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.

doi:10.1088/0004-637X/707/1/482

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

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

MPS-Authors

/persons/resource/persons103872

Curdt, W.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104247

Tian, H.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-02F5-8

Abstract

There is no abstract available