The solar wind interaction with Venus: Pioneer Venus observations of bow shock location and structure
- 30 December 1980
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 85 (A13), 7625-7641
- https://doi.org/10.1029/ja085ia13p07625
Abstract
No abstract availableKeywords
This publication has 78 references indexed in Scilit:
- The location of the dayside ionopause of Venus: Pioneer Venus Orbiter Magnetometer observationsGeophysical 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
- Evidence for Earth magnetospheric tail associated phenomena at 3100 REGeophysical Research Letters, 1979
- Observation of magnetic flux ropes in the Venus ionosphereNature, 1979
- A model of the variability of the Venus ionopause altitudeGeophysical Research Letters, 1979
- The Mariner 10 Radio Occultation Measurements of the Ionosphere of VenusJournal of the Atmospheric Sciences, 1975
- Venus ionosphere: An interpretation of Mariner 10 observationsGeophysical Research Letters, 1974
- The structure of the earth’s bow shockLa Rivista del Nuovo Cimento, 1973
- Solar wind interaction with planetary atmospheresReviews of Geophysics, 1971