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  Semiempirical Models of the Solar Atmosphere. III. Set of Non-Lte Models for Far-Ultraviolet/Extreme-Ultraviolet Irradiance Computation

Fontenla, J. M., Curdt, W., Haberreiter, M., Harder, J., & Tian, H. (2009). Semiempirical Models of the Solar Atmosphere. III. Set of Non-Lte Models for Far-Ultraviolet/Extreme-Ultraviolet Irradiance Computation. Astrophysical Journal, 707(1), 482-502. doi:10.1088/0004-637X/707/1/482.

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 Creators:
Fontenla, J. M., Author
Curdt, W.1, 2, Author           
Haberreiter, M., Author
Harder, J., Author
Tian, H.3, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
3IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: SOHO: SUMER
 Abstract: -

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 Dates: 2009
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/0004-637X/707/1/482
BibTex Citekey: Fontenla:2009-274
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Title: Astrophysical Journal
Source Genre: Journal
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Pages: - Volume / Issue: 707 (1) Sequence Number: - Start / End Page: 482 - 502 Identifier: -