Magnetic Field Diagnostics in the Solar Upper Atmosphere
The magnetic field is the main driver of the activity in the solar upper atmosphere, but its measurement is notoriously difficult. In order to determine the magnetic field in the chromosphere, transition region, and corona, we need to measure and interpret the polarization signals that the scattering of anisotropic radiation and the Hanle and
Trujillo Bueno, J. et al.
Advertised on:
8
2022