М. Б. Крайнев

1.2k total citations
102 papers, 763 citations indexed

About

М. Б. Крайнев is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Artificial Intelligence. According to data from OpenAlex, М. Б. Крайнев has authored 102 papers receiving a total of 763 indexed citations (citations by other indexed papers that have themselves been cited), including 94 papers in Astronomy and Astrophysics, 26 papers in Atmospheric Science and 23 papers in Artificial Intelligence. Recurrent topics in М. Б. Крайнев's work include Solar and Space Plasma Dynamics (90 papers), Ionosphere and magnetosphere dynamics (52 papers) and Atmospheric Ozone and Climate (25 papers). М. Б. Крайнев is often cited by papers focused on Solar and Space Plasma Dynamics (90 papers), Ionosphere and magnetosphere dynamics (52 papers) and Atmospheric Ozone and Climate (25 papers). М. Б. Крайнев collaborates with scholars based in Russia, South Africa and Germany. М. Б. Крайнев's co-authors include G. A. Bazilevskaya, В. С. Махмутов, N. S. Svirzhevsky, A. K. Svirzhevskaya, E. O. Flückiger, Y. I. Stozhkov, M. Storini, L. Desorgher, R. G. Harrison and G. A. Kovaltsov and has published in prestigious journals such as SHILAP Revista de lepidopterología, Space Science Reviews and Solar Physics.

In The Last Decade

М. Б. Крайнев

92 papers receiving 711 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
М. Б. Крайнев Russia	11	679	255	133	95	88	102	763
A. K. Svirzhevskaya Russia	10	615 0.9×	263 1.0×	141 1.1×	62 0.7×	92 1.0×	65	715
N. S. Svirzhevsky Russia	10	552 0.8×	249 1.0×	119 0.9×	49 0.5×	93 1.1×	64	645
Y. I. Stozhkov Russia	11	732 1.1×	324 1.3×	231 1.7×	61 0.6×	134 1.5×	138	922
В. С. Махмутов Russia	18	976 1.4×	383 1.5×	235 1.8×	88 0.9×	147 1.7×	117	1.2k
Agnieszka Gil Poland	14	574 0.8×	125 0.5×	119 0.9×	105 1.1×	25 0.3×	62	657
Jose F. Valdés Galicia Mexico	15	560 0.8×	86 0.3×	314 2.4×	47 0.5×	45 0.5×	99	771
Konstantin Herbst Germany	17	672 1.0×	185 0.7×	133 1.0×	37 0.4×	36 0.4×	56	817
P. Velinov Bulgaria	15	629 0.9×	215 0.8×	117 0.9×	24 0.3×	36 0.4×	91	698
E. Eroshenko Russia	17	801 1.2×	167 0.7×	145 1.1×	103 1.1×	15 0.2×	77	867
É. V. Vashenyuk Russia	15	613 0.9×	92 0.4×	169 1.3×	50 0.5×	20 0.2×	86	698

Countries citing papers authored by М. Б. Крайнев

Since Specialization

Citations

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

Fields of papers citing papers by М. Б. Крайнев

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by М. Б. Крайнев. 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 М. Б. Крайнев. The network helps show where М. Б. Крайнев may publish in the future.

Co-authorship network of co-authors of М. Б. Крайнев

This figure shows the co-authorship network connecting the top 25 collaborators of М. Б. Крайнев. A scholar is included among the top collaborators of М. Б. Крайнев 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 М. Б. Крайнев. М. Б. Крайнев 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

Крайнев, М. Б., et al.. (2023). Fifty years of studying the GCR intensity during inversion of heliospheric magnetic fields I. Observations. Solar-Terrestrial Physics. 9(4). 3–16. 2 indexed citations

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

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

Крайнев, М. Б., et al.. (2012). On the formation of spot and magnetic cycles in the galactic cosmic ray intensity in the minima of solar activity. Bulletin of the Lebedev Physics Institute. 39(6). 175–180. 1 indexed citations

Крайнев, М. Б.. (2012). On the intensity of galactic cosmic rays in the inner heliosphere during epochs of minimum solar activity. Bulletin of the Lebedev Physics Institute. 39(6). 185–190. 1 indexed citations

Крайнев, М. Б.. (2012). On the heliosphere characteristics important for galactic cosmic rays in the phase of minimum solar activity. Bulletin of the Lebedev Physics Institute. 39(6). 170–174. 1 indexed citations

Крайнев, М. Б.. (2007). On the detailed information in the regular balloon monitoring of cosmic rays: the description of the method and some new results. ICRC. 1. 465–468.

Махмутов, В. С., et al.. (2003). Semiannual Variation in the Number of Energetic Electron Precipitation Events Recorded in the Polar Atmosphere. International Cosmic Ray Conference. 7. 4233. 1 indexed citations

Bazilevskaya, G. A., et al.. (2001). Distribution of solar energetic particle events over an 11-year solar cycle. International Cosmic Ray Conference. 8. 3413. 4 indexed citations

10.

Крайнев, М. Б.. (1999). The Gnevyshev gap effect in galactic cosmic rays. ICRC. 7. 155. 6 indexed citations

11.

Bazilevskaya, G. A., et al.. (1997). On the Angular Distribution of Cosmic Ray Intensity in the Earth's Atmosphere. International Cosmic Ray Conference. 7. 321. 1 indexed citations

12.

Bazilevskaya, G. A., et al.. (1995). Long-Term Changes in Galactic Cosmic Ray Variation Caused by the Solar Rotation. International Cosmic Ray Conference. 4. 572. 3 indexed citations

13.

Svirzhevsky, N. S., G. A. Bazilevskaya, М. Б. Крайнев, В. С. Махмутов, & A. K. Svirzhevskaya. (1995). The Energy Hysteresis of the Galactic Cosmic Ray Intensity in 1988-1993. International Cosmic Ray Conference. 4. 550. 2 indexed citations

14.

Крайнев, М. Б., et al.. (1995). On the 2D and 3D Cosmic Ray Transport Equations. International Cosmic Ray Conference. 4. 688. 2 indexed citations

15.

Bazilevskaya, G. A., М. Б. Крайнев, Y. I. Stozhkov, A. K. Svirzhevskaya, & N. S. Svirzhevsky. (1993). Cosmic Ray Intensity in Four Successive Sunspot Maxima. 3. 601. 5 indexed citations

16.

Крайнев, М. Б. & W. R. Webber. (1993). The Galactic Cosmic Rays Near the Solar Activity Minimum II. The Model for the Behavior of Positive and Negative Cosmic Rays Near the Current Sheet. 3. 555. 2 indexed citations

17.

Крайнев, М. Б.. (1987). The Long-Term Variation of the Highlatitude Interplanetary Magnetic Field and the Galactic Cosmic Rays. International Cosmic Ray Conference. 3. 381. 1 indexed citations

18.

Крайнев, М. Б., et al.. (1983). On the Energetic "hysteresis" in the Galactic Cosmic Ray Intensity. International Cosmic Ray Conference. 3. 23. 2 indexed citations

19.

Крайнев, М. Б., et al.. (1983). On the "anomalous" Phenomena in the Galactic Cosmic Ray Intensity in the Periods of the Inversion of General Magnetic Field of the Sun. International Cosmic Ray Conference. 3. 95. 1 indexed citations

20.

Крайнев, М. Б.. (1981). The Electromagnetic Field in and Outside the Solar Wind Cavity and the Galactic Cosmic Rays. International Cosmic Ray Conference. 3. 357. 3 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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