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Lyman Lines in Prominences and Filaments: NLTE Modelling Strategies
Published online by Cambridge University Press: 12 April 2016
Abstract
We briefly summarize the most important aspects of NLTE formation of hydrogen Lyman lines in prominences and filaments. A modified MALI code of Heinzel (1995) is described and its applicability to the interpretation of SOHO/SUMER data is discussed.
- Type
- Filaments and Their Environment
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 188 - 189
- Copyright
- Copyright © Astronomical Society of the Pacific 1998