Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma
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doi.org/10.1086/149674 →Countries where authors are citing Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma
This map shows the geographic impact of Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma. 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 Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma more than expected).
Fields of papers citing Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma
This network shows the impact of Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the Turbulence, Viscosity, and Dissipation in the Solar-Wind Plasma.
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.
This paper is also available at doi.org/10.1086/149674.