The Hanle Effect of Lyα in a Magnetohydrodynamic Model of the Solar Transition Region
In order to understand the heating of the solar corona it is crucial to obtain empirical information on the magnetic field in its lower boundary (the transition region). To this end, we need to measure and model the linear polarization produced by scattering processes in strong UV lines, such as the hydrogen Lyα line. The interpretation of the
Štěpán, J. et al.
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10
2012