Open rlbyrne opened 3 years ago
If the sky model contains linearly polarized emission, we need to account for ionospheric Faraday rotation. We would like to be able to supply FHD with an RM and account for Stokes Q-U mode mixing and depolarization.
If the sky model contains linearly polarized emission, we need to account for ionospheric Faraday rotation. We would like to be able to supply FHD with an RM and account for Stokes Q-U mode mixing and depolarization.