Stellar Occultations by turbulent planetary atmospheres: A wave-optical theory including a finite scale height
- 31 May 1978
- Vol. 34 (2) , 374-395
- https://doi.org/10.1016/0019-1035(78)90174-4
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Occultation of Epsilon Geminorum by Mars. II - The structure and extinction of the Martian upper atmosphereThe Astrophysical Journal, 1977
- The occultation of Epsilon Geminorum by Mars - Analysis of McDonald dataThe Astrophysical Journal, 1977
- Turbulent scattering in an exponential atmosphere - A wave-optical solutionThe Astrophysical Journal, 1977
- Stellar occultations by turbulent planetary atmospheres: The Beta Scorpii eventsIcarus, 1977
- Stellar occultations by turbulent planetary atmospheres: A heuristic scattering modelIcarus, 1977
- Scintillations during occultations by planets I. An approximate theoryIcarus, 1976
- Stellar occultation spikes as probes of atmospheric structure and compositionIcarus, 1976
- The Occultation of Beta Scorpii by Jupiter. 11. the Hydrogen-Helium Abundance in the Jovian AtmosphereThe Astrophysical Journal, 1974
- on the "thin Screen" Model of Interplanetary ScintillationsThe Astrophysical Journal, 1970
- Interplanetary Scintillations. I. TheoryThe Astrophysical Journal, 1967