Solar wind control of plasma number density in the near Earth plasma sheet: three- dimensional structure

Details Solar wind control of plasma number density in the near Earth plasma sheet: three- dimensional structure Solar wind control of plasma number density in the near Earth plasma sheet: three- dimensional structure

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm12b..02n&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM12B-02

Physics

2744 Magnetotail, 2748 Magnetotail Boundary Layers, 2760 Plasma Convection (2463), 2764 Plasma Sheet, 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

Plasma number density in the near-Earth plasma sheet depends strongly on solar wind and IMF: (1) plasma sheet number density positively correlates with solar wind number density [Borovsky et al., 1998]. (2) plasma sheet number density positively correlates with theta angle of IMF with time lag of several-hours [Terasawa et al., 1997]. Recently, Nagata et al. [JGR in press] shows two-dimensional structure of such dependences in the near- Earth central plasma sheet (X<0, 9

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