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Lyman Lines in Prominences and Filaments: NLTE Modelling Strategies

Published online by Cambridge University Press:  12 April 2016

P. Heinzel
P. Heinzel*
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic CZ–25165 Ondřejov, Czech Republic

Abstract

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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

References

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