This map shows the geographic impact of В. Н. Обридко'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 В. Н. Обридко with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites В. Н. Обридко more than expected).
This network shows the impact of papers produced by В. Н. Обридко. 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 В. Н. Обридко. The network helps show where В. Н. Обридко may publish in the future.
Co-authorship network of co-authors of В. Н. Обридко
This figure shows the co-authorship network connecting the top 25 collaborators of В. Н. Обридко.
A scholar is included among the top collaborators of В. Н. Обридко 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 В. Н. Обридко. В. Н. Обридко is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Обридко, В. Н., et al.. (2005). Some Fractal Properties of Solar Magnetic Fields. ESASP. 596.1 indexed citations
9.
Badalyan, O. G., В. Н. Обридко, & J. Sýkora. (2002). Direction of the coronal green line polarization as derived from the eclipse measurements. Contributions of the Astronomical Observatory Skalnaté Pleso. 32(1). 49–61.1 indexed citations
10.
Обридко, В. Н., et al.. (2002). Meridional drifts of large-scale solar magnetic fields and meridional circulation. 2. 851–854.1 indexed citations
11.
Обридко, В. Н., et al.. (2002). Secular and cycle variations of the IMF Bz component and some associated geophysical effects. ESASP. 477. 405–407.2 indexed citations
12.
Sýkora, J., et al.. (1999). Structure and magnetic field of the July 11, 1991 eclipse corona from the solar cycle viewpoint. Contributions of the Astronomical Observatory Skalnaté Pleso. 29(2). 89–104.2 indexed citations
13.
Обридко, В. Н., et al.. (1999). Studies of the rotation periods of photospheric magnetic fields in the 20th-22nd solar cycles. Astronomy Reports. 43(12). 831–837.3 indexed citations
14.
Шубин, В.Н., et al.. (1997). Dependence of the Density of the Upper Atmosphere on Solar Activity from Satellite Drag Data. Cosmic Research. 35(2). 114.1 indexed citations
15.
Ivanov, Evgeniy V., В. Н. Обридко, & B. D. Shelting. (1997). Large-scale structure of solar magnetic fields and coronal mass ejections. 41(2). 236–239.6 indexed citations
16.
Обридко, В. Н., et al.. (1996). Calculating Solar Wind Parameters from Solar Magnetic Field Data. ASPC. 95. 366.1 indexed citations
17.
Обридко, В. Н., et al.. (1992). Frequency composition of long-period magnetic field variations of the sun as a star. AZh. 69(5). 1083–1089.3 indexed citations
18.
Гершберг, Р. Е., et al.. (1987). Energetics of activity of flare stars and the Sun: a synergetical approach.. 3. 3–17.
19.
Staude, J., J. Hildebrandt, A. Krüger, et al.. (1984). The atmosphere of a sunspot based on observations in the X-ray, extreme ultraviolet, optical, and radio ranges. 28. 557–563.1 indexed citations
20.
Обридко, В. Н., et al.. (1974). Solar Proton Flares and the Sector Structure of the Interplanetary Magnetic Field. Geomagnetism and Aeronomy. 14(1). 1.1 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.