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NASA NTRS · 19660059977

Extended source of energetic cosmic X rays.

Boldt, E.·Mcdonald, F. B.·Riegler, G.·Serlemitsos, P.
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Abstract

Cosmic X-ray source near direction of north galactic pole, noting empirical results from balloon observations

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COSMIC RADIATIONBALLOON SOUNDINGX-RAY ANALYSIS

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BibTeXRIS

Boldt, E., Mcdonald, F. B., Riegler, G., Serlemitsos, P.. 1966-08-22. Extended source of energetic cosmic X rays.. https://ntrs.nasa.gov/citations/19660059977

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Cosmic-ray background fluxes were modeled based on existing measurements and theories and are presented here. The model, originally developed for the Gamma-ray Large Area Space Telescope (GLAST) Balloon Experiment, covers the entire solid angle (4(pi) sr), the sensitive energy range of the instrument ((approx) 10 MeV to 100 GeV) and abundant components (proton, alpha, e(sup -), e(sup +), (mu)(sup -), (mu)(sup +) and gamma). It is expressed in analytic functions in which modulations due to the solar activity and the Earth geomagnetism are parameterized. Although the model is intended to be used primarily for the GLAST Balloon Experiment, model functions in low-Earth orbit are also presented and can be used for other high energy astrophysical missions. The model has been validated via comparison with the data of the GLAST Balloon Experiment.

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