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dc.contributor.authorThuillier, G.
dc.contributor.authorSimon, P.C.
dc.contributor.authorLabs, D.
dc.contributor.authorPastiels, R.
dc.contributor.authorNeckel, H.
dc.date1981
dc.date.accessioned2017-09-06T09:07:42Z
dc.date.available2017-09-06T09:07:42Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/6177
dc.descriptionThis instrument, at the present time in development, will fly on board Spacelab I in May 1983. Other flights are foreseen during the following missions. This instrument is composed by three double monochromators covering the range 170 to 3200 nm. The spectrometers have band-passes of 1 nm up to 900 nm and 20 nm from 850 to 3200 nm with an accuracy 10-2 nm. Calibration lamps are included in the instrument to monitor any change of its sensitivity and wavelength scale.
dc.languageeng
dc.titleAn instrument to measure the solar spectrum from 170 to 3200 nm on board Spacelab
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSolar Physics
dc.source.volume74
dc.source.issue2
dc.source.page531-537
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/BF00154536
dc.identifier.scopus2-s2.0-0042023630


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