void smurf_sc2pca( int *status ) {
smfData *amplitudes=NULL; /* Amplitudes of each component */
smfArray *bbms=NULL; /* Bad bolometer masks */
smfData *components=NULL; /* Components */
smfArray *darks=NULL ; /* Dark data */
int ensureflat; /* Flag for flatfielding data */
smfData *data=NULL; /* Pointer to input smfData */
Grp *fgrp=NULL; /* Filtered group, no darks */
smfArray *flatramps=NULL; /* Flatfield ramps */
AstKeyMap *heateffmap = NULL; /* Heater efficiency data */
size_t i=0; /* Counter, index */
Grp *igrp=NULL; /* Input group of files */
Grp *outampgrp=NULL; /* Output amplitude group of files */
Grp *outcompgrp=NULL; /* Output component group of files */
size_t outampsize; /* Total number of NDF names in ocompgrp */
size_t outcompsize; /* Total number of NDF names in ocompgrp */
size_t size; /* Number of files in input group */
ThrWorkForce *wf=NULL; /* Pointer to a pool of worker threads */
/* 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 );
/* Are we flatfielding? */
parGet0l( "FLAT", &ensureflat, status );
/* Filter out useful data (revert to darks if no science data) */
smf_find_science( wf, 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;
if( size > 0 ) {
/* Get output file(s) */
kpg1Wgndf( "OUTAMP", igrp, size, size, "More output files required...",
&outampgrp, &outampsize, status );
kpg1Wgndf( "OUTCOMP", igrp, size, size, "More output files required...",
&outcompgrp, &outcompsize, status );
} else {
msgOutif(MSG__NORM, " ","All supplied input frames were DARK,"
" nothing to flatfield", status );
}
/* Get group of bolometer masks and read them into a smfArray */
smf_request_mask( wf, "BBM", &bbms, status );
for( i=1; i<=size; i++ ) {
if( *status != SAI__OK ) break;
/* Load data, flatfielding and/or opening raw as double as necessary */
smf_open_asdouble( wf, igrp, i, darks, flatramps, heateffmap, ensureflat, &data, status );
/* Mask out bad bolometers */
smf_apply_mask( wf, data, bbms, SMF__BBM_DATA|SMF__BBM_QUAL, 0, status );
/* Sync quality with bad values */
smf_update_quality( wf, data, 1, NULL, 0, 0.05, status );
/* Calculate the PCA */
smf_clean_pca( wf, data, 0, 0, 0, &components, &litudes, 0, 1, NULL,
status );
/* Write out to the new files */
smf_write_smfData( wf, amplitudes, NULL, NULL, outampgrp, i, 0, MSG__VERB,
0, status );
smf_write_smfData( wf, components, NULL, NULL, outcompgrp, i, 0, MSG__VERB,
0, status );
/* Free resources for output data */
smf_close_file( wf, &data, status );
smf_close_file( wf, &litudes, status );
smf_close_file( wf, &components, status );
}
/* Write out the list of output NDF names, annulling the error if a null
parameter value is supplied. */
if( *status == SAI__OK && outampgrp ) {
grpList( "OUTAMPFILES", 0, 0, NULL, outampgrp, status );
if( *status == PAR__NULL ) errAnnul( status );
}
if( *status == SAI__OK && outcompgrp ) {
grpList( "OUTCOMPFILES", 0, 0, NULL, outcompgrp, status );
if( *status == PAR__NULL ) errAnnul( status );
}
/* Tidy up after ourselves: release the resources used by the grp routines */
if( igrp ) grpDelet( &igrp, status);
if( outampgrp ) grpDelet( &outampgrp, status);
if( outcompgrp ) grpDelet( &outcompgrp, status);
if( darks ) smf_close_related( wf, &darks, status );
if( bbms ) smf_close_related( wf, &bbms, status );
if( flatramps ) smf_close_related( wf, &flatramps, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
ndfEnd( status );
}
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 smurf_calcqu( int *status ) {
/* Local Variables: */
AstFitsChan *fc; /* Holds FITS headers for output NDFs */
AstKeyMap *config; /* Holds all cleaning parameters */
AstKeyMap *dkpars; /* Holds dark squid cleaning parameters */
AstKeyMap *heateffmap = NULL; /* Heater efficiency data */
AstKeyMap *sub_instruments;/* Indicates which instrument is being used */
Grp *bgrp = NULL; /* Group of base names for each chunk */
Grp *igrp = NULL; /* Group of input files */
Grp *ogrp = NULL; /* Group of output files */
Grp *sgrp = NULL; /* Group of science files */
HDSLoc *loci = NULL; /* Locator for output I container file */
HDSLoc *locq = NULL; /* Locator for output Q container file */
HDSLoc *locu = NULL; /* Locator for output U container file */
NdgProvenance *oprov; /* Provenance to store in each output NDF */
ThrWorkForce *wf; /* Pointer to a pool of worker threads */
char headval[ 81 ]; /* FITS header value */
char ndfname[ 30 ]; /* Name of output Q or U NDF */
char polcrd[ 81 ]; /* FITS 'POL_CRD' header value */
char subarray[ 10 ]; /* Subarray name (e.g. "s4a", etc) */
double angrot; /* Angle from focal plane X axis to fixed analyser */
double paoff; /* WPLATE value corresponding to POL_ANG=0.0 */
float arcerror; /* Max acceptable error (arcsec) in one block */
int block_end; /* Index of last time slice in block */
int block_start; /* Index of first time slice in block */
int dkclean; /* Clean dark squids? */
int fix; /* Fix the POL-2 triggering issue? */
int iblock; /* Index of current block */
int iplace; /* NDF placeholder for current block's I image */
int ipolcrd; /* Reference direction for waveplate angles */
int maxsize; /* Max no. of time slices in a block */
int minsize; /* Min no. of time slices in a block */
int nc; /* Number of characters written to a string */
int pasign; /* +1 or -1 indicating sense of POL_ANG value */
int qplace; /* NDF placeholder for current block's Q image */
int submean; /* Subtract mean value from each time slice? */
int uplace; /* NDF placeholder for current block's U image */
size_t ichunk; /* Continuous chunk counter */
size_t idx; /* Subarray counter */
size_t igroup; /* Index for group of related input NDFs */
size_t inidx; /* Index into group of science input NDFs */
size_t nchunk; /* Number continuous chunks outside iter loop */
size_t ssize; /* Number of science files in input group */
smfArray *concat = NULL; /* Pointer to smfArray holding bolometer data */
smfArray *darks = NULL; /* dark frames */
smfArray *dkarray = NULL; /* Pointer to smfArray holding dark squid data */
smfArray *flatramps = NULL;/* Flatfield ramps */
smfData *data = NULL; /* Concatenated data for one subarray */
smfData *dkdata = NULL; /* Concatenated dark squid data for one subarray */
smfGroup *sgroup = NULL; /* smfGroup corresponding to sgrp */
/* Check inhereited status */
if( *status != SAI__OK ) return;
/* Start new AST and NDF contexts. */
astBegin;
ndfBegin();
/* Find the number of cores/processors available and create a work force
holding the same number of threads. */
wf = thrGetWorkforce( thrGetNThread( SMF__THREADS, status ), status );
/* Get a group of input files */
kpg1Rgndf( "IN", 0, 1, " Give more NDFs...", &igrp, &ssize, status );
/* Get a group containing just the files holding science data. */
smf_find_science( igrp, &sgrp, 0, NULL, NULL, 1, 1, SMF__NULL, &darks,
&flatramps, &heateffmap, NULL, status );
/* Check we have at least once science file. */
ssize = grpGrpsz( sgrp, status );
if( ssize == 0 ) {
msgOutif( MSG__NORM, " ", "All supplied input frames were DARK.",
status );
} else {
/* See if a correction should be made for the POL2 triggering issue. */
parGet0l( "FIX", &fix, status );
/* Create HDS container files to hold the output NDFs. */
datCreat( "OUTQ", "CALCQU", 0, 0, status );
datCreat( "OUTU", "CALCQU", 0, 0, status );
/* Associate the locators with the structures. */
datAssoc( "OUTQ", "WRITE", &locq, status );
datAssoc( "OUTU", "WRITE", &locu, status );
/* The I images are optional. */
if( *status == SAI__OK ) {
datCreat( "OUTI", "CALCQU", 0, 0, status );
datAssoc( "OUTI", "WRITE", &loci, status );
if( *status == PAR__NULL ) {
errAnnul( status );
loci = NULL;
}
}
/* Group the input files so that all files within a single group have the
same wavelength and belong to the same subscan of the same observation.
Also identify chunks of data that are contiguous in time, and
determine to which such chunk each group belongs. All this information
is returned in a smfGroup structure ("*sgroup"). */
smf_grp_related( sgrp, ssize, 1, 1, 0, NULL, NULL, NULL,
NULL, &sgroup, &bgrp, NULL, status );
/* Obtain the number of contiguous chunks. */
if( *status == SAI__OK ) {
nchunk = sgroup->chunk[ sgroup->ngroups - 1 ] + 1;
} else {
nchunk = 0;
}
/* Indicate we have not yet found a value for the ARCERROR parameter. */
arcerror = 0.0;
/* Loop over all contiguous chunks */
for( ichunk = 0; ichunk < nchunk && *status == SAI__OK; ichunk++ ) {
/* Display the chunk number. */
if( nchunk > 1 ) {
msgOutiff( MSG__VERB, "", " Doing chunk %d of %d.",
status, (int) ichunk + 1, (int) nchunk );
}
/* Concatenate the data within this contiguous chunk. This produces a
smfArray ("concat") containing a smfData for each subarray present in
the chunk. Each smfData holds the concatenated data for a single
subarray. */
smf_concat_smfGroup( wf, NULL, sgroup, darks, NULL, flatramps,
heateffmap, ichunk, 1, 1, NULL, 0, NULL, NULL,
0, 0, 0, &concat, NULL, status );
/* Get a KeyMap holding values for the configuration parameters. Since we
sorted by wavelength when calling smf_grp_related, we know that all
smfDatas in the current smfArray (i.e. chunk) will relate to the same
wavelength. Therefore we can use the same parameters for all smfDatas in
the current smfArray. */
sub_instruments = smf_subinst_keymap( SMF__SUBINST_NONE,
concat->sdata[ 0 ], NULL,
0, status );
config = kpg1Config( "CONFIG", "$SMURF_DIR/smurf_calcqu.def",
sub_instruments, status );
sub_instruments = astAnnul( sub_instruments );
/* Get the CALCQU specific parameters. */
if( !astMapGet0I( config, "PASIGN", &pasign ) ) pasign = 1;
msgOutiff( MSG__VERB, "", "PASIGN=%d", status, pasign );
if( !astMapGet0D( config, "PAOFF", &paoff ) ) paoff = 0.0;
msgOutiff( MSG__VERB, "", "PAOFF=%g", status, paoff );
if( !astMapGet0D( config, "ANGROT", &angrot ) ) angrot = 90.0;
msgOutiff( MSG__VERB, "", "ANGROT=%g", status, angrot );
if( !astMapGet0I( config, "SUBMEAN", &submean ) ) submean = 0;
msgOutiff( MSG__VERB, "", "SUBMEAN=%d", status, submean );
/* See if the dark squids should be cleaned. */
if( !astMapGet0I( config, "DKCLEAN", &dkclean ) ) dkclean = 0;
/* If required, clean the dark squids now since we might need to use them to
clean the bolometer data. */
if( dkclean ) {
/* Create a smfArray containing the dark squid data. For each one, store
a pointer to the main header so that smf_clean_smfArray can get at the
JCMTState information. */
dkarray = smf_create_smfArray( status );
for( idx = 0; idx < concat->ndat && *status == SAI__OK; idx++ ) {
data = concat->sdata[ idx ];
if( data && data->da && data->da->dksquid ) {
dkdata = data->da->dksquid;
dkdata->hdr = data->hdr;
smf_addto_smfArray( dkarray, dkdata, status );
}
}
/* Clean the smfArray containing the dark squid data. Use the "CLEANDK.*"
parameters. */
(void) astMapGet0A( config, "CLEANDK", &dkpars );
smf_clean_smfArray( wf, dkarray, NULL, NULL, NULL, dkpars, status );
dkpars = astAnnul( dkpars );
/* Nullify the header pointers so that we don't accidentally close any. */
if( dkarray ) {
for( idx = 0; idx < dkarray->ndat; idx++ ) {
dkdata = dkarray->sdata[ idx ];
dkdata->hdr = NULL;
}
/* Free the smfArray holding the dark squid data, but do not free the
individual smfDatas within it. */
dkarray->owndata = 0;
smf_close_related( &dkarray, status );
}
}
/* Now clean the bolometer data */
smf_clean_smfArray( wf, concat, NULL, NULL, NULL, config, status );
/* If required correct for the POL2 triggering issue. */
if( fix ) smf_fix_pol2( wf, concat, status );
/* Loop round each sub-array in the current contiguous chunk of data. */
for( idx = 0; idx < concat->ndat && *status == SAI__OK; idx++ ) {
data = concat->sdata[ idx ];
/* Find the name of the subarray that generated the data. */
smf_find_subarray( data->hdr, subarray, sizeof(subarray), NULL,
status );
/* Display the sub-array. */
if( concat->ndat > 1 ) {
msgOutiff( MSG__VERB, "", " Doing sub-array %s.",
status, subarray );
}
/* Create an empty provenance structure. Each input NDF that contributes
to the current chunk and array will be added as an ancestor to this
structure, which will later be stored in each output NDF created for
this chunk and array. */
oprov = ndgReadProv( NDF__NOID, "SMURF:CALCQU", status );
/* Indicate we do not yet have any FITS headers for the output NDFs */
fc = NULL;
/* Indicate we do not yet know the coordinate reference frame for the
half-waveplate angle. */
polcrd[ 0 ] = 0;
ipolcrd = 0;
/* Go through the smfGroup looking for groups of related input NDFs that
contribute to the current chunk. */
for( igroup = 0; igroup < sgroup->ngroups; igroup++ ) {
if( sgroup->chunk[ igroup ] == ichunk ) {
/* Get the integer index into the GRP group (sgrp) that holds the input NDFs.
This index identifies the input NDF that provides the data for the current
chunk and subarray. This assumes that the order in which smf_concat_smfGroup
stores arrays in the "concat" smfArray matches the order in which
smf_grp_related stores arrays within the sgroup->subgroups. */
inidx = sgroup->subgroups[ igroup ][ idx ];
/* Add this input NDF as an ancestor into the output provenance structure. */
smf_accumulate_prov( NULL, sgrp, inidx, NDF__NOID,
"SMURF:CALCQU", &oprov, status );
/* Merge the FITS headers from the current input NDF into the FitsChan
that holds headers for the output NDFs. The merging retains only those
headers which have the same value in all input NDFs. */
smf_fits_outhdr( data->hdr->fitshdr, &fc, status );
/* Get the polarimetry related FITS headers and check that all input NDFs
have usabie values. */
headval[ 0 ] = 0;
smf_getfitss( data->hdr, "POL_MODE", headval,
sizeof(headval), status );
if( strcmp( headval, "CONSTANT" ) && *status == SAI__OK ) {
*status = SAI__ERROR;
grpMsg( "N", sgrp, inidx );
errRep( " ", "Input NDF ^N does not contain "
"polarimetry data obtained with a spinning "
"half-waveplate.", status );
}
headval[ 0 ] = 0;
smf_getfitss( data->hdr, "POLWAVIN", headval,
sizeof(headval), status );
if( strcmp( headval, "Y" ) && *status == SAI__OK ) {
*status = SAI__ERROR;
grpMsg( "N", sgrp, inidx );
errRep( " ", "Half-waveplate was not in the beam for "
"input NDF ^N.", status );
}
headval[ 0 ] = 0;
smf_getfitss( data->hdr, "POLANLIN", headval,
sizeof(headval), status );
if( strcmp( headval, "Y" ) && *status == SAI__OK ) {
*status = SAI__ERROR;
grpMsg( "N", sgrp, inidx );
errRep( " ", "Analyser was not in the beam for input "
"NDF ^N.", status );
}
if( polcrd[ 0 ] ) {
headval[ 0 ] = 0;
smf_getfitss( data->hdr, "POL_CRD", headval,
sizeof(headval), status );
if( strcmp( headval, polcrd ) && *status == SAI__OK ) {
*status = SAI__ERROR;
errRep( " ", "Input NDFs have differing values for "
"FITS header 'POL_CRD'.", status );
}
} else {
smf_getfitss( data->hdr, "POL_CRD", polcrd,
sizeof(polcrd), status );
if( !strcmp( polcrd, "FPLANE" ) ) {
ipolcrd = 0;
} else if( !strcmp( polcrd, "AZEL" ) ) {
ipolcrd = 1;
} else if( !strcmp( polcrd, "TRACKING" ) ) {
ipolcrd = 2;
} else if( *status == SAI__OK ) {
*status = SAI__ERROR;
msgSetc( "N", data->file->name );
msgSetc( "V", polcrd );
errRep( " ", "Input NDF ^N contains unknown value "
"'^V' for FITS header 'POL_CRD'.", status );
}
}
}
}
/* If not already done, get the maximum spatial drift (in arc-seconds) that
can be tolerated whilst creating a single I/Q/U image. The default value is
half the makemap default pixel size. Also get limits on the number of
time slices in any block. */
if( arcerror == 0.0 ) {
parDef0d( "ARCERROR", 0.5*smf_calc_telres( data->hdr->fitshdr,
status ), status );
parGet0r( "ARCERROR", &arcerror, status );
parGet0i( "MAXSIZE", &maxsize, status );
parGet0i( "MINSIZE", &minsize, status );
if( maxsize > 0 && maxsize < minsize && *status == SAI__OK ) {
*status = SAI__ERROR;
errRepf( "", "Value of parameter MAXSIZE (%d) is less "
"than value of parameter MINSIZE (%d)", status,
maxsize, minsize );
}
}
/* The algorithm that calculates I, Q and U assumes that all samples for a
single bolometer measure flux from the same point on the sky. Due to
sky rotation, this will not be the case - each bolometer will drift
slowly across the sky. However, since the drift is (or should be)
slow we can apply the I/Q/U algorithm to blocks of contiguous data over
which the bolometers do not move significantly. We produce a separate
I, Q and U image for each such block. The first block starts at the first
time slice in the smfData. */
block_start = 0;
/* Find the time slice at which the corner bolometers have moved
a critical distance (given by parameter ARCERROR) from their
positions at the start of the block. Then back off some time slices
to ensure that the block holds an integral number of half-waveplate
rotations. */
block_end = smf_block_end( data, block_start, ipolcrd, arcerror,
maxsize, status );
/* Loop round creating I/Q/U images for each block. Count them. */
iblock = 0;
while( block_end >= 0 && *status == SAI__OK ) {
/* Skip very short blocks. */
if( block_end - block_start > minsize ) {
/* Display the start and end of the block. */
msgOutiff( MSG__VERB, "", " Doing time slice block %d "
"-> %d", status, (int) block_start,
(int) block_end );
/* Get the name for the Q NDF for this block. Start of with "Q" followed by
the block index. */
iblock++;
nc = sprintf( ndfname, "Q%d", iblock );
/* Append the subarray name to the NDF name. */
nc += sprintf( ndfname + nc, "_%s", subarray );
/* Append the chunk index to the NDF name. */
nc += sprintf( ndfname + nc, "_%d", (int) ichunk );
/* Get NDF placeholder for the Q NDF. The NDFs are created inside the
output container file. */
ndfPlace( locq, ndfname, &qplace, status );
/* The name of the U NDF is the same except the initial "Q" is changed to
"U". */
ndfname[ 0 ] = 'U';
ndfPlace( locu, ndfname, &uplace, status );
/* The name of the I NDF is the same except the initial "Q" is changed to
"I". */
if( loci ) {
ndfname[ 0 ] = 'I';
ndfPlace( loci, ndfname, &iplace, status );
} else {
iplace = NDF__NOPL;
}
/* Store the chunk and block numbers as FITS headers. */
atlPtfti( fc, "POLCHUNK", (int) ichunk, "Chunk index used by CALCQU", status );
atlPtfti( fc, "POLBLOCK", iblock, "Block index used by CALCQU", status );
/* Create the Q and U images for the current block of time slices from
the subarray given by "idx", storing them in the output container
file. */
smf_calc_iqu( wf, data, block_start, block_end, ipolcrd,
qplace, uplace, iplace, oprov, fc,
pasign, AST__DD2R*paoff, AST__DD2R*angrot,
submean, status );
/* Warn about short blocks. */
} else {
msgOutiff( MSG__VERB, "", " Skipping short block of %d "
"time slices (parameter MINSIZE=%d).", status,
block_end - block_start - 1, minsize );
}
/* The next block starts at the first time slice following the previous
block. */
block_start = block_end + 1;
/* Find the time slice at which the corner bolometers have moved
a critical distance (given by parameter ARCERROR) from their
positions at the start of the block. Then back off some time slices
to ensure that the block holds an integral number of half-waveplate
rotations. This returns -1 if all time slices have been used. */
block_end = smf_block_end( data, block_start, ipolcrd,
arcerror, maxsize, status );
}
/* Free resources */
oprov = ndgFreeProv( oprov, status );
fc = astAnnul( fc );
}
config = astAnnul( config );
/* Close the smfArray. */
smf_close_related( &concat, status );
}
/* Annul the locators for the output container files. */
datAnnul( &locq, status );
datAnnul( &locu, status );
if( loci ) datAnnul( &loci, status );
/* The parameter system hangs onto a primary locator for each container
file, so cancel the parameters to annul these locators. */
datCancl( "OUTQ", status );
datCancl( "OUTU", status );
datCancl( "OUTI", status );
}
/* Free resources. */
smf_close_related( &darks, status );
smf_close_related( &flatramps, status );
if( igrp ) grpDelet( &igrp, status);
if( sgrp ) grpDelet( &sgrp, status);
if( bgrp ) grpDelet( &bgrp, status );
if( ogrp ) grpDelet( &ogrp, status );
if( sgroup ) smf_close_smfGroup( &sgroup, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
/* End the NDF and AST contexts. */
ndfEnd( status );
astEnd;
/* Issue a status indication.*/
if( *status == SAI__OK ) {
msgOutif( MSG__VERB, " ", "CALCQU succeeded.", status);
} else {
msgOutif( MSG__VERB, " ", "CALCQU failed.", status);
}
}
void smurf_sc2clean( int *status ) {
smfArray *array = NULL; /* Data to be cleaned */
Grp *basegrp=NULL; /* Grp containing first file each chunk */
size_t basesize; /* Number of files in base group */
smfArray *bbms = NULL; /* Bad bolometer masks */
smfArray *concat=NULL; /* Pointer to a smfArray */
size_t contchunk; /* Continuous chunk counter */
smfArray *darks = NULL; /* Dark data */
int ensureflat; /* Flag for flatfielding data */
smfArray *flatramps = NULL;/* Flatfield ramps */
AstKeyMap *heateffmap = NULL; /* Heater efficiency data */
smfData *odata = NULL; /* Pointer to output data struct */
Grp *fgrp = NULL; /* Filtered group, no darks */
size_t gcount=0; /* Grp index counter */
size_t idx; /* Subarray counter */
Grp *igrp = NULL; /* Input group of files */
smfGroup *igroup=NULL; /* smfGroup corresponding to igrp */
dim_t maxconcat=0; /* Longest continuous chunk length in samples */
double maxlen=0; /* Constrain maxconcat to this many seconds */
size_t ncontchunks=0; /* Number continuous chunks outside iter loop */
Grp *ogrp = NULL; /* Output group of files */
size_t osize; /* Total number of NDF names in the output group */
dim_t padStart=0; /* How many samples padding at start */
dim_t padEnd=0; /* How many samples padding at end */
size_t size; /* Number of files in input group */
int temp; /* Temporary signed integer */
int usedarks; /* flag for using darks */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
int writecom; /* Write COMmon mode to NDF if calculated? */
int writegai; /* Write GAIns to NDF if calculated? */
/* 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 );
/* Read the input file */
kpg1Rgndf( "IN", 0, 1, "", &igrp, &size, status );
/* Filter out darks */
smf_find_science( wf, 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;
if (size == 0) {
msgOutif(MSG__NORM, " ","All supplied input frames were filtered,"
" nothing to do", status );
goto CLEANUP;
}
/* --- Parse ADAM parameters ---------------------------------------------- */
/* Maximum length of a continuous chunk */
parGdr0d( "MAXLEN", 0, 0, VAL__MAXD, 1, &maxlen, status );
/* Padding */
parGdr0i( "PADSTART", 0, 0, VAL__MAXI, 1, &temp, status );
padStart = (dim_t) temp;
parGdr0i( "PADEND", 0, 0, VAL__MAXI, 1, &temp, status );
padEnd = (dim_t) temp;
/* Are we using darks? */
parGet0l( "USEDARKS", &usedarks, status );
/* Are we flatfielding? */
parGet0l( "FLAT", &ensureflat, status );
/* Write COM/GAI to NDFs if calculated? */
parGet0l( "COM", &writecom, status );
parGet0l( "GAI", &writegai, status );
/* Get group of bolometer masks and read them into a smfArray */
smf_request_mask( wf, "BBM", &bbms, status );
/* Group the input files by subarray and continuity ----------------------- */
smf_grp_related( igrp, size, 1, 0, maxlen-padStart-padEnd, NULL, NULL,
&maxconcat, NULL, &igroup, &basegrp, NULL, status );
/* Obtain the number of continuous chunks and subarrays */
if( *status == SAI__OK ) {
ncontchunks = igroup->chunk[igroup->ngroups-1]+1;
}
basesize = grpGrpsz( basegrp, status );
/* Get output file(s) */
kpg1Wgndf( "OUT", basegrp, basesize, basesize,
"More output files required...",
&ogrp, &osize, status );
/* Loop over continuous chunks and clean -----------------------------------*/
gcount = 1;
for( contchunk=0;(*status==SAI__OK)&&contchunk<ncontchunks; contchunk++ ) {
AstKeyMap *keymap=NULL;
int dkclean;
AstKeyMap *sub_instruments=NULL;
/* Place cleaning parameters into a keymap and set defaults. Do
this inside the loop in case we are cleaning files with
differing sub-instruments. Note that we use the map-maker
defaults file here (which loads the sc2clean defaults) so that
we populate the locked keymap with all the parameters that
people may come across to allow them to load their map-maker
config directly into sc2clean.
*/
sub_instruments = smf_subinst_keymap( SMF__SUBINST_NONE,
NULL, igrp,
igroup->subgroups[contchunk][0],
status );
keymap = kpg1Config( "CONFIG", "$SMURF_DIR/smurf_makemap.def",
sub_instruments, 1, status );
if( sub_instruments ) sub_instruments = astAnnul( sub_instruments );
/* Now rerun smf_grp_related to figure out how long each downsampled
chunk of data will be. */
if( basegrp ) grpDelet( &basegrp, status );
if( igroup ) smf_close_smfGroup( &igroup, status );
smf_grp_related( igrp, size, 1, 0, maxlen-padStart-padEnd, NULL, keymap,
&maxconcat, NULL, &igroup, &basegrp, NULL, status );
/* Concatenate this continuous chunk */
smf_concat_smfGroup( wf, NULL, igroup, usedarks ? darks:NULL, bbms, flatramps,
heateffmap, contchunk, ensureflat, 1, NULL, 0, NULL,
NULL, NO_FTS, padStart, padEnd, 0, &concat, NULL, status );
if( *status == SAI__OK) {
/* clean the dark squids now since we might need to use them
to clean the bolometer data */
smf_get_cleanpar( keymap, NULL, NULL, NULL, NULL, NULL, NULL, NULL, NULL,
&dkclean, NULL, NULL, NULL, NULL, NULL, NULL, NULL,
NULL, NULL, NULL, NULL, NULL, NULL, NULL, NULL, NULL,
NULL, NULL, NULL, NULL, NULL, NULL, NULL, NULL, NULL,
NULL, NULL, NULL, status );
for( idx=0; dkclean&&(*status==SAI__OK)&&idx<concat->ndat; idx++ ) {
odata = concat->sdata[idx];
if( odata && odata->da && odata->da->dksquid ) {
smfData *dksquid = odata->da->dksquid;
AstKeyMap *kmap=NULL;
msgOut("", TASK_NAME ": cleaning dark squids", status);
/* fudge the header so that we can get at JCMTState */
dksquid->hdr = odata->hdr;
/* clean darks using cleandk.* parameters */
astMapGet0A( keymap, "CLEANDK", &kmap );
array = smf_create_smfArray( status );
smf_addto_smfArray( array, dksquid, status );
smf_clean_smfArray( wf, array, NULL, NULL, NULL, kmap, status );
if( array ) {
array->owndata = 0;
smf_close_related( wf, &array, status );
}
if( kmap ) kmap = astAnnul( kmap );
/* Unset hdr pointer so that we don't accidentally close it */
dksquid->hdr = NULL;
}
}
/* Then the main data arrays */
if( *status == SAI__OK ) {
smfArray *com = NULL;
smfArray *gai = NULL;
char filename[GRP__SZNAM+1];
msgOut("", TASK_NAME ": cleaning bolometer data", status );
smf_clean_smfArray( wf, concat, NULL, &com, &gai, keymap, status );
/* If ADAM parameters for COM or GAI were specified, and the
common-mode was calculated, export to files here */
if( writecom && com ) {
for( idx=0; (*status==SAI__OK)&&(idx<com->ndat); idx++ ) {
smf_model_createHdr( com->sdata[idx], SMF__COM, concat->sdata[idx],
status );
smf_stripsuffix( com->sdata[idx]->file->name,
SMF__DIMM_SUFFIX, filename, status );
smf_dataOrder( wf, com->sdata[idx], 1, status );
smf_write_smfData( wf, com->sdata[idx], NULL, filename, NULL, 0,
NDF__NOID, MSG__NORM, 0, NULL, NULL, status );
}
}
if( writegai && gai ) {
for( idx=0; (*status==SAI__OK)&&(idx<gai->ndat); idx++ ) {
smf_model_createHdr( gai->sdata[idx], SMF__GAI, concat->sdata[idx],
status );
smf_stripsuffix( gai->sdata[idx]->file->name,
SMF__DIMM_SUFFIX, filename, status );
smf_dataOrder( wf, gai->sdata[idx], 1, status );
smf_write_smfData( wf, gai->sdata[idx], NULL, filename, NULL, 0,
NDF__NOID, MSG__NORM, 0, NULL, NULL, status );
}
}
/* Close com and gai */
if( com ) smf_close_related( wf, &com, status );
if( gai ) smf_close_related( wf, &gai, status );
}
/* Report statistics (currently need a smfArray for that) */
if (*status == SAI__OK) {
size_t last_qcount[SMF__NQBITS];
size_t last_nmap = 0;
smf_qualstats_report( wf, MSG__VERB, SMF__QFAM_TSERIES, 1, concat,
last_qcount, &last_nmap, 1, NULL, NULL, status );
}
/* Clean up for contchunk loop */
if( keymap ) keymap = astAnnul( keymap );
}
/* Export concatenated/cleaned data for each subarray to NDF file */
for( idx=0; (*status==SAI__OK)&&idx<concat->ndat; idx++ ) {
odata = concat->sdata[idx];
/* Complete the history information in the output NDF so that it
includes group parameters accessed since the default history
information was written to the NDF (in smf_open_and_flatfield). */
smf_puthistory( odata, "SMURF:SC2CLEAN", status );
/* Ensure ICD data order */
smf_dataOrder( wf, odata, 1, status );
if( odata->file && odata->file->name ) {
smf_write_smfData( wf, odata, NULL, NULL, ogrp, gcount, NDF__NOID,
MSG__VERB, 0, NULL, NULL, status );
} else {
*status = SAI__ERROR;
errRep( FUNC_NAME,
"Unable to determine file name for concatenated data.",
status );
}
/* Increment the group index counter */
gcount++;
}
/* Close the smfArray */
smf_close_related( wf, &concat, status );
}
/* Write out the list of output NDF names, annulling the error if a null
parameter value is supplied. */
if( *status == SAI__OK && ogrp ) {
grpList( "OUTFILES", 0, 0, NULL, ogrp, status );
if( *status == PAR__NULL ) errAnnul( status );
}
CLEANUP:
/* Tidy up after ourselves: release the resources used by the grp routines */
if( darks ) smf_close_related( wf, &darks, status );
if( flatramps ) smf_close_related( wf, &flatramps, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
if( bbms ) smf_close_related( wf, &bbms, status );
if( igrp ) grpDelet( &igrp, status);
if( ogrp ) grpDelet( &ogrp, status);
if( basegrp ) grpDelet( &basegrp, status );
if( igroup ) smf_close_smfGroup( &igroup, status );
fftw_cleanup();
ndfEnd( status );
}
void smurf_extinction( int * status ) {
/* Local Variables */
smfArray *bbms = NULL; /* Bad bolometer masks */
smfArray *darks = NULL; /* Dark data */
AstKeyMap *extpars = NULL; /* Tau relation keymap */
Grp *fgrp = NULL; /* Filtered group, no darks */
smfArray *flatramps = NULL;/* Flatfield ramps */
int has_been_sky_removed = 0;/* Data are sky-removed */
AstKeyMap *heateffmap = NULL; /* Heater efficiency data */
size_t i; /* Loop counter */
Grp *igrp = NULL; /* Input group */
AstKeyMap *keymap=NULL; /* Keymap for storing parameters */
smf_tausrc tausrc; /* enum value of optical depth source */
smf_extmeth extmeth; /* Extinction correction method */
char tausource[LEN__METHOD]; /* String for optical depth source */
char method[LEN__METHOD]; /* String for extinction airmass method */
smfData *odata = NULL; /* Output data struct */
Grp *ogrp = NULL; /* Output group */
size_t outsize; /* Total number of NDF names in the output group */
size_t size; /* Number of files in input group */
double tau = 0.0; /* Zenith tau at this wavelength */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
if (*status != SAI__OK) return;
/* 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 );
/* Read the input file */
kpg1Rgndf( "IN", 0, 1, "", &igrp, &size, status );
/* Filter out darks */
smf_find_science( igrp, &fgrp, 0, 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;
if (size > 0) {
/* Get output file(s) */
kpg1Wgndf( "OUT", igrp, size, size, "More output files required...",
&ogrp, &outsize, status );
} else {
msgOutif(MSG__NORM, " ","All supplied input frames were DARK,"
" nothing to extinction correct", status );
}
/* Get group of pixel masks and read them into a smfArray */
smf_request_mask( "BBM", &bbms, status );
/* Read the tau relations from config file or group. We do not
allow sub instrument overloading because these are all values
based on filter name. */
keymap = kpg1Config( "TAUREL", "$SMURF_DIR/smurf_extinction.def", NULL,
1, status );
/* and we need to use the EXT entry */
astMapGet0A( keymap, "EXT", &extpars );
keymap = astAnnul( keymap );
/* Get tau source */
parChoic( "TAUSRC", "Auto",
"Auto,CSOtau,CSOFit, Filtertau, WVMraw", 1,
tausource, sizeof(tausource), status);
/* Decide how the correction is to be applied - convert to flag */
parChoic( "METHOD", "ADAPTIVE",
"Adaptive,Quick,Full,", 1, method, sizeof(method), status);
/* Place parameters into a keymap and extract values */
if( *status == SAI__OK ) {
keymap = astKeyMap( " " );
if( astOK ) {
astMapPut0C( keymap, "TAUSRC", tausource, NULL );
astMapPut0C( keymap, "TAUMETHOD", method, NULL );
smf_get_extpar( keymap, &tausrc, &extmeth, NULL, status );
}
}
for (i=1; i<=size && ( *status == SAI__OK ); i++) {
/* Flatfield - if necessary */
smf_open_and_flatfield( igrp, ogrp, i, darks, flatramps, heateffmap,
&odata, status );
if (*status != SAI__OK) {
/* Error flatfielding: tell the user which file it was */
msgSeti("I",i);
errRep(TASK_NAME, "Unable to open the ^I th file", status);
}
/* Mask out bad pixels - mask data array not quality array */
smf_apply_mask( odata, bbms, SMF__BBM_DATA, 0, status );
/* Now check that the data are sky-subtracted */
if ( !smf_history_check( odata, "smf_subtract_plane", status ) ) {
/* Should we override remsky check? */
parGet0l("HASSKYREM", &has_been_sky_removed, status);
if ( !has_been_sky_removed && *status == SAI__OK ) {
*status = SAI__ERROR;
msgSeti("I",i);
errRep("", "Input data from file ^I are not sky-subtracted", status);
}
}
/* If status is OK, make decisions on source keywords the first
time through. */
if ( *status == SAI__OK && i == 1 ) {
if (tausrc == SMF__TAUSRC_CSOTAU ||
tausrc == SMF__TAUSRC_AUTO ||
tausrc == SMF__TAUSRC_TAU) {
double deftau;
const char * param = NULL;
smfHead *ohdr = odata->hdr;
/* get default CSO tau -- this could be calculated from CSO fits */
deftau = smf_calc_meantau( ohdr, status );
/* Now ask for desired CSO tau */
if ( tausrc == SMF__TAUSRC_CSOTAU || tausrc == SMF__TAUSRC_AUTO) {
param = "CSOTAU";
} else if (tausrc == SMF__TAUSRC_TAU) {
param = "FILTERTAU";
deftau = smf_cso2filt_tau( ohdr, deftau, extpars, status );
}
parGdr0d( param, deftau, 0.0,1.0, 1, &tau, status );
} else if ( tausrc == SMF__TAUSRC_CSOFIT || tausrc == SMF__TAUSRC_WVMRAW ) {
/* Defer a message until after extinction correction */
} else {
*status = SAI__ERROR;
errRep("", "Unsupported opacity source. Possible programming error.",
status);
}
}
/* Apply extinction correction - note that a check is made to
determine whether the data have already been extinction
corrected */
smf_correct_extinction( wf, odata, &tausrc, extmeth, extpars, tau, NULL, NULL, status );
if ( tausrc == SMF__TAUSRC_WVMRAW ) {
msgOutif(MSG__VERB," ", "Used Raw WVM data for extinction correction", status);
} else if ( tausrc == SMF__TAUSRC_CSOFIT ) {
msgOutif(MSG__VERB," ", "Used fit to CSO data for extinction correction", status);
} else if ( tausrc == SMF__TAUSRC_CSOTAU ) {
msgOutif(MSG__VERB," ", "Used an explicit CSO tau value for extinction correction", status);
} else if ( tausrc == SMF__TAUSRC_TAU ) {
msgOutif(MSG__VERB," ", "Used an explicit filter tau value for extinction correction", status);
} else {
if (*status == SAI__OK) {
const char * taustr = smf_tausrc_str( tausrc, status );
*status = SAI__ERROR;
errRepf( "", "Unexpected opacity source used for extinction correction of %s."
" Possible programming error.", status, taustr );
}
}
/* Set character labels */
smf_set_clabels( "Extinction corrected",NULL, NULL, odata->hdr, status);
smf_write_clabels( odata, status );
/* Free resources for output data */
smf_close_file( &odata, status );
}
/* Write out the list of output NDF names, annulling the error if a null
parameter value is supplied. */
if( *status == SAI__OK && ogrp ) {
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 */
if (darks) smf_close_related( &darks, status );
if (bbms) smf_close_related( &bbms, status );
if( flatramps ) smf_close_related( &flatramps, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
grpDelet( &igrp, status);
grpDelet( &ogrp, status);
if( keymap ) keymap = astAnnul( keymap );
if (extpars) extpars = astAnnul( extpars );
ndfEnd( status );
}
void smurf_sc2concat( int *status ) {
/* Local Variables */
Grp *basegrp=NULL; /* Grp containing first file each chunk */
size_t basesize; /* Number of files in base group */
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 idx; /* Subarray counter */
int usedarks; /* flag for using darks */
Grp *igrp = NULL; /* Group of input files */
smfGroup *igroup=NULL; /* smfGroup corresponding to igrp */
size_t isize; /* Number of files in input group */
dim_t maxconcat=0; /* Longest continuous chunk length in samples */
double maxlen; /* Constrain maxconcat to this many seconds */
size_t ncontchunks=0; /* Number continuous chunks outside iter loop */
Grp *ogrp = NULL; /* Output files */
size_t osize; /* Number of files in input group */
dim_t padStart=0; /* How many samples padding at start */
dim_t padEnd=0; /* How many samples padding at end */
int temp; /* Temporary signed integer */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
if (*status != SAI__OK) return;
/* 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 );
/* Read the input file */
kpg1Rgndf( "IN", 0, 1, "", &igrp, &isize, 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 */
isize = grpGrpsz( fgrp, status );
grpDelet( &igrp, status);
igrp = fgrp;
fgrp = NULL;
if (isize == 0) {
msgOutif(MSG__NORM, " ","All supplied input frames were filtered,"
" nothing to do", status );
goto CLEANUP;
}
/* --- Parse ADAM parameters ------------------------ */
/* Maximum length of a continuous chunk */
parGdr0d( "MAXLEN", 0, 0, VAL__MAXD, 1, &maxlen, status );
/* Padding */
parGdr0i( "PADSTART", 0, 0, VAL__MAXI, 1, &temp, status );
padStart = (dim_t) temp;
parGdr0i( "PADEND", 0, 0, VAL__MAXI, 1, &temp, status );
padEnd = (dim_t) temp;
/* Are we using darks? */
parGet0l( "USEDARKS", &usedarks, status );
/* Are we flatfielding? */
parGet0l( "FLAT", &ensureflat, status );
/* Group the input files by subarray and continuity */
smf_grp_related( igrp, isize, 1, 0, maxlen-padStart-padEnd, NULL, NULL,
&maxconcat, NULL, &igroup, &basegrp, NULL, status );
/* Obtain the number of continuous chunks and subarrays */
if( *status == SAI__OK ) {
ncontchunks = igroup->chunk[igroup->ngroups-1]+1;
}
basesize = grpGrpsz( basegrp, status );
/* Get output file(s) */
kpg1Wgndf( "OUT", basegrp, basesize, basesize,
"More output files required...",
&ogrp, &osize, status );
/* Loop over continuous chunks */
gcount = 1;
for( contchunk=0;(*status==SAI__OK)&&contchunk<ncontchunks; contchunk++ ) {
/* Concatenate this continuous chunk */
smf_concat_smfGroup( wf, NULL, igroup, usedarks ? darks:NULL, NULL, flatramps,
heateffmap, contchunk, ensureflat, 1, NULL, 0, NULL, NULL,
NO_FTS, padStart, padEnd, 0, &concat, NULL, status );
/* Export concatenated data for each subarray to NDF file */
for( idx=0; (*status==SAI__OK)&&idx<concat->ndat; idx++ ) {
if( concat->sdata[idx]->file && concat->sdata[idx]->file->name ) {
smf_write_smfData( concat->sdata[idx], NULL, NULL, ogrp, gcount,
NDF__NOID, MSG__VERB, 0, status );
} else {
*status = SAI__ERROR;
errRep( FUNC_NAME,
"Unable to determine file name for concatenated data.",
status );
}
/* Increment the group index counter */
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 && ogrp ) {
grpList( "OUTFILES", 0, 0, NULL, ogrp, status );
if( *status == PAR__NULL ) errAnnul( status );
}
CLEANUP:
if( darks ) smf_close_related( &darks, status );
if( flatramps ) smf_close_related( &flatramps, status );
if (heateffmap) heateffmap = smf_free_effmap( heateffmap, status );
if( igrp ) grpDelet( &igrp, status);
if( basegrp ) grpDelet( &basegrp, status );
if( ogrp ) grpDelet( &ogrp, status );
if( igroup ) smf_close_smfGroup( &igroup, status );
ndfEnd( status );
if( *status == SAI__OK ) {
msgOutif(MSG__VERB," ","SC2CONCAT succeeded.", status);
} else {
msgOutif(MSG__VERB," ","SC2CONCAT failed.", status);
}
}
/* Main entry */
void smurf_fixsteps( int *status ) {
/* Local Variables */
AstKeyMap *keymap; /* Default config parameter values */
AstKeyMap *sub_instruments; /* Info about sub-instruments */
FILE *fd = NULL; /* File descriptor */
Grp *igrp = NULL; /* Input group of files */
Grp *ogrp = NULL; /* Output group of files */
dim_t dcfitbox; /* DCFITBOX config parameter */
dim_t dcsmooth; /* DCSMOOTH config parameter */
dim_t nx; /* Length of first pixel axis */
double dcthresh; /* DCTHRESH config parameter */
double sizetol; /* Tolerance allowed on step height */
int changed; /* Have any step fixes changed? */
int dclimcorr; /* DCLIMCORR config parameter */
int dcmaxsteps; /* DCMAXSTEPS config parameter */
int first; /* Index of first change to report */
int itemp; /* Intermediate value */
int meanshift; /* Use a mean shift filter? */
int nnew; /* Number of new step fixes */
int nold; /* Number of old step fixes */
size_t nrej; /* Number of rejected bolometers */
size_t outsize; /* Total number of NDF names in the output group */
size_t size; /* Number of files in input group */
smfData *data = NULL; /* Output smfData */
smfData *indata = NULL; /* Input smfData */
smfStepFix *newsteps = NULL; /* New step fix descriptions */
smfStepFix *oldsteps = NULL; /* Old step fix descriptions */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
/* Check inherited status */
if (*status != SAI__OK) return;
/* begin an NDF context. */
ndfBegin();
/* Get the name of the input NDF. */
kpg1Rgndf( "IN", 1, 1, "", &igrp, &size, status );
/* Get output file(s) */
kpg1Wgndf( "OUT", igrp, size, 0, "More output files required...",
&ogrp, &outsize, status );
/* Open the input data file, read-only. */
smf_open_file( igrp, 1, "Read", 0, &indata, status );
/* Since we will be modifying the data values, we need a deep copy. */
data = smf_deepcopy_smfData( indata, 0, 0, 0, 0, status );
/* Place cleaning parameters into a keymap and set defaults. Note that we
use the map-maker defaults file here so that we populate the locked
keymap with all the parameters that people may come across to allow
them to load their map-maker config directly this application. */
sub_instruments = smf_subinst_keymap( SMF__SUBINST_NONE, data, NULL, 0,
status );
keymap = kpg1Config( "CONFIG", "$SMURF_DIR/smurf_makemap.def",
sub_instruments, status );
sub_instruments = astAnnul( sub_instruments );
/* Set the default for each of the step fixing config parameters. */
astMapGet0I( keymap, "DCSMOOTH", &itemp );
parDef0i( "DCSMOOTH", itemp, status );
astMapGet0I( keymap, "DCFITBOX", &itemp );
parDef0i( "DCFITBOX", itemp, status );
astMapGet0I( keymap, "DCMAXSTEPS", &itemp );
parDef0i( "DCMAXSTEPS", itemp, status );
astMapGet0I( keymap, "DCLIMCORR", &itemp );
parDef0i( "DCLIMCORR", itemp, status );
astMapGet0D( keymap, "DCTHRESH", &dcthresh );
parDef0d( "DCTHRESH", dcthresh, status );
/* Get values for the config params */
parGet0i( "DCSMOOTH", &itemp, status );
dcsmooth = itemp;
parGet0i( "DCFITBOX", &itemp, status );
dcfitbox = itemp;
parGet0i( "DCMAXSTEPS", &itemp, status );
dcmaxsteps = itemp;
parGet0i( "DCLIMCORR", &itemp, status );
dclimcorr = itemp;
parGet0d( "DCTHRESH", &dcthresh, status );
parGet0l( "MEANSHIFT", &meanshift, status );
/* Find the number of cores/processors available and create a pool of
threads of the same size. */
wf = thrGetWorkforce( thrGetNThread( SMF__THREADS, status ), status );
/* Fix the steps. */
smf_fix_steps( wf, data, dcthresh, dcsmooth, dcfitbox, dcmaxsteps,
dclimcorr, meanshift, &nrej, &newsteps, &nnew, status );
/* Display a summary of what was done by the step fixer. */
msgBlank( status );
if( nrej == 0 ) {
msgOut( "", "No bolometers were rejected", status );
} else if( nrej == 1 ) {
msgOut( "", "One bolometer was rejected", status );
} else {
msgSeti( "NREJ", nrej );
msgOut( "", "^NREJ bolometers were rejected", status );
}
parPut0i( "NREJECTED", nrej, status );
if( nnew == 0 ) {
msgOut( "", "No steps were fixed", status );
} else if( nnew == 1 ) {
msgOut( "", "One step was fixed", status );
} else {
msgSeti( "NNEW", nnew );
msgOut( "", "^NNEW steps were fixed", status );
}
parPut0i( "NFIXED", nnew, status );
/* If required, write out to a text file details of the steps that were
fixed. */
fd = smf_open_textfile( "NEWSTEPS", "w", "<none>", status );
if( fd ) {
smf1_write_steps( fd, indata, nnew, newsteps, dcthresh, dcsmooth,
dcfitbox, dcmaxsteps, dclimcorr, nrej, status );
fclose( fd );
}
/* If required, create the output NDF. */
if( outsize > 0 && indata && indata->file ) {
smf_write_smfData( data, NULL, NULL, ogrp, 1,
indata->file->ndfid, MSG__VERB, 0, status );
}
/* Save the length of the first pixel axis. */
nx = data ? data->dims[ 0 ] : 0;
/* Close the NDFs. */
smf_close_file( &data, status );
smf_close_file( &indata, status );
/* Attempt to open a file containing descriptions of steps fixed by a
previous invocation of this program. */
fd = smf_open_textfile( "OLDSTEPS", "r", "<none>", status );
if( fd ) {
/* Get SIZETOL - the minimum significant fractional error in step sizes. */
parGet0d( "SIZETOL", &sizetol, status );
/* Read the contents of the file, issuing a warning if the global
properties read from the file (e.g. parameters used, no. of steps
found, etc) differ from those of the current invocation. */
msgBlank( status );
oldsteps = smf1_read_steps( fd, dcthresh, dcsmooth,
dcfitbox, dcmaxsteps, dclimcorr,
nrej, nnew, &nold, status );
/* Get the index of the first change to report. */
parGet0i( "FIRST", &first, status );
/* Compare the new step fixes with the old step fixes, issuing a warning
for the first step fix that has changed. */
changed = smf1_check_steps( "CONTINUE", first, nx, sizetol,
nold, nnew, oldsteps, newsteps, status );
/* Store a flag indicating if any sstep fixes have chnaged. */
parPut0l( "CHANGED", changed, status );
/* Tell the user if nothing has changed. */
if( ! changed ) {
msgOut( "", "There are no significant differences "
"between old and new step fixes.", status );
}
msgBlank( status );
/* Close the old steps file, and free the memory holding the old step
descriptions. */
fclose( fd );
oldsteps = astFree( oldsteps );
}
/* Free resources. */
newsteps = astFree( newsteps );
grpDelet( &igrp, status );
grpDelet( &ogrp, status );
/* End the NDF context. */
ndfEnd( status );
/* If anything went wrong issue a context message. */
if( *status != SAI__OK ) msgOutif( MSG__VERB, " ", "FIXSTEPS failed.",
status );
}
void smurf_unmakemap( int *status ) {
/* Local Variables */
AstFrameSet *wcsin = NULL; /* WCS Frameset for input cube */
AstMapping *skymap; /* GRID->SkyFrame Mapping from input WCS */
AstSkyFrame *abskyfrm; /* Input SkyFrame (always absolute) */
AstSkyFrame *skyfrm = NULL;/* SkyFrame from the input WCS Frameset */
Grp *igrp1 = NULL; /* Group of input sky files */
Grp *igrp2 = NULL; /* Group of input template files */
Grp *igrpc = NULL; /* Group of input COM files */
Grp *igrpg = NULL; /* Group of input GAI files */
Grp *igrpq = NULL; /* Group of input Q sky files */
Grp *igrpu = NULL; /* Group of input U sky files */
Grp *ogrp = NULL; /* Group containing output file */
HDSLoc *cloc = NULL; /* HDS locator for component ipdata structure */
HDSLoc *iploc = NULL; /* HDS locator for top level ipdata structure */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
char ipdata[ 200 ]; /* Text buffer for IPDATA value */
char pabuf[ 10 ]; /* Text buffer for parameter value */
char subarray[ 5 ]; /* Name of SCUBA-2 subarray (s8a,s8b,etc) */
dim_t iel; /* Index of next element */
dim_t ndata; /* Number of elements in array */
dim_t ntslice; /* Number of time slices in array */
double *ang_data = NULL; /* Pointer to the FP orientation angles */
double *angc_data = NULL; /* Pointer to the instrumental ANGC data */
double *c0_data = NULL; /* Pointer to the instrumental C0 data */
double *gai_data = NULL; /* Pointer to the input GAI map */
double *in_data = NULL; /* Pointer to the input I sky map */
double *inc_data = NULL; /* Pointer to the input COM data */
double *inq_data = NULL; /* Pointer to the input Q sky map */
double *inu_data = NULL; /* Pointer to the input U sky map */
double *outq_data = NULL; /* Pointer to the Q time series data */
double *outu_data = NULL; /* Pointer to the U time series data */
double *p0_data = NULL; /* Pointer to the instrumental P0 data */
double *p1_data = NULL; /* Pointer to the instrumental P1 data */
double *pd; /* Pointer to next element */
double *pq = NULL; /* Pointer to next Q time series value */
double *pu = NULL; /* Pointer to next U time series value */
double *qinst_data = NULL; /* Pointer to the instrumental Q data */
double *uinst_data = NULL; /* Pointer to the instrumental U data */
double amp16; /* Amplitude of 16 Hz signal */
double amp2; /* Amplitude of 2 Hz signal */
double amp4; /* Amplitude of 4 Hz signal */
double angrot; /* Angle from focal plane X axis to fixed analyser */
double paoff; /* WPLATE value corresponding to POL_ANG=0.0 */
double params[ 4 ]; /* astResample parameters */
double phase16; /* Phase of 16 Hz signal */
double phase2; /* Phase of 2 Hz signal */
double phase4; /* Phase of 4 Hz signal */
double sigma; /* Standard deviation of noise to add to output */
int alignsys; /* Align data in the map's system? */
int cdims[ 3 ]; /* Common-mode NDF dimensions */
int dims[ NDF__MXDIM ]; /* NDF dimensions */
int flag; /* Was the group expression flagged? */
int gdims[ 3 ]; /* GAI model NDF dimensions */
int harmonic; /* The requested harmonic */
int ifile; /* Input file index */
int indf; /* Input sky map NDF identifier */
int indfangc; /* IP ANGC values NDF identifier */
int indfc0; /* IP C0 values NDF identifier */
int indfc; /* Input COM NDF identifier */
int indfcs; /* NDF identifier for matching section of COM */
int indfg; /* Input GAI NDF identifier */
int indfin; /* Input template cube NDF identifier */
int indfiq; /* Input instrumental Q NDF */
int indfiu; /* Input instrumental U NDF */
int indfout; /* Output cube NDF identifier */
int indfp0; /* IP P0 values NDF identifier */
int indfp1; /* IP P1 values NDF identifier */
int indfq; /* Input Q map NDF identifier */
int indfu; /* Input U map NDF identifier */
int interp = 0; /* Pixel interpolation method */
int lbndc[ 3 ]; /* Array of lower bounds of COM NDF */
int moving; /* Is the telescope base position changing? */
int ndim; /* Number of pixel axes in NDF */
int ndimc; /* Number of pixel axes in common-mode NDF */
int ndimg; /* Number of pixel axes in GAI NDF */
int nel; /* Number of elements in array */
int nelc; /* Number of elements in COM array */
int nelg; /* Number of elements in GAI array */
int nelqu; /* Number of elements in Q or U array */
int ngood; /* No. of good values in putput cube */
int nparam = 0; /* No. of parameters required for interpolation scheme */
int pasign; /* Indicates sense of POL_ANG value */
int sdim[ 2 ]; /* Array of significant pixel axes */
int slbnd[ 2 ]; /* Array of lower bounds of input map */
int subnd[ 2 ]; /* Array of upper bounds of input map */
int ubndc[ 3 ]; /* Array of upper bounds of COM NDF */
size_t ncom; /* Number of com files */
size_t ngai; /* Number of gai files */
size_t nskymap; /* Number of supplied sky cubes */
size_t outsize; /* Number of files in output group */
size_t size; /* Number of files in input group */
smfData *odata = NULL; /* Pointer to output data struct */
/* Check inherited status */
if( *status != SAI__OK ) return;
/* Begin an AST context */
astBegin;
/* Begin an NDF context. */
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 an identifier for the input NDF. We use NDG (via kpg1Rgndf)
instead of calling ndfAssoc directly since NDF/HDS has problems with
file names containing spaces, which NDG does not have. */
kpg1Rgndf( "IN", 1, 1, "", &igrp1, &nskymap, status );
ndgNdfas( igrp1, 1, "READ", &indf, status );
/* Map the data array in the input sky map. */
ndfMap( indf, "DATA", "_DOUBLE", "READ", (void **) &in_data, &nel,
status );
/* Get the WCS FrameSet from the sky map, together with its pixel index
bounds. */
kpg1Asget( indf, 2, 0, 1, 1, sdim, slbnd, subnd, &wcsin, status );
/* Check the current Frame is a SKY frame. */
skyfrm = astGetFrame( wcsin, AST__CURRENT );
if( !astIsASkyFrame( skyfrm ) && *status == SAI__OK ) {
ndfMsg( "N", indf );
*status = SAI__ERROR;
errRep( " ", " Current Frame in ^N is not a SKY Frame.", status );
}
/* Get a copy of the current frame that represents absolute coords rather
than offsets. We assume the target is moving if the map represents
offsets. */
moving = ( *status == SAI__OK &&
!strcmp( astGetC( skyfrm, "SkyRefIs" ), "Origin" ) ) ? 1 : 0;
abskyfrm = astCopy( skyfrm );
astClear( abskyfrm, "SkyRefIs" );
/* If the ALIGNSYS parameter is TRUE then we align the raw data with the
map in the current system of the map, rather than the default ICRS. */
parGet0l( "ALIGNSYS", &alignsys, status );
if( alignsys ) astSetC( abskyfrm, "AlignSystem", astGetC( abskyfrm,
"System" ) );
/* Get the Mapping from the Sky Frame to grid axis in the iput map. */
skymap = astGetMapping( wcsin, AST__CURRENT, AST__BASE );
/* Get the pixel interpolation scheme to use. */
parChoic( "INTERP", "NEAREST", "NEAREST,LINEAR,SINC,"
"SINCSINC,SINCCOS,SINCGAUSS,SOMB,SOMBCOS",
1, pabuf, 10, status );
if( !strcmp( pabuf, "NEAREST" ) ) {
interp = AST__NEAREST;
nparam = 0;
} else if( !strcmp( pabuf, "LINEAR" ) ) {
interp = AST__LINEAR;
nparam = 0;
} else if( !strcmp( pabuf, "SINC" ) ) {
interp = AST__SINC;
nparam = 1;
} else if( !strcmp( pabuf, "SINCSINC" ) ) {
interp = AST__SINCSINC;
nparam = 2;
} else if( !strcmp( pabuf, "SINCCOS" ) ) {
interp = AST__SINCCOS;
nparam = 2;
} else if( !strcmp( pabuf, "SINCGAUSS" ) ) {
interp = AST__SINCGAUSS;
nparam = 2;
} else if( !strcmp( pabuf, "SOMB" ) ) {
interp = AST__SOMB;
nparam = 1;
} else if( !strcmp( pabuf, "SOMBCOS" ) ) {
interp = AST__SOMBCOS;
nparam = 2;
} else if( *status == SAI__OK ) {
nparam = 0;
*status = SAI__ERROR;
msgSetc( "V", pabuf );
errRep( "", "Support not available for INTERP = ^V (programming "
"error)", status );
}
/* Get an additional parameter vector if required. */
if( nparam > 0 ) parExacd( "PARAMS", nparam, params, status );
/* Get a group of reference time series files to use as templates for
the output time series files.*/
ndgAssoc( "REF", 1, &igrp2, &size, &flag, status );
/* Get output file(s) */
kpg1Wgndf( "OUT", igrp2, size, size, "More output files required...",
&ogrp, &outsize, status );
/* Get he noise level to add to the output data. */
parGet0d( "SIGMA", &sigma, status );
/* Get any Q and U input maps. */
if( *status == SAI__OK ) {
kpg1Rgndf( "QIN", 1, 1, "", &igrpq, &nskymap, status );
ndgNdfas( igrpq, 1, "READ", &indfq, status );
ndfMap( indfq, "DATA", "_DOUBLE", "READ", (void **) &inq_data, &nelqu,
status );
if( nelqu != nel && *status == SAI__OK ) {
ndfMsg( "Q", indfq );
*status = SAI__ERROR;
errRep( "", "Q image '^Q' is not the same size as the I image.",
status );
}
kpg1Rgndf( "UIN", 1, 1, "", &igrpu, &nskymap, status );
ndgNdfas( igrpu, 1, "READ", &indfu, status );
ndfMap( indfu, "DATA", "_DOUBLE", "READ", (void **) &inu_data, &nelqu,
status );
if( nelqu != nel && *status == SAI__OK ) {
ndfMsg( "U", indfu );
*status = SAI__ERROR;
errRep( "", "U image '^U' is not the same size as the I image.",
status );
}
if( *status == PAR__NULL ) {
ndfAnnul( &indfq, status );
ndfAnnul( &indfu, status );
inq_data = NULL;
inu_data = NULL;
errAnnul( status );
} else {
parGet0d( "ANGROT", &angrot, status );
parGet0d( "PAOFF", &paoff, status );
parGet0l( "PASIGN", &pasign, status );
}
}
/* Get any common-mode files. */
if( *status == SAI__OK ) {
kpg1Rgndf( "COM", size, size, "", &igrpc, &ncom, status );
if( *status == PAR__NULL ) {
errAnnul( status );
ncom = 0;
}
}
/* Get any GAI files. */
if( *status == SAI__OK ) {
kpg1Rgndf( "GAI", size, size, "", &igrpg, &ngai, status );
if( *status == PAR__NULL ) {
errAnnul( status );
ngai = 0;
}
}
/* Get any instrumental polarisation files. */
if( *status == SAI__OK ) {
/* First see if the user wants to use the "INSTQ/INSTU" scheme for
specifying instrumental polarisation. */
ndfAssoc( "INSTQ", "Read", &indfiq, status );
ndfAssoc( "INSTU", "Read", &indfiu, status );
if( *status == PAR__NULL ) {
ndfAnnul( &indfiq, status );
ndfAnnul( &indfiu, status );
errAnnul( status );
} else {
msgOut( " ", "Using user-defined IP model", status );
ndfDim( indfiq, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfiq );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfiq, "DATA", "_DOUBLE", "READ", (void **) &qinst_data,
&nel, status );
}
ndfDim( indfiu, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfiu );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfiu, "DATA", "_DOUBLE", "READ", (void **) &uinst_data,
&nel, status );
}
}
/* If not, see if the user wants to use the Johnstone/Kennedy instrumental
polarisation model. The IPDATA parameter gives the path to an HDS
container file contining NDFs holding the required IP data for all
subarrays. */
if( !qinst_data ) {
parGet0c( "IPDATA", ipdata, sizeof(ipdata), status );
if( *status == PAR__NULL ) {
errAnnul( status );
} else {
msgOutf( " ", "Using Johnstone/Kennedy IP model in %s",
status, ipdata );
hdsOpen( ipdata, "READ", &iploc, status );
}
}
}
/* Loop round all the template time series files. */
for( ifile = 1; ifile <= (int) size && *status == SAI__OK; ifile++ ) {
/* Start a new NDF context. */
ndfBegin();
/* Create the output NDF by propagating everything from the input, except
for quality and variance. */
ndgNdfas( igrp2, ifile, "READ", &indfin, status );
ndfMsg( "FILE", indfin );
msgSeti( "THISFILE", ifile );
msgSeti( "NUMFILES", size );
msgOutif( MSG__NORM, " ", "Simulating ^THISFILE/^NUMFILES ^FILE",
status );
ndgNdfpr( indfin, "DATA,HISTORY,LABEL,TITLE,WCS,UNITS,EXTENSION(*)",
ogrp, ifile, &indfout, status );
ndfAnnul( &indfin, status );
ndfAnnul( &indfout, status );
/* We now re-open the output NDF and then modify its data values. */
smf_open_file( wf, ogrp, ifile, "UPDATE", 0, &odata, status );
/* Issue a suitable message and abort if anything went wrong. */
if( *status != SAI__OK ) {
errRep( FUNC_NAME, "Could not open input template file.", status );
break;
} else {
if( odata->file == NULL ) {
*status = SAI__ERROR;
errRep( FUNC_NAME, "No smfFile associated with smfData.",
status );
break;
} else if( odata->hdr == NULL ) {
*status = SAI__ERROR;
errRep( FUNC_NAME, "No smfHead associated with smfData.",
status );
break;
}
}
/* Check the reference time series contains double precision values. */
smf_dtype_check_fatal( odata, NULL, SMF__DOUBLE, status );
/* Get the total number of data elements, and the number of time slices. */
smf_get_dims( odata, NULL, NULL, NULL, &ntslice, &ndata, NULL,
NULL, status );
/* Get the subarray name */
smf_fits_getS( odata->hdr, "SUBARRAY", subarray, sizeof(subarray),
status );
/* If we are using the Johnstone/Kennedy IP model, open and map the
relevant parameter NDFs within the IPDATA container file. */
if( iploc ) {
datFind( iploc, subarray, &cloc, status );
ndfFind( cloc, "C0", &indfc0, status );
ndfDim( indfc0, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfc0 );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfc0, "DATA", "_DOUBLE", "READ", (void **) &c0_data,
&nel, status );
}
ndfFind( cloc, "P0", &indfp0, status );
ndfDim( indfp0, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfp0 );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfp0, "DATA", "_DOUBLE", "READ", (void **) &p0_data,
&nel, status );
}
ndfFind( cloc, "P1", &indfp1, status );
ndfDim( indfp1, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfp1 );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfp1, "DATA", "_DOUBLE", "READ", (void **) &p1_data,
&nel, status );
}
ndfFind( cloc, "ANGC", &indfangc, status );
ndfDim( indfangc, 2, dims, &ndim, status );
if( dims[ 0 ] != 32 || dims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "N", indfangc );
errRep( " ", "Instrumental polarisation file ^N has bad "
"dimensions - should be 32x40.", status );
} else {
ndfMap( indfangc, "DATA", "_DOUBLE", "READ", (void **) &angc_data,
&nel, status );
}
}
/* Open any COM file. */
if( ncom ) {
ndgNdfas( igrpc, ifile, "READ", &indfc, status );
ndfDim( indfc, 3, cdims, &ndimc, status );
/* Check its dimensions. */
if( *status == SAI__OK ) {
if( ndimc == 1 ) {
if( cdims[ 0 ] < (int) ntslice ) {
*status = SAI__ERROR;
ndfMsg( "C", indfc );
ndfMsg( "R", indfin );
msgSeti( "N", cdims[ 0 ] );
msgSeti( "M", ntslice );
errRep( " ", "Supplied COM file (^C) has ^N time-slices, but "
"the reference NDF (^R) has ^M time-slices.", status );
} else {
ndfBound( indfc, 3, lbndc, ubndc, &ndimc, status );
ubndc[ 0 ] = lbndc[ 0 ] + ntslice - 1;
ndfSect( indfc, 1, lbndc, ubndc, &indfcs, status );
}
} else if( ndimc == 3 ) {
if( cdims[ 0 ] != 1 || cdims[ 1 ] != 1 ) {
*status = SAI__ERROR;
ndfMsg( "C", indfc );
errRep( " ", "Supplied 3D COM file (^C) has bad "
"dimensions for axis 1 and/or 2 (should "
"both be 1 pixel long).", status );
} else if( cdims[ 2 ] < (int) ntslice ) {
*status = SAI__ERROR;
ndfMsg( "C", indfc );
ndfMsg( "R", indfin );
msgSeti( "N", cdims[ 2 ] );
msgSeti( "M", ntslice );
errRep( " ", "Supplied COM file (^C) has ^N time-slices, but "
"the reference NDF (^R) has ^M time-slices.", status );
} else {
ndfBound( indfc, 3, lbndc, ubndc, &ndimc, status );
ubndc[ 2 ] = lbndc[ 2 ] + ntslice - 1;
ndfSect( indfc, 3, lbndc, ubndc, &indfcs, status );
}
} else {
*status = SAI__ERROR;
ndfMsg( "C", indfc );
msgSeti( "N", ndimc );
errRep( " ", "Supplied COM file (^C) has ^N dimensions - "
"must be 3.", status );
}
}
ndfMap( indfcs, "DATA", "_DOUBLE", "READ", (void **) &inc_data,
&nelc, status );
} else {
indfcs = NDF__NOID;
inc_data = NULL;
}
/* Open any GAI files. */
if( ngai ) {
ndgNdfas( igrpg, ifile, "READ", &indfg, status );
ndfDim( indfg, 3, gdims, &ndimg, status );
/* Check its dimensions, and map it if OK. */
if( *status == SAI__OK ) {
if( ndimg != 2 ) {
*status = SAI__ERROR;
ndfMsg( "C", indfg );
msgSeti( "N", ndimg );
errRep( " ", "Supplied GAI file (^C) has ^N dimensions - "
"must be 2.", status );
} else if( gdims[ 0 ] != 32 || gdims[ 1 ] != 40 ) {
*status = SAI__ERROR;
ndfMsg( "C", indfg );
errRep( " ", "Supplied GAI file (^C) has has bad "
"dimensions - should be 32x40.", status );
}
}
ndfMap( indfg, "DATA", "_DOUBLE", "READ", (void **) &gai_data,
&nelg, status );
} else {
indfg = NDF__NOID;
gai_data = NULL;
}
/* Fill the output with bad values. */
if( *status == SAI__OK ) {
pd = odata->pntr[ 0 ];
for( iel = 0; iel < ndata; iel++ ) *(pd++) = VAL__BADD;
}
/* Resample the sky map data into the output time series. */
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, in_data, odata->pntr[ 0 ],
NULL, &ngood, status );
/* Add on any COM data. */
smf_addcom( wf, odata, inc_data, status );
/* Issue a wrning if there is no good data in the output cube. */
if( ngood == 0 ) msgOutif( MSG__NORM, " ", " Output contains no "
"good data values.", status );
/* If Q and U maps have been given, allocate room to hold resampled Q and
U values, and fill them with bad values. */
if( inq_data && inu_data ) {
pq = outq_data = astMalloc( ndata*sizeof( *outq_data ) );
pu = outu_data = astMalloc( ndata*sizeof( *outu_data ) );
if( *status == SAI__OK ) {
for( iel = 0; iel < ndata; iel++ ) {
*(pu++) = VAL__BADD;
*(pq++) = VAL__BADD;
}
}
/* Determine the harmonic to use. */
parGet0i( "HARMONIC", &harmonic, status );
/* If producing the normal 8 Hz harmonic, get the amplitude and phase of a
other signals to add onto the 8 Hz signal. */
if( harmonic == 4 ) {
parGet0d( "AMP2", &2, status );
parGet0d( "PHASE2", &phase2, status );
parGet0d( "AMP4", &4, status );
parGet0d( "PHASE4", &phase4, status );
parGet0d( "AMP16", &16, status );
parGet0d( "PHASE16", &phase16, status );
} else {
amp2 = 0.0;
phase2 = 0.0;
amp4 = 0.0;
phase4 = 0.0;
amp16 = 0.0;
phase16 = 0.0;
}
/* Allocate room for an array to hold the angle from the Y pixel axis
in the sky map to the focal plane Y axis, in radians, at each time
slice. Positive rotation is in the same sense as rotation from
focal plane X to focal plane Y. */
ang_data = astMalloc( ntslice*sizeof( *ang_data ) );
/* Resample them both into 3D time series. These Q/U values arw with
respect to the sky image Y axis. */
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, inq_data, outq_data,
ang_data, &ngood, status );
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, inu_data, outu_data,
NULL, &ngood, status );
/* Combine these time series with the main output time series so that the
main output is analysed intensity. */
smf_uncalc_iqu( wf, odata, odata->pntr[ 0 ], outq_data, outu_data,
ang_data, pasign, AST__DD2R*paoff, AST__DD2R*angrot,
amp2, AST__DD2R*phase2, amp4, AST__DD2R*phase4,
amp16, AST__DD2R*phase16, qinst_data, uinst_data,
c0_data, p0_data, p1_data, angc_data, harmonic,
status );
/* Release work space. */
outq_data = astFree( outq_data );
outu_data = astFree( outu_data );
ang_data = astFree( ang_data );
}
/* Factor in any GAI data. */
smf_addgai( wf, odata, gai_data, status );
/* Close the output time series file. */
smf_close_file( wf, &odata, status );
/* Close the IP data container for the current subarray, if it is open. */
if( cloc ) datAnnul( &cloc, status );
/* End the NDF context. */
ndfEnd( status );
}
/* Close any input data file that is still open due to an early exit from
the above loop. */
if( odata != NULL ) {
smf_close_file( wf, &odata, status );
odata = NULL;
}
/* Free remaining resources. */
if( igrp1 != NULL) grpDelet( &igrp1, status);
if( igrp2 != NULL) grpDelet( &igrp2, status);
if( igrpq != NULL) grpDelet( &igrpq, status);
if( igrpu != NULL) grpDelet( &igrpu, status);
if( igrpc != NULL) grpDelet( &igrpc, status);
if( igrpg != NULL) grpDelet( &igrpg, status);
if( ogrp != NULL) grpDelet( &ogrp, status);
if( iploc ) datAnnul( &iploc, status );
/* End the NDF context. */
ndfEnd( status );
/* End the tile's AST context. */
astEnd;
/* Issue a status indication.*/
if( *status == SAI__OK ) {
msgOutif(MSG__VERB," ",TASK_NAME " succeeded, time series written.", status);
} else {
msgOutif(MSG__VERB," ",TASK_NAME " failed.", status);
}
}
void smurf_sc2threadtest( int *status ) {
/* Local Variables */
smfArray **res=NULL; /* array of smfArrays of test data */
smfData *data=NULL; /* Pointer to SCUBA2 data struct */
dim_t datalen; /* Number of data points */
smfFilter *filt=NULL; /* Frequency domain filter */
size_t i; /* Loop counter */
size_t j; /* Loop counter */
smfTimeChunkData *job_data=NULL; /* Array of pointers for job data */
size_t joblen; /* Number of chunks per job */
size_t k; /* Loop counter */
size_t nchunks; /* Number of chunks */
size_t nsub; /* Number of subarrays */
int nthread; /* Number of threads */
smfTimeChunkData *pdata=NULL; /* Pointer to data for single job */
int temp; /* Temporary integer */
size_t tsteps; /* How many time steps in chunk */
struct timeval tv1, tv2; /* Timers */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
double *dat=NULL;
dim_t nbolo;
dim_t ntslice;
dim_t ndata;
size_t bstride;
size_t tstride;
dim_t offset;
if (*status != SAI__OK) return;
/* Get input parameters */
parGdr0i( "NTHREAD", 1, 1, NUM__MAXI, 1, &nthread, status );
parGdr0i( "TSTEPS", 6000, 0, NUM__MAXI, 1, &temp, status );
tsteps = (size_t) temp;
parGdr0i( "NCHUNKS", 1, 1, NUM__MAXI, 1, &temp, status );
nchunks = (size_t) temp;
parGdr0i( "NSUB", 1, 1, 4, 1, &temp, status );
nsub = (size_t) temp;
msgSeti("N",nthread);
msgOut( "", TASK_NAME ": Running test with ^N threads", status );
/*** TIMER ***/
smf_timerinit( &tv1, &tv2, status );
/* Create some fake test data in the form of an array of smfArrays */
msgSeti("T",tsteps);
msgSeti("C",nchunks);
msgSeti("NS",nsub);
msgOut( "", TASK_NAME
": Creating ^NS subarrays of data with ^C chunks * ^T samples",
status );
res = astCalloc( nchunks, sizeof(*res) );
for( k=0; (*status==SAI__OK)&&(k<nchunks); k++ ) {
res[k] = smf_create_smfArray( status );
for( i=0; (*status==SAI__OK)&&(i<nsub); i++ ) {
/* Create individual smfDatas and add to array */
data = smf_create_smfData( SMF__NOCREATE_FILE |
SMF__NOCREATE_DA |
SMF__NOCREATE_FTS, status );
if( *status==SAI__OK ) {
data->dtype=SMF__DOUBLE;
data->ndims=3;
data->dims[0]=40;
data->dims[1]=32;
data->dims[2]=(dim_t) tsteps;
datalen=1;
data->isFFT=-1;
for( j=0; j<data->ndims; j++ ) datalen *= data->dims[j];
data->hdr->steptime = 0.005;
data->pntr[0] = astCalloc( datalen, smf_dtype_sz(data->dtype,status) );
data->qual = astCalloc( datalen, sizeof(*data->qual) );
}
smf_addto_smfArray( res[k], data, status );
}
}
/*** TIMER ***/
msgOutf( "", "** %f seconds generating data", status,
smf_timerupdate(&tv1,&tv2,status) );
msgOut( "", TASK_NAME
": Starting test 1 __parallel time: dataOrder__", status );
/* Create a pool of threads. */
wf = thrGetWorkforce( nthread, status );
/* Work out number of chunks per thread */
joblen = nchunks/nthread;
if( joblen == 0 ) joblen = 1; /* At least one chunk per thread */
/* The first test will process separate time chunks of data in
parallel, re-ordering each to bolo-ordered format. All subarrays
and an integer number of input file chunks all go into a single
thread. Start by allocating and initializing a number of
smfTimeChunkData's that hold the information required for each
thread */
job_data = astCalloc( nthread, sizeof(*job_data) );
for( i=0; (i<(size_t)nthread) && (*status==SAI__OK); i++ ) {
pdata = job_data + i;
pdata->type = 0; /* Start with a data re-order */
pdata->data = res; /* Pointer to main data array */
pdata->chunk1 = i*joblen; /* Index of first chunk for job */
pdata->nchunks = nchunks; /* Total number of time chunks in data */
pdata->ijob = -1; /* Flag job as available to do work */
/* The last thread has to pick up the remainder of chunks */
if( i==(size_t)(nthread-1) ) pdata->chunk2=nchunks-1;
else pdata->chunk2 = (i+1)*joblen-1; /* Index of last chunk for job */
/* Ensure a valid chunk range, or set to a length that we know to ignore */
if( pdata->chunk1 >= nchunks ) {
pdata->chunk1 = nchunks;
pdata->chunk2 = nchunks;
} else if( pdata->chunk2 >= nchunks ) {
pdata->chunk2 = nchunks-1;
}
if( pdata->chunk1 >= nchunks ) {
/* Nothing for this thread to do */
msgSeti( "W", i+1);
msgOutif( MSG__DEBUG, "",
"-- parallel time: skipping thread ^W, nothing to do",
status);
} else {
/* Since we know there is one job_data per thread, just submit jobs
immediately */
pdata->ijob = thrAddJob( wf, THR__REPORT_JOB, pdata, smfParallelTime,
0, NULL, status );
}
}
/* Wait until all of the submitted jobs have completed */
thrWait( wf, status );
/* Annul the bad status that we set in smfParallelTime */
if( *status == SMF__INSMP ) {
errAnnul( status );
msgOut( "", " *** Annulled SMF__INSMP set in smfParallelTime *** ",
status );
} else {
msgOut( "", " *** Flushing good status *** ", status );
errFlush( status );
}
/*** TIMER ***/
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
/* The second test will boxcar smooth bolometers from time chunks in
parallel */
msgOut( "", TASK_NAME
": Starting test 2 __parallel time: boxcar smooth__", status );
for( i=0; (i<(size_t)nthread) && (*status==SAI__OK); i++ ) {
pdata = job_data + i;
pdata->type = 1; /* Boxcar smooth */
if( pdata->chunk1 >= nchunks ) {
/* Nothing for this thread to do */
msgSeti( "W", i+1);
msgOutif( MSG__DEBUG, "",
"-- parallel time: skipping thread ^W, nothing to do",
status);
} else {
/* Since we know there is one job_data per thread, just submit jobs
immediately */
pdata->ijob = thrAddJob( wf, THR__REPORT_JOB, pdata, smfParallelTime,
0, NULL, status );
}
}
/* Wait until all of the submitted jobs have completed */
thrWait( wf, status );
/*** TIMER ***/
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
msgOut( "", TASK_NAME
": *** Next 2 tests will be done twice due to FFTW planning *****",
status );
for( k=0; k<2; k++ ) {
/* The third test will FFT filter bolometers from time chunks in
parallel */
msgOut( "", TASK_NAME
": Starting test 3 __parallel time: FFT filter__", status );
for( i=0; (i<(size_t)nthread) && (*status==SAI__OK); i++ ) {
pdata = job_data + i;
pdata->type = 2; /* FFT filter */
if( pdata->chunk1 >= nchunks ) {
/* Nothing for this thread to do */
msgSeti( "W", i+1);
msgOutif( MSG__DEBUG, "",
"-- parallel time: skipping thread ^W, nothing to do",
status);
} else {
/* Since we know there is one job_data per thread, just submit jobs
immediately */
pdata->ijob = thrAddJob( wf, THR__REPORT_JOB, pdata, smfParallelTime,
0, NULL, status );
}
}
/* Wait until all of the submitted jobs have completed */
thrWait( wf, status );
/*** TIMER ***/
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
msgOut( "", TASK_NAME
": Starting test 4 __FFTW filter using internal threading__",
status );
for( i=0; (*status==SAI__OK)&&(i<nchunks); i++ ) {
filt = smf_create_smfFilter( res[i]->sdata[0], status );
smf_filter_ident( filt, 1, status );
for( j=0; (*status==SAI__OK)&&(j<nsub); j++ ) {
msgOutiff( MSG__DEBUG, "", " filter chunk %zu/%zu, bolo %zu/%zu",
status, i+1, nchunks, j+1, nsub );
smf_filter_execute( wf, res[i]->sdata[j], filt, 0, 0, status );
}
if( filt ) filt = smf_free_smfFilter( filt, status );
}
/*** TIMER ***/
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
}
msgOut( "", TASK_NAME
": **************************************************************",
status );
/* Series of short single-thread array index tests */
data = res[0]->sdata[0];
dat = data->pntr[0];
smf_get_dims( data, NULL, NULL, &nbolo, &ntslice, &ndata, &bstride,
&tstride, status );
msgOut("","Array index test #1: two multiplies in inner loop",status);
smf_timerinit( &tv1, &tv2, status );
for( i=0; i<nbolo; i++ ) {
for( j=0; j<ntslice; j++ ) {
dat[i*bstride + j*tstride] += 5;
}
}
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
msgOut("","Array index test #2: only index increments",status);
smf_timerinit( &tv1, &tv2, status );
for( i=0; i<nbolo*bstride; i+=bstride ) {
for( j=i; j<(i+ntslice*tstride); j+=tstride ) {
dat[j] += 5;
}
}
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
msgOut("","Array index test #3: one multiply in outer loop",status);
smf_timerinit( &tv1, &tv2, status );
offset = 0;
for( i=0; i<nbolo; i++ ) {
offset = i*bstride;
for( j=0; j<ntslice; j++ ) {
dat[offset] += 5;
offset += tstride;
}
}
msgOutf( "", "** %f seconds to complete test", status,
smf_timerupdate(&tv1,&tv2,status) );
/* Clean up */
if( res ) {
for( i=0; i<nchunks; i++ ) {
if( res[i] ) {
smf_close_related( &res[i], status );
}
}
res = astFree( res );
}
job_data = astFree( job_data );
/* Ensure that FFTW doesn't have any used memory kicking around */
fftw_cleanup();
}
void smurf_unmakemap( int *status ) {
/* Local Variables */
AstFrameSet *wcsin = NULL; /* WCS Frameset for input cube */
AstMapping *skymap; /* GRID->SkyFrame Mapping from input WCS */
AstSkyFrame *abskyfrm; /* Input SkyFrame (always absolute) */
AstSkyFrame *skyfrm = NULL;/* SkyFrame from the input WCS Frameset */
Grp *igrp1 = NULL; /* Group of input sky files */
Grp *igrp2 = NULL; /* Group of input template files */
Grp *igrpq = NULL; /* Group of input Q sky files */
Grp *igrpu = NULL; /* Group of input U sky files */
Grp *ogrp = NULL; /* Group containing output file */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
char pabuf[ 10 ]; /* Text buffer for parameter value */
dim_t iel; /* Index of next element */
dim_t ndata; /* Number of elements in array */
dim_t ntslice; /* Number of time slices in array */
double *ang_data = NULL; /* Pointer to the FP orientation angles */
double *in_data = NULL; /* Pointer to the input I sky map */
double *inq_data = NULL; /* Pointer to the input Q sky map */
double *inu_data = NULL; /* Pointer to the input U sky map */
double *outq_data = NULL; /* Pointer to the Q time series data */
double *outu_data = NULL; /* Pointer to the U time series data */
double *pd; /* Pointer to next element */
double *pq = NULL; /* Pointer to next Q time series value */
double *pu = NULL; /* Pointer to next U time series value */
double angrot; /* Angle from focal plane X axis to fixed analyser */
double paoff; /* WPLATE value corresponding to POL_ANG=0.0 */
double params[ 4 ]; /* astResample parameters */
double sigma; /* Standard deviation of noise to add to output */
int alignsys; /* Align data in the map's system? */
int flag; /* Was the group expression flagged? */
int harmonic; /* The requested harmonic */
int ifile; /* Input file index */
int indf; /* Input sky map NDF identifier */
int indfin; /* Input template cube NDF identifier */
int indfout; /* Output cube NDF identifier */
int indfq; /* Input Q map NDF identifier */
int indfu; /* Input U map NDF identifier */
int interp = 0; /* Pixel interpolation method */
int moving; /* Is the telescope base position changing? */
int nel; /* Number of elements in array */
int nelqu; /* Number of elements in Q or U array */
int ngood; /* No. of good values in putput cube */
int nparam = 0; /* No. of parameters required for interpolation scheme */
int pasign; /* Indicates sense of POL_ANG value */
int sdim[ 2 ]; /* Array of significant pixel axes */
int slbnd[ 2 ]; /* Array of lower bounds of input map */
int subnd[ 2 ]; /* Array of upper bounds of input map */
size_t nskymap; /* Number of supplied sky cubes */
size_t outsize; /* Number of files in output group */
size_t size; /* Number of files in input group */
smfData *odata = NULL; /* Pointer to output data struct */
/* Check inherited status */
if( *status != SAI__OK ) return;
/* Begin an AST context */
astBegin;
/* Begin an NDF context. */
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 an identifier for the input NDF. We use NDG (via kpg1Rgndf)
instead of calling ndfAssoc directly since NDF/HDS has problems with
file names containing spaces, which NDG does not have. */
kpg1Rgndf( "IN", 1, 1, "", &igrp1, &nskymap, status );
ndgNdfas( igrp1, 1, "READ", &indf, status );
/* Map the data array in the input sky map. */
ndfMap( indf, "DATA", "_DOUBLE", "READ", (void **) &in_data, &nel,
status );
/* Get the WCS FrameSet from the sky map, together with its pixel index
bounds. */
kpg1Asget( indf, 2, 0, 1, 1, sdim, slbnd, subnd, &wcsin, status );
/* Check the current Frame is a SKY frame. */
skyfrm = astGetFrame( wcsin, AST__CURRENT );
if( !astIsASkyFrame( skyfrm ) && *status == SAI__OK ) {
ndfMsg( "N", indf );
*status = SAI__ERROR;
errRep( " ", " Current Frame in ^N is not a SKY Frame.", status );
}
/* Get a copy of the current frame that represents absolute coords rather
than offsets. We assume the target is moving if the map represents
offsets. */
moving = ( *status == SAI__OK &&
!strcmp( astGetC( skyfrm, "SkyRefIs" ), "Origin" ) ) ? 1 : 0;
abskyfrm = astCopy( skyfrm );
astClear( abskyfrm, "SkyRefIs" );
/* If the ALIGNSYS parameter is TRUE then we align the raw data with the
map in the current system of the map, rather than the default ICRS. */
parGet0l( "ALIGNSYS", &alignsys, status );
if( alignsys ) astSetC( abskyfrm, "AlignSystem", astGetC( abskyfrm,
"System" ) );
/* Get the Mapping from the Sky Frame to grid axis in the iput map. */
skymap = astGetMapping( wcsin, AST__CURRENT, AST__BASE );
/* Get the pixel interpolation scheme to use. */
parChoic( "INTERP", "NEAREST", "NEAREST,LINEAR,SINC,"
"SINCSINC,SINCCOS,SINCGAUSS,SOMB,SOMBCOS",
1, pabuf, 10, status );
if( !strcmp( pabuf, "NEAREST" ) ) {
interp = AST__NEAREST;
nparam = 0;
} else if( !strcmp( pabuf, "LINEAR" ) ) {
interp = AST__LINEAR;
nparam = 0;
} else if( !strcmp( pabuf, "SINC" ) ) {
interp = AST__SINC;
nparam = 1;
} else if( !strcmp( pabuf, "SINCSINC" ) ) {
interp = AST__SINCSINC;
nparam = 2;
} else if( !strcmp( pabuf, "SINCCOS" ) ) {
interp = AST__SINCCOS;
nparam = 2;
} else if( !strcmp( pabuf, "SINCGAUSS" ) ) {
interp = AST__SINCGAUSS;
nparam = 2;
} else if( !strcmp( pabuf, "SOMB" ) ) {
interp = AST__SOMB;
nparam = 1;
} else if( !strcmp( pabuf, "SOMBCOS" ) ) {
interp = AST__SOMBCOS;
nparam = 2;
} else if( *status == SAI__OK ) {
nparam = 0;
*status = SAI__ERROR;
msgSetc( "V", pabuf );
errRep( "", "Support not available for INTERP = ^V (programming "
"error)", status );
}
/* Get an additional parameter vector if required. */
if( nparam > 0 ) parExacd( "PARAMS", nparam, params, status );
/* Get a group of reference time series files to use as templates for
the output time series files.*/
ndgAssoc( "REF", 1, &igrp2, &size, &flag, status );
/* Get output file(s) */
kpg1Wgndf( "OUT", igrp2, size, size, "More output files required...",
&ogrp, &outsize, status );
/* Get he noise level to add to the output data. */
parGet0d( "SIGMA", &sigma, status );
/* Get any Q and U input maps. */
if( *status == SAI__OK ) {
kpg1Rgndf( "QIN", 1, 1, "", &igrpq, &nskymap, status );
ndgNdfas( igrpq, 1, "READ", &indfq, status );
ndfMap( indfq, "DATA", "_DOUBLE", "READ", (void **) &inq_data, &nelqu,
status );
if( nelqu != nel && *status == SAI__OK ) {
ndfMsg( "Q", indfq );
*status = SAI__ERROR;
errRep( "", "Q image '^Q' is not the same size as the I image.",
status );
}
kpg1Rgndf( "UIN", 1, 1, "", &igrpu, &nskymap, status );
ndgNdfas( igrpu, 1, "READ", &indfu, status );
ndfMap( indfu, "DATA", "_DOUBLE", "READ", (void **) &inu_data, &nelqu,
status );
if( nelqu != nel && *status == SAI__OK ) {
ndfMsg( "U", indfu );
*status = SAI__ERROR;
errRep( "", "U image '^U' is not the same size as the I image.",
status );
}
if( *status == PAR__NULL ) {
ndfAnnul( &indfq, status );
ndfAnnul( &indfu, status );
inq_data = NULL;
inu_data = NULL;
errAnnul( status );
} else {
parGet0d( "ANGROT", &angrot, status );
parGet0d( "PAOFF", &paoff, status );
parGet0l( "PASIGN", &pasign, status );
}
}
/* Loop round all the template time series files. */
for( ifile = 1; ifile <= (int) size && *status == SAI__OK; ifile++ ) {
/* Start a new NDF context. */
ndfBegin();
/* Create the output NDF by propagating everything from the input, except
for quality and variance. */
ndgNdfas( igrp2, ifile, "READ", &indfin, status );
ndfMsg( "FILE", indfin );
msgSeti( "THISFILE", ifile );
msgSeti( "NUMFILES", size );
msgOutif( MSG__NORM, " ", "Simulating ^THISFILE/^NUMFILES ^FILE",
status );
ndgNdfpr( indfin, "DATA,HISTORY,LABEL,TITLE,WCS,UNITS,EXTENSION(*)",
ogrp, ifile, &indfout, status );
ndfAnnul( &indfin, status );
ndfAnnul( &indfout, status );
/* We now re-open the output NDF and then modify its data values. */
smf_open_file( wf, ogrp, ifile, "UPDATE", 0, &odata, status );
/* Issue a suitable message and abort if anything went wrong. */
if( *status != SAI__OK ) {
errRep( FUNC_NAME, "Could not open input template file.", status );
break;
} else {
if( odata->file == NULL ) {
*status = SAI__ERROR;
errRep( FUNC_NAME, "No smfFile associated with smfData.",
status );
break;
} else if( odata->hdr == NULL ) {
*status = SAI__ERROR;
errRep( FUNC_NAME, "No smfHead associated with smfData.",
status );
break;
}
}
/* Check the reference time series contains double precision values. */
smf_dtype_check_fatal( odata, NULL, SMF__DOUBLE, status );
/* Get the total number of data elements, and the number of time slices. */
smf_get_dims( odata, NULL, NULL, NULL, &ntslice, &ndata, NULL,
NULL, status );
/* Fill the output with bad values. */
if( *status == SAI__OK ) {
pd = odata->pntr[ 0 ];
for( iel = 0; iel < ndata; iel++ ) *(pd++) = VAL__BADD;
}
/* Resample the sky map data into the output time series. */
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, in_data, odata->pntr[ 0 ],
NULL, &ngood, status );
/* Issue a wrning if there is no good data in the output cube. */
if( ngood == 0 ) msgOutif( MSG__NORM, " ", " Output contains no "
"good data values.", status );
/* If Q and U maps have been given, allocate room to hold resampled Q and
U values, and fill them with bad values. */
if( inq_data && inu_data ) {
pq = outq_data = astMalloc( ndata*sizeof( *outq_data ) );
pu = outu_data = astMalloc( ndata*sizeof( *outu_data ) );
if( *status == SAI__OK ) {
for( iel = 0; iel < ndata; iel++ ) {
*(pu++) = VAL__BADD;
*(pq++) = VAL__BADD;
}
}
/* Determine the harmonic to use. */
parGet0i( "HARMONIC", &harmonic, status );
/* Allocate room for an array to hold the anti-clockwise angle from the
focal plane Y axis to the Y pixel axis in the reference map, at each
time slice. */
ang_data = astMalloc( ntslice*sizeof( *ang_data ) );
/* Resample them both into 3D time series. */
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, inq_data, outq_data,
ang_data, &ngood, status );
smf_resampmap( wf, odata, abskyfrm, skymap, moving, slbnd, subnd,
interp, params, sigma, inu_data, outu_data,
NULL, &ngood, status );
/* Combine these time series with the main output time series so that the
main output is analysed intensity. */
smf_uncalc_iqu( wf, odata, odata->pntr[ 0 ], outq_data, outu_data,
ang_data, pasign, AST__DD2R*paoff, AST__DD2R*angrot,
harmonic, status );
/* Release work space. */
outq_data = astFree( outq_data );
outu_data = astFree( outu_data );
ang_data = astFree( ang_data );
}
/* Close the output time series file. */
smf_close_file( wf, &odata, status );
/* End the NDF context. */
ndfEnd( status );
}
/* Close any input data file that is still open due to an early exit from
the above loop. */
if( odata != NULL ) {
smf_close_file( wf, &odata, status );
odata = NULL;
}
/* Free remaining resources. */
if( igrp1 != NULL) grpDelet( &igrp1, status);
if( igrp2 != NULL) grpDelet( &igrp2, status);
if( igrpq != NULL) grpDelet( &igrpq, status);
if( igrpu != NULL) grpDelet( &igrpu, status);
if( ogrp != NULL) grpDelet( &ogrp, status);
/* End the NDF context. */
ndfEnd( status );
/* End the tile's AST context. */
astEnd;
/* Issue a status indication.*/
if( *status == SAI__OK ) {
msgOutif(MSG__VERB," ",TASK_NAME " succeeded, time series written.", status);
} else {
msgOutif(MSG__VERB," ",TASK_NAME " failed.", status);
}
}
void smurf_sc2filtermap( int *status ) {
Grp *fgrp = NULL; /* Output filter group */
smfFilter *filt=NULL; /* Filter */
double filt_edgehigh=0; /* High-pass filter */
double filt_edgelow=0; /* Low-pass filter */
size_t fsize; /* Number of files in fgrp */
size_t i; /* Loop (grp) counter */
smfData *idata; /* Pointer to input smfData */
Grp *igrp = NULL; /* Input group of files */
int isfft=0; /* Are data fft or real space? */
int *mask=NULL; /* Mask indicating where bad data are */
size_t ndata=0; /* Number of pixels in the map */
size_t ndims; /* Number of real space dimensions */
smfData *odata=NULL; /* Pointer to output smfData to be exported */
Grp *ogrp = NULL; /* Output group of files */
size_t outsize; /* Number of files in output group */
size_t size; /* Number of files in input group */
ThrWorkForce *wf = NULL; /* Pointer to a pool of worker threads */
smfData *wrefmap=NULL; /* Whitening reference map */
int whiten; /* Applying whitening filter? */
Grp *wgrp = NULL; /* Whitening reference map group */
size_t wsize; /* Size of wgrp */
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 );
size = grpGrpsz( igrp, status );
if (size > 0) {
int parstate=0; /* ADAM parameter state */
/* Get output file(s) */
kpg1Wgndf( "OUT", igrp, size, size, "More output files required...",
&ogrp, &outsize, status );
/* Write out the filter? */
parState( "OUTFILTER", &parstate, status );
if( parstate != PAR__GROUND ) {
kpg1Wgndf( "OUTFILTER", igrp, size, size,
"More output filter files required...",
&fgrp, &fsize, status );
}
}
/* Are we going to zero bad values first? */
parGet0l( "ZEROBAD", &zerobad, status );
/* High/low-pass filters? */
parGet0d( "FILT_EDGEHIGH", &filt_edgehigh, status );
parGet0d( "FILT_EDGELOW", &filt_edgelow, status );
/* Are we applying a spatial whitening filter? */
parGet0l( "WHITEN", &whiten, status );
if( whiten ) {
/* We also need the reference map to measure the whitening filter. We
make a deep copy of it so that we can set bad values to 0 etc. */
smfData *tempdata=NULL;
kpg1Rgndf( "whiterefmap", 0, 1, "", &wgrp, &wsize, status );
if( (*status == SAI__OK) && (wsize != 1) ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME ": WHITEREFMAP must be a single reference map",
status );
}
smf_open_file( wgrp, 1, "READ", SMF__NOTTSERIES, &tempdata, status );
wrefmap = smf_deepcopy_smfData( tempdata, 0, 0, 0, 0, status );
smf_close_file( &tempdata, status );
/* Set VAL__BADD to zero if requested */
if( (*status==SAI__OK) && zerobad ) {
double *d=NULL;
size_t j;
ndata=1;
for( j=0; j<wrefmap->ndims; j++ ) ndata *= wrefmap->dims[j];
d = wrefmap->pntr[0];
if( d ) {
for( j=0; j<ndata; j++ ) {
if( d[j] == VAL__BADD ) {
d[j] = 0;
}
}
}
}
}
for( i=1;(*status==SAI__OK)&&i<=size; i++ ) {
smf_open_file( igrp, i, "READ", SMF__NOTTSERIES, &idata, status );
isfft = smf_isfft( idata, NULL, NULL, NULL, NULL, &ndims, status);
if( (*status==SAI__OK) && isfft ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME ": Input data are FFT, not real-space!\n",
status );
break;
}
if( (*status==SAI__OK) && (ndims != 2) ) {
*status = SAI__ERROR;
errRep( "", FUNC_NAME ": Input data not a 2D map!\n",
status );
break;
}
/* smf_filter_execute operates in-place, so first create the output
data as a copy of the input */
odata = smf_deepcopy_smfData( idata, 0, 0, 0, 0, status );
/* Set VAL__BADD to zero if requested */
if( (*status==SAI__OK) && zerobad ) {
double *d=NULL;
size_t j, k;
ndata=1;
for( j=0; j<odata->ndims; j++ ) ndata *= odata->dims[j];
mask = astCalloc( ndata, sizeof(*mask) );
/* Do both DATA and VARIANCE */
if( *status == SAI__OK ) {
for( k=0; k<2; k++ ) {
d = odata->pntr[k];
if( d ) {
for( j=0; j<ndata; j++ ) {
if( d[j] == VAL__BADD ) {
d[j] = 0;
mask[j] = 1;
}
}
}
}
}
}
/* Measure and apply the whitening filter. We need to do this
every time because the dimensions of filt need to match idata
(not the wrefmap) and they might be different each time. We
could try to be more clever in the future if this is too slow. */
filt = smf_create_smfFilter( idata, status );
/* Set to the identity in case no whitening is applied */
msgOut( "", TASK_NAME ": initializing filter", status );
smf_filter_ident( filt, 0, status );
if( whiten ) {
msgOut( "", TASK_NAME ": whitening the filter", status );
smf_filter2d_whiten( wf, filt, wrefmap, 0, 0, 3, status );
}
if( filt_edgelow ) {
msgOutf( "", TASK_NAME ": applying low-pass at < %lg 1/arcsec", status,
filt_edgelow );
smf_filter2d_edge( filt, filt_edgelow, 1, status );
}
if( filt_edgehigh ) {
msgOutf( "", TASK_NAME ": applying high-pass at >= %lg 1/arcsec", status,
filt_edgehigh );
smf_filter2d_edge( filt, filt_edgehigh, 0, status );
}
smf_filter_execute( wf, odata, filt, 0, 0, status );
/* Set bad values from the mask */
if( mask ) {
double *d=NULL;
size_t j, k;
/* Do both DATA and VARIANCE */
for( k=0; k<2; k++ ) {
d = odata->pntr[k];
if( d ) {
for( j=0; j<ndata; j++ ) {
if( mask[j] ) {
d[j] = VAL__BADD;
}
}
}
}
}
/* Export the data to a new file */
smf_write_smfData( odata, NULL, NULL, ogrp, i, 0, MSG__NORM, status );
/* Write out filters? */
if( fgrp ) smf_write_smfFilter( filt, NULL, fgrp, i, status );
if( filt ) smf_free_smfFilter( filt, status );
}
/* Tidy up after ourselves */
if( fgrp ) grpDelet( &fgrp, status);
if( igrp ) grpDelet( &igrp, status);
if( ogrp ) grpDelet( &ogrp, status);
if( wgrp ) grpDelet( &wgrp, status );
if( odata ) smf_close_file( &odata, status );
if( wrefmap ) smf_close_file( &wrefmap, status );
if( mask ) mask = astFree( mask );
ndfEnd( status );
/* Ensure that FFTW doesn't have any used memory kicking around */
fftw_cleanup();
}