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.
Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties
2010634 citationsI. G. Richardson, H. V. Caneprofile →
Interplanetary coronal mass ejections in the near‐Earth solar wind during 1996–2002
2003485 citationsH. V. Cane, I. G. Richardsonprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of H. V. Cane'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. V. Cane with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. V. Cane more than expected).
This network shows the impact of papers produced by H. V. Cane. 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. V. Cane. The network helps show where H. V. Cane may publish in the future.
Co-authorship network of co-authors of H. V. Cane
This figure shows the co-authorship network connecting the top 25 collaborators of H. V. Cane.
A scholar is included among the top collaborators of H. V. Cane 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. V. Cane. H. V. Cane is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Richardson, I. G. & H. V. Cane. (2011). Identification of Interplanetary Coronal Mass Ejections at Ulysses Using Multiple Solar Wind Signatures, and Comparison with ICMEs Observed at the Earth and in the Inner Heliosphere. AGU Fall Meeting Abstracts. 2011.1 indexed citations
3.
Richardson, I. G. & H. V. Cane. (2007). Interplanetary Coronal Mass Ejections During 1996 - 2007. International Cosmic Ray Conference. 1. 319–322.3 indexed citations
4.
Richardson, I. G., H. V. Cane, T. T. von Rosenvinge, & R. E. McGuire. (2006). IMP 8 GME Energetic Particle Observations Over Three Solar Cycles. AGU Spring Meeting Abstracts. 1. 323–326.1 indexed citations
5.
Cyr, O. C. St., H. V. Cane, N. Nitta, et al.. (2001). Two Recent Electron-Rich Energetic Particle Events and Their Associated CMEs. AGUFM. 2001.1 indexed citations
6.
Cane, H. V.. (2001). Are There Two Classes of Solar Energetic Particle Events. International Cosmic Ray Conference. 1. 3231.3 indexed citations
7.
Cane, H. V., et al.. (2001). Cosmic Ray Evidence for Magnetic Field Line Disconnection Inside Interplanetary Coronal Mass Ejections. International Cosmic Ray Conference. 9. 3531.2 indexed citations
8.
Lepri, S. T., T. H. Zurbuchen, L. A. Fisk, et al.. (2001). Iron Charge State Distributions as an Identifier of Interplanetary Coronal Mass Ejections. AGU Spring Meeting Abstracts. 2001.3 indexed citations
9.
Richardson, I. G., et al.. (2001). Bidirectional Cosmic Ray and 1 MeV Ion Flows, and their Association With Ejecta.. ICRC. 9. 3498.3 indexed citations
10.
Wibberenz, G., H. V. Cane, & I. G. Richardson. (1997). Two-step Forbush Decreases in thecInner Solar System and their Relevance for Models of Transient Disturbances. International Cosmic Ray Conference. 1. 397.3 indexed citations
11.
Richardson, I. G. & H. V. Cane. (1995). Corotating >60 MeV/amu Cosmic Ray Depressions Observed by Spacecraft Anti-Coincidence Guards. ICRC. 4. 960.2 indexed citations
12.
Cliver, E. W., S. W. Kahler, D. F. Neidig, et al.. (1995). Extreme "Propagation" of Solar Energetic Particles. ICRC. 4. 257.16 indexed citations
13.
Richardson, I. G. & H. V. Cane. (1995). Anisotropies of Solar Particle Onsets Observed Within Ejecta. International Cosmic Ray Conference. 4. 373.2 indexed citations
14.
Cane, H. V., I. G. Richardson, & G. Wibberenz. (1995). The Response of Energetic Particles to the Presence of Ejecta Material. ICRC. 4. 377.18 indexed citations
15.
Wibberenz, G. & H. V. Cane. (1993). Multi-Spacecraft Observations of Particles and Shocks in the Inner Heliosphere. 3. 274.2 indexed citations
16.
Cliver, E. W., D. V. Reames, S. W. Kahler, & H. V. Cane. (1991). Size distributions of solar energetic particle events. International Cosmic Ray Conference. 3. 25.2 indexed citations
17.
Cane, H. V., D. V. Reames, & T. T. von Rosenvinge. (1990). The origin of solar particle events with low Fe/O. ICRC. 5. 370.1 indexed citations
18.
Reames, D. V., H. V. Cane, & T. T. von Rosenvinge. (1990). Energetic-Particle Abundances in Impulsive Solar Flares. ICRC. 5. 108.1 indexed citations
19.
Cane, H. V.. (1983). Velocity profiles of interplanetary shocks. NASA Technical Reports Server (NASA). 228.10 indexed citations
20.
Cane, H. V., R. G. Stone, J. Fainberg, J. L. Steinberg, & S. Hoang. (1980). Type 2 solar radio events observed in the interplanetary medium. Part 1: General characteristics. NASA STI/Recon Technical Report N. 81. 15927.17 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.