Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsm54a..01z&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SM54A-01
Physics
2706 Cusp, 2724 Magnetopause And Boundary Layers, 2753 Numerical Modeling, 2764 Plasma Sheet, 2784 Solar Wind/Magnetosphere Interactions
Scientific paper
Multiple cusps have been observed by the Cluster spacecraft when the satellites were travelling outbound on Mar 21 and Mar 22, 2001. Evidences show that multiple cusps are a temporal effect which is due to the change of the solar wind azimuthal flow. The cusp properties derived from two MHD codes, Open GGCM and BATSRUS, have been compared with the Cluster observations. We find that although the simulated magnetospheres are smaller than the real magnetosphere, the simulated magnetic fields and the amplitude of the model-derived plasma parameters (velocity, density, temperature and thermal pressure) agree well with Cluster observations. The MHD code qualitatively simulated the responses of the cusp positions to the solar wind azimuthal flow (the wind sock effect).
Fritz Teresa A.
Raeder Joachim
Ridley Aaron J.
Siscoe George
Zhang Huazhong
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