1992
DOI: 10.1016/0273-1177(92)90124-g
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Gamma-ray measurements from the space shuttle during a solar flare

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Cited by 7 publications
(2 citation statements)
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“…It is well known that optical elements that are placed into orbit around the Earth experience harsh radiation environments that originate from trapped-particle belts, cosmic rays, and solar events 9 . Of particular interest to optical materials is the continuous flux of energetic protons, hard x-rays, and gamma photons that the materials encounter 9,10 . These types of radiation exposures lead to the excitation of electrons and the subsequent formation of color centers in the materials 7,11 .…”
Section: Introductionmentioning
confidence: 99%
“…It is well known that optical elements that are placed into orbit around the Earth experience harsh radiation environments that originate from trapped-particle belts, cosmic rays, and solar events 9 . Of particular interest to optical materials is the continuous flux of energetic protons, hard x-rays, and gamma photons that the materials encounter 9,10 . These types of radiation exposures lead to the excitation of electrons and the subsequent formation of color centers in the materials 7,11 .…”
Section: Introductionmentioning
confidence: 99%
“…During the last high latitude passage (south) for the SAM measurement the detector recorded gamma-ray flux levels that exceed all but one of the preceding S A A passages. While it is likely that those fluxes were primarily due to electron bremsstrahlung, there may also be a contribution from the secondary reaction products from high energy protons [9].…”
Section: Pre-flight Measurementsmentioning
confidence: 99%