Energy spectra of cosmic rays with energies higher than 10 to the 19th eV for different directions of the celestial sphere

Details Energy spectra of cosmic rays with energies higher than 10 to the 19th eV for different directions of the celestial sphere Energy spectra of cosmic rays with energies higher than 10 to the 19th eV for different directions of the celestial sphere

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..597m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, July 1989, p. 597-602. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Celestial Sphere, Energy Spectra, Galactic Cosmic Rays, Astronomical Spectroscopy, Local Group (Astronomy), Milky Way Galaxy

Scientific paper

The directions of arrival of cosmic rays with energies of greater than
10 to the 19th eV are studied. It is shown that, up to 4 x 10 to the
19th eV, the cosmic ray flux maximum is observed from the direction of
the galactic plane. This is above 4 x 10 to the 19th eV from the central
part of the local supercluster.

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