex));
INIT = 1;
} else if (N / nx != ny) {
fftw_cleanup();
fftw_free(in);
fftw_free(out);
N = nx * ny;
in = fftw_malloc(N * sizeof(fftw_complex));
out = fftw_malloc(N * sizeof(fftw_complex));
INIT = 1;
}
fft = fftw_plan_dft_2d(nx, ny, in, out, +1, FFTW_ESTIMATE);
for (j = 0; j < ny; j++) {
for (i = 0; i < nx; i++) {
idx(i, j, nx, r1);
shift_idx(i, j, nx / 2, ny / 2, nx, ny, r2);
phs_idx(i, j, nx, r3);
in[r2][0] = amp[r1] * phs[r3] * mask[r1];
in[r2][1] = amp[r1] * phs[r3 + 1] * mask[r1];
}
}
fftw_execute(fft);
for (j = 0; j < ny; j++) {
for (i = 0; i < nx; i++) {
idx(i, j, nx, r1);
rec[r1] = (float) out[r1][0];
}
}
fftw_cleanup();
free(mask);
}