Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...411..690m&link_type=abstract
Astrophysical Journal - Part 1 (ISSN 0004-637X), vol. 411, no. 2, p. 690-707.
Astronomy and Astrophysics
Astrophysics
6
Computerized Simulation, Cosmic Rays, Particle Acceleration, Supernova Remnants, Three Dimensional Models, Astronomical Models, Milky Way Galaxy, Shock Wave Interaction, Spatial Distribution
Scientific paper
The present 3D code for simulating SNR distributed cosmic-ray acceleration encompasses the decoupling of the main acceleration region and secondary particle production region. Two transport mechanisms are taken into account: diffusion and random wandering of the convective cells. The geometry of the Galaxy is approximated by a thick disk within which the remnants are located; this disk is immersed in a larger, porous-walled box within which the medium density is negligible, and the diffusion coefficient is constant. Several observed features of galactic cosmic rays are reproduced.
Medina Tanco Gustavo A.
Opher Reuven
No associations
LandOfFree
Spatial and temporal distributed acceleration of cosmic rays by supernova remnants three-dimensional simulations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spatial and temporal distributed acceleration of cosmic rays by supernova remnants three-dimensional simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatial and temporal distributed acceleration of cosmic rays by supernova remnants three-dimensional simulations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1069371