MHD Simulations of the Solar Wind and ICME Dynamics from the Inner to the Outer Heliosphere

Details MHD Simulations of the Solar Wind and ICME Dynamics from the Inner to the Outer Heliosphere MHD Simulations of the Solar Wind and ICME Dynamics from the Inner to the Outer Heliosphere

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..359..220w&link_type=abstract

Numerical Modeling of Space Plasma Flows: Astronum-2006 ASP Conference Series, Volume 359, Proceedings of the Conference Held 26

Astronomy and Astrophysics

Astronomy

Scientific paper

We summarize recent work on MHD modeling of solar wind and interplanetary coronal mass ejection (ICME) evolution from the inner to the outer heliosphere. First, we describe the multi-fluid MHD model, which takes into account the effects of pickup ions, that we use to propagate the solar wind to the outer heliosphere. Then we use observations from spacecraft distributed throughout the heliosphere to trace ICMEs and shocks they drive from the inner heliosphere to the location of Voyager 2.

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