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astro-ph.SR2025
The H line as a probe of chromospheric magnetic fields
Harsh Mathur, Jayant Joshi, Thore Espedal Moe +2
We explore the diagnostic potential of the H line for probing the chromospheric magnetic field using a realistic 3D radiative magnetohydrodynamic (rMHD) model. The Stokes profil…
astro-ph.SR2025
Clustering analysis of Ca {\sc i} 4227 line polarization using magnetohydrodynamic simulations of the solar atmosphere
Harsh Mathur, L. S. Anusha, Devang Agnihotri
Ca {\sc i} 4227 Å\, line is a strong resonance line formed in the Solar chromosphere. At the limb, it produces the largest scattering polarization signal. So far, modeling the line…