Physics
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003georl..30qssc3z&link_type=abstract
Geophysical Research Letters, Volume 30, Issue 17, pp. SSC 3-1, CiteID 1883, DOI 10.1029/2003GL017456
Physics
13
Magnetospheric Physics: Magnetospheric Configuration And Dynamics, Magnetospheric Physics: Current Systems (2409), Magnetospheric Physics: Magnetosphere-Inner, Magnetospheric Physics: Storms And Substorms
Scientific paper
Two important observed substorm growth phase phenomena are modeled: the formation of a near-Earth (|X| ~ 8 RE) thin cross-tail current sheet, as well as the equatorward shift of the ionospheric Birkeland currents. Our study is performed by solving the 3D force-balance equation with realistic boundary conditions and pressure distributions. The obtained cross-tail current sheet has large current density (Jφ ~ 10 nA/m2) and a half-thickness in the north-south direction of ~1 RE, while plasma β is very high (β ~ 40) in the current sheet region. The Region-1 and Region-2 Birkeland currents, formed on closed field lines due to pressure gradients, move equatorward and become more intense (J∥max ~ 3 μA/m2) compared to quiet times. The results agree with growth phase observations. We also find that the cross-tail current sheet maps into the ionosphere in the transition region between the Region-1 and Region-2 currents.
Cheng C. Z.
Zaharia Sorin
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