2-D Radiative Transfer Simulations with Angle-Dependent Partial Frequency Redistribution

We demonstrate how the angle-dependent redistribution function can be incorporated into the 2-D transfer modelling of solar prominences. Some preliminary numerical simulations have been performed and we present their results by comparing the emergent hydrogen L α line profiles computed with the angl...

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Veröffentlicht in:International Astronomical Union Colloquium 1998, Vol.167, p.209-212
Hauptverfasser: Gorshkov, A.B., Heinzel, P.
Format: Artikel
Sprache:eng
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Zusammenfassung:We demonstrate how the angle-dependent redistribution function can be incorporated into the 2-D transfer modelling of solar prominences. Some preliminary numerical simulations have been performed and we present their results by comparing the emergent hydrogen L α line profiles computed with the angle-averaged and angle-dependent redistributions.
ISSN:0252-9211
DOI:10.1017/S0252921100047606