Daum, Patrick and Wild, J.A. (2006) MHD models for multi-spacecraft / ground-based data analysis and conjunction visualizations. In: Numerical modeling of space plasma flows, 1900-01-01.
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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.
|Item Type:||Conference or Workshop Item (Paper)|
|Journal or Publication Title:||Numerical modeling of space plasma flows|
|Uncontrolled Keywords:||DCS-publications-id ; inproc-517 ; DCS-publications-personnel-id ; 108 ; 104|
|Subjects:||Q Science > QC Physics|
|Departments:||Faculty of Science and Technology > School of Computing & Communications|
Faculty of Science and Technology > Physics
|Deposited By:||Dr Steve Marple|
|Deposited On:||06 Sep 2009 14:00|
|Last Modified:||24 May 2016 00:02|
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