Kinetic theory of propagation and 'runaway' of Galactic cosmic rays

Details Kinetic theory of propagation and 'runaway' of Galactic cosmic rays Kinetic theory of propagation and 'runaway' of Galactic cosmic rays

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..356d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 1, p. 356-359.

Astronomy and Astrophysics

Astrophysics

6

Charged Particles, Galactic Cosmic Rays, Halos, Particle Interactions, Particle Motion, Astronomical Models, Electromagnetic Scattering

Scientific paper

The size of the cosmic-ray halo is determined from the solution of the
kinetic equation describing particle propagation in a scattering medium.
For the case investigated it is shown that the halo scale depends on
particle energy. A possible consequence of this effect on cosmic-ray
grammage and anisotropy is discussed.

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