Modelling of the heliosphere and cosmic ray transport / Jasper L. Snyman
A two dimensional hydrodynamic model describing the solar wind interaction with the local interstellar medium, which surrounds the solar system, is used to study the heliosphere both as a steady-state- and dynamic structure. The finite volume method used to solve the associated system of hydrodynami...
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North-West University
2009
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| Online Access: | http://hdl.handle.net/10394/1814 |
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