E. A. Eroshenko

975 total citations
57 papers, 750 citations indexed

About

E. A. Eroshenko is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Molecular Biology. According to data from OpenAlex, E. A. Eroshenko has authored 57 papers receiving a total of 750 indexed citations (citations by other indexed papers that have themselves been cited), including 45 papers in Astronomy and Astrophysics, 15 papers in Nuclear and High Energy Physics and 8 papers in Molecular Biology. Recurrent topics in E. A. Eroshenko's work include Solar and Space Plasma Dynamics (45 papers), Ionosphere and magnetosphere dynamics (31 papers) and Astrophysics and Cosmic Phenomena (15 papers). E. A. Eroshenko is often cited by papers focused on Solar and Space Plasma Dynamics (45 papers), Ionosphere and magnetosphere dynamics (31 papers) and Astrophysics and Cosmic Phenomena (15 papers). E. A. Eroshenko collaborates with scholars based in Russia, Italy and Israel. E. A. Eroshenko's co-authors include А. V. Belov, V. G. Yanke, V. A. Oleneva, А. А. Аbunin, М. А. Аbunina, A. B. Struminsky, Л. И. Дорман, G. Villoresi, N. Iucci and L. I. Gromova and has published in prestigious journals such as SHILAP Revista de lepidopterología, Monthly Notices of the Royal Astronomical Society and IEEE Transactions on Plasma Science.

In The Last Decade

E. A. Eroshenko

56 papers receiving 724 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
E. A. Eroshenko Russia	15	658	145	127	125	122	57	750
Miranda Parisi Italy	16	798 1.2×	208 1.4×	116 0.9×	100 0.8×	141 1.2×	75	896
E. Eroshenko Russia	17	801 1.2×	118 0.8×	93 0.7×	167 1.3×	145 1.2×	77	867
А. А. Аbunin Russia	16	773 1.2×	149 1.0×	73 0.6×	194 1.6×	115 0.9×	96	828
Yu Yi South Korea	16	642 1.0×	148 1.0×	55 0.4×	93 0.7×	70 0.6×	93	719
Е. Г. Ерошенко Russia	15	601 0.9×	126 0.9×	83 0.7×	114 0.9×	104 0.9×	54	664
М. А. Аbunina Russia	15	724 1.1×	140 1.0×	63 0.5×	180 1.4×	106 0.9×	98	771
V. A. Oleneva Russia	14	659 1.0×	129 0.9×	38 0.3×	180 1.4×	112 0.9×	68	699
P. Preka‐Papadema Greece	18	553 0.8×	147 1.0×	69 0.5×	52 0.4×	63 0.5×	43	659
M. Gerontidou Greece	14	511 0.8×	73 0.5×	82 0.6×	63 0.5×	60 0.5×	49	581
Pingbing Zuo China	16	691 1.1×	157 1.1×	120 0.9×	42 0.3×	89 0.7×	102	756

Countries citing papers authored by E. A. Eroshenko

Since Specialization

Citations

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

Fields of papers citing papers by E. A. Eroshenko

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by E. A. Eroshenko. 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 E. A. Eroshenko. The network helps show where E. A. Eroshenko may publish in the future.

Co-authorship network of co-authors of E. A. Eroshenko

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Belov, А. V., et al.. (2008). Variations of Parameters of Rigidity Spectrum of Cosmic Rays during events of January, 2005. ICRC. 1. 155–158. 1 indexed citations

Belov, А. V., et al.. (2005). Frequency of Forbush effects as an index of solar activity. CERN Document Server (European Organization for Nuclear Research). 1. 375. 5 indexed citations

Belov, А. V., R. Bütikofer, E. A. Eroshenko, et al.. (2003). Interplanetary Magnetic Field Disturbances with Particularly High Cosmic Ray Modulation Efficiency. ICRC. 6. 3581. 3 indexed citations

Дорман, Л. И., А. V. Belov, E. A. Eroshenko, et al.. (2003). Possible Cosmic Ray Using for Forecasting of Major Geo- magnetic Storms, Accompanied by Forbush-Effects. ICRC. 6. 3553. 6 indexed citations

Belov, А. V., et al.. (2002). Model of The Solar Cosmic Ray Propagation and Its Use In The Short Time Prognosis of The Proton Enhancements.. EGS General Assembly Conference Abstracts. 1387. 1 indexed citations

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

Belov, А. V., E. A. Eroshenko, B. Heber, et al.. (2001). Latitudinal and radial variation of >2 GeV/n protons and alpha particles in the southern heliosphere at solar maximum: Ulysses cospinket and neutron monitor network observations. International Cosmic Ray Conference. 10. 3996. 1 indexed citations

Belov, А. V., E. A. Eroshenko, V. A. Oleneva, A. B. Struminsky, & V. G. Yanke. (2001). What determines the magnitude of forbush decreases?. Advances in Space Research. 27(3). 625–630. 98 indexed citations

Belov, А. V., E. A. Eroshenko, & V. G. Yanke. (1997). Modulation Effects in 1991-1992 Years. ICRC. 1. 437. 7 indexed citations

10.

Belov, А. V., et al.. (1993). The Amplitude-Phase Interrelation of CR Anisotropy in the Two Last Solar Minima. 3. 641. 1 indexed citations

11.

Belov, А. V., et al.. (1993). Long Time Modulation of the Neutron Monitors Barometric Coefficients. 3. 613. 1 indexed citations

12.

Белов, А. А., et al.. (1991). The Amplitude-Phase Interrelation and Other Peculiarities of the First Cosmic Ray Anisotropy Harmonic. ICRC. 3. 457. 1 indexed citations

13.

Belov, А. V., Л. И. Дорман, E. A. Eroshenko, et al.. (1991). The Features of the Ground Level Increase of Cosmic Ray Intensity on September 29, 1989. International Cosmic Ray Conference. 3. 105. 6 indexed citations

14.

Belov, А. V., Л. И. Дорман, E. A. Eroshenko, & V. A. Oleneva. (1987). Cosmic Ray Gradient Variations in 1974. International Cosmic Ray Conference. 4. 137. 2 indexed citations

15.

Belov, А. V., et al.. (1983). Interplanetary modulation of the anisotropy and density of cosmic rays.. 47. 1864–1866. 1 indexed citations

16.

Belov, А. V. & E. A. Eroshenko. (1981). The Reception Coefficients of Neutron Monitors. International Cosmic Ray Conference. 4. 97. 4 indexed citations

17.

Belov, А. V., et al.. (1978). Solar cosmic rays of 22 November 1977 from data of the neutron component.. Ge&Ae. 18. 1017–1021. 1 indexed citations

18.

Belov, А. V., et al.. (1978). Variations of cosmic rays in the period from the 7 to 24 September 1977 from data of the neutron component.. Geomagnetism and Aeronomy. 18. 804–808. 1 indexed citations

19.

Belov, А. V., et al.. (1977). Joint Analysis of the Data on the Cosmic Ray Anisotropy and the Interplanetary Magnetic Field. ICRC. 4. 117. 1 indexed citations

20.

Belov, А. V., et al.. (1973). Studies of isotropic and anisotropic cosmic-ray variations in the Earth's vicinities during disturbed periods. International Cosmic Ray Conference. 2. 1247. 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.

Explore authors with similar magnitude of impact