Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
Hebbur Dayananda, Supriya et al.
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2021