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            <title xml:lang="en">2D radiative modelling of He I spectral lines formed in solar prominences</title>
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                <forename>Frédéric</forename>
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                <title xml:lang="en">2D radiative modelling of He I spectral lines formed in solar prominences</title>
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              <p>We present preliminary results of 2D radiative modelling of He I lines in solar prominences, using a new numerical code developed by us (Leger, Chevallier and 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 THeMIS are very satisfactory.</p>
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