Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Internal Structure and Early Thermal Evolution of Mars from Mars Global Surveyor Topography and Gravity
Citations per year, relative to G. L. Tyler G. L. Tyler (= 1×)
peers
V. R. Eshleman
Countries citing papers authored by G. L. Tyler
Since
Specialization
Citations
This map shows the geographic impact of G. L. Tyler'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 G. L. Tyler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. L. Tyler more than expected).
This network shows the impact of papers produced by G. L. Tyler. 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 G. L. Tyler. The network helps show where G. L. Tyler may publish in the future.
Co-authorship network of co-authors of G. L. Tyler
This figure shows the co-authorship network connecting the top 25 collaborators of G. L. Tyler.
A scholar is included among the top collaborators of G. L. Tyler 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 G. L. Tyler. G. L. Tyler is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
DeBoy, Christopher C., S. A. Stern, Michael A. Vincent, et al.. (2019). Pluto's Surface Properties from the New Horizons Uplink Bistatic Radar Experiment. AGU Fall Meeting Abstracts. 2019.
Andert, T. P., P. Rosenblatt, M. Pätzold, B. Häusler, & G. L. Tyler. (2011). The internal structure of Phobos and hints to its origin derived from Mars Express Radio Science observations. 2011. 210.3 indexed citations
5.
Rosenblatt, P., T. P. Andert, M. Päetzold, et al.. (2010). Revisiting Phobos' origin issue from Mars Express Radio-Science observations.. epsc. 652.2 indexed citations
6.
Peter, Kerstin, et al.. (2008). The Structure of the Mars Ionosphere. 37. 2328.1 indexed citations
7.
Peter, Kerstin, et al.. (2007). Ionopause Features of Mars as Observed by the Radio Science Experiment MaRS on Mars Express. AGU Fall Meeting Abstracts. 2007. 2414.1 indexed citations
8.
Simpson, R. A., G. L. Tyler, B. Häusler, & M. Pätzold. (2007). Search for Anomalous Surface Properties at Maxwell Montes with Venus Express Bistatic Radar. Lunar and Planetary Science Conference. 2240.1 indexed citations
9.
Pätzold, M., S. Tellmann, B. Häusler, D. P. Hinson, & G. L. Tyler. (2006). Radio-sounding of the neutral martian atmosphere with Mars Express: overview of the observations. 132.1 indexed citations
10.
Simpson, R. A., G. L. Tyler, M. C. Nolan, M. Pätzold, & B. Häusler. (2006). Mars Express Bistatic Radar Explores Stealth. 38.1 indexed citations
11.
Linscott, I. R., et al.. (2005). Bistatic UHF Radar Experiments at Mars Using the SRI 150-ft Dish and the Mars Odyssey Spacecraft. AGUFM. 2005.1 indexed citations
12.
Bird, M. K., R. Dutta‐Roy, Yvonne Dzierma, et al.. (2005). A Measurement of Titan's Zonal Winds by the Huygens Doppler Wind Experiment. DPS.2 indexed citations
13.
Baron, E. J., R. A. Simpson, & G. L. Tyler. (2002). Radar Backscatter from Surface and Subsurface Rocks: Angular Dependenceand Polarization Ratios. LPI. 1456.1 indexed citations
14.
Baron, J. E., G. L. Tyler, & R. A. Simpson. (1998). New Results for Scattering from Buried Craters and Refractive Lenses: Implications for Remote Sensing of Icy Surfaces. Bulletin of the American Astronomical Society. 30. 1087.6 indexed citations
15.
Gurrola, E. M., V. R. Eshleman, G. L. Tyler, & E. A. Marouf. (1993). Simulations of a Radio Occultation Experiment for Measuring Pluto's Atmosphere: Lessons from Triton. 25.1 indexed citations
16.
Gurrola, E. M., E. A. Marouf, V. R. Eshleman, & G. L. Tyler. (1991). Voyager Radio Occultation Observations of Triton's Neutral Atmosphere. Bulletin of the American Astronomical Society. 23. 1207.3 indexed citations
17.
Rosen, P. A., G. L. Tyler, & E. A. Marouf. (1988). Thirty Wave Features in Radio Occultation Data of Saturn's Rings: Summary of Results. Bulletin of the American Astronomical Society. 20. 853.1 indexed citations
18.
Simpson, R. A., G. L. Tyler, & J. B. Holberg. (1982). Saturn's Pole Vector from Combined Ring Occultation Data.. Bulletin of the American Astronomical Society. 14. 731.1 indexed citations
19.
Lindal, G. F., Henry B. Hotz, D. N. Sweetnam, V. R. Eshleman, & G. L. Tyler. (1981). The Atmosphere of Titan: An Analysis of the Voyager 1 Radio Occultation Measurements.. Bulletin of the American Astronomical Society. 13. 700.5 indexed citations
20.
Howard, H. T. & G. L. Tyler. (1972). Bistatic-Radar Observations of the Lunar Surface with Apollos 14 and 15. Lunar and Planetary Science Conference. 3. 398.1 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.