T. E. Bunch
About
In The Last Decade
T. E. Bunch
119 papers receiving 1.5k citations
Peers
Comparison fields: 5 of 80
- Astronomy and Astrophysics 1.2k
- Geophysics 606
- Atmospheric Science 390
- Ecology 239
- Paleontology 114
Countries citing papers authored by T. E. Bunch
This map shows the geographic impact of T. E. Bunch's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by T. E. Bunch with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. E. Bunch more than expected).
Fields of papers citing papers by T. E. Bunch
This network shows the impact of papers produced by T. E. Bunch. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by T. E. Bunch. The network helps show where T. E. Bunch may publish in the future.
Co-authorship network of co-authors of T. E. Bunch
This figure shows the co-authorship network connecting the top 25 collaborators of T. E. Bunch. A scholar is included among the top collaborators of T. E. Bunch based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with T. E. Bunch. T. E. Bunch is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Assessment of the Mesosiderite-Diogenite Connection and an Impact Model for the Genesis of Mesosiderites | 1 |
| 2 | A Nomenclature System for Diogenites Consistent with the IUGS System for Naming Terrestrial Ultramafic Rocks | 1 |
| 3 | Al-26, Be-10, and Mn-53 in Martian Meteorites | 1 |
| 4 | Oxygen Isotopic and Petrological Diversity Among Brachinites NWA 4872, NWA 4874, NWA 4882 and NWA 4969: How Many Ancient Parent Bodies? | 9 |
| 5 | Melt Spherules from Peter's Pond, a Carolina Bay, South Carolina | 1 |
| 6 | ASSESSMENT OF MULTI-COMPONENT MIXING, OXIDATION, METAMORPHISM AND PARTIAL MELTING ON THE ACAPULCOITE-LODRANITE PARENT BODY. A. J. Irving | 4 |
| 7 | Lunar Meteorites NWA 2700, NWA 2727 and NWA 2977: Mare Basalt/Gabbro Breccias with Affinities to NWA 773 | 3 |
| 8 | Evidence for a Carbonaceous Chondrite Parent Body With Near-TFL Oxygen Isotopes From Unique Metachondrite Northwest Africa 2788 | 1 |
| 9 | Proximal Ejecta at Meteor Crater, Arizona: Discovery of Impact Melt-bearing Breccias | 2 |
| 10 | "Primitive" and Igneous Achondrites Related to the Large and Differentiated CR Parent Body | 2 |
| 11 | Olivine-Orthopyroxene-Phyric Shergottites NWA 2626 and DaG 476: The Tharsis Connection | 3 |
| 12 | Metachondrites: Recrystallized and/or Residual Mantle Rocks from Multiple, Large Chondritic Parent Bodies | 4 |
| 13 | Evidence for Shocked Feldspars and Ballen Quartz in 450,000 Year Old Argentine Impact Melt Breccias | 2 |
| 14 | A Primitive Achondrite With Oxygen Isotopic Affinities to CV Chondrites: Implications for Differentiation and Size of the CV Parent Body | 8 |
| 15 | 1 | |
| 16 | The Role of Brecciation in Controlling Morphology at Haughton Crater: Climatic Implications for Mars | 3 |
| 17 | Hypervelocity Impact Penetration Experiments--A Guide to the Origin of Rims on Chondrules | 2 |
| 18 | Regolith Origin for Allende Meteorite | 6 |
| 19 | Noble Gases in Fine-Grained Olivine-Carbon Assemblages from an Allende Dark Inclusion | 1 |
| 20 | Euxenite from Ampangabe, Madagascar | 1 |
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.