Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 81-88 |
| Number of pages | 8 |
| Journal | Journal of Astrophysics and Astronomy |
| Volume | 31 |
| Issue number | 2 |
| DOIs | |
| State | Published - 2010 |
| Externally published | Yes |
Keywords
- Cosmic rays
- ISM: galactic locations
- stochastic processes
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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