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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| Veröffentlicht in: | Кинематика и физика небесных тел |
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| Datum: | 2005 |
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Головна астрономічна обсерваторія НАН України
2005
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| Schlagworte: | |
| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/79633 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | On the consequences of Fisk's type magnetic field configuration for galactic cosmic ray modulation / Z. Kobylinski, A. Ajabshirizadeh, A. Wysokinski // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 159-164. — Бібліогр.: 26 назв. — англ. |