Numerical study of GCR proton transport
Fuente:
arXiv
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| Autori principali: | , , |
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| Natura: | Preprint |
| Pubblicazione: |
2022
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| Soggetti: | |
| Accesso online: | |
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| _version_ | 1866917829939298304 |
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| author | Yurovsky, V. O Peryatinskaya, A. I. Kudryashov, I. |
| author_facet | Yurovsky, V. O Peryatinskaya, A. I. Kudryashov, I. |
| contents | The paper numerically investigates the propagation of galactic cosmic rays in a model magnetic field, which is a composition of an isotropic turbulent field with the Kolmogorov turbulence spectrum and a regular constant field. The dependence of the diffusion tensor components on the particle energy is studied. It is shown that the transport anisotropy increases with decreasing energy. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2211_08873 |
| institution | arXiv |
| publishDate | 2022 |
| record_format | arxiv |
| spellingShingle | Numerical study of GCR proton transport Yurovsky, V. O Peryatinskaya, A. I. Kudryashov, I. High Energy Astrophysical Phenomena The paper numerically investigates the propagation of galactic cosmic rays in a model magnetic field, which is a composition of an isotropic turbulent field with the Kolmogorov turbulence spectrum and a regular constant field. The dependence of the diffusion tensor components on the particle energy is studied. It is shown that the transport anisotropy increases with decreasing energy. |
| title | Numerical study of GCR proton transport |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2211.08873 |