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1 : //# ImageSkyModel.h: Definition for ImageSkyModel 2 : //# Copyright (C) 1996,1997,1998,1999,2000,2002 3 : //# Associated Universities, Inc. Washington DC, USA. 4 : //# 5 : //# This library is free software; you can redistribute it and/or modify it 6 : //# under the terms of the GNU Library General Public License as published by 7 : //# the Free Software Foundation; either version 2 of the License, or (at your 8 : //# option) any later version. 9 : //# 10 : //# This library is distributed in the hope that it will be useful, but WITHOUT 11 : //# ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or 12 : //# FITNESS FOR A PARTICULAR PURPOSE. See the GNU Library General Public 13 : //# License for more details. 14 : //# 15 : //# You should have received a copy of the GNU Library General Public License 16 : //# along with this library; if not, write to the Free Software Foundation, 17 : //# Inc., 675 Massachusetts Ave, Cambridge, MA 02139, USA. 18 : //# 19 : //# Correspondence concerning AIPS++ should be adressed as follows: 20 : //# Internet email: casa-feedback@nrao.edu. 21 : //# Postal address: AIPS++ Project Office 22 : //# National Radio Astronomy Observatory 23 : //# 520 Edgemont Road 24 : //# Charlottesville, VA 22903-2475 USA 25 : //# 26 : //# 27 : //# $Id$ 28 : 29 : #ifndef SYNTHESIS_IMAGESKYMODEL_H 30 : #define SYNTHESIS_IMAGESKYMODEL_H 31 : 32 : #include <casacore/ms/MeasurementSets/MeasurementSet.h> 33 : #include <synthesis/MeasurementComponents/SkyModel.h> 34 : #include <casacore/casa/Arrays/Matrix.h> 35 : #include <casacore/images/Images/ImageInterface.h> 36 : #include <casacore/images/Images/PagedImage.h> 37 : #include <casacore/images/Images/TempImage.h> 38 : #include <casacore/casa/Logging/LogMessage.h> 39 : #include <casacore/casa/Logging/LogSink.h> 40 : #include <casacore/casa/System/PGPlotter.h> 41 : 42 : namespace casa { //# NAMESPACE CASA - BEGIN 43 : 44 : // <summary> 45 : // Image Sky Model: Image-based Model for the Sky Brightness 46 : // </summary> 47 : 48 : // <use visibility=export> 49 : 50 : // <reviewed reviewer="" date="" tests="" demos=""> 51 : 52 : // <prerequisite> 53 : // <li> <linkto class=SkyModel>SkyModel</linkto> class 54 : // <li> <linkto class=SkyEquation>SkyEquation</linkto> class 55 : // <li> <linkto class=casacore::ImageInterface>ImageInterface</linkto> class 56 : // <li> <linkto class=casacore::PagedImage>PagedImage</linkto> class 57 : // <li> <linkto module=MeasurementComponents>MeasurementComponents</linkto> module 58 : // <li> <linkto class=VisSet>VisSet</linkto> class 59 : // </prerequisite> 60 : // 61 : // <etymology> 62 : // ImageSkyModel describes an interface for Models to be used in 63 : // the SkyEquation. It is derived from <linkto class=SkyModel>SkyModel</linkto>. 64 : // </etymology> 65 : // 66 : // <synopsis> 67 : // A ImageSkyModel contains a number of separate models. The interface to 68 : // SkyEquation is via an image per model. <linkto class=SkyEquation>SkyEquation</linkto> uses this image to 69 : // calculate Fourier transforms, etc. Some (most) SkyModels are 70 : // solvable: the SkyEquation can be used by the SkyModel to return 71 : // gradients with respect to itself (via the image interface). Thus 72 : // for a SkyModel to solve for itself, it calls the SkyEquation 73 : // methods to get gradients of chi-squared with respect to the 74 : // image pixel values (thus returning an image: basically a residual 75 : // image). The SkyModel then uses these gradients as appropriate to 76 : // update itself. 77 : // </synopsis> 78 : // 79 : // <example> 80 : // See the example for <linkto class=SkyModel>SkyModel</linkto>. 81 : // </example> 82 : // 83 : // <motivation> 84 : // The properties of a model of the sky must be described 85 : // for the <linkto class=SkyEquation>SkyEquation</linkto>. 86 : // </motivation> 87 : // 88 : // <todo asof="97/10/01"> 89 : // <li> Multiple images in SkyModel 90 : // <li> ComponentModel 91 : // </todo> 92 : 93 : class ImageSkyModel : public SkyModel { 94 : public: 95 : 96 : // Empty constructor 97 : ImageSkyModel(const casacore::Int maxNumModels=1); 98 : 99 : void setMaxNumberModels(const casacore::Int maxNumModels); 100 : 101 : // Copy constructor 102 : ImageSkyModel(const ImageSkyModel& sm); 103 : 104 : // Add a componentlist 105 : virtual casacore::Bool add(ComponentList& compList); 106 : //update componentlist 107 : virtual casacore::Bool updatemodel(ComponentList& compList); 108 : 109 : 110 : // Add an image. maxNumXfr is the maximum Number of transfer functions 111 : // that we might want to associate with this image. 112 : virtual casacore::Int add(casacore::ImageInterface<casacore::Float>& image, const casacore::Int maxNumXfr=100); 113 : //update model image...you have to have added it before...nmodels_p held has to be bigger that image here 114 : //its left to the caller to make sure the image is conformant...otherwise you are in trouble. 115 : virtual casacore::Bool updatemodel(const casacore::Int thismodel, casacore::ImageInterface<casacore::Float>& image); 116 : // Add a residual image 117 : virtual casacore::Bool addResidual(casacore::Int image, casacore::ImageInterface<casacore::Float>& residual); 118 : 119 : // Destructor 120 : virtual ~ImageSkyModel(); 121 : 122 : // Assignment operator 123 : ImageSkyModel& operator=(const ImageSkyModel& other); 124 : 125 : // Number of models contained 126 0 : virtual casacore::Int numberOfModels() {return nmodels_p;}; 127 : 128 : // MFS : Number of taylor terms per model 129 0 : virtual casacore::Int numberOfTaylorTerms() {return 1;}; 130 : 131 : // MFS : In-place coefficient residual calculations 132 0 : virtual casacore::Bool calculateCoeffResiduals(){return false;}; 133 : 134 : // MFS : Calculate restored alpha and beta. 135 0 : virtual casacore::Bool calculateAlphaBeta(const casacore::Vector<casacore::String>& /*restoredNames*/, const casacore::Vector<casacore::String>& /*residualNames*/){return false;}; 136 : 137 : // MFS : Reference Frequency 138 0 : virtual casacore::Double getReferenceFrequency(){return 0.0;} 139 : 140 : // MFS : Index of Taylor term in array of nmodels x ntaylorterms 141 : //virtual casacore::Int getTaylorIndex(casacore::Int index){return 0;} 142 0 : virtual casacore::Int getTaylorIndex(casacore::Int index){return (casacore::Int)(index/nfields_p);} 143 : 144 : // Is this model solveable? 145 : casacore::Bool isSolveable(casacore::Int model=0); 146 : 147 : // Free and fix the model (returns previous status). Free means that 148 : // it will be solved for in any solution. 149 : casacore::Bool free(casacore::Int model=0); 150 : casacore::Bool fix(casacore::Int model=0); 151 : 152 : // Initialize for gradient search 153 : virtual void initializeGradients(); 154 : 155 : // Finalize for gradient search 156 0 : virtual void finalizeGradients() {}; 157 : 158 : // Does this have a component list? 159 : casacore::Bool hasComponentList(); 160 : 161 : casacore::Bool isEmpty(casacore::Int model=0); 162 : 163 : // Return the component list 164 : virtual ComponentList& componentList(); 165 : 166 : // Return actual images to be used by SkyEquation. 167 : // <group> 168 : casacore::ImageInterface<casacore::Float>& image(casacore::Int model=0); 169 : casacore::ImageInterface<casacore::Complex>& cImage(casacore::Int model=0); 170 : casacore::ImageInterface<casacore::Complex>& XFR(casacore::Int model=0, casacore::Int numXFR=0); 171 : casacore::ImageInterface<casacore::Float>& PSF(casacore::Int model=0); 172 : casacore::ImageInterface<casacore::Float>& gS(casacore::Int model=0); 173 : casacore::ImageInterface<casacore::Float>& residual(casacore::Int model=0); 174 : casacore::ImageInterface<casacore::Float>& ggS(casacore::Int model=0); 175 : // if (doFluxScale(mod)) image(mod) * fluxScale(mod) 176 : // gives actual brightness distribution 177 : casacore::ImageInterface<casacore::Float>& fluxScale(casacore::Int model=0); 178 : casacore::ImageInterface<casacore::Float>& work(casacore::Int model=0); 179 : casacore::ImageInterface<casacore::Float>& deltaImage(casacore::Int model=0); 180 : // </group> 181 : 182 : // tells if this model needs to be multiplied by a flux scale image 183 : casacore::Bool doFluxScale(casacore::Int model=0); 184 : // require use of flux scale image 185 : void mandateFluxScale(casacore::Int model=0); 186 : 187 : casacore::Bool hasXFR(casacore::Int model=0); 188 : 189 : // Add to Sum weights, Chi-Squared 190 0 : void addStatistics(casacore::Float sumwt, casacore::Float chisq) {sumwt_p+=sumwt;chisq_p+=chisq;} 191 : 192 : // Weight per model (channels, polarizations) 193 : casacore::Matrix<casacore::Float>& weight(casacore::Int model=0); 194 : 195 : // Solve for this SkyModel: This replaces the image with 196 : // the residual image 197 : virtual casacore::Bool solve (SkyEquation& me); 198 : 199 : // Solve explicitly for the residuals: same as solve for 200 : // this class 201 : // modelToMs determines if predicted vis is put in the MODEL_DATA column 202 : casacore::Bool solveResiduals (SkyEquation& me, casacore::Bool modelToMS=false); 203 : 204 : // Make the approximate PSFs needed for each model 205 : virtual void makeApproxPSFs(SkyEquation& se); 206 : 207 : // Get current residual image: this is either that image specified via 208 : // addResidual, or a scratch image. 209 : // For example in WFImageSkyModel it might return the whole main image 210 : //rather than facets 211 : virtual casacore::ImageInterface<casacore::Float>& getResidual (casacore::Int model=0); 212 : 213 : // Return the fitted beam for each model 214 : casacore::ImageBeamSet& beam(casacore::Int model=0); 215 : 216 : // Set casacore::PGPlotter to be used 217 : void setPGPlotter(casacore::PGPlotter& pgp) { pgplotter_p = &pgp; } 218 : 219 : // This is the factor by which you multiply the worst outer 220 : // sidelobe by to get the threshold for the current cycle 221 0 : void setCycleFactor(float x) { cycleFactor_p = x; } 222 : 223 : // Cycle threshold will double in this number of iterations 224 : // (ie, use a large number if you don't want cycle threshold 225 : // to inch up) 226 0 : void setCycleSpeedup(float x) { cycleSpeedup_p = x; } 227 : 228 : // Yet another control for the minor cycle threshold. 229 : // This is in response to CAS-2673 230 : // This allows control similar to 'cyclefactor' - used in MFClarkCleanSkyModel 231 0 : void setCycleMaxPsfFraction(float x) { cycleMaxPsfFraction_p = x; } 232 : 233 : // Set the variable that switches on the progress display 234 0 : void setDisplayProgress (const casacore::Bool display ) {displayProgress_p = display; }; 235 : 236 : // Set a variable to indicate the polarization frame in the data (circular or linear). 237 : // This is used along with the user's choice of output casacore::Stokes parameter 238 : // to decide the stokesCoordinate of the temporary images "cImage". 239 0 : void setDataPolFrame(StokesImageUtil::PolRep datapolrep) {dataPolRep_p = datapolrep;}; 240 : 241 : // Tries to return a pointer to a casacore::TempImage (allocated with new, so remember 242 : // to use delete) with the given shape and CoordinateSystem. 243 : // 244 : // @param imgShp 245 : // @param imgCoords 246 : // @param nMouthsToFeed: If > 1 it is taken as a hint that it should leave 247 : // room for nMouthsToFeed - 1 more TempImages. 248 : // 249 : // <throws> 250 : // casacore::AipsError on memory allocation error. 251 : // </throws> 252 : template<class M> 253 : static casacore::TempImage<M>* getTempImage(const casacore::TiledShape& imgShp, 254 : const casacore::CoordinateSystem& imgCoords, 255 : const casacore::uInt nMouthsToFeed=1); 256 : 257 0 : virtual casacore::Int getModelIndex(casacore::uInt field, casacore::uInt /*taylor*/){return field;}; 258 : 259 : //try to make templattices use memory if possible 260 : //if set to false then always use disk 261 : virtual void setMemoryUse(casacore::Bool useMem=false); 262 0 : virtual casacore::Bool getMemoryUse(){return useMem_p;}; 263 : //Set templattice tile vol in pixels 264 : void setTileVol(const casacore::Int tileVol=1000000); 265 : protected: 266 : 267 : // Make Newton Raphson step internally. This is really an implementation 268 : // detail: it is useful for derived classes. 269 : // The modelToMS parameter is for committing to MODEL_DATA column of the MS 270 : // the predicted visibilities. 271 : 272 : casacore::Bool makeNewtonRaphsonStep(SkyEquation& se, 273 : casacore::Bool incremental=false, casacore::Bool modelToMS=false); 274 : 275 : 276 : // Get casacore::PGPlotter to be used 277 : casacore::PGPlotter* getPGPlotter() { return pgplotter_p; } 278 : 279 : casacore::Int maxnmodels_p; 280 : casacore::Int nmodels_p; 281 : //MFS 282 : casacore::Int nfields_p; 283 : 284 : casacore::Int maxNumXFR_p; 285 : 286 : casacore::Float sumwt_p; 287 : casacore::Float chisq_p; 288 : 289 : // ComponentList 290 : ComponentList* componentList_p; 291 : 292 : // Images 293 : casacore::Vector<casacore::String> imageNames_p; 294 : // Everything here can be just interface 295 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > image_p; 296 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > residual_p; 297 : 298 : // We actually create these 299 : casacore::PtrBlock<casacore::ImageInterface<casacore::Complex> * > cimage_p; 300 : casacore::PtrBlock<casacore::ImageInterface<casacore::Complex> * > cxfr_p; 301 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > residualImage_p; 302 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > gS_p; 303 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > psf_p; 304 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > ggS_p; 305 : // if (doFluxScale_p), image_p * fluxScale_p gives the true brightness 306 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > fluxScale_p; 307 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > work_p; 308 : casacore::PtrBlock<casacore::ImageInterface<casacore::Float> * > deltaimage_p; 309 : casacore::Block<casacore::Bool> solve_p; 310 : casacore::Block<casacore::Bool> doFluxScale_p; 311 : 312 : casacore::PtrBlock<casacore::Matrix<casacore::Float> * > weight_p; 313 : 314 : casacore::PtrBlock<casacore::ImageBeamSet * > beam_p; 315 : 316 : casacore::LogSink logSink_p; 317 0 : casacore::LogSink& logSink() {return logSink_p;}; 318 : 319 : casacore::Long cacheSize(casacore::Int model); 320 : casacore::IPosition tileShape(casacore::Int model); 321 : 322 : casacore::PGPlotter *pgplotter_p; 323 : casacore::Bool displayProgress_p; 324 : // This is the factor by which you multiply the worst outer 325 : // sidelobe by to get the threshold for the current cycle 326 : casacore::Float cycleFactor_p; 327 : // Cycle threshold will double in this number of iterations 328 : // (ie, use a large number if you don't want cycle threshold 329 : // to inch up) 330 : casacore::Float cycleSpeedup_p; 331 : // Cycle threshold = maxResidual x min(Max-Psf-Fraction , cyclefactor x maxpsfsidelobe) 332 : casacore::Float cycleMaxPsfFraction_p; 333 : // If PSF is done..should not redo it. 334 : casacore::Bool donePSF_p; 335 : // check if model has been modified especially for continuing 336 : // a deconvolution 337 : casacore::Bool modified_p; 338 : // Parameter to indicate the polaraization type of the data (circular or linear) 339 : // Required by cImage() to decide shapes. 340 : StokesImageUtil::PolRep dataPolRep_p; 341 : casacore::Bool workDirOnNFS_p; 342 : casacore::Bool useMem_p; 343 : casacore::Int tileVol_p; 344 : }; 345 : 346 : 347 : 348 : } //# NAMESPACE CASA - END 349 : 350 : 351 : #ifndef AIPS_NO_TEMPLATE_SRC 352 : #include <synthesis/MeasurementComponents/ImageSkyModel.tcc> 353 : #endif //# AIPS_NO_TEMPLATE_SRC 354 : 355 : #endif 356 : 357 :