Image Details
Caption: Figure 4.
Two-dimensional anisotropy angular distributions (for a slab where ﹩{\hat{{\boldsymbol{n}}}}_{{ \mathcal S }}\cdot \hat{{\boldsymbol{B}}}=0﹩) as a function of the cosine of the zenith angle, ﹩{\mu }_{kn}=\cos {\theta }_{kn}﹩, and the azimuthal angle ϕkB, of the intensity (Equation (38), left column), and the averaged electric field components ﹩| {\bar{{ \mathcal E }}}_{\parallel }^{2}| ﹩ (middle column) and ﹩| {\bar{{ \mathcal E }}}_{\perp }^{2}| ﹩ (right column), obtained in MAGTHOMSCATT. Rows correspond, from top to bottom, to ω/B = 0.01, 0.1, 0.25, 0.5, 2.0, and 100.0, spanning the strong field to effectively nonmagnetic scattering regimes discussed in Section 2.5. Note the varying normalization color scale for each row for HI.
© 2026. The Author(s). Published by the American Astronomical Society.