M. S. Robinson
About
In The Last Decade
M. S. Robinson
493 papers receiving 10.6k citations
Hit Papers
Peers
Comparison fields: 5 of 144
- Astronomy and Astrophysics 10.2k
- Atmospheric Science 3.1k
- Aerospace Engineering 1.8k
- Geophysics 1.1k
- Ecology 700
Countries citing papers authored by M. S. Robinson
This map shows the geographic impact of M. S. Robinson'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 M. S. Robinson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. S. Robinson more than expected).
Fields of papers citing papers by M. S. Robinson
This network shows the impact of papers produced by M. S. Robinson. 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 M. S. Robinson. The network helps show where M. S. Robinson may publish in the future.
Co-authorship network of co-authors of M. S. Robinson
This figure shows the co-authorship network connecting the top 25 collaborators of M. S. Robinson. A scholar is included among the top collaborators of M. S. Robinson 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 M. S. Robinson. M. S. Robinson is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 3 | |
| 3 | 0 | |
| 4 | 61 | |
| 5 | Areal Crater Density Analysis of Volcanic Smooth Plains: Mare Imbrium, a Revised Approach | 3 |
| 6 | Tectonic Mapping of Mare Frigoris Using Lunar Reconnaissance Orbiter Camera Images | 1 |
| 7 | Topography of Mercury from stereo images: first samples from MESSENGER orbital mapping | 5 |
| 8 | South Pole-Aitken Basin: Crater Size-Frequency Distribution Measurements | 0 |
| 9 | Geologic Mapping of the King Crater Region with an Emphasis on Melt Pond Anatomy — Evidence for Subsurface Drainage on the Moon | 3 |
| 10 | Giordano Bruno: The Young and the Restless | 19 |
| 11 | Permanent Sunlight at the Lunar North Pole | 7 |
| 12 | Permanent Shadow in Simple Craters near the Lunar Poles | 0 |
| 13 | Automated Extraction of Planetary Digital Elevation Models | 1 |
| 14 | NEAR MSI Mosaics of 433 Eros | 1 |
| 15 | Structural Geology of Eros from NEAR Shoemaker Imaging | 1 |
| 16 | The Topography of Lobate Scarps in Northern Arabia Terra from MOLA Data | 1 |
| 17 | The Clementine Bistatic Radar Experiment: Evidence for Ice on the Moon | 7 |
| 18 | Spectral Heterogeneity of Lunar Local Dark Mantle Deposits | 2 |
| 19 | Remote Sensing Studies of the Northeastern Portion of the Lunar Nearside | 1 |
| 20 | Galileo Imaging Results from the Second Earth-Moon Flyby: Lunar Mariaand Related Units | 4 |
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.