Physics
Scientific paper
Oct 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998georl..25.3751e&link_type=abstract
Geophysical Research Letters, Volume 25, Issue 20, p. 3751-3754
Physics
29
Magnetospheric Physics: Magnetosphere-Inner, Magnetospheric Physics: Numerical Modeling, Magnetospheric Physics: Ring Current, Magnetospheric Physics: Storms And Substorms
Scientific paper
The ring current buildup depending on the solar wind density and the time-dependent convection field is examined by using a particle tracing scheme. To obtain the current density, energetic protons injected from the night side boundary at L=9 are traced under the dipolar magnetic field and the Kp dependent model of the Volland-Stern type convection field. The source distribution function at the boundary is assumed to be isotropic Maxwellian with a temperature of 5 keV and a number density depending on the solar wind density. We derive the corrected Dst (Dst*) from the Biot-Savart integral over the whole three-dimensional distribution of the calculated current density. The results are compared with the observed Dst* in the three successive storms in April 1997; the major variation of the Dst* is mainly due to the convection electric field and the solar wind density as well.
Ebihara Yasuhiro
Ejiri Masaki
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