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The visible solar spectral irradiance from 350 to 850 nm as measured by the solspec spectrometer during the ATLAS I mission

dc.contributor.authorThuillier, G.
dc.contributor.authorHersé, M.
dc.contributor.authorSimon, P.C.
dc.contributor.authorLabs, D.
dc.contributor.authorMandel, H.
dc.contributor.authorGillotay, D.
dc.contributor.authorFoujols, T.
dc.date1998
dc.date.accessioned2017-05-19T11:16:15Z
dc.date.available2017-05-19T11:16:15Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5424
dc.descriptionThe SOLSPEC instrument has been built to carry out solar spectral irradiance measurements from 200 to 3000 nm. It consists of three spectrometers designed to measure the solar spectral irradiance in ultraviolet, visible, and infrared domains. It flew with the ATLAS I mission in March 1992. This paper is dedicated to the visible part of the solar spectrum. Comparisons with recent data are shown and differences below 450 nm are discussed.
dc.languageeng
dc.titleThe visible solar spectral irradiance from 350 to 850 nm as measured by the solspec spectrometer during the ATLAS I mission
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSolar Physics
dc.source.volume177
dc.source.issue1-2
dc.source.page41-61
Orfeo.peerreviewedYes
dc.identifier.doi10.1023/A:1004953215589
dc.identifier.scopus2-s2.0-0032397234


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