B. B. Gvozdevsky

863 total citations
77 papers, 630 citations indexed

About

B. B. Gvozdevsky is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics. According to data from OpenAlex, B. B. Gvozdevsky has authored 77 papers receiving a total of 630 indexed citations (citations by other indexed papers that have themselves been cited), including 62 papers in Astronomy and Astrophysics, 25 papers in Geophysics and 18 papers in Nuclear and High Energy Physics. Recurrent topics in B. B. Gvozdevsky's work include Ionosphere and magnetosphere dynamics (54 papers), Solar and Space Plasma Dynamics (50 papers) and Earthquake Detection and Analysis (24 papers). B. B. Gvozdevsky is often cited by papers focused on Ionosphere and magnetosphere dynamics (54 papers), Solar and Space Plasma Dynamics (50 papers) and Earthquake Detection and Analysis (24 papers). B. B. Gvozdevsky collaborates with scholars based in Russia, Denmark and United States. B. B. Gvozdevsky's co-authors include В. А. Сергеев, É. V. Vashenyuk, Yu. V. Balabin, A. G. Yahnin, T. A. Yahnina, S. Vennerstrøm, Y. P. Maltsev, К. Мурсула, L. I. Miroshnichenko and A. G. Demekhov and has published in prestigious journals such as SHILAP Revista de lepidopterología, Journal of Geophysical Research Atmospheres and Journal of Geophysical Research Atmospheres.

In The Last Decade

B. B. Gvozdevsky

70 papers receiving 601 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
B. B. Gvozdevsky Russia 12 594 196 129 85 74 77 630
J. R. Cummings United States 15 1.0k 1.8× 128 0.7× 114 0.9× 202 2.4× 76 1.0× 54 1.1k
Brian Kress United States 21 1.2k 2.0× 349 1.8× 261 2.0× 73 0.9× 146 2.0× 56 1.2k
P. Velinov Bulgaria 15 629 1.1× 138 0.7× 47 0.4× 117 1.4× 215 2.9× 91 698
Е. Г. Ерошенко Russia 15 601 1.0× 83 0.4× 126 1.0× 104 1.2× 114 1.5× 54 664
Hanna Rothkaehl Poland 11 434 0.7× 154 0.8× 70 0.5× 73 0.9× 39 0.5× 68 517
I. N. Myagkova Russia 12 567 1.0× 104 0.5× 183 1.4× 34 0.4× 28 0.4× 107 607
D. W. Datlowe United States 18 852 1.4× 341 1.7× 167 1.3× 70 0.8× 61 0.8× 45 889
M. Gerontidou Greece 14 511 0.9× 82 0.4× 73 0.6× 60 0.7× 63 0.9× 49 581
J. T. Niehof United States 9 638 1.1× 272 1.4× 185 1.4× 31 0.4× 48 0.6× 20 660
Miranda Parisi Italy 16 798 1.3× 116 0.6× 208 1.6× 141 1.7× 100 1.4× 75 896

Countries citing papers authored by B. B. Gvozdevsky

Since Specialization
Citations

This map shows the geographic impact of B. B. Gvozdevsky'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. B. Gvozdevsky with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. B. Gvozdevsky more than expected).

Fields of papers citing papers by B. B. Gvozdevsky

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by B. B. Gvozdevsky. 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. B. Gvozdevsky. The network helps show where B. B. Gvozdevsky may publish in the future.

Co-authorship network of co-authors of B. B. Gvozdevsky

This figure shows the co-authorship network connecting the top 25 collaborators of B. B. Gvozdevsky. A scholar is included among the top collaborators of B. B. Gvozdevsky 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. B. Gvozdevsky. B. B. Gvozdevsky 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.
Gvozdevsky, B. B., et al.. (2023). Precipitation-related increase events of the electromagnetic component of secondary cosmic rays: Spectral analysis. Solar-Terrestrial Physics. 9(2). 37–47.
2.
Kirillov, A. S., et al.. (2023). Vibrational Kinetics of NO and N2 in the Earth's Middle Atmosphere During GLE69 on January 20, 2005. Journal of Geophysical Research Atmospheres. 128(17). 2 indexed citations
3.
Balabin, Yu. V., et al.. (2022). GLE73 Event (October 28, 2021) in Solar Cosmic Rays. Bulletin of the Russian Academy of Sciences Physics. 86(12). 1542–1548. 1 indexed citations
4.
Крайнев, М. Б., et al.. (2021). On the transition from 3D to 2D transport equations for a study of long-term cosmic-ray intensity variations in the heliosphere. Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021). 1323–1323. 5 indexed citations
5.
Bazilevskaya, G. A., М. Б. Крайнев, В. С. Махмутов, et al.. (2020). Temporal Characteristics of Energetic Magnetospheric Electron Precipitation as Observed During Long‐Term Balloon Observations. Journal of Geophysical Research Space Physics. 125(11). 9 indexed citations
7.
Gvozdevsky, B. B., et al.. (2018). Geomagnetic cutoff rigidities of cosmic rays and their secular changes.. 42. 1 indexed citations
8.
Gvozdevsky, B. B., et al.. (2016). Nature of gamma radiation variations during atmospheric precipitations. Solar-Terrestrial Physics. 2(1). 78–88.
9.
Balabin, Yu. V., et al.. (2013). THE FIRST GLE OF THE NEW 24 th SOLAR CYCLE. International Cosmic Ray Conference. 33. 1467. 1 indexed citations
10.
Balabin, Yu. V., et al.. (2013). Transport of solar protons through the atmosphere during GLE. Journal of Physics Conference Series. 409. 12200–12200. 2 indexed citations
11.
Balabin, Yu. V., et al.. (2011). Hadrons with energies higher than 50 MeV in EASes with N e = 105–107. Bulletin of the Russian Academy of Sciences Physics. 75(3). 360–363. 1 indexed citations
12.
Balabin, Yu. V., et al.. (2008). Observing Multiplicity Effect during December 13, 2006 event on the Barentsburg Neutron Monitor. ICRC. 1. 257–260. 3 indexed citations
13.
Vashenyuk, É. V., G. A. Bazilevskaya, B. B. Gvozdevsky, et al.. (2008). The GLE of December 13, 2006 according to the ground level and balloon observations. International Cosmic Ray Conference. 1. 221–224. 2 indexed citations
14.
Vashenyuk, É. V., Yu. V. Balabin, B. B. Gvozdevsky, & L. I. Miroshnichenko. (2007). Characteristics of relativistic solar cosmic rays in large ground-level events in 1956–2005. Bulletin of the Russian Academy of Sciences Physics. 71(7). 933–937. 5 indexed citations
15.
Vashenyuk, É. V., B. B. Gvozdevsky, L. I. Miroshnichenko, et al.. (2005). Energetic solar particle dynamics during 28 October, 2003 GLE. CERN Document Server (European Organization for Nuclear Research). 1. 217. 1 indexed citations
16.
Vashenyuk, É. V., et al.. (2003). Relativistic Solar proton Dynamics in Large GLE of 23rd Solar Cycle. International Cosmic Ray Conference. 6. 3401. 4 indexed citations
17.
Belov, А. V., J. W. Bieber, E. A. Eroshenko, et al.. (2001). The "Bastille Day"; GLE 14 July, 2000 as observed by the worldwide neutron monitor network. International Cosmic Ray Conference. 8. 3446. 5 indexed citations
18.
Yahnina, T. A., B. B. Gvozdevsky, & A. G. Yahnin. (1999). Anisotropic Precipitation of Energetic Protons from the Inner Magnetosphere. Cosmic Research. 37(1). 40–2720. 3 indexed citations
19.
Gvozdevsky, B. B. & В. А. Сергеев. (1996). MT-index — A possible new index to characterize the configuration of the magnetotail. Advances in Space Research. 18(8). 51–54. 7 indexed citations
20.
Vashenyuk, É. V., S. Fischer, & B. B. Gvozdevsky. (1993). Short Term SCR Intensity Variations During GLE. 3. 266. 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.

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