MHD Models for Multi-Spacecraft / Ground-based Data Analysis and Conjunction Visualizations

Details MHD Models for Multi-Spacecraft / Ground-based Data Analysis and Conjunction Visualizations MHD Models for Multi-Spacecraft / Ground-based Data Analysis and Conjunction Visualizations

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..359..125d&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

2

Scientific paper

The BATS-R-US MHD code is used to describe the large-scale structure of the magnetosphere whereby the model parameters are constrained by multi spacecraft Cluster data in the post-noon high-latitude magnetopause region. We discuss the potentials of the model in combination with the experimental data to accurately describe the dynamics of these regions in three-dimensions. A major aspect of this potential is to make predictions about the configuration of flux tubes at the magnetopause boundary and to visualize the open flux tubes passing by the spacecraft and observed simultaneously by ionospheric radars.

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