An instrument to measure the solar spectrum from 170 to 3200 nm on board Spacelab
dc.contributor.author | Thuillier, G. | |
dc.contributor.author | Simon, P.C. | |
dc.contributor.author | Labs, D. | |
dc.contributor.author | Pastiels, R. | |
dc.contributor.author | Neckel, H. | |
dc.date | 1981 | |
dc.date.accessioned | 2017-09-06T09:07:42Z | |
dc.date.available | 2017-09-06T09:07:42Z | |
dc.identifier.uri | https://orfeo.belnet.be/handle/internal/6177 | |
dc.description | This 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.language | eng | |
dc.title | An instrument to measure the solar spectrum from 170 to 3200 nm on board Spacelab | |
dc.type | Article | |
dc.subject.frascati | Physical sciences | |
dc.audience | Scientific | |
dc.source.title | Solar Physics | |
dc.source.volume | 74 | |
dc.source.issue | 2 | |
dc.source.page | 531-537 | |
Orfeo.peerreviewed | Yes | |
dc.identifier.doi | 10.1007/BF00154536 | |
dc.identifier.scopus | 2-s2.0-0042023630 |