Particle background effects for Hubble Space Telescope (HST) and the Lyman Far Ultraviolet Spectroscopic Explorer

Details Particle background effects for Hubble Space Telescope (HST) and the Lyman Far Ultraviolet Spectroscopic Explorer Particle background effects for Hubble Space Telescope (HST) and the Lyman Far Ultraviolet Spectroscopic Explorer

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aipc..186..468w&link_type=abstract

IN: High-energy radiation background in space (A90-25305 09-93). New York, American Institute of Physics, 1989, p. 468-482.

Physics

Far Uv Spectroscopic Explorer, Hubble Space Telescope, Light (Visible Radiation), Lyman Spectra, Radiation Detectors, Radiation Hazards, Cerenkov Radiation, Charge Coupled Devices, Energetic Particles, Fluorescence, Phosphorescence, Trapped Particles

Scientific paper

Requirements on orbital background counting rates are described for the UV and visible detectors on the planned second generation instrument Space Telescope Imaging Spectrograph (STIS) and for the proposed Lyman Far Ultraviolet Spectroscopic Explorer. Expected background rates and shielding requirements are analyzed for detector types in both instruments for low earth orbits, and for high orbits in the case of Lyman.

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