Simple models of time-dependent reconnection in a collision-free plasma with an application to substorms in the geomagnetic tail
- 30 April 1987
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 35 (4) , 451-466
- https://doi.org/10.1016/0032-0633(87)90102-4
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- ISEE‐3 distant Geotail resultsGeophysical Research Letters, 1984
- Detailed examination of a plasmoid in the distant magnetotail with ISEE 3Geophysical Research Letters, 1984
- Direct observations of passages of the distant neutral line (80‐140 RE) following substorm pnsets: ISEE‐3Geophysical Research Letters, 1984
- Substorm associated traveling compression regions in the distant tail: Isee‐3 Geotail observationsGeophysical Research Letters, 1984
- Evidence for the tailward retreat of a magnetic neutral line in the magnetotail during substorm recoveryGeophysical Research Letters, 1981
- Some properties of a steady‐state geomagnetic tailGeophysical Research Letters, 1980
- The warm current sheet model, and its implications on the temporal behaviour of the geomagnetic tailPlanetary and Space Science, 1974
- The self-consistent geomagnetic tail under static conditionsPlanetary and Space Science, 1972
- Consistency of fields and particle motion in the ‘Speiser’ model of the current sheetPlanetary and Space Science, 1972
- Magneto-Hydrodynamic ShocksPhysical Review B, 1950