Physics
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107..203l&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 107, no. 2, 1987, p. 203-219. Research supported by the Ministere de l'Education Nationale
Physics
53
Calibrating, Solar Flux Density, Solar Spectra, Spacecraft Instruments, Spacelab, Ultraviolet Spectrometers, Black Body Radiation, Earth Atmosphere, Iue
Scientific paper
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.
Labs Dietrich
Neckel Heinz
Simon Paul C.
Thuillier Gerard
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