A semiempirical magnetosheath model to analyze the solar wind‐magnetosphere interaction
- 1 December 2000
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 105 (A12) , 27469-27479
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- On the processes in the terrestrial magnetosheath: 1. Scheme developmentJournal of Geophysical Research, 1999
- A test particle simulation of the motion of oxygen ions and solar wind protons near MarsJournal of Geophysical Research, 1999
- A new functional form to study the solar wind control of the magnetopause size and shapeJournal of Geophysical Research, 1997
- Magnetic field orientation effects on the standoff distance of Earth's bow shockGeophysical Research Letters, 1996
- Modeling the entry of magnetosheath electrons into the dayside ionosphereJournal of Geophysical Research, 1996
- An empirical model of the solar wind flow around MarsJournal of Geophysical Research, 1996
- Magnetic field and plasma flow structure near the magnetopauseJournal of Geophysical Research, 1995
- The magnetosheath region adjacent to the dayside magnetopause: AMPTE/IRM observationsJournal of Geophysical Research, 1994
- On the spatial range of validity of the gas dynamic model in the magnetosheath of VenusGeophysical Research Letters, 1993
- A mathematical magnetospheric field model with independent physical parametersPlanetary and Space Science, 1981