No CrossRef data available.
Article contents
2-D Radiative Transfer Simulations with Angle-Dependent Partial Frequency Redistribution
Published online by Cambridge University Press: 12 April 2016
Abstract
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