A global magnetohydrodynamic simulation of the magnetosphere when the interplanetary magnetic field is southward: The onset of magnetotail reconnection
- 1 October 1993
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 98 (A10), 17235-17249
- https://doi.org/10.1029/93ja01321
Abstract
No abstract availableKeywords
This publication has 51 references indexed in Scilit:
- The magnetic topology of the plasmoid flux rope in a MHD-simulation of magnetotail reconnectionPublished by Wiley ,1990
- Average plasma properties in the central plasma sheetJournal of Geophysical Research, 1989
- Three-dimensional computer modeling of dynamic reconnection in the magnetotail: Plasmoid signatures in the near and distant tailPublished by Wiley ,1984
- Particle and field signatures of substorms in the near magnetotailPublished by Wiley ,1984
- Self‐consistent theory of three‐dimensional convection in the geomagnetic tailJournal of Geophysical Research, 1983
- A time dependent three‐dimensional simulation of the Earth's magnetosphere: Reconnection eventsJournal of Geophysical Research, 1982
- Magnetospheric substorms: A newly emerging modelPlanetary and Space Science, 1981
- Three‐dimensional computer modeling of dynamic reconnection in the geomagnetic tailJournal of Geophysical Research, 1981
- Dynamics of the aurora—IVJournal of Atmospheric and Terrestrial Physics, 1966
- The dynamics of the aurora—II Westward traveling surgesJournal of Atmospheric and Terrestrial Physics, 1965