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 |
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| container_title | International Astronomical Union Colloquium |
| container_volume | 167 |
| creator | Gorshkov, A.B. Heinzel, P. |
| description | 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. |
| doi_str_mv | 10.1017/S0252921100047606 |
| format | Article |
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| ispartof | International Astronomical Union Colloquium, 1998, Vol.167, p.209-212 |
| issn | 0252-9211 |
| language | eng |
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| source | Alma/SFX Local Collection |
| title | 2-D Radiative Transfer Simulations with Angle-Dependent Partial Frequency Redistribution |
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