Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | SSC 3-1 - 3-4 |
| Journal | Geophysical Research Letters |
| Volume | 30 |
| Issue number | 17 |
| DOIs | |
| Publication status | Published - 2003 Sept 1 |
All Science Journal Classification (ASJC) codes
- Geophysics
- General Earth and Planetary Sciences