AFARS | Is used after FARS to determine Position and Value of the maximum |
ALBUS | Calculate ionospheric delay and Faraday rotation using ALBUS |
AVERSION | Specify a version of the ALBUS container |
BANDPOL | specifies polarizations of individual IFs |
BDEPO | computes depolarization due to rotation measure gradients |
BLPCL | Do divide by I,Q,U models for circular polarization BLCHN |
BLPOLCAL | Do BLCHN for I, Q, U, V models |
COMB | combines two images by a variety of mathematical methods |
CXPOLN | Procedure to make complex polarization images and beam |
DOFARS | Procedure to aid in Faraday rotation synthesis using the FARS task |
DOPOL | selects application of any polarization calibration |
DT2PD | Write PD table from a PD table text file |
FARAD | add ionospheric Faraday rotation to CL table |
FARS | Faraday rotation synthesis based on the brightness vs wavelength |
FTARS | Fits 1-dimensional polarization spectrum to Q/U text file |
HLPRMFIT | Polarization fitting task RMFIT - run-time help |
HLPZAMAN | Fits 1-dimensional Zeeman model to absorption data - run-time help |
HLPZEMAN | Fits 1-dimensional Zeeman model to data - run-time help |
LPCAL | Determines instrumental polarization for UV data |
MAPBM | Map VLA beam polarization |
MARSP | Check planetary polarization angles, plot histogram of differences |
MEDI | combines four images by a variety of mathematical methods |
MFIMG | Image the Earth magnetic field model or TEC data used by TECOR |
MODAB | Makes simple absorption/emission spectral-line image in I/V |
MODIM | adds images of model objects to image cubes in IQU polarization |
MODSP | adds images of model objects to image cubes in I/V polarization |
MTARS | Compute model inputs to TARS |
PCAL | Determines instrumental polarization for UV data |
PCNTR | Generate plot file with contours plus polarization vectors |
PCUT | Cutoff in polarized intensity |
PDEDT | Interactive TV task to edit polarization D-term (PD) tables |
PDPLT | Plots selected contents of PD tables |
PDVER | specifies the version of the spetral polarization table to use |
PMODEL | Polarization model parameters |
POLANGLE | Intrinsic polarization angles for up to 30 sources |
POLCO | Task to correct polarization maps for Ricean bias |
POLPLOT | specifies the desired polarization ratio before plotting. |
POLSN | Make a SN table from cross polarized fringe fit |
PPAPP | Applies Right minus Left phase difference to a 2nd data set |
PROGRAM | Specify a program to be used |
QUFIX | determines Right minus Left phase difference, corrects cal files |
QUOUT | writes text file of Q, U versus frequency to be used by RLDIF |
QUXTR | extracts text files from Q,U cubes for input to TARS |
RFARS | Correct Q/U cubes for Faraday rotation synthesis results |
RIFRM | Task to modify a CL and TE table with IFRM values from ALBUS files |
RLCAL | Determines instrumental right-left phase versus time (a self-cal) |
RLCOR | corrects a data set for R-L phase differences |
RLDIF | determines Right minus Left phase difference, corrects cal files |
RM | Task to calculate rotation measure and magnetic field |
RM2PL | Plots spectrum of a pixel with RMFIT fit |
RMFIT | Fits 1-dimensional polarization spectrum to Q/U cube |
ROTMEAS | Tells the rotation measure of a source |
SWPOL | Swap polarizations in a UV data base |
TARPL | Plot input and output text files of the TARS task |
TARS | Simulation of Faraday rotation synthesis (mainly task FARS) |
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