Physics
Scientific paper
May 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsm53a..02b&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SM53A-02
Physics
2730 Magnetosphere: Inner, 2768 Plasmasphere, 2784 Solar Wind/Magnetosphere Interactions, 2788 Magnetic Storms And Substorms (7954)
Scientific paper
When geomagnetic activity commences, sometimes the magnetosphere has a built up outer plasmasphere and sometimes it does not. The presence or absence of an outer plasmasphere may change the evolution of the solar-wind-driven magnetosphere. We investigate three things could differ owing to the effects of plasmaspheric plasma. (1) The high-mass-density plasmaspheric plasma may mass load magnetospheric convection. (2) The high-density plasmaspheric plasma could lead to enhanced loss of radiation-belt electrons. (3) The high-mass-density plasmaspheric plasma may choke reconnection at the dayside neutral line. Theoretical, experimental, and simulation evidence for all three processes are given.
Borovsky Joseph E.
Denton Michael H.
Hesse Matthias
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