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...
| Main Author: | |
|---|---|
| Published: |
North-West University
2009
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/10394/1814 |