Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T14:36:13.777Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  12 April 2016

A.B. Gorshkov  and
P. Heinzel
A.B. Gorshkov
Affiliation:
Sternberg Astronomical Institute, 119899 Moscow, Russia
P. Heinzel
Affiliation:
Astronomical Institute, 25165 Ondřejov, Czech Republic

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 Lα line profiles computed with the angle-averaged and angle-dependent redistributions.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 209 - 212
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Gorshkov, A.B. 1996, in Mein, N. and Sahal-Brechot, S. (eds.), Science with THEMIS, Proc. Forum THEMIS, Observatoire de Paris-Meudon, p. 273 Google Scholar
Gouttebroze, P., Heinzel, P. and Vial, J.-C. 1993, A&AS, 99, 513 Google Scholar
Heinzel, P. 1995, A&A, 299, 563 Google Scholar
Hubený, I. 1985, Bull. Astron. Inst. Czech, 36, 1 Google Scholar
Hummer, D.G. 1962, MNRAS, 125, 21 CrossRefGoogle Scholar
Paletou, F. 1995, A&A, 302, 587 Google Scholar
Rybicki, G.B. and Hummer, D.G. 1991, A&A, 245, 171 Google Scholar