An empirical model of the Venusian outer environment 2. The shape and location of the bow shock
- 30 December 1980
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 85 (A13), 7651-7654
- https://doi.org/10.1029/ja085ia13p07651
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- Plasma Observations Near Venus Onboard the Venera 9 and 10 Satellites by Means of Wide-Angle Plasma DetectorsPublished by Wiley ,2013
- Ion Flux Parameters in the Solar Wind-Venus Interaction Region According to Venera-9 and Venera-10 DataPublished by Wiley ,2013
- 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
- Initial Pioneer Venus Magnetic Field Results: Dayside ObservationsScience, 1979
- Plasma near Venus from the Venera 9 and 10 wide‐angle analyzer dataJournal of Geophysical Research, 1978
- The Venus bow shock: Detached or attached?Journal of Geophysical Research, 1977
- Solar wind flow past nonmagnetic planets—Venus and MarsPlanetary and Space Science, 1970
- Mariner V: Plasma and Magnetic Fields Observed near VenusScience, 1967