[tel-00726959, v1] Caractériser le milieu interstellaire ... - HAL - INRIA

WIFISYNA. implementation planWIFISYNB. wifisyn language internal helpas a function of frequency, implying the computation of a singledirty beam for all the frequencies.BWIFISYN Language Internal HelpThis appendix describes the user interface of the WIFISYN package.tel-00726959, version 1 - 31 Aug 2012WIFISYNaxes.B.4 LOAD[WIFISYN\] LOAD Buffer Varname16B. wifisyn language internal helpLoad the specified internal buffer (VISI, WEIGHT, BEAM, DIRTY) into thespecified SIC variable (Varname).B.5 READ[WIFISYN\]READ Buffer File [/PLANE First Last]Read the specified internal buffer (UV, BEAM, DIRTY) from the specifiedinput File. Default extensions are respectively .tuv, .beam, .lmv. Arange of channels can be specified using the /PLANE option.B.6 SETUP[WIFISYN\]SETUPSetup and display the imaging parameters for the internal uvxy table.B.7 UVBEAM[WIFISYN\]UVBEAMCompute the dirty beams associated to the internal uvxy table.B.8 UVGRID[WIFISYN\]UVGRID [/NOCONV]Grid the internal uvxy table into a wificube. The /NOCONV option createsthe wificube of the right dimension and initializes it so that the usercan fill it through the COMPLEX command.B.9 UVMAP[WIFISYN\]UVMAPCompute the dirty image associated to the internal uvxy table. This commandis equivalent to the following sequence: SETUP, UVGRID, FFT WIFI/DIRECT /XY, WIFI2VISI, FFT VISI /INVERSE, COMPLEX VISI TO REAL.B.1 LanguageCOMPLEX : Transfer complex internal buffers into SIC real images andvice-versaFFT : Compute direct or inverse FFT of internal buffersLOAD : Load an internal buffer into a SIC variableREAD : Read the input files in internal buffersSETUP : Setup and display the imaging parameters for the internaluvxy tableUVBEAM : Compute the dirty beams associated to the internal uvxytableUVGRID : Grid the internal uvxy tableUVMAP : Compute the dirty image associated to the internal uvxytableUVSHIFT : Shift the phase center of the internal uvxy table(Not working yet)UVSORT : Sort the internal uvxy table(Not working yet)UVSWAP : Swap the UVT and UVR buffers(Not working yet)UVSYMMETRY : Check the Hermitian symmetry of the internal buffersVARIABLE : Map the imaging internal parameters onto the WIFI% SICstructureWIFI2VISI : Shift-and-average the wide-field hypercube to get a’’standard’’ visibility planeWRITE : Write internal buffers into output filesB.2 COMPLEX[WIFISYN\]COMPLEX VISICUBE|WIFICUBE TO|FROM AMPLITUDE|PHASE|RE-AL|IMAGINARYTransfer complex internal buffers (visicube or wificube) into SIC realimages for display. The inverse operation is possible to set or to modifythe complex internal buffers.B.3 FFT[WIFISYN\]FFT VISICUBE|WIFICUBE /DIRECT|INVERSE /UV|XYCompute the direct or inverse 2D Fast Fourier Transform of internal complexbuffers (visicube or wificube). When the FFT is applied to thewificube buffer, the 2D FFT can be applied along either the uv or the xyWIFISYNB.10 UVSYMMETRY[WIFISYN\]UVSYMMETRY17B. wifisyn language internal helpCheck the Hermitian symmetry of the wificube (or visicube???) buffer.B.11 VARIABLE[WIFISYN\]VARIABLEMap the imaging internal parameters onto the WIFI% SIC structure.B.12 WIFI2VISI[WIFISYN\]WIFI2VISIShift-and-average the wide-field hypercube to get a ’’standard’’ visibilityUV plane, which can then be FFTed to get the dirty image.B.13 WRITE[WIFISYN\]WRITE Buffer File [/PLANE First Last]Write the specified output File from the specified internal buffer (UV,BEAM, DIRTY). Default extensions are respectively .tuv, .beam, .lmv. Arange of channels can be specified using the /PLANE option.1819