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Bremsstrahlung effects in energetic particle detectors
Author(s) -
Tuszewski M.,
Cayton T. E.,
Ingraham J. C.,
Kippen R. M.
Publication year - 2004
Publication title -
space weather
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.254
H-Index - 56
ISSN - 1542-7390
DOI - 10.1029/2003sw000057
Subject(s) - bremsstrahlung , detector , physics , computational physics , charged particle , satellite , electron , van allen radiation belt , magnetosphere , particle detector , radiation , nuclear physics , particle (ecology) , particle radiation , noise (video) , ion , optics , plasma , astronomy , computer science , oceanography , quantum mechanics , artificial intelligence , image (mathematics) , geology
The energetic charged particles of the Earth's magnetosphere are routinely detected by solid‐state satellite instruments. Quantitative data are increasingly required for engineering dose calculations and for space weather science. However, the design of some energetic particle detectors can be severely constrained. Background effects must be accurately modeled in such cases to extract quantitative information. In particular, bremsstrahlung radiation from electrons impacting the detector and the satellite often dominates the background noise. Numerical tools are presented here to calculate total bremsstrahlung effects in energetic electron detectors. The calculations are illustrated for the low‐energy particle detector of current Global Positioning System satellites.

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