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Paper: 2D Radiative Modeling of He I Spectral Lines Formed in Solar Prominences
Volume: 405, Solar Polarization 5: In Honor of Jan Olof Stenflo
Page: 325
Authors: Léger, L.; Paletou, F.
Abstract: We present preliminary results of 2D radiative modeling of He I lines in solar prominences, using a new numerical code developed by us (Léger, Chevallier, & Paletou 2007). It treats self-consistently the radiation transfer and the non-LTE statistical equilibrium of H and, in a second stage, the one of He using a detailed atomic model. Preliminary comparisons with new visible plus near-infrared observations made at high spectral resolution with THéMIS are very satisfactory.
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