Prediction of galactic cosmic ray intensity variation for a few (up to 10-12) years ahead on the basis of convection-diffusion and drift model
We determine the dimension of the Heliosphere (modulation region), radial diffusion coefficient and other parameters of convection-diffusion and drift mechanisms of cosmic ray (CR) long-term variation, depending on particle energy, the level of solar activity (SA) and general solar magnetic fiel...
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2005-11-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/23/3003/2005/angeo-23-3003-2005.pdf |