Altitude profile of H in the atmosphere of Venus from Lyman α observations of Venera 11 and Venera 12 and origin of the hot exospheric component
- 30 November 1982
- Vol. 52 (2), 221-244
- https://doi.org/10.1016/0019-1035(82)90110-5
Abstract
No abstract availableKeywords
This publication has 35 references indexed in Scilit:
- On the variability of Lyman-alpha with solar activityPlanetary and Space Science, 1981
- Venera 11 and Venera 12 observations of e.u.v. emissions from the upper atmosphere of VenusPlanetary and Space Science, 1981
- Venus nighttime hydrogen bulgeGeophysical Research Letters, 1980
- Extreme Ultraviolet Observations from Voyager 1 Encounter with JupiterScience, 1979
- Consequences of the day-to-night variation of the exospheric temperature of VenusNature, 1979
- Lyman-alpha observations of venera-9 and 10 I. The non-thermal hydrogen population in the exosphere of venusPlanetary and Space Science, 1978
- The Mariner 5 Ultraviolet Photometer Experiment: Analysis of hydrogen lyman alpha dataJournal of Geophysical Research, 1976
- Observed variations of the exospheric hydrogen density with the exospheric temperatureJournal of Geophysical Research, 1975
- Interpretation of the Mariner 5 Lyman Alpha MeasurementsJournal of the Atmospheric Sciences, 1968
- Ultraviolet Emissions Observed near Venus from Mariner VScience, 1967