Solar flux determination in the spectral range 150-210 nm

dc.contributor.author	Samain, D.
dc.contributor.author	Simon, P.C.
dc.date	1976
dc.date.accessioned	2017-09-01T12:11:13Z
dc.date.available	2017-09-01T12:11:13Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/6099
dc.description	Solar irradiation fluxes are determined between 150 and 210 nm from stigmatic spectra of the Sun obtained by means of a rocket-borne spectrograph. Absolute intensities at the disk center with a spectral resolution of 0.04 nm and a spatial resolution of 7 arc sec are presented. From center-to-limb intensity variations determined from the same spectra, mean full disk intensities of the quiet Sun can be deduced. In order to compare them with other measurements, the new solar fluxes have been averaged over a bandpass of 1 nm.
dc.language	eng
dc.title	Solar flux determination in the spectral range 150-210 nm
dc.type	Article
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Solar Physics
dc.source.volume	49
dc.source.issue	1
dc.source.page	33-41
Orfeo.peerreviewed	Yes
dc.identifier.doi	10.1007/BF00221483
dc.identifier.scopus	2-s2.0-0008483675