Radial intensity gradients of galactic cosmic rays in the heliosphere at solar maximum: 1D no-shock simulation
We study the spatial distribution of galactic cosmic rays in the heliosphere at solar maximum of cycles 21, 22 and 23, using a one-dimensional no-shock model of the cosmic ray transport equation. We investigate the radial intensity gradients from 1 AU to the distant heliosphere and interpret the dat...
Gorde:
| Argitaratua izan da: | Geofísica Internacional |
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| Egile Nagusiak: | , |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2009
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| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=56813223006 |
| Etiketak: |
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