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.
Rapid local acceleration of relativistic radiation-belt electrons by magnetospheric chorus
2013623 citationsQianli Ma, Jacob Bortnik et al.profile →
Electron Acceleration in the Heart of the Van Allen Radiation Belts
2013458 citationsG. D. Reeves, M. G. Henderson et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by M. G. Henderson
Since
Specialization
Citations
This map shows the geographic impact of M. G. Henderson'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 M. G. Henderson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. G. Henderson more than expected).
This network shows the impact of papers produced by M. G. Henderson. 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 M. G. Henderson. The network helps show where M. G. Henderson may publish in the future.
Co-authorship network of co-authors of M. G. Henderson
This figure shows the co-authorship network connecting the top 25 collaborators of M. G. Henderson.
A scholar is included among the top collaborators of M. G. Henderson 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 M. G. Henderson. M. G. Henderson is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
MacDonald, E., L. Kepko, Joseph E. Borovsky, et al.. (2017). Mission Concept to Connect Magnetospheric Physical Processes to Ionospheric Phenomena. AGUFM. 2017.1 indexed citations
Tu, Weichao, et al.. (2014). Modeling the Impenetrable Barrier to Inward Transport of Ultra-relativistic Radiation Belt Electrons. AGU Fall Meeting Abstracts. 2014.1 indexed citations
Reeves, G. D., Steven K. Morley, R. H. Friedel, et al.. (2010). On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake Revisited. AGUFM. 2010.1 indexed citations
16.
Wilson, R. J., R. L. Tokar, M. G. Henderson, et al.. (2007). Thermal Plasma Flow in Saturn's Inner Magnetosphere.. AGU Fall Meeting Abstracts. 2007.1 indexed citations
17.
Clauer, C. R., Xia Cai, D. T. Welling, A. D. DeJong, & M. G. Henderson. (2005). Characterizing the April 18, 2002 Storm-time Sawtooth Events using Ground Magnetic Data. AGUSM. 2005.4 indexed citations
18.
Henderson, M. G., R. H. Friedel, R. M. Skoug, et al.. (2002). Simultaneous Multipoint Observations of Stormtime Substorms with the CLUSTER, IMAGE, POLAR, Geosynchronous, and GPS Spacecraft. AGUSM. 2002.3 indexed citations
19.
Reeves, G. D., M. G. Henderson, R. M. Skoug, et al.. (2001). The ENA, Ring Current, and Auroral Response to ``Sawtooth Injections" in the October 4-6, 2000 Storm. AGUFM. 2001.2 indexed citations
20.
Reeves, G. D., et al.. (1996). Los Alamos space weather data products: on line and on time. ESASP. 389. 689.9 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.