The Effects of the Sun Rotation on the Solar Wind Propagation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

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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