On Kelvin–Helmholtz instability due to the solar wind interaction with unmagnetized planets
- 31 October 2007
- journal article
- Published by Elsevier BV in Planetary and Space Science
- Vol. 55 (12), 1811-1816
- https://doi.org/10.1016/j.pss.2007.01.015
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Solar wind flow past Venus and its implications for the occurrence of the Kelvin–Helmholtz instabilityPlanetary and Space Science, 2007
- The stability of the pristine magnetopausePlanetary and Space Science, 2003
- A two‐dimensional simulation of the Kelvin‐Helmholtz instability with magnetic shearJournal of Geophysical Research, 1999
- Simulation of the Kelvin‐Helmholtz Instability in the Magnetized Slab JetThe Astrophysical Journal, 1997
- Kelvin‐Helmholtz instability at the magnetospheric boundary: Dependence on the magnetosheath sonic Mach numberJournal of Geophysical Research, 1992
- On the stability of the ionopause of VenusJournal of Geophysical Research, 1984
- Anomalous transport by magnetohydrodynamic Kelvin‐Helmholtz instabilities in the solar wind‐magnetosphere interactionJournal of Geophysical Research, 1984
- On the penetration of the solar wind into the cometary ionosphereThe Astrophysical Journal, 1983
- Plasma clouds above the ionopause of Venus and their implicationsPlanetary and Space Science, 1982
- The dynamic behavior of the Venus ionosphere in response to solar wind interactionsJournal of Geophysical Research, 1980