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.
Global Distribution of Neutrons from Mars: Results from Mars Odyssey
2002425 citationsW. C. Feldman, W. V. Boynton et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of K. R. Moore'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 K. R. Moore with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. R. Moore more than expected).
This network shows the impact of papers produced by K. R. Moore. 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 K. R. Moore. The network helps show where K. R. Moore may publish in the future.
Co-authorship network of co-authors of K. R. Moore
This figure shows the co-authorship network connecting the top 25 collaborators of K. R. Moore.
A scholar is included among the top collaborators of K. R. Moore 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 K. R. Moore. K. R. Moore 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.
Jacobs, J M, Wojciech Dec, Jamie P. Levine, et al.. (2012). Best Face Forward. Plastic & Reconstructive Surgery. 131(1). 64–70.16 indexed citations
Prettyman, T. H., W. C. Feldman, R. C. Elphic, et al.. (2003). Mid-latitude composition of mars from thermal and epithermal neutrons. University of North Texas Digital Library (University of North Texas).3 indexed citations
Tokar, R. L., W. C. Feldman, K. R. Moore, et al.. (2002). Comparison of Measured Thermal/Epithermal Neutron Flux and Simulation Predictions for the Odyssey Neutron Spectrometer in Orbit About Mars. Lunar and Planetary Science Conference. 1803.2 indexed citations
6.
Feldman, W. C., R. L. Tokar, T. H. Prettyman, et al.. (2002). Initial Results of the Mars Odyssey Neutron Spectrometer at Mars. Lunar and Planetary Science Conference. 1718.1 indexed citations
Moore, K. R., et al.. (1993). A space-based classification system for RF transients. University of North Texas Digital Library (University of North Texas).4 indexed citations
Moore, K. R., D. J. McComas, C. T. Russell, S. S. Stahara, & J. R. Spreiter. (1991). Gasdynamic modeling of the Venus magnetotail. Journal of Geophysical Research Atmospheres. 96(A4). 5667–5681.19 indexed citations
Moore, K. R.. (1990). The Role of Pickup Ions in the Solar Wind Interaction with Venus as Deduced from Observations and Numerical Simulations..1 indexed citations
17.
Phillips, J. L., J. G. Luhmann, C. T. Russell, & K. R. Moore. (1987). Finite Larmor radius effect on ion pickup at Venus. Journal of Geophysical Research Atmospheres. 92(A9). 9920–9930.68 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.