Image Details
Caption: Figure 14.
Impact of reversing the polarity of the magnetic field on the time-averaged KHARMA MAD R high = 160, a * = 0.5, i = 130° model. In radiative transfer, the handedness of Faraday rotation and intrinsic circularly polarized emission flip sign when the magnetic field flipped. This can lead to changes in the morphologies of both linearly and circularly polarized images.
© 2024. The Author(s). Published by the American Astronomical Society.