This map shows the geographic impact of S. M. Brooks'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 S. M. Brooks with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. M. Brooks more than expected).
This network shows the impact of papers produced by S. M. Brooks. 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 S. M. Brooks. The network helps show where S. M. Brooks may publish in the future.
Co-authorship network of co-authors of S. M. Brooks
This figure shows the co-authorship network connecting the top 25 collaborators of S. M. Brooks.
A scholar is included among the top collaborators of S. M. Brooks 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 S. M. Brooks. S. M. Brooks is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Diniega, S., S. M. Brooks, M. S. Gilmore, et al.. (2020). Recognizing our colleagues of color in Planetary Science. 52(6).1 indexed citations
6.
Edgington, S. G., R. F. Beebe, B. J. Buratti, et al.. (2019). Cassini-Huygens Scientific Legacy: The Cassini Mission Archive at the Planetary Data System. LPI. 2932.1 indexed citations
Spilker, L. J., R. Morishima, C. Leyrat, et al.. (2010). Saturn ring temperature changes before and after ring equinox. EGUGA. 5675.1 indexed citations
9.
Ferrari, C., et al.. (2009). CIRS-CASSINI Prime mission on Saturn’s B ring : infrared optical depths and energy balance. AGU Fall Meeting Abstracts. 2009.1 indexed citations
10.
Spilker, L. J., R. Morishima, N. Altobelli, et al.. (2009). Saturn Ring Temperatures at Equinox with Cassini CIRS. AGU Fall Meeting Abstracts. 2009.2 indexed citations
Pilorz, S., L. J. Spilker, B. Wallis, et al.. (2005). Sensitivity Studies of Thermal Observations of Saturn's Rings Using a Coupled Thermal/Radiative Transfer Model.1 indexed citations
13.
Spilker, L. J., S. Pilorz, B. Wallis, et al.. (2005). Cassini CIRS: Thermal Changes In Saturn's Main Rings With Increasing Phase Angle. 37.1 indexed citations
14.
Ferrari, C., L. J. Spilker, S. M. Brooks, et al.. (2005). Azimuthal temperature variations in Saturn's rings as seen by the CIRS spectrometer onboard Cassini. 37.5 indexed citations
15.
Spilker, L. J., S. Pilorz, B. Wallis, et al.. (2005). Saturn Ring Temperature Roll-off at Submillimeter Wavelengths From Cassini CIRS Observations. AGU Spring Meeting Abstracts. 2005.2 indexed citations
16.
Spilker, L. J., S. Pilorz, C. Ferrari, et al.. (2004). Cassini CIRS: Preliminary Results on Saturn's Rings. AGU Fall Meeting Abstracts. 2004.1 indexed citations
17.
Chapman, C. R., et al.. (1998). Cratering in the Jovian System: Intersatellite Comparisons. LPI. 1927.12 indexed citations
18.
Merline, W. J., C. R. Chapman, S. M. Brooks, et al.. (1998). Cratering on Callisto from the Galileo Prime Mission. Bulletin of the American Astronomical Society. 30. 1122.1 indexed citations
19.
Chapman, C. R., W. J. Merline, J. W. Keller, et al.. (1997). Populations of small craters on Europa, Ganymede, and Callisto: initial Galileo imaging results. elib (German Aerospace Center). 217.6 indexed citations
20.
Chapman, C. R., et al.. (1997). Impactor Populations on the Galilean Satellites. DPS.2 indexed citations
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.