Solar Wind Transport Into Magnetosphere Caused by Magnetic Reconnection During Southward and Northward IMF

Details Solar Wind Transport Into Magnetosphere Caused by Magnetic Reconnection During Southward and Northward IMF Solar Wind Transport Into Magnetosphere Caused by Magnetic Reconnection During Southward and Northward IMF

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agusmsm32a..02y&link_type=abstract

American Geophysical Union, Spring Meeting 2009, abstract #SM32A-02

Physics

2723 Magnetic Reconnection (7526, 7835), 2724 Magnetopause And Boundary Layers, 2784 Solar Wind/Magnetosphere Interactions, 7859 Transport Processes

Scientific paper

Reconnection is considered as the dominant mechanism of the solar wind transport into magnetosphere. Here, two cases under southward and northward IMF respectively are analyzed, with the results as follows: Firstly, by analyzing measurements from Cluster, an event of magnetopause crossing has been investigated. At the latitude of about 40

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