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AbstractAbstract
[en] From measured COS-B gamma ray data it is possible to derive the variation of the ratio of the galactic gamma ray flux in the two energy intervals 70-300 MeV and 300-2,000 MeV as a function of galactic latitude for two longitudinal regions. It is shown that this energy ratio is a good test between a more proton and a more electron induced origin of galactic gamma rays. (orig.)
[de]
Aus gemessenen COS-B-Gammastrahlungsdaten kann die Variation des galaktischen Gamma-Flussverhaeltnisses in den beiden Energieintervallen 70-300 MeV und 300-2.000 MeV in Abhaengigkeit von der galaktischen Breite fuer zwei Breitenbereiche bestimmt werden. Es zeigt sich, dass dieses Energieverhaeltnis zur Unterscheidung eines eher proton- bzw. eines eher elektron-induzierten Ursprungs galaktischer Gammastrahlung gut geeignet ist. (orig.)Primary Subject
Source
1977; 7 p; 37. annual meeting of the Deutsche Physikalische Gesellschaft e.V. in conjunction with the spring meeting of the Arbeitsgemeinschaft Extraterrestrische Physik; Braunschweig, Germany, F.R; 28 Mar - 1 Apr 1977; 2 figs.; 14 refs.
Record Type
Miscellaneous
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Conference
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BASIC INTERACTIONS, BOSONS, COSMIC RADIATION, COSMIC RAY SOURCES, ELASTIC SCATTERING, ELECTROMAGNETIC INTERACTIONS, ELECTROMAGNETIC RADIATION, ELEMENTARY PARTICLES, ENERGY RANGE, HADRONS, INTERACTIONS, IONIZING RADIATIONS, MESONS, MEV RANGE, PIONS, PSEUDOSCALAR MESONS, RADIATION FLUX, RADIATIONS, SCATTERING
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