1979
DOI: 10.1029/ja084ia03p00967
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Bremsstrahlwung produced by precipitating electrons

Abstract: Theoretical values are presented of the bremsstrahlung flux escaping the atmosphere for various incident electron fluxes. The assumed incident electron fluxes were isotropic with exponential energy spectra. The escaping bremsstrahlung intensity, energy spectra, and angular d•stributions depend on the incident electron flux characteristics, indicating that measurements of bremsstrahlung can be used to derive information on the electron precipitation.

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Cited by 36 publications
(28 citation statements)
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“…The ®rst model was developed by Berger and Seltzer (1972) and Seltzer and Berger (1974), and the second model by Walt et al (1979). These models are used to calculate the X-ray bremsstrahlung produced by energetic electrons that precipitate into the atmosphere.…”
Section: The Modelsmentioning
confidence: 99%
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“…The ®rst model was developed by Berger and Seltzer (1972) and Seltzer and Berger (1974), and the second model by Walt et al (1979). These models are used to calculate the X-ray bremsstrahlung produced by energetic electrons that precipitate into the atmosphere.…”
Section: The Modelsmentioning
confidence: 99%
“…Then we apply the model of Walt et al (1979) to ®nd the X-ray yield in the direction of the FOV of our X-ray detector. In our chosen azimuth sector 0 ±30 and time-interval (135±199-s¯ight time) the detector was looking at X-rays coming up at elevation angles of 33X4 to 54X3…”
Section: The Modelsmentioning
confidence: 99%
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