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 |