Effects from diffusive reacceleration on propagating cosmic rays

Details Effects from diffusive reacceleration on propagating cosmic rays Effects from diffusive reacceleration on propagating cosmic rays

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19..781s&link_type=abstract

Advances in Space Research, Volume 19, Issue 5, p. 781-786.

Physics

Scientific paper

According to the diffusive reacceleration model the transport of cosmic ray particles is controlled by diffusion where the particles scatter on hydromagnetic waves. As a consequence they encounter stochastic 2nd order Fermi acceleration. This physical scenario can explain the cosmic ray observations but it leads to a mean escape length which is different from that obtained from Leaky Box calculations. We will explain how this works.

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