Interior Structure Modeling
Interior Structure Modeling is a computational and theoretical framework within planetary seismology that infers the radial and compositional architecture of a planetary body by integrating seismic observations with physical constraints to constrain density, layering, phase transitions, and material properties of its deep interior.
97
Publications
6.3K
Citations
410
Authors
184
Institutions
Publications per year
2017–2026
53
Parents
97
1–5 of 97
410
9
h-index
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184
Planetary Science Institute
Tucson, United States
16 h-index
25 publications
2.2K citations

Centre National de la Recherche Scientifique
Paris, France
15 h-index
51 publications
3.7K citations
University of California, Santa Cruz
Santa Cruz, United States
13 h-index
20 publications
1.9K citations
Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)
Cologne, Germany
12 h-index
45 publications
2.5K citations
University of Zurich
Zurich, Switzerland
12 h-index
20 publications
1.2K citations
Observatoire de la Côte d’Azur
Nice, France
11 h-index
16 publications
1.8K citations
Jet Propulsion Laboratory
Pasadena, United States
11 h-index
21 publications
896 citations
University of Arizona
Tucson, United States
11 h-index
13 publications
1K citations
1–8 of 184
17 publications · 1.2K citations
15
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ApJ · 12 publications · 915 citations
11
h-index
9 publications · 559 citations
9
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JGR · 7 publications · 630 citations
7
h-index
6 publications · 154 citations
6
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