Scattering Polarization of the Ca II IR Triplet for Probing the Quiet Solar Chromosphere
The chromosphere of the quiet Sun is a very important stellar atmospheric region whose thermal and magnetic structure we need to decipher in order to unlock new discoveries in solar and stellar physics. To this end, we need to identify and exploit observables sensitive to weak magnetic fields (B
Manso-Sainz, R. et al.
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2010