Ultraviolet solar irradiance measurement from 200 to 358 nm during spacelab 1 mission

dc.contributor.author	Labs, D.
dc.contributor.author	Neckel, H.
dc.contributor.author	Simon, P.C.
dc.contributor.author	Thuillier, G.
dc.date	1987
dc.date.accessioned	2017-06-13T09:35:56Z
dc.date.available	2017-06-13T09:35:56Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/5803
dc.description	The paper presents the results obtained from the UV-spectrometer of the 'Solar Spectrum Experiment' during the Spacelab 1 mission in December 1983. The irradiance data concern 492 passbands, which are located between 200 and 358 nm at almost equidistant wavelengths separated by about 0.3 nm. The passbands have a well-defined, bell-shaped profile with a full width at half maximum of about 1.3 nm. The data, which have an error budget between 4 and 5%, agree closely with the spectral distributions observed by Heath (1980) and Mentall et al. (1981) and confirm that the solar irradiance and the fluxes of Sun-like stars show about the same spectral distribution down to at least 240 nm.
dc.language	eng
dc.title	Ultraviolet solar irradiance measurement from 200 to 358 nm during spacelab 1 mission
dc.type	Article
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Solar Physics
dc.source.volume	107
dc.source.issue	2
dc.source.page	203-219
Orfeo.peerreviewed	Yes
dc.identifier.doi	10.1007/BF00152019
dc.identifier.scopus	2-s2.0-0002920978