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On the consequences of Fisk's type magnetic field configuration for galactic cosmic ray modulation
Three-dimensional steady state transport equation of galactic cosmic rays with drift included is solved by means of newly achieved Fortran code in two cases: 1) Fisk’s type of heliospheric magnetic field dominates in the heliosphere; 2) standard Parker field fills the interplanetary space. The spher...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2005
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| Series: | Кинематика и физика небесных тел |
| Subjects: | |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/79633 |
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