Hanle signatures of the coronal magnetic field in the linear polarization of the hydrogen LyAlpha line
M. Derouich (1), F. Auchere (1), J. C. Vial (1), and M. Zhang (2)
TL;DR
This paper evaluates how future coronal spectro-polarimetric observations of hydrogen LyAlpha can be used to infer the magnetic field vector in the solar corona.
Contribution
It provides a framework for interpreting linear polarization measurements of hydrogen LyAlpha in terms of coronal magnetic fields.
Findings
Assessment of the validity of future observations
Preparation of interpretation methods for magnetic field inference
Guidelines for spectro-polarimetric data analysis
Abstract
This paper is dedicated to the assessment of the validity of future coronal spectro-polarimetric observations and to prepare their interpretation in terms of the magnetic field vector.
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