Deep radio occultations and “evolute flashes”; their characteristics and utility for planetary studies
- 31 March 1979
- Vol. 37 (3), 612-626
- https://doi.org/10.1016/0019-1035(79)90017-4
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- Effects of turbulence on average refraction angles in occultations by planetary atmospheresIcarus, 1978
- Radio science investigations with VoyagerSpace Science Reviews, 1977
- Occultation of Epsilon Geminorum by Mars. II - The structure and extinction of the Martian upper atmosphereThe Astrophysical Journal, 1977
- Jupiter's Atmosphere: Problems and Potential of Radio OccultationScience, 1975
- The radio occultation method for the study of planetary atmospheresPlanetary and Space Science, 1973
- The Neutral Atmosphere of Venus as Studied with the Mariner V Radio Occultation ExperimentsThe Astronomical Journal, 1971
- Atmosphere of Venus as Studied with the Mariner 5 Dual Radio‐Frequency Occultation ExperimentRadio Science, 1969
- Lens effect of the earth's ionosphere on radio waves reaching the moonPlanetary and Space Science, 1968
- The bistatic radar-occultation method for the study of planetary atmospheresJournal of Geophysical Research, 1965
- Lens-Like Action of a Star by the Deviation of Light in the Gravitational FieldScience, 1936