Citations per year, relative to G. P. Chernov G. P. Chernov (= 1×)
peers
Michael Heinemann
Countries citing papers authored by G. P. Chernov
Since
Specialization
Citations
This map shows the geographic impact of G. P. Chernov'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 G. P. Chernov with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. P. Chernov more than expected).
This network shows the impact of papers produced by G. P. Chernov. 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 G. P. Chernov. The network helps show where G. P. Chernov may publish in the future.
Co-authorship network of co-authors of G. P. Chernov
This figure shows the co-authorship network connecting the top 25 collaborators of G. P. Chernov.
A scholar is included among the top collaborators of G. P. Chernov 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 G. P. Chernov. G. P. Chernov is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Chernov, G. P. & В. В. Фомичев. (2023). Slowly drifting radio fibres. Monthly Notices of the Royal Astronomical Society. 522(2). 1930–1938.1 indexed citations
Chernov, G. P., et al.. (1999). Coronal Magnetic Structure during Long Lasting and Impulsive Type IV Radio Bursts With Fine Structures. 9. 765.1 indexed citations
9.
Chernov, G. P.. (1997). The relationship between fine structure of the solar radio emission at meter wavelengths and coronal transients. 23(6). 827–837.2 indexed citations
10.
Chernov, G. P.. (1996). A manifestation of quasilinear diffusion in whistlers in the fine structure of type IV solar radio bursts. 40(4). 561–568.5 indexed citations
Chernov, G. P.. (1990). Some Features of the Formation of Filaments in Type IV Radio Bursts. 34. 66.2 indexed citations
13.
Chernov, G. P. & В. В. Фомичев. (1989). Testing of Conservation Laws for the Interaction of Plasma Waves with Difference Frequency Whistlers in the Solar Corona. 15. 410.1 indexed citations
14.
Chernov, G. P.. (1989). Behaviour of low-frequency waves in coronal magnetic traps.. Astronomicheskii Zhurnal. 33. 1258–1270.1 indexed citations
15.
Chernov, G. P., et al.. (1989). Whistler ray tracing calculations in the solar corona.. 5. 32–43.2 indexed citations
Chernov, G. P., et al.. (1985). Broad-band solar bursts of the 'spike' type. 29. 564–568.2 indexed citations
18.
Chernov, G. P.. (1977). Morphological characteristics of solar radio bursts of the "spike" type. Soviet Astronomy. 21. 1081.1 indexed citations
19.
Chernov, G. P.. (1976). Microstructure in the continuous radiation of type IV meter bursts. Observations and model of the source. 20. 449.2 indexed citations
20.
Chernov, G. P.. (1976). Microstructure in continuous emission of type IV meter bursts. Modulation of continuous emission by wave packets of whistlers. 20. 1027.6 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.