Radial distribution of cosmic ray intensity in the galaxy from gamma-ray data

Details Radial distribution of cosmic ray intensity in the galaxy from gamma-ray data Radial distribution of cosmic ray intensity in the galaxy from gamma-ray data

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..325g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 325-328 (SEE N85-33902 22-93)

Physics

Cosmic Rays, Galactic Radiation, Gamma Rays, Gas Density, Radial Distribution, Radiant Flux Density, Bremsstrahlung, Electrons, Emissivity, Gradients, Hydrogen, Longitude, Nucleons, Particle Energy, Sas-2

Scientific paper

The radial distributions of galactic γ-ray emissivity and cosmic ray intensity are derived by unfolding the SAS 2 line flux data. The results show a marked gradient, with the cosmic ray intensity in the region 3 < R < 7 kpc being 3 - 4 times as much as locally. There is also an indication for a higher gradient for cosmic rays of lower energy.

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