Markov stochastic technique to determine galactic cosmic ray sources distribution

Details Markov stochastic technique to determine galactic cosmic ray sources distribution Markov stochastic technique to determine galactic cosmic ray sources distribution

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010japa...31...81f&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 31, Issue 2, pp.81-88

Astronomy and Astrophysics

Astrophysics

Cosmic Rays, Ism: Galactic Locations, Stochastic Processes

Scientific paper

A new numerical model of particle propagation in the Galaxy has been developed, which allows the study of cosmic-ray production and propagation in 2D. The model has been used to solve cosmic ray diffusive transport equation with a complete network of nuclear interactions using the time backward Markov stochastic process by tracing the particles’ trajectories starting from the Solar System back to their sources in the Galaxy. This paper describes a further development of the model to calculate the contribution of various galactic locations to the production of certain cosmic ray nuclei observed at the Solar System.

Affiliated with

Also associated with

No associations

Rating

Markov stochastic technique to determine galactic cosmic ray sources distribution 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 Markov stochastic technique to determine galactic cosmic ray sources distribution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Markov stochastic technique to determine galactic cosmic ray sources distribution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1831280