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.
Cosmic ray production rates of 10Be and 26Al in quartz from glacially polished rocks
1989477 citationsK. Nishiizumi, C. P. Kohl 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 J. R. Arnold'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 J. R. Arnold with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. R. Arnold more than expected).
This network shows the impact of papers produced by J. R. Arnold. 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 J. R. Arnold. The network helps show where J. R. Arnold may publish in the future.
Co-authorship network of co-authors of J. R. Arnold
This figure shows the co-authorship network connecting the top 25 collaborators of J. R. Arnold.
A scholar is included among the top collaborators of J. R. Arnold 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 J. R. Arnold. J. R. Arnold 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.
Parker, Richard H., R. C. Reedy, A. E. Metzger, J. I. Trombka, & J. R. Arnold. (2022). Preliminary design and performance of an advanced gamma ray spectrometer for future orbiter missions. NASA STI Repository (National Aeronautics and Space Administration).
2.
Arnold, J. R.. (2013). GRAVITATION, FORCE, AND TIME. viXra. 9(24).
3.
Nishiizumi, K., J. R. Arnold, Marc W. Caffee, et al.. (1993). Exposure ages of carbonaceous chondrites, 1. 1085.4 indexed citations
4.
Bada, Jeffrey L., et al.. (1993). A reexamination of amino acids in lunar soil. 193.2 indexed citations
5.
Nishiizumi, K., J. R. Arnold, & P. Sharma. (1993). Two-Stage Exposure of the Fayetteville Meteorite Based on 129I. Metic. 28(3). 412.1 indexed citations
6.
Nishiizumi, K., J. R. Arnold, Robert C. Finkel, et al.. (1992). 10Be and 26Al in Individual Cosmic Spherules. Meteoritics and Planetary Science. 27(3). 269.3 indexed citations
7.
Nishiizumi, K., J. R. Arnold, Marc W. Caffee, Robert C. Finkel, & John Southon. (1992). Exposure Histories of Calcalong Creek and LEW 88516 Meteorites. Meteoritics and Planetary Science. 27(3). 270.14 indexed citations
8.
Shoemaker, E. M., C. S. Shoemaker, K. Nishiizumi, et al.. (1990). Ages of Australian meteorite craters-A preliminary report. Metic. 25. 409.13 indexed citations
9.
Reedy, R. C., K. Nishiizumi, & J. R. Arnold. (1989). Solar Cosmic Rays: Fluxes and Reaction Cross Sections. LPI. 20. 890.1 indexed citations
10.
Nishiizumi, K., J. R. Arnold, David Fink, et al.. (1989). Cosmogenic Radionuclides in Individual Cosmic Particles. Meteoritics and Planetary Science. 24. 178.2 indexed citations
11.
Nishiizumi, K., et al.. (1986). Exposure History of Four Lunar Meteorites. Meteoritics and Planetary Science. 11. 294–59.13 indexed citations
12.
Nishiizumi, K., J. R. Arnold, Jeff Klein, R. Middleton, & J. N. Goswami. (1985). Cosmogenic Nuclides in 15011 Rocklets. LPI. 620–621.1 indexed citations
13.
Nishiizumi, K., D. Elmore, & J. R. Arnold. (1984). Cosmogenic Nuclides in Peculiar Meteorites. Meteoritics and Planetary Science. 19. 283.4 indexed citations
14.
Nishiizumi, K., J. R. Arnold, Jeff Klein, & R. Middleton. (1982). 10 Be and Other Radionuclides in Antarctic Meteorites and in Associated Ice. Metic. 17. 260.2 indexed citations
15.
Nishiizumi, K., M. T. Murrell, J. R. Arnold, M. Imamura, & M. Honda. (1980). Cosmogenic 53Mn Survey of Yamato Meteorites. Memoirs of National Institute of Polar Research. Special issue. 17. 202–209.8 indexed citations
16.
Nishiizumi, K., M. T. Murrell, J. R. Arnold, & M. Imamura. (1980). 53MN Measurements in Individual Rocklets from 60010 and in Lunar Core 70009. LPI. 818–820.1 indexed citations
17.
Nishiizumi, K., M. Imamura, M. Honda, M. T. Murrell, & J. R. Arnold. (1978). A Study of Gardening in the Lunar Regolith Using 53MN. Lunar and Planetary Science Conference. 811–813.1 indexed citations
18.
Arnold, J. R.. (1975). Monte Carlo simulation of turnover processes in the lunar regolith. Lunar and Planetary Science Conference Proceedings. 2. 2375–2395.43 indexed citations
19.
Finkel, Robert C., M. Wahlen, J. R. Arnold, C. P. Kohl, & M. Imamura. (1973). The Gradient of Cosmogenic Radionuclides to a Depth of 400 g/cm2 in the Moon. Lunar and Planetary Science Conference. 4. 242.1 indexed citations
20.
Arnold, J. R., A. C. Delany, J. C. Evans, et al.. (1971). Depth variation of cosmogenic nuclides in a lunar surface rock and lunar soil. Lunar and Planetary Science Conference Proceedings. 2. 1773.25 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.