V. G. Kurt

630 total citations
31 papers, 410 citations indexed

About

V. G. Kurt is a scholar working on Astronomy and Astrophysics, Geophysics and Molecular Biology. According to data from OpenAlex, V. G. Kurt has authored 31 papers receiving a total of 410 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 7 papers in Geophysics and 5 papers in Molecular Biology. Recurrent topics in V. G. Kurt's work include Solar and Space Plasma Dynamics (25 papers), Ionosphere and magnetosphere dynamics (18 papers) and Astro and Planetary Science (10 papers). V. G. Kurt is often cited by papers focused on Solar and Space Plasma Dynamics (25 papers), Ionosphere and magnetosphere dynamics (18 papers) and Astro and Planetary Science (10 papers). V. G. Kurt collaborates with scholars based in Russia, Slovakia and Tajikistan. V. G. Kurt's co-authors include А. V. Belov, H. Mavromichalaki, M. Gerontidou, Jean‐Loup Bertaux, H. A. Garcia, B. Yu. Yushkov, K. Kudela, S. N. Kuznetsov, E. Eroshenko and V. G. Yanke and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, Solar Physics and Journal of Atmospheric and Solar-Terrestrial Physics.

In The Last Decade

V. G. Kurt

28 papers receiving 378 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
V. G. Kurt Russia	11	392	46	39	35	28	31	410
Yu. I. Logachëv Russia	10	403 1.0×	31 0.7×	34 0.9×	27 0.8×	46 1.6×	118	422
Karl‐Ludwig Klein France	14	499 1.3×	41 0.9×	17 0.4×	55 1.6×	21 0.8×	27	517
R. A. Leske United States	9	462 1.2×	70 1.5×	47 1.2×	36 1.0×	27 1.0×	47	488
Evangelos Paouris Greece	11	298 0.8×	27 0.6×	49 1.3×	55 1.6×	38 1.4×	28	331
H. M. Bain United States	14	450 1.1×	25 0.5×	25 0.6×	66 1.9×	14 0.5×	36	471
Э. Валтонен Finland	13	606 1.5×	76 1.7×	22 0.6×	103 2.9×	26 0.9×	55	635
J. Rodríguez‐Pacheco Spain	11	506 1.3×	36 0.8×	20 0.5×	60 1.7×	12 0.4×	70	544
M. Dierckxsens Belgium	10	331 0.8×	48 1.0×	23 0.6×	69 2.0×	29 1.0×	24	390
V. G. Kurt Russia	10	322 0.8×	30 0.7×	15 0.4×	21 0.6×	35 1.3×	31	328
A. B. Struminsky Russia	10	381 1.0×	43 0.9×	56 1.4×	23 0.7×	10 0.4×	57	403

Countries citing papers authored by V. G. Kurt

Since Specialization

Citations

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

Fields of papers citing papers by V. G. Kurt

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by V. G. Kurt. 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 V. G. Kurt. The network helps show where V. G. Kurt may publish in the future.

Co-authorship network of co-authors of V. G. Kurt

This figure shows the co-authorship network connecting the top 25 collaborators of V. G. Kurt. A scholar is included among the top collaborators of V. G. Kurt 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 V. G. Kurt. V. G. Kurt is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Yushkov, B. Yu., V. G. Kurt, & V. I. Galkin. (2023). High-Energy Emissions Observed in the Impulsive Phase of the 2001 August 25 Eruptive Flare. Solar Physics. 298(2). 1 indexed citations

Kurt, V. G., B. Yu. Yushkov, K. Kudela, V. I. Galkin, & L. K. Kashapova. (2015). CORONAS-F observation of HXR and gamma-ray emissions from the solar flare X10 on 29 October 2003 as a probe of accelerated proton spectrum. Contributions of the Astronomical Observatory Skalnaté Pleso. 45(1). 42–59. 2 indexed citations

Kurt, V. G., С. И. Свертилов, B. Yu. Yushkov, et al.. (2010). Dynamics and energetics of the thermal and nonthermal components in the solar flare of January 20, 2005, based on data from hard electromagnetic radiation detectors onboard the CORONAS-F satellite. Astronomy Letters. 36(4). 280–291. 5 indexed citations

Kuznetsov, S. N., V. G. Kurt, B. Yu. Yushkov, K. Kudela, & V. I. Galkin. (2010). Gamma-Ray and High-Energy-Neutron Measurements on CORONAS-F during the Solar Flare of 28 October 2003. Solar Physics. 268(1). 175–193. 20 indexed citations

Preka‐Papadema, P., et al.. (2010). Radio Observations of the 20 January 2005 X-class Flare. Solar Physics. 267(2). 343–359. 8 indexed citations

Kuznetsov, S. N., et al.. (2006). Proton acceleration during 20 January 2005 solar flare: CORONAS-F observations of high-energy γ emission and GLE. 36(2). 85–92. 5 indexed citations

Belov, А. V., H. A. Garcia, V. G. Kurt, H. Mavromichalaki, & M. Gerontidou. (2005). Proton Enhancements and Their Relation to the X-Ray Flares During the Three Last Solar Cycles. Solar Physics. 229(1). 135–159. 75 indexed citations

Plainaki, Christina, et al.. (2004). Unexpectable burst of solar activity recorded by neutron monitors during October-November 2003. cosp. 35. 2696. 3 indexed citations

Myagkova, I. N., et al.. (2004). Gamma-ray observations of solar flares from August 2001 to November 2003: SONG experiment onboard CORONAS-F satellite results. Proceedings of the International Astronomical Union. 2004(IAUS223). 471–472. 2 indexed citations

10.

Mavromichalaki, H., P. Preka‐Papadema, Ioannis Liritzis, B. Pétropoulos, & V. G. Kurt. (2003). Short-term variations of cosmic-ray intensity and flare related data in 1981–1983. New Astronomy. 8(8). 777–794. 31 indexed citations

11.

Kuznetsov, S. N., A. V. Bogomolov, Yu. I. Denisov, et al.. (2003). The Solar Flare of November 4, 2001, and Its Manifestations in Energetic Particles from Coronas-F Data. Solar System Research. 37(2). 121–127. 2 indexed citations

12.

Belov, А. V., V. G. Kurt, & H. Mavromichalaki. (2002). The Efficiency of Solar Flares With Gamma-ray Emission of Solar Cosmic Rays Production.. EGS General Assembly Conference Abstracts. 5752. 1 indexed citations

13.

Gerontidou, M., et al.. (2002). Frequency distributions of solar proton events. Journal of Atmospheric and Solar-Terrestrial Physics. 64(5-6). 489–496. 14 indexed citations

14.

Kahler, S. W., H. V. Cane, H. S. Hudson, et al.. (1998). The solar energetic particle event of April 14, 1994, as a probe of shock formation and particle acceleration. Journal of Geophysical Research Atmospheres. 103(A6). 12069–12076. 9 indexed citations

15.

Belov, А. V., et al.. (1994). Some evidences of prolonged particle acceleration in the high-energy gamma-ray flare of June 15, 1991. AIP conference proceedings. 294. 106–111. 5 indexed citations

16.

Belov, А. V., et al.. (1993). High Energy Gamma-Rays at the Late State of the Large Solar Flare of June 15, 1991 and Accompanying Phenomena. 3. 111. 1 indexed citations

17.

Belov, А. V., et al.. (1993). The high-energy gamma-ray flare of June, 15, 1991: Some evidence of prolonged particle acceleration at the post-eruption phase. 371–374. 2 indexed citations

18.

Giovannelli, F., P. Persi, R. Manchanda, et al.. (1990). BD+37°1160 : a probable optical counterpart of the X-ray source 1H 0521+373. 231(2). 354–364. 2 indexed citations

19.

Giovannelli, F., P. Persi, R. Manchanda, et al.. (1989). Search of the Optical Counterpart of the X-Rays Source 1H:0521+373. ESASP. 1. 579.

20.

Dalaudier, F., et al.. (1984). Characteristics of interstellar helium observed with Prognoz 6 58.4-nm photometers. 134(1). 171–184. 32 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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