Orientation of planetary O+ fluxes and magnetic field lines in the Venus wake
- 1 September 1982
- journal article
- Published by Springer Nature in Nature
- Vol. 299 (5881) , 325-326
- https://doi.org/10.1038/299325a0
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Observations of mass addition to the shocked solar wind of the Venusian ionosheathGeophysical Research Letters, 1982
- The distant bow shock and magnetotail of Venus: Magnetic field and plasma wave observationsGeophysical Research Letters, 1981
- Solar wind pickup of ionized Venus exosphere atomsJournal of Geophysical Research, 1981
- A source of plasma turbulence at the ionopause of VenusJournal of Geophysical Research, 1981
- Pioneer Venus plasma observations of the solar wind‐Venus interactionJournal of Geophysical Research, 1980
- Evidence for a viscous boundary layer at the Venus ionopause from the preliminary Pioneer Venus resultsJournal of Geophysical Research, 1980
- The Pioneer Venus Orbiter Plasma Analyzer ExperimentIEEE Transactions on Geoscience and Remote Sensing, 1980
- Plasma near Venus from the Venera 9 and 10 wide‐angle analyzer dataJournal of Geophysical Research, 1978
- Strongly-cooled ionizing plasma flows with application to venusPlanetary and Space Science, 1975
- Atmospheric ion wakes of Venus and Mars in the solar windPlanetary and Space Science, 1974