A remote imaging method for interplanetary magnetic fields based on GSA and Hanle effect polarization in spectral lines, with collisional effects included and feasibility shown via forward modeling of Mercury's magnetosphere.
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Observed CR pitch-angle diffusion matches quasi-slab fast-mode turbulence predictions shaped by damping, but not Alfvénic turbulence, evidencing fast-mode dominance and constraining LISM to low beta ≈0.1 with δB/B0 ≈0.5.
citing papers explorer
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A Method for Imaging Interplanetary Magnetic Field Strength and Orientation
A remote imaging method for interplanetary magnetic fields based on GSA and Hanle effect polarization in spectral lines, with collisional effects included and feasibility shown via forward modeling of Mercury's magnetosphere.