Atmosphere of Venus as Studied with the Mariner 5 Dual Radio‐Frequency Occultation Experiment
- 1 October 1969
- journal article
- Published by American Geophysical Union (AGU) in Radio Science
- Vol. 4 (10) , 879-897
- https://doi.org/10.1029/rs004i010p00879
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Venus: Lower Atmosphere Not MeasuredScience, 1968
- The Radius of Venus as Determined by Planetary Radar and Mariner 5 Radio Tracking DataJournal of the Atmospheric Sciences, 1968
- The atmosphere of mars analyzed by integral inversion of the Mariner IV occultation dataPlanetary and Space Science, 1968
- Model of the Atmosphere of the Planet Venus Based on Results of Measurements made by the Soviet Automatic Interplanetary Station Venera 4Journal of the Atmospheric Sciences, 1968
- Theory of the Curve of Growth and Phase Effects in a Cloudy Atmosphere. Applications to VenusJournal of the Atmospheric Sciences, 1968
- Interpretation of the Mariner 5 Lyman Alpha MeasurementsJournal of the Atmospheric Sciences, 1968
- The Case for the Radar Radius of VenusScience, 1968
- Mariner V: Plasma and Magnetic Fields Observed near VenusScience, 1967
- The two-frequency bistatic radar-occultation method for the study of planetary ionospheresJournal of Geophysical Research, 1965
- Results of the Occultation of Regulus by Venus, July 7, 1959Nature, 1960