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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
physics.space-ph 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Parker Solar Probe observations indicate intrinsically enhanced transverse magnetic power inside switchbacks at MHD-ion scales, independent of field angle, coinciding with elevated proton temperatures.
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.
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Wave Activity at MHD-ion Scales Associated with Switchbacks
Parker Solar Probe observations indicate intrinsically enhanced transverse magnetic power inside switchbacks at MHD-ion scales, independent of field angle, coinciding with elevated proton temperatures.