Propagation of cosmic Rays Using the Time Parameter

Details Propagation of cosmic Rays Using the Time Parameter Propagation of cosmic Rays Using the Time Parameter

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..199s&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

A new code for calculation of the propagation of cosmic rays has been developed. The code uses time as the 2 integration variable, instead of the g/cm , that has been used historically. The computational technique and parameters used in the code are described. Two results from application of the code are presented: (1) a 10 9 numerically exact solution for the Be/ Be ratio over a wide range of energies in the Leaky Box model; (2) 10 9 the consequences for the Be/ Be ratio when cosmic rays are observed from inside a cavity ("bubble") of low density.

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