Photoelectric array detectors for use at XUV wavelengths

Details Photoelectric array detectors for use at XUV wavelengths Photoelectric array detectors for use at XUV wavelengths

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...29..461t&link_type=abstract

(Schweizerische Naturforschende Gesellschaft and Eidgenoesische Technische Hochschule Zuerich, Conference on Solar Physics from

Astronomy and Astrophysics

Astronomy

1

Extreme Ultraviolet Radiation, Photometers, Solar Spectra, Spacelab Payloads, Ultraviolet Astronomy, X Ray Astronomy, Far Ultraviolet Radiation, Grist (Telescope), Spaceborne Astronomy

Scientific paper

The characteristics of photoelectric detector systems for use at visible-light, ultraviolet, and X-ray wavelengths are briefly reviewed in the context of the needs of the Spacelab solar-physics facilities. Photoelectric array detectors for use at XUV wavelengths between 90 and 1500 A are described, and their use in the ESA Grazing-Incidence Solar Telescope (GRIST) facility is discussed.

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