void smurf_sc2fft( int *status ) {
int avpspec=0; /* Flag for doing average power spectrum */
double avpspecthresh=0; /* Threshold noise for detectors in avpspec */
Grp * basegrp = NULL; /* Basis group for output filenames */
smfArray *bbms = NULL; /* Bad bolometer masks */
smfArray *concat=NULL; /* Pointer to a smfArray */
size_t contchunk; /* Continuous chunk counter */
smfArray *darks = NULL; /* dark frames */
int ensureflat; /* Flag for flatfielding data */
Grp *fgrp = NULL; /* Filtered group, no darks */
smfArray *flatramps = NULL;/* Flatfield ramps */
AstKeyMap *heateffmap = NULL; /* Heater efficiency data */
size_t gcount=0; /* Grp index counter */
size_t i; /* Loop counter */
smfGroup *igroup=NULL; /* smfGroup corresponding to igrp */
Grp *igrp = NULL; /* Input group of files */
int inverse=0; /* If set perform inverse transform */
int isfft=0; /* Are data fft or real space? */
dim_t maxconcat=0; /* Longest continuous chunk length in samples */
size_t ncontchunks=0; /* Number continuous chunks outside iter loop */
smfData *odata=NULL; /* Pointer to output smfData to be exported */
Grp *ogrp = NULL; /* Output group of files */
size_t outsize; /* Total number of NDF names in the output group */
int polar=0; /* Flag for FFT in polar coordinates */
int power=0; /* Flag for squaring amplitude coeffs */
size_t size; /* Number of files in input group */
smfData *tempdata=NULL; /* Temporary smfData pointer */
int weightavpspec=0; /* Flag for 1/noise^2 weighting */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
int zerobad; /* Zero VAL__BADD before taking FFT? */
/* Main routine */
ndfBegin();
/* Find the number of cores/processors available and create a pool of
threads of the same size. */
wf = thrGetWorkforce( thrGetNThread( SMF__THREADS, status ), status );
/* Get input file(s) */
kpg1Rgndf( "IN", 0, 1, "", &igrp, &size, status );
/* Filter out darks */
smf_find_science( igrp, &fgrp, 1, NULL, NULL, 1, 1, SMF__NULL, &darks,
&flatramps, &heateffmap, NULL, status );
/* input group is now the filtered group so we can use that and
free the old input group */
size = grpGrpsz( fgrp, status );
grpDelet( &igrp, status);
igrp = fgrp;
fgrp = NULL;
/* We now need to combine files from the same subarray and same sequence
to form a continuous time series */
smf_grp_related( igrp, size, 1, 0, 0, NULL, NULL, &maxconcat, NULL, &igroup,
&basegrp, NULL, status );
/* Get output file(s) */
size = grpGrpsz( basegrp, status );
if( size > 0 ) {
kpg1Wgndf( "OUT", basegrp, size, size, "More output files required...",
&ogrp, &outsize, status );
} else {
msgOutif(MSG__NORM, " ", TASK_NAME ": All supplied input frames were DARK,"
" nothing to do", status );
}
/* Get group of bolometer masks and read them into a smfArray */
smf_request_mask( "BBM", &bbms, status );
/* Obtain the number of continuous chunks and subarrays */
if( *status == SAI__OK ) {
ncontchunks = igroup->chunk[igroup->ngroups-1]+1;
}
msgOutiff( MSG__NORM, "", "Found %zu continuous chunk%s", status, ncontchunks,
(ncontchunks > 1 ? "s" : "") );
/* Are we flatfielding? */
parGet0l( "FLAT", &ensureflat, status );
/* Are we doing an inverse transform? */
parGet0l( "INVERSE", &inverse, status );
/* Are we using polar coordinates instead of cartesian for the FFT? */
parGet0l( "POLAR", &polar, status );
/* Are we going to assume amplitudes are squared? */
parGet0l( "POWER", &power, status );
/* Are we going to zero bad values first? */
parGet0l( "ZEROBAD", &zerobad, status );
/* Are we calculating the average power spectrum? */
parGet0l( "AVPSPEC", &avpspec, status );
if( avpspec ) {
power = 1;
parGet0d( "AVPSPECTHRESH", &avpspecthresh, status );
parGet0l( "WEIGHTAVPSPEC", &weightavpspec, status );
}
/* If power is true, we must be in polar form */
if( power && !polar) {
msgOutif( MSG__NORM, " ", TASK_NAME
": power spectrum requested so setting POLAR=TRUE", status );
polar = 1;
}
gcount = 1;
for( contchunk=0;(*status==SAI__OK)&&contchunk<ncontchunks; contchunk++ ) {
size_t idx;
/* Concatenate this continuous chunk but forcing a raw data read.
We will need quality. */
smf_concat_smfGroup( wf, NULL, igroup, darks, NULL, flatramps, heateffmap,
contchunk, ensureflat, 1, NULL, 0, NULL, NULL, 0, 0, 0,
&concat, NULL, status );
/* Now loop over each subarray */
/* Export concatenated data for each subarray to NDF file */
for( idx=0; (*status==SAI__OK)&&idx<concat->ndat; idx++ ) {
if( concat->sdata[idx] ) {
smfData * idata = concat->sdata[idx];
int provid = NDF__NOID;
dim_t nbolo; /* Number of detectors */
dim_t ndata; /* Number of data points */
/* Apply a mask to the quality array and data array */
smf_apply_mask( idata, bbms, SMF__BBM_QUAL|SMF__BBM_DATA, 0, status );
smf_get_dims( idata, NULL, NULL, &nbolo, NULL, &ndata, NULL, NULL,
status );
/* Check for double precision data */
if( idata->dtype != SMF__DOUBLE ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME ": data are not double precision.", status );
}
/* Are we zeroing VAL__BADD? */
if( (*status==SAI__OK) && zerobad ) {
double *data= (double *) idata->pntr[0];
for( i=0; i<ndata; i++ ) {
if( data[i] == VAL__BADD ) {
data[i] = 0;
}
}
}
/* Check whether we need to transform the data at all */
isfft = smf_isfft(idata,NULL,NULL,NULL,NULL,NULL,status);
if( isfft && avpspec && (*status == SAI__OK) ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME
": to calculate average power spectrum input data cannot "
"be FFT", status );
}
if( (*status == SAI__OK) && (isfft == inverse) ) {
if( avpspec ) {
/* If calculating average power spectrum do the transforms with
smf_bolonoise so that we can also measure the noise of
each detector */
double *whitenoise=NULL;
smf_qual_t *bolomask=NULL;
double mean, sig, freqlo;
size_t ngood, newgood;
whitenoise = astCalloc( nbolo, sizeof(*whitenoise) );
bolomask = astCalloc( nbolo, sizeof(*bolomask) );
freqlo = 1. / (idata->hdr->steptime * idata->hdr->nframes);
smf_bolonoise( wf, idata, 1, freqlo, SMF__F_WHITELO,
SMF__F_WHITEHI, 1, 0, whitenoise, NULL, &odata,
status );
/* Initialize quality */
for( i=0; i<nbolo; i++ ) {
if( whitenoise[i] == VAL__BADD ) {
bolomask[i] = SMF__Q_BADB;
} else {
/* smf_bolonoise returns a variance, so take sqrt */
whitenoise[i] = sqrt(whitenoise[i]);
}
}
ngood=-1;
newgood=0;
/* Iteratively cut n-sigma noisy outlier detectors */
while( ngood != newgood ) {
ngood = newgood;
smf_stats1D( whitenoise, 1, nbolo, bolomask, 1, SMF__Q_BADB,
&mean, &sig, NULL, NULL, status );
msgOutiff( MSG__DEBUG, "", TASK_NAME
": mean=%lf sig=%lf ngood=%li\n", status,
mean, sig, ngood);
newgood=0;
for( i=0; i<nbolo; i++ ) {
if( whitenoise[i] != VAL__BADD ){
if( (whitenoise[i] - mean) > avpspecthresh *sig ) {
whitenoise[i] = VAL__BADD;
bolomask[i] = SMF__Q_BADB;
} else {
newgood++;
}
}
}
}
msgOutf( "", TASK_NAME
": Calculating average power spectrum of best %li "
" bolometers.", status, newgood);
/* If using 1/noise^2 weights, calculate 1/whitenoise^2 in-place
to avoid allocating another array */
if( weightavpspec ) {
msgOutif( MSG__VERB, "", TASK_NAME ": using 1/noise^2 weights",
status );
for( i=0; i<nbolo; i++ ) {
if( whitenoise[i] && (whitenoise[i] != VAL__BADD) ) {
whitenoise[i] = 1/(whitenoise[i]*whitenoise[i]);
}
}
}
/* Calculate the average power spectrum of good detectors */
tempdata = smf_fft_avpspec( odata, bolomask, 1, SMF__Q_BADB,
weightavpspec ? whitenoise : NULL,
status );
smf_close_file( &odata, status );
whitenoise = astFree( whitenoise );
bolomask = astFree( bolomask );
odata = tempdata;
tempdata = NULL;
/* Store the number of good bolometers */
parPut0i( "NGOOD", newgood, status );
} else {
/* Otherwise do forward/inverse transforms here as needed */
/* If inverse transform convert to cartesian representation first */
if( inverse && polar ) {
smf_fft_cart2pol( wf, idata, 1, power, status );
}
/* Tranform the data */
odata = smf_fft_data( wf, idata, NULL, inverse, 0, status );
smf_convert_bad( wf, odata, status );
if( inverse ) {
/* If output is time-domain, ensure that it is ICD bolo-ordered */
smf_dataOrder( odata, 1, status );
} else if( polar ) {
/* Store FFT of data in polar form */
smf_fft_cart2pol( wf, odata, 0, power, status );
}
}
/* open a reference input file for provenance propagation */
ndgNdfas( basegrp, gcount, "READ", &provid, status );
/* Export the data to a new file */
smf_write_smfData( odata, NULL, NULL, ogrp, gcount, provid,
MSG__VERB, 0, status );
/* Free resources */
ndfAnnul( &provid, status );
smf_close_file( &odata, status );
} else {
msgOutif( MSG__NORM, " ",
"Data are already transformed. No output will be produced",
status );
}
}
/* Update index into group */
gcount++;
}
/* Close the smfArray */
smf_close_related( &concat, status );
}
/* Write out the list of output NDF names, annulling the error if a null
parameter value is supplied. */
if( *status == SAI__OK ) {
grpList( "OUTFILES", 0, 0, NULL, ogrp, status );
if( *status == PAR__NULL ) errAnnul( status );
}
/* Tidy up after ourselves: release the resources used by the grp routines */
grpDelet( &igrp, status);
grpDelet( &ogrp, status);
if (basegrp) grpDelet( &basegrp, status );
if( igroup ) smf_close_smfGroup( &igroup, status );
if( flatramps ) smf_close_related( &flatramps, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
if (bbms) smf_close_related( &bbms, status );
ndfEnd( status );
/* Ensure that FFTW doesn't have any used memory kicking around */
fftw_cleanup();
}
void smf_bolonoise( ThrWorkForce *wf, smfData *data, double gfrac,
size_t window, double f_low,
double f_white1, double f_white2,
int nep, size_t len, double *whitenoise, double *fratio,
smfData **fftpow,int *status ) {
double *base=NULL; /* Pointer to base coordinates of array */
size_t bstride; /* bolometer index stride */
double df=1; /* Frequency step size in Hz */
size_t i; /* Loop counter */
size_t i_low; /* Index in power spectrum to f_low */
size_t i_w1; /* Index in power spectrum to f_white1 */
size_t i_w2; /* Index in power spectrum to f_white2 */
size_t j; /* Loop counter */
size_t mingood; /* Min. required no. of good values in bolometer */
dim_t nbolo; /* Number of bolometers */
dim_t ndata; /* Number of data points */
dim_t nf=0; /* Number of frequencies */
size_t ngood; /* Number of good samples */
dim_t ntslice; /* Number of time slices */
double p_low; /* Power at f_low */
double p_white; /* Average power from f_white1 to f_white2 */
smfData *pow=NULL; /* Pointer to power spectrum data */
smf_qual_t *qua=NULL; /* Pointer to quality component */
double steptime=1; /* Length of a sample in seconds */
size_t tstride; /* time index stride */
if (*status != SAI__OK) return;
/* Check inputs */
if (!smf_dtype_check_fatal( data, NULL, SMF__DOUBLE, status )) return;
if( !data->hdr ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME ": smfData has no header", status );
return;
}
/* Obtain dimensions */
smf_get_dims( data, NULL, NULL, &nbolo, &ntslice, &ndata, &bstride, &tstride,
status );
if( *status==SAI__OK ) {
steptime = data->hdr->steptime;
if( steptime < VAL__SMLD ) {
*status = SAI__ERROR;
errRep("", FUNC_NAME ": FITS header error, STEPTIME must be > 0",
status);
} else {
/* Frequency steps in the FFT */
df = 1. / (steptime * (double) ntslice );
}
}
/* Initialize arrays */
if( whitenoise ) for(i=0; i<nbolo; i++) whitenoise[i] = VAL__BADD;
if( fratio ) for(i=0; i<nbolo; i++) fratio[i] = VAL__BADD;
/* FFT the data and convert to polar power spectral density form */
pow = smf_fft_data( wf, data, NULL, 0, len, status );
smf_convert_bad( wf, pow, status );
smf_fft_cart2pol( wf, pow, 0, 1, status );
{
dim_t fdims[2];
smf_isfft( pow, NULL, NULL, fdims, NULL, NULL, status );
if( *status == SAI__OK ) nf=fdims[0];
}
/* Check for reasonble frequencies, and integer offsets in the array */
i_low = smf_get_findex( f_low, df, nf, status );
i_w1 = smf_get_findex( f_white1, df, nf, status );
i_w2 = smf_get_findex( f_white2, df, nf, status );
/* Get the quality pointer from the smfData so that we can mask known
bad bolometer. */
qua = smf_select_qualpntr( data, NULL, status );
/* The minimum required number of good values in a bolometer. */
mingood = ( gfrac > 0.0 ) ? ntslice*gfrac : 0;
/* Loop over detectors */
for( i=0; (*status==SAI__OK)&&(i<nbolo); i++ )
if( !qua || !(qua[i*bstride]&SMF__Q_BADB) ) {
/* Pointer to start of power spectrum */
base = pow->pntr[0];
base += nf*i;
/* Smooth the power spectrum */
smf_boxcar1D( base, nf, 1, window, NULL, 0, 1, NULL, status );
/* Measure the power */
if( *status == SAI__OK ) {
p_low = base[i_low];
smf_stats1D( base+i_w1, 1, i_w2-i_w1+1, NULL, 0, 0, &p_white, NULL, NULL,
&ngood, status );
/* It's OK if bad status was generated as long as a mean was calculated */
if( *status==SMF__INSMP ) {
errAnnul( status );
/* if we had no good data there was probably a problem with SMF__Q_BADB
so we simply go to the next bolometer */
if (ngood == 0) continue;
}
/* Count the number of initially good values for the current
bolometer. */
if( (*status==SAI__OK) && qua ) {
ngood = 0;
for( j=0; j<ntslice; j++ ) {
if( qua[i*bstride + j*tstride] == 0 ) ngood++;
}
/* Set bolometer to bad if no power detected, or the number of good
values is too low. */
if( (p_low <= 0) || (p_white <= 0) || (ngood < mingood) ) {
for( j=0; j<ntslice; j++ ) {
qua[i*bstride + j*tstride] |= SMF__Q_BADB;
}
}
}
}
if( (*status==SAI__OK) && (!qua || !(qua[i*bstride]&SMF__Q_BADB)) ) {
/* Power ratio requested */
if ( fratio ) {
fratio[i] = p_low/p_white;
}
/* Store values */
if( whitenoise ) {
/* Integrate the PSD by multiplying the average white noise
level by total number of samples and the frequency spacing:
this calculates the time-domain variance (in 200 Hz SCUBA-2
samples for example) assuming this level holds at all
frequencies. */
whitenoise[i] = p_white * ntslice * df;
/* If NEP set, scale this to variance in a 1-second average by
dividing by the sampling frequency (equivalent to
multiplying by sample length). */
if( nep ) {
whitenoise[i] *= steptime;
}
}
}
}
/* Clean up if the caller does not want to take over the power spectrum */
if( pow ) {
if (fftpow) {
*fftpow = pow;
} else {
smf_close_file( &pow, status );
}
}
}