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Precision Meter-wavelength Polarimetry with the Very Large Array
Precision Meter-wavelength Polarimetry with the Very Large Array
Accurate imaging polarimetry at meter wavelengths requires removal of the highly variable ionospheric Faraday rotation (IFRM) with an accuracy of 0.1 rad/m^2 or better. Models to estimate the VTEC using GNSS timing data, combined with global terrestrial magnetic field models have been developed over the past 25 years. Estimating the accuracy of these models requires observations of a source of known intrinsic electric vector position angle (EVPA) over a wide rage of ionospheric conditions.
