Measurement of the solar spectral irradiance from 200 to 3000 nanometers

dc.contributor.author	Thuillier, G.
dc.contributor.author	Goutail, J.P.
dc.contributor.author	Simon, P.C.
dc.contributor.author	Pastiels, R.
dc.contributor.author	Labs, D.
dc.contributor.author	Neckel, H.
dc.date	1984
dc.date.accessioned	2017-06-28T09:36:37Z
dc.date.available	2017-06-28T09:36:37Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/5896
dc.description	The solar spectrum experiment on Spacelab 1 measured 98 percent of the sun's total energy output. It improved the absolute accuracy of solar irradiance data, especially in the ultraviolet and infrared regions. In order to detect any variation in the spectrum on future shuttle flights, the data were obtained in a radiation scale that can be preserved with high precision over many years. The instrument performance and preliminary data reduction are described.
dc.language	eng
dc.title	Measurement of the solar spectral irradiance from 200 to 3000 nanometers
dc.type	Article
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Science
dc.source.volume	225
dc.source.issue	4658
dc.source.page	182-184
Orfeo.peerreviewed	Yes
dc.identifier.doi	10.1126/science.225.4658.182
dc.identifier.scopus	2-s2.0-0346107891