This map shows the geographic impact of H. K. Hills'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 H. K. Hills with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. K. Hills more than expected).
This network shows the impact of papers produced by H. K. Hills. 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 H. K. Hills. The network helps show where H. K. Hills may publish in the future.
Co-authorship network of co-authors of H. K. Hills
This figure shows the co-authorship network connecting the top 25 collaborators of H. K. Hills.
A scholar is included among the top collaborators of H. K. Hills 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 H. K. Hills. H. K. Hills is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Nagihara, S., Yasuyuki Nakamura, D. R. Williams, et al.. (2017). Recent Achievement by the SSERVI ALSEP Data Recovery Focus Group. 2041. 5017.2 indexed citations
2.
Williams, D. R., et al.. (2013). Lunar Data Node: Apollo Data Restoration and Archiving Update. NASA STI Repository (National Aeronautics and Space Administration). 1620.2 indexed citations
3.
McBride, M. J., D. R. Williams, H. K. Hills, & N. E. Turner. (2013). First-Time Analysis of Completely Restored DTREM Instrument Data from Apollo 14 and 15. NASA Technical Reports Server (NASA). 2868.1 indexed citations
4.
Williams, D. R., H. K. Hills, E. A. Guinness, Patrick T. Taylor, & M. J. McBride. (2011). Restoration of APOLLO Data by the NSSDC and PDS Lunar Data Node. NASA Technical Reports Server (NASA). 2476.
5.
Collier, M. R., T. J. Stubbs, & H. K. Hills. (2008). Lunar Surface Potential Changes Possible Associated with Traversals of the Bow Shock. NASA Technical Reports Server (NASA).1 indexed citations
Sanderson, T. R., Michael T. Brett, H. K. Hills, et al.. (1990). World-wide interactive access to scientific databases via satellite and terrestrial data network.
9.
Schofield, Norman, R. Parthasarathy, & H. K. Hills. (1988). Data Catalog Series for Space Science and Applications Flight Missions. NASA Technical Reports Server (NASA).2 indexed citations
Harel, M., R. A. Wolf, P. H. Reiff, & H. K. Hills. (1977). Study of plasma flow near the earth's plasmapause. Final report, 1 October 1976--30 September 19 77. OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information).1 indexed citations
Freeman, J. W., et al.. (1975). The Lunar Ionosphere. Lunar and Planetary Science Conference. 6. 39.2 indexed citations
14.
Freeman, J. W., et al.. (1975). The lunar terminator ionosphere.. Lunar and Planetary Science Conference Proceedings. 3. 3013–3021.12 indexed citations
Freeman, J. W., et al.. (1973). The electric potential of the lunar surface. Lunar and Planetary Science Conference. 4. 2877.8 indexed citations
17.
Freeman, J. W., H. K. Hills, & R. R. Vondrak. (1972). Water vapor, whence comest thou.. Lunar and Planetary Science Conference Proceedings. 3. 2217.6 indexed citations
18.
Hills, H. K.. (1967). Investigation of Energetic Electron Intensities in the Earth's Outer Radiation Zone with OGO 1.. NASA Technical Reports Server (NASA).4 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.