A new approach for deriving the solar irradiance from nonflaring solar upper atmosphere plasmas at 2 × 10<SUP>4</SUP> ≤ T ≤ 2 × 10<SUP>7</SUP> K

Feldman U.; Brown C. M.; Seely J. F.; Dammasch I. E.; Landi E.; Doschek G. A.; Colgan J.; Abdallah J.; Fontes C. J.; Sherrill M. E.

Authors

Feldman U.

Brown C. M.

Seely J. F.

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Discipline

Physical sciences

Audience

Scientific

Date

3/2010

Metadata

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Description

http://esoads.eso.org/abs/2010JGRA..115.3101F

Citation

Feldman U.; Brown C. M.; Seely J. F.; Dammasch I. E.; Landi E.; Doschek G. A.; Colgan J.; Abdallah J.; Fontes C. J.; Sherrill M. E. (3/2010). A new approach for deriving the solar irradiance from nonflaring solar upper atmosphere plasmas at 2 × 10⁴ ≤ T ≤ 2 × 10⁷ K. (AGU, Ed.), Journal of Geophysical Research (Space Physics), Vol. 115, A03101, DOI: 10.1029/2008JA013926.

Identifiers

uri: https://orfeo.belnet.be/handle/internal/3673

doi: http://dx.doi.org/10.1029/2008JA013926

url: http://esoads.eso.org/abs/2010JGRA..115.3101F

Type

Article

Peer-Review

Yes

Language

eng

A new approach for deriving the solar irradiance from nonflaring solar upper atmosphere plasmas at 2 × 104 ≤ T ≤ 2 × 107 K