Solar wind flow about the terrestrial planets: 2. Comparison with gas dynamic theory and implications for solar‐planetary interactions
- 1 January 1983
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 88 (A1), 19-35
- https://doi.org/10.1029/ja088ia01p00019
Abstract
No abstract availableThis publication has 104 references indexed in Scilit:
- Observations of mass addition to the shocked solar wind of the Venusian ionosheathGeophysical Research Letters, 1982
- Loss of oxygen from VenusGeophysical Research Letters, 1982
- Magnetic field and plasma wave observations in a plasma cloud at VenusGeophysical Research Letters, 1982
- Evidence for the acceleration of ionospheric O+ in the magnetosheath of VenusGeophysical Research Letters, 1981
- The effects on the Earth's magnetotail from shocks in the solar windGeophysical Research Letters, 1980
- A comparison of Pioneer Venus and Venera bow shock observations: Evidence for a solar cycle variationGeophysical Research Letters, 1979
- Position and shape of the Venus bow shock: Pioneer Venus Orbiter observationsGeophysical Research Letters, 1979
- Axisymmetric Implicit Blunt-Body Computation of Solar Wind Flows Past PlanetsAIAA Journal, 1978
- Solar wind interaction with planetary atmospheresReviews of Geophysics, 1971
- III. The electrical conductivity of the Moon - The electrical conductivity of the Moon’s interiorProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1967