This map shows the geographic impact of R. Tousey'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 R. Tousey with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Tousey more than expected).
This network shows the impact of papers produced by R. Tousey. 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 R. Tousey. The network helps show where R. Tousey may publish in the future.
Co-authorship network of co-authors of R. Tousey
This figure shows the co-authorship network connecting the top 25 collaborators of R. Tousey.
A scholar is included among the top collaborators of R. Tousey 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 R. Tousey. R. Tousey 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.
Underwood, J. H., et al.. (1976). Observations of Coronal Holes Throughout Sunspot Cycle 20.. Bulletin of the American Astronomical Society. 8. 557.1 indexed citations
2.
Howard, R. A., M. J. Koomen, D. J. Michels, et al.. (1975). Synoptic observations of the solar. STIN. 76. 16001.1 indexed citations
3.
Sheeley, N. R., J. D. Bohlin, G. E. Brueckner, et al.. (1975). Interpreting XUV Spectroheliograms in Terms of Coronal Magnetic Field Structures. Bulletin of the American Astronomical Society. 7. 346.2 indexed citations
4.
Bohlin, J. D., J. D. Purcell, N. R. Sheeley, & R. Tousey. (1975). Polar Plumes in XUV Emission-Line Corona. Bulletin of the American Astronomical Society. 7. 356.5 indexed citations
5.
Bohlin, J. D., G. E. Brueckner, J. D. Purcell, et al.. (1974). The eruptive prominence of August 21, 1973 observed from Skylab in the white light corona and in the He II 304 Å chromosphere.. Bulletin of the American Astronomical Society. 6. 219.2 indexed citations
6.
Milone, E. F., et al.. (1974). An Atlas of the Solar Ultraviolet Spectrum between 2220 and 2990Å. Bulletin of the American Astronomical Society. 6. 292.1 indexed citations
7.
Tousey, R.. (1973). The solar corona.. 2. 713–730.120 indexed citations
8.
Tousey, R.. (1973). First Results from Skylab.. Bulletin of the American Astronomical Society. 5. 419.8 indexed citations
9.
Tousey, R. & M. J. Koomen. (1972). Movement of a Bright Source in the White-Light Corona. Bulletin of the American Astronomical Society. 4. 394.5 indexed citations
Michels, D. J. & R. Tousey. (1971). The Sun's Changing XUV Corona, As Viewed from OSO-7.. Bulletin of the American Astronomical Society. 3. 439.1 indexed citations
Purcell, J. D. & R. Tousey. (1969). Gyrosynchrotron Radiation and Solar Microwave Bursts. Bulletin of the American Astronomical Society. 1. 290.5 indexed citations
14.
Koomen, M. J., et al.. (1967). Photographs of particles from an Aerobee rocket at 130-km to 204-km altitude. 11. 333.1 indexed citations
Tousey, R.. (1964). Sun, Spectrum of, in Extreme Ultraviolet (George Darwin Lecture). Quarterly journal of the Royal Astronomical Society. 5. 123.2 indexed citations
17.
Purcell, J. D., et al.. (1963). Solar Spectra from 3500 to 2200 A at 30 mA Resolution. 781.2 indexed citations
Purcell, J. D., et al.. (1960). The ultraviolet spectrum of the sun. 581.3 indexed citations
20.
Purcell, J. D. & R. Tousey. (1960). The profile of solar Lyman Alpha. 590.3 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.