2D Radiative Modeling of He I Spectral Lines Formed in Solar Prominences

Details 2D Radiative Modeling of He I Spectral Lines Formed in Solar Prominences 2D Radiative Modeling of He I Spectral Lines Formed in Solar Prominences

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..325l&link_type=abstract

Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results of 2D radiative modeling of He I lines in solar prominences, using a new numerical code developed by us \citep*{leger_leger07}. 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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