Published May 1984 | Version v1
Journal article Metadata-only

Cosmic ray anisotropy at energies of 5 x 1011 - 1014 eV in the diffusion approximation

Creators

  • 1. AN SSSR, Moscow. Inst. Zemnogo Magnetizma, Ionosfery i Rasprostraneniya Radiovoln

Description

The 2nd and 3rd angular harmonic amplitudes for cosmic ray diffusing in the interstellar medium ape calculated. The observed amplitude of the 2nd harmonic is due apparently to the inhomogeneity of the local galactic magnetic field at a scale of 3-10 pc

Additional details

Additional titles

Original title (Russian)
Анизотропия космических лучей при энергиях 5 x 10

Publishing Information

Journal Title
Astron. Zh.
Journal Volume
61
Journal Issue
3
Series
Astron. Zh.
Journal Page Range
610-613
ISSN
0004-6299

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
16029005
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ANGULAR DISTRIBUTION; ANISOTROPY; COSMIC RAY FLUX; GEV RANGE 100-1000; HARD COMPONENT; INTERSTELLAR SPACE; PRIMARY COSMIC RADIATION; TEV RANGE 01-10; TEV RANGE 10-100
Descriptors DEC
COSMIC RADIATION; DISTRIBUTION; ENERGY RANGE; GEV RANGE; IONIZING RADIATIONS; RADIATION FLUX; RADIATIONS; SPACE; TEV RANGE

Optional Information

Notes
For English translation see the journal Soviet Astronomy (USA).