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Paper: The Effects of the Sun Rotation on the Solar Wind Propagation
Volume: 444, 5th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2010)
Page: 105
Authors: Borovikov, S. N.; Pogorelov, N. V.
Abstract: We develop a numerical model of the corotating interaction regions which form as a consequence of the fast and slow wind interaction. The numerical model is verified against similar simulations performed by Pizzo and a good agreement with his results are found. Finally, we show preliminary results of propagating corotating interaction regions into the inner heliosheath.
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