Modeling of galactic cosmic rays in the heliosphere / Mabedle Donald Ngobeni
The modulation of galactic cosmic ray (GCR) Carbon in a north-south asymmetrical heliosphere is studied, using a two-dimensional numerical model that contains a solar wind termination shock (TS), a heliosheath, as well as particle drifts and diffusive shock re-acceleration of GCRs. The asymmetry in...
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| Language: | en |
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2015
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| Online Access: | http://hdl.handle.net/10394/15476 |