A solar spectrograph for occultation and solar flux measurements in the solar system

Details A solar spectrograph for occultation and solar flux measurements in the solar system A solar spectrograph for occultation and solar flux measurements in the solar system

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1745..110s&link_type=abstract

In: Instrumentation for planetary and terrestrial atmospheric remote sensing; Proceedings of the Meeting, San Diego, CA, July 23

Computer Science

Sound

Extreme Ultraviolet Radiation, Planetary Atmospheres, Solar Flux, Solar Planetary Interactions, Solar Spectrometers, Atmospheric Sounding, Solar System, Spectrographs, Stellar Occultation

Scientific paper

A compact solar spectrograph based on the Rowland grazing-incidence design has been developed that covers 200-3200 A and has no moving parts; it will record the entire spectrum within its range in a single exposure on the basis of pinhole optics. Three gratings are used and these are recorded on a single CCD focal plane detector. Methods used to minimize the effects of scattering include its suppression with coatings and optical components; a detector layout that subtracts scattered light effects, and a photocathode that discriminates against long wavelengths.

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