13.26 POLARIZA

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)
TRUEP    determines true antenna polarization from special data sets
VH2RL    Converts from linear to circular polarization and vice versa
VHCAL    Do divide by I,Q,U models for linear polarization data
VHCALIB    Do CALIB for linear polarization with I, Q, U models
VHDIF    find/apply V minus H linear polarization phase difference
VLABP    VLA antenna beam polarization correction for snapshot images
VLBACPOL    Procedure to calibrate cross-polarization delays
XG2PL    Plots spectrum of a pixel with XGAUS/AGAUS and ZEMAN/ZAMAN fits
XYDIF    find/apply X minus Y linear polarization phase difference
ZAMAN    Fits 1-dimensional Zeeman model to absorption-line data
ZEMAN    Fits 1-dimensional Zeeman model to data