Published August 1985 | Version v1
Report Metadata-only

Simulation of high energy cosmic ray propagation 2

Creators

  • 1. Kobe Univ., Japan
  • 2. Kyoto Univ., Japan

Description

The cosmic ray propagation in the Galactic arm is simulated. The Galactic magnetic fields are known to go along with so called Galactic arms as a main structure with turbulences of the scale about 30pc. The distribution of cosmic ray in Galactic arm is studied. The escape time and the possible anisotropies caused by the arm structure are discussed

Additional details

Publishing Information

Imprint Title
Ninteenth International Cosmic Ray Conference. OG sessions, volume 2
Journal Page Range
vp.
Report number
NASA-CP--2376-VOL-2

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17080828
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Non-conventional Literature
Descriptors DEI
ANISOTROPY; COSMIC RAY PROPAGATION; COSMIC SHOWERS; MAGNETIC FIELDS; MILKY WAY; MORPHOLOGICAL CHANGES; SIMULATION; SPATIAL DISTRIBUTION
Descriptors DEC
COSMIC RADIATION; DISTRIBUTION; GALAXIES; IONIZING RADIATIONS; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS