The atmosphere of Titan: An analysis of the Voyager 1 radio occultation measurements
- G. F. Lindal, G. E. Wood, H. Hotz, D. Sweetnam, V. Eshleman, G. Tyler
- Physics, Environmental Science
- 1 June 1981
Internal structure and early thermal evolution of Mars from Mars Global Surveyor topography and gravity.
- M. Zuber, S. Solomon, S. Zhong
- GeologyScience
- 10 March 2000
The strength of the lithosphere beneath the ancient southern highlands suggests that the northern hemisphere was a locus of high heat flow early in martian history and the thickness of the elastic lithosphere increases with time of loading in the northern plains and Tharsis.
The atmosphere of Uranus: Results of radio occultation measurements with Voyager 2
- G. F. Lindal, J. Lyons, D. Sweetnam, V. Eshleman, D. Hinson, G. Tyler
- Physics, Environmental Science
- 30 December 1987
During Voyager 2's occultation by Uranus the radio link from the spacecraft probed the atmosphere of the planet at latitudes ranging from 2° to 7° south. The measurements, which were conducted at two…
Initial results from radio occultation measurements with Mars Global Surveyor
- D. Hinson, R. A. Simpson, J. Twicken, G. Tyler, F. Flasar
- Environmental Science, Physics
- 25 November 1999
A series of radio occultation experiments conducted with Mars Global Surveyor in early 1998 has yielded 88 vertical profiles of the neutral atmosphere. The measurements cover latitudes of 29°N to…
Structure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express
- S. Tellmann, M. Pätzold, B. Häusler, M. Bird, G. Tyler
- Physics, Environmental Science
- 1 September 2009
[1] The European Space Agency Venus Express Radio Science experiment (VeRa) obtained 118 radio occultation measurements of the Venusian atmosphere between July 2006 and June 2007. Southern latitudes…
A Sporadic Third Layer in the Ionosphere of Mars
- M. Pätzold, S. Tellmann, B. Häusler, D. Hinson, R. Schaa, G. Tyler
- Physics, GeologyScience
- 4 November 2005
The authors' observations imply that a third ionospheric layer at altitude ranges of 65 to 110 kilometers, which has been predicted to be permanent and continuous is present sporadically and locally.
The vertical profile of winds on Titan
- M. Bird, M. Allison, G. Tyler
- Environmental Science, PhysicsNature
- 8 December 2005
A high resolution vertical profile of Titan's winds is reported, with an estimated accuracy of better than 1 m s-1, providing in situ confirmation of superrotation on Titan.
The depth of the convective boundary layer on Mars
- D. Hinson, M. Pätzold, S. Tellmann, B. Häusler, G. Tyler
- Environmental Science, Physics
- 1 November 2008
The gravity field of Mars: results from Mars Global Surveyor.
- D. Smith, W. Sjogren, G. Tyler, G. Balmino, F. LeMoine, A. Konopliv
- GeologyScience
- 1 October 1999
Observations of the gravity field of Mars reveal a planet that has responded differently in its northern and southern hemispheres to major impacts and volcanic processes. The rough, elevated southern…
...
...