Simulation Study of Dayside Magnetospheric Boundary Dynamics

Details Simulation Study of Dayside Magnetospheric Boundary Dynamics Simulation Study of Dayside Magnetospheric Boundary Dynamics

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsm31a..07p&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SM31A-07

Physics

2724 Magnetopause, Cusp, And Boundary Layers, 2753 Numerical Modeling, 2772 Plasma Waves And Instabilities, 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

Measurements by HEOS 2, Polar and Cluster II often indicate that dayside magnetospheric boundary regions at high latitudes are highly turbulent. Different and rather irregular flows are observed; density and temperature do not exhibit significant changes across the magnetopause; plasma mixing and transport are believed to occur (Haerendel and Paschmann, 1982). To obtain a better understanding of physics associated with these remarkable properties, we have made a detailed study of possible dynamical processes occurring in the boundary layers by using 2-D and 3-D simulations, resistive MHD and collisionless Hall MHD simulations. Simulation results and relevant discussions are present.

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