Cosmic ray path length distributions from superbubble/giant HII regions

Details Cosmic ray path length distributions from superbubble/giant HII regions Cosmic ray path length distributions from superbubble/giant HII regions

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..528..429h&link_type=abstract

ACCELERATION AND TRANSPORT OF ENERGETIC PARTICLES OBSERVED IN THE HELIOSPHERE: ACE 2000 Symposium. AIP Conference Proceedings, V

Astronomy and Astrophysics

Astronomy

2

Cosmic Rays, Interstellar Medium And Nebulae In Milky Way, Supernovae

Scientific paper

We have constructed a Monte Carlo Simulation program for the space and time dependent distribution of Galactic supernovae, as a source of both shock energy and particles for cosmic ray acceleration, based on recent astronomical observations and theory. From these simulated spatial and temporal distributions of discrete sources, we then determine the form and variance of the expected local cosmic ray path length distributions, together with anisotropies and local intensity histories, for a wide range of effective mean free paths. .

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