This map shows the geographic impact of B. V. Jackson'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 B. V. Jackson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. V. Jackson more than expected).
This network shows the impact of papers produced by B. V. Jackson. 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 B. V. Jackson. The network helps show where B. V. Jackson may publish in the future.
Co-authorship network of co-authors of B. V. Jackson
This figure shows the co-authorship network connecting the top 25 collaborators of B. V. Jackson.
A scholar is included among the top collaborators of B. V. Jackson 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 B. V. Jackson. B. V. Jackson is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Liou, K., D. G. Socker, R. A. Howard, et al.. (2015). The first super geomagnetic storm of solar cycle 24: "The St. Patrick day (17 March 2015)" event. AGU Fall Meeting Abstracts. 2015.2 indexed citations
4.
Bisi, M. M., et al.. (2011). Current and Planned Solar Wind Observations Using the EISCAT and LOFAR Radio-Telescope Systems. AGU Fall Meeting Abstracts. 2011.1 indexed citations
Jackson, B. V., A. Buffington, P. P. Hick, M. Kojima, & M. Tokumaru. (2004). Comparison of Solar Mass Ejection Imager (SMEI) White Light Observations with IPS Velocity. AGUFM. 2004.1 indexed citations
Kojima, M., B. V. Jackson, Paul Hick, et al.. (1998). Solar Wind Structure at 0.1-1 AU Reconstructed from IPS Observations Using Tomography. 207.1 indexed citations
11.
Jackson, B. V., et al.. (1995). Three-dimensional reconstruction of a coronal mass ejection.. 299. 885.16 indexed citations
Schwenn, R., E. Marsch, & B. V. Jackson. (1993). Book-Review - Physics of the Inner Heliosphere - Part Two - Particles Waves and Turbulence. Solar Physics. 145. 405.3 indexed citations
14.
Švestka, Z., B. V. Jackson, & M. E. Machado. (1992). Eruptive solar flares : proceedings of Colloquium no. 133 of the International Astronomical Union held at Iguazú, Argentina, 2-6 August, 1991. Springer eBooks.1 indexed citations
15.
Webb, D. F., B. V. Jackson, & D. V. Reames. (1992). Study of CMES Observed in the Heliosphere Using HELIOS Photometer, Magnetic Field and Plasma Data. 180.1 indexed citations
16.
Jackson, B. V., et al.. (1987). Detection of CMEs in the Interplanetary Medium from 1976-1979 Using Helios-2 Photometer data. 2. 267.1 indexed citations
17.
Jackson, B. V., R. A. Howard, M. J. Koomen, D. J. Michels, & N. R. Sheeley. (1985). White Light and X-ray Studies of the Coronal Mass Ejection Onset Phase. Bulletin of the American Astronomical Society. 17. 636.2 indexed citations
18.
Jackson, B. V.. (1984). Helios Spacecraft and Earth Perspective Observations of the Loop-Like Solar Mass Ejection of 24 May 1979. Bulletin of the American Astronomical Society. 16. 453.1 indexed citations
Jackson, B. V.. (1976). A Polar Coronal Hole: I. The Three Dimensional Boundary. Bulletin of the American Astronomical Society. 8. 325.2 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.