Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets—II. Two-fluid HD model
- 31 January 1992
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 40 (1) , 131-138
- https://doi.org/10.1016/0032-0633(92)90155-h
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets—I. Features of the solar wind interaction with planetsPlanetary and Space Science, 1992
- First measurements of plasma waves near MarsNature, 1989
- Magnetic fields near Mars: first resultsNature, 1989
- First measurements of the ionospheric plasma escape from MarsNature, 1989
- Mass loading in the solar wind interaction with Venus and MarsJournal of Geophysical Research, 1989
- On a hot oxygen corona of MarsIcarus, 1988
- Hot oxygen atoms in the upper atmospheres of Venus and MarsGeophysical Research Letters, 1988
- Interaction of mass-loaded solar wind flow with blunt bodyPlanetary and Space Science, 1987
- The effect of the hot oxygen corona on the interaction of the solar wind with VenusGeophysical Research Letters, 1987
- Comparison of gas dynamic model with steady solar wind flow around VenusJournal of Geophysical Research, 1982