Diffuse cosmic gamma-ray observations from 0.3 to 6 MeV in two regions near the Galactic center and anticenter

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cosmic Rays, Diffuse Radiation, Galactic Nuclei, Gamma Ray Astronomy, Background Radiation, Gamma Ray Telescopes, Graphs (Charts), X Ray Spectra

Scientific paper

The results obtained on the diffuse component of cosmic radiation between 0.3 and 6 MeV from two gamma-ray telescope balloon observations in two regions - near the Galactic center and near the anticenter - are presented. The spectra obtained are deduced from fluxes measured by the detector; the background induced by various atmospheric components, such as photons, neutrons, and protons, at two flight latitudes (44 deg 30 min N and 22 deg 48 min S) is calculated. Although the accuracy of the results does not permit a final conclusion, the comparison of spectra obtained under very different background conditions for the two regions observed gives evidence for the isotropy of the diffuse component.

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