This map shows the geographic impact of Hunter Waite'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 Hunter Waite with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Hunter Waite more than expected).
This network shows the impact of papers produced by Hunter Waite. 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 Hunter Waite. The network helps show where Hunter Waite may publish in the future.
Co-authorship network of co-authors of Hunter Waite
This figure shows the co-authorship network connecting the top 25 collaborators of Hunter Waite.
A scholar is included among the top collaborators of Hunter Waite 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 Hunter Waite. Hunter Waite is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Stofan, E. R., J. I. Lunine, R. D. Lorenz, et al.. (2011). The Titan Mare Explorer Mission (TiME): A Discovery mission to a Titan sea. 2011. 909.2 indexed citations
9.
Stofan, E. R., R. D. Lorenz, J. I. Lunine, et al.. (2010). Titan Mare Explorer (TiME): First In Situ Exploration of an Extraterrestrial Sea. Open Research Online (The Open University). 1538. 5270.5 indexed citations
10.
Cravens, T. E., R. L. Tokar, I. P. Robertson, et al.. (2010). Plasma in the Water Plume of Enceladus. EGU General Assembly Conference Abstracts. 2981.1 indexed citations
11.
Stofan, E. R., J. I. Lunine, R. D. Lorenz, et al.. (2010). Exploring the seas of Titan: the Titan Mare Eplorer (TiME) mission. Open Research Online (The Open University). 1236.7 indexed citations
12.
Bell, J. M., Hunter Waite, J. H. Westlake, & B. Magee. (2009). Simulating the 3-D Structure of Titan's Upper Atmosphere. AGUSM. 2009.1 indexed citations
Gladstone, G. R., T. Majeed, S. W. Bougher, Hunter Waite, & J. T. Clarke. (2005). Using HST-STIS Observations of Auroral Lyα Line Profiles to Map High-Altitude Winds on Jupiter. AGUSM. 2005.1 indexed citations
15.
Branduardi‐Raymont, G., Anil Bhardwaj, P. M. Rodriguez‐Pascual, et al.. (2005). X-ray exploration of the giant planets, their magnetospheres and the solar connection: from XMM-Newton to XEUS. UCL Discovery (University College London). 588. 393.2 indexed citations
16.
Bhardwaj, Anil, R. F. Elsner, G. R. Gladstone, et al.. (2005). A Comparative View of X-rays from the Solar System. NASA Technical Reports Server (NASA). 2005.1 indexed citations
17.
Mahaffy, P. R., David Beaty, M. S. Anderson, et al.. (2004). Science Priorities Related to the Organic Contamination of Martian Landers.6 indexed citations
18.
Beaty, D. W., P. R. Mahaffy, M. S. Anderson, et al.. (2003). Report of the Organic Contamination Science Steering Group.4 indexed citations
19.
Clarke, J. T., Denis Grodent, J. E. P. Connerney, et al.. (2001). HST Observations of Aurora from the Magnetic Footprints of Io, Ganymede, and Europa during the Millennium Campaign. Open Repository and Bibliography (University of Liège).1 indexed citations
20.
Clarke, J. T., John T. Trauger, & Hunter Waite. (1988). Doppler Shifted H Ly α Emission from Jupiter's Aurora. Bulletin of the American Astronomical Society. 20. 868.1 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.