Structure of irregular galactic magnetic fields

Details Structure of irregular galactic magnetic fields Structure of irregular galactic magnetic fields

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.255..689s&link_type=abstract

Nature, vol. 255, June 26, 1975, p. 689, 690.

Computer Science

4

Galactic Structure, High Energy Interactions, Magnetic Field Configurations, Primary Cosmic Rays, Anisotropy, Diffuse Radiation, Energy Spectra, Particle Motion, Proton Energy, X Ray Density Measurement

Scientific paper

A description is given of a method for determining the structural composition of random galactic fields on the basis of cosmic-ray measurements. The applicability of the described method depends essentially on the validity of the diffusion approximation in describing the propagation of cosmic rays in the energy range from 1 TeV to 1,000 TeV.

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