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.
9,400 years of cosmic radiation and solar activity from ice cores and tree rings
2012557 citationsF. Steinhilber, J. A. Abreu et al.Proceedings of the National Academy of Sciencesprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by K. G. McCracken
Since
Specialization
Citations
This map shows the geographic impact of K. G. McCracken'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. G. McCracken with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. G. McCracken more than expected).
This network shows the impact of papers produced by K. G. McCracken. 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. G. McCracken. The network helps show where K. G. McCracken may publish in the future.
Co-authorship network of co-authors of K. G. McCracken
This figure shows the co-authorship network connecting the top 25 collaborators of K. G. McCracken.
A scholar is included among the top collaborators of K. G. McCracken 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. G. McCracken. K. G. McCracken is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Beer, J., K. G. McCracken, J. A. Abreu, U. Heikkilä, & F. Steinhilber. (2008). Long-term changes in cosmic rays derived from cosmogenic radionuclides. DORA Eawag (Swiss Federal Institute of Aquatic Science and Technology (Eawag)). 1. 765–768.5 indexed citations
4.
Moraal, H., K. G. McCracken, & P. H. Stoker. (2008). Analysis of the 20 January 2005 cosmic ray ground level enhancement. International Cosmic Ray Conference. 1. 265–268.1 indexed citations
Moraal, H., R. A. Caballero─López, K. G. McCracken, & J. E. Humble. (2005). An explanation for the unusual cosmic ray diurnal variation in 1954. CERN Document Server (European Organization for Nuclear Research). 2. 105.
7.
Moraal, H., Raimund Muscheler, Peter W. Kubik, et al.. (2005). 10Be concentration in the ice shelf of Queen Maud Land, Antarctica. South African Journal of Science. 101. 299–301.6 indexed citations
8.
McCracken, K. G.. (2003). The Accuracy of Cosmogenic 10 Be as a Quantitative Measurement of the GCR. International Cosmic Ray Conference. 7. 4127.1 indexed citations
9.
Shea, M. A., D. F. Smart, G. Dreschhoff, & K. G. McCracken. (2003). The Seasonal Dependency of the NO(Y) Impulsive Precipitation Events in Arctic Polar Ice. ICRC. 7. 4225.1 indexed citations
10.
Beer, J., M. Vonmoos, Raimund Muscheler, K. G. McCracken, & W. Mende. (2003). Heliospheric Modulation over the past 10,000 Years as de- rived from Co smogenic Nuclides. ICRC. 7(2). 4147–4.7 indexed citations
11.
McCracken, K. G. & B. C. Heikkila. (2003). The Cosmic Ray Intensity between 1933-1965. ICRC. 7. 4117.4 indexed citations
12.
McCracken, K. G., D. F. Smart, M. A. Shea, & G. Dreschhoff. (2001). 400 years of large fluence solar proton events. International Cosmic Ray Conference. 8. 3209.11 indexed citations
13.
Dreschhoff, G., M. A. Shea, D. F. Smart, & K. G. McCracken. (1997). Evidence for Historical Solar Proton Events from NO(X) Precipitation in Polar Ice Cores. International Cosmic Ray Conference. 1. 89.2 indexed citations
Barnden, Leighton & K. G. McCracken. (1973). Attenuation of a Galactic Anisotropy by 2 and 4 Sector Interplanetary Magnetic Fields. ICRC. 2. 963.1 indexed citations
18.
McCracken, K. G.. (1966). A celestial source of X rays in the energy range 20 to 58 keV. International Cosmic Ray Conference. 1. 449.1 indexed citations
19.
McCracken, K. G. & U. R. Rao. (1965). A survey of the diurnal anisotropy. International Cosmic Ray Conference. 1. 213.17 indexed citations
20.
McCracken, K. G.. (1964). Solar cosmic ray propagation characteristics.. International Cosmic Ray Conference. 1. 83.1 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.