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The Solar Irradiance Spectrum at Solar Activity Minimum Between Solar Cycles 23 and 24

dc.contributor.authorThuillier, G.
dc.contributor.authorBolsée, D.
dc.contributor.authorSchmidtke, G.
dc.contributor.authorFoujols, T.
dc.contributor.authorNikutowski, B.
dc.contributor.authorShapiro, A.I.
dc.contributor.authorBrunner, R.
dc.contributor.authorWeber, M.
dc.contributor.authorErhardt, C.
dc.contributor.authorHersé, M.
dc.contributor.authorGillotay, D.
dc.contributor.authorPeetermans, W.
dc.contributor.authorDecuyper, W.
dc.contributor.authorPereira, N.
dc.contributor.authorHaberreiter, M.
dc.contributor.authorMandel, H.
dc.contributor.authorSchmutz, W.
dc.date2014
dc.date.accessioned2016-03-25T09:42:10Z
dc.date.available2016-03-25T09:42:10Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2846
dc.descriptionOn 7 February 2008, the SOLAR payload was placed onboard the International Space Station. It is composed of three instruments, two spectrometers and a radiometer. The two spectrometers allow us to cover the 16 - 2900 nm spectral range. In this article, we first briefly present the instrumentation, its calibration and its performance in orbit. Second, the solar spectrum measured during the transition between Solar Cycles 23 to 24 at the time of the minimum is shown and compared with other data sets. Its accuracy is estimated as a function of wavelength and the solar atmosphere brightness-temperature is calculated and compared with those derived from two theoretical models.
dc.languageeng
dc.titleThe Solar Irradiance Spectrum at Solar Activity Minimum Between Solar Cycles 23 and 24
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeSolACES
dc.subject.freeSolar minimum
dc.subject.freeSolar spectrum
dc.subject.freeSOLSPEC
dc.subject.freeSpace Station
dc.source.titleSolar Physics
dc.source.volume289
dc.source.issue6
dc.source.page1931-1958
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11207-013-0461-y
dc.identifier.scopus2-s2.0-84893944834


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