Gasdynamic and magnetohydrodynamic modeling of the magnetosheath: A tutorial
- 1 July 1994
- journal article
- Published by Elsevier in Advances In Space Research
- Vol. 14 (7) , 5-19
- https://doi.org/10.1016/0273-1177(94)90042-6
Abstract
No abstract availableThis publication has 10 references indexed in Scilit:
- Solar cycle variations in the neutral exosphere inferred from the location of the Venus bow shockAdvances In Space Research, 1990
- A three dimensional gasdynamic model for solar wind flow past nonaxisymmetric magnetospheres: Application to Jupiter and SaturnJournal of Geophysical Research, 1989
- The effect of the hot oxygen corona on the interaction of the solar wind with VenusGeophysical Research Letters, 1987
- A gas dynamic magnetosheath field model for unsteady interplanetary fields: Application to the solar wind interaction with VenusJournal of Geophysical Research, 1986
- Solar wind flow about the outer planets: Gas dynamic modeling of the Jupiter and Saturn bow shocksJournal of Geophysical Research, 1985
- The magnetic field of Mars: Implications from gas dynamic modelingJournal of Geophysical Research, 1984
- Hot oxygen atoms in the upper atmosphere of VenusGeophysical Research Letters, 1981
- A new predictive model for determining solar wind‐terrestrial planet interactionsJournal of Geophysical Research, 1980
- Aligned magnetohydrodynamic solution for solar wind flow past the earth's magnetosphereActa Astronautica, 1974
- Hydromagnetic flow around the magnetospherePlanetary and Space Science, 1966