Airglow-solar spectrometer instrument (20-700 nm) aboard the San Marco D/L satellite

Details Airglow-solar spectrometer instrument (20-700 nm) aboard the San Marco D/L satellite Airglow-solar spectrometer instrument (20-700 nm) aboard the San Marco D/L satellite

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apopt..24.3206s&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 24, Oct. 1, 1985, p. 3206-3213.

Physics

Optics

22

Aeronomy, Airglow, Extraterrestrial Radiation, San Marco Satellites, Solar Radiation, Solar Spectrometers, Calibrating, Molecular Spectra, Satellite-Borne Instruments

Scientific paper

The ASSI experiment aboard the San Marco D/L aeronomy satellite will monitor the airglow, solar, and interplanetary radiations from the EUV through the visible spectral regions. Four spectrometers with solar pointing control cover this broad region using channels with eighteen overlapping wavelength ranges with spectral resolutions from 0.8 to 3.0 nm, which are adequate for aeronomy. Large dynamic ranges up to 1:10 to the 11th permit the measurement of faint airglow or interplanetary radiation and intense solar emissions with one and the same instrument. Instrumental details such as the special optical design and calibration procedures are presented in detail.

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