Radio occultation of the Venusian atmosphere and bistatic radiolocation of the surface of Venus using the Venera‐9 and Venera‐10 satellites
- 1 January 1979
- journal article
- Published by American Geophysical Union (AGU) in Radio Science
- Vol. 14 (1) , 163-173
- https://doi.org/10.1029/rs014i001p00163
Abstract
No abstract availableKeywords
This publication has 6 references indexed in Scilit:
- Venus: Mass, Gravity Field, Atmosphere, and Ionosphere as Measured by the Mariner 10 Dual-Frequency Radio SystemScience, 1974
- Venus: Topography Revealed by Radar DataScience, 1972
- The Neutral Atmosphere of Venus as Studied with the Mariner V Radio Occultation ExperimentsThe Astronomical Journal, 1971
- Radar Mapping of Venus With Interf Erometric Resolution of the Range‐Doppler AmbiguityRadio Science, 1970
- A Radar Determination of the Rotation of VenusThe Astronomical Journal, 1970
- Atmosphere of Venus as Studied with the Mariner 5 Dual Radio‐Frequency Occultation ExperimentRadio Science, 1969