Planetary Geoid
Planetary Geoid is the equipotential surface of a planet's gravity field that best approximates the mean shape of its fluid envelope, distinguishing itself from other reference surfaces by representing the global mean sea level in the absence of tidal, atmospheric, and dynamic oceanic forces.
45
Publications
2.5K
Citations
107
Authors
57
Institutions
Publications per year
2017–2026
2
Parents
45
Stagnant lid convection on Venus
V. S. Solomatov, Louis Moresi · Journal of Geophysical Research Atmospheres · 1996 · 289 citations
Gravity Field, Shape, and Moment of Inertia of Titan
L. Iess, N. J. Rappaport, Robert A. Jacobson et al. · Science · 2010 · 202 citations
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57
California Institute of Technology
Pasadena, United States
3 h-index
5 publications
530 citations
Charles University
Prague, Czechia
3 h-index
5 publications
165 citations
University of New Brunswick
Fredericton, Canada
3 h-index
3 publications
154 citations
University of Stuttgart
Stuttgart, Germany
3 h-index
4 publications
50 citations

Institut de physique du globe de Paris
Paris, France
3 h-index
4 publications
364 citations
United States Geological Survey
Reston, United States
2 h-index
2 publications
128 citations
Jet Propulsion Laboratory
Pasadena, United States
2 h-index
6 publications
1K citations

University of Tehran
Tehran, Iran
2 h-index
3 publications
51 citations
1–8 of 57
JGR · 12 publications · 1.1K citations
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5 publications · 299 citations
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4 publications · 256 citations
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3 publications · 386 citations
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2 publications · 32 citations
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