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

dc.contributor.authorFeldman U.
dc.contributor.authorBrown C. M.
dc.contributor.authorSeely J. F.
dc.contributor.authorDammasch I. E.
dc.contributor.authorLandi E.
dc.contributor.authorDoschek G. A.
dc.contributor.authorColgan J.
dc.contributor.authorAbdallah J.
dc.contributor.authorFontes C. J.
dc.contributor.authorSherrill M. E.
dc.date3/2010
dc.date.accessioned2016-04-13T10:04:32Z
dc.date.available2016-04-13T10:04:32Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3673
dc.descriptionhttp://esoads.eso.org/abs/2010JGRA..115.3101F
dc.languageeng
dc.rightsRestricted Access
dc.titleA 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
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research (Space Physics)
dc.source.volume115
dc.source.pageA03101
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2008JA013926
dc.identifier.urlhttp://esoads.eso.org/abs/2010JGRA..115.3101F
dc.source.editorAGU


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