V. A. Slemzin

1.2k total citations
72 papers, 610 citations indexed

About

V. A. Slemzin is a scholar working on Astronomy and Astrophysics, Molecular Biology and Aerospace Engineering. According to data from OpenAlex, V. A. Slemzin has authored 72 papers receiving a total of 610 indexed citations (citations by other indexed papers that have themselves been cited), including 63 papers in Astronomy and Astrophysics, 14 papers in Molecular Biology and 10 papers in Aerospace Engineering. Recurrent topics in V. A. Slemzin's work include Solar and Space Plasma Dynamics (61 papers), Ionosphere and magnetosphere dynamics (33 papers) and Astro and Planetary Science (22 papers). V. A. Slemzin is often cited by papers focused on Solar and Space Plasma Dynamics (61 papers), Ionosphere and magnetosphere dynamics (33 papers) and Astro and Planetary Science (22 papers). V. A. Slemzin collaborates with scholars based in Russia, Belgium and France. V. A. Slemzin's co-authors include I. A. Zhitnik, A. A. Pertsov, A. P. Ignat’ev, A. V. Mitrofanov, Sergey Kuzin, V. V. Grechnev, S. V. Kuzin, I. M. Chertok, S. N. Oparin and A. M. Urnov and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

V. A. Slemzin

70 papers receiving 587 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
V. A. Slemzin Russia 15 520 108 54 53 42 72 610
I. A. Zhitnik Russia 14 444 0.9× 64 0.6× 67 1.2× 34 0.6× 55 1.3× 71 584
J. P. Delaboudinière France 12 694 1.3× 160 1.5× 14 0.3× 43 0.8× 32 0.8× 48 744
I. Kondò Japan 11 635 1.2× 67 0.6× 46 0.9× 44 0.8× 14 0.3× 64 698
C. J. Eyles United Kingdom 14 823 1.6× 122 1.1× 38 0.7× 36 0.7× 26 0.6× 34 904
A. K. Richter Germany 15 634 1.2× 115 1.1× 24 0.4× 21 0.4× 42 1.0× 44 686
M. R. Aellig Germany 11 374 0.7× 83 0.8× 15 0.3× 10 0.2× 22 0.5× 24 460
Albert Y. Shih United States 11 641 1.2× 70 0.6× 30 0.6× 96 1.8× 15 0.4× 59 736
S. Pensotti Italy 14 205 0.4× 17 0.2× 128 2.4× 49 0.9× 39 0.9× 49 554
Noriyuki Narukage Japan 18 1.3k 2.4× 265 2.5× 23 0.4× 83 1.6× 22 0.5× 59 1.3k
G. Mannocchi Italy 14 135 0.3× 28 0.3× 73 1.4× 10 0.2× 27 0.6× 89 643

Countries citing papers authored by V. A. Slemzin

Since Specialization
Citations

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

Fields of papers citing papers by V. A. Slemzin

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of V. A. Slemzin

This figure shows the co-authorship network connecting the top 25 collaborators of V. A. Slemzin. A scholar is included among the top collaborators of V. A. Slemzin 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. A. Slemzin. V. A. Slemzin 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.
Slemzin, V. A., et al.. (2024). Observation and modeling of complex transient structure in heliosphere followed by geomagnetic storm on May 10–11, 2024. Advances in Space Research. 76(12). 7230–7240. 2 indexed citations
2.
Slemzin, V. A., et al.. (2024). Prediction of Geomagnetic Storms Associated with Interplanetary Coronal Mass Ejections. Astronomy Reports. 68(2). 192–199. 1 indexed citations
3.
4.
Yermolaev, Yu. I., И. Г. Лодкина, M. Yu. Yermolaev, et al.. (2020). Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance. Journal of Geophysical Research Space Physics. 125(7). 8 indexed citations
5.
Slemzin, V. A., et al.. (2018). Influence of coronal mass ejections on parameters of high-speed solar wind: a case study. Journal of Space Weather and Space Climate. 8. A28–A28. 9 indexed citations
6.
Pagano, P., et al.. (2017). Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011. Solar Physics. 292(7). 16 indexed citations
7.
Veselovsky, I. S., et al.. (2017). Possible causes of the discrepancy between the predicted and observed parameters of high-speed solar wind streams. Cosmic Research. 55(1). 20–29. 5 indexed citations
8.
Slemzin, V. A., et al.. (2016). Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24. Bulletin of the Lebedev Physics Institute. 43(9). 287–290. 4 indexed citations
9.
Slemzin, V. A., et al.. (2012). Signatures of Slow Solar Wind Streams from Active Regions in the Inner Corona. Solar Physics. 286(1). 157–184. 20 indexed citations
10.
Koutchmy, S., et al.. (2008). Analysis and interpretation of a fast limb CME with eruptive prominence, C-flare, and EUV dimming. Springer Link (Chiba Institute of Technology). 8 indexed citations
11.
Slemzin, V. A., et al.. (2008). Off-limb EUV observations of the solar corona and transients with the CORONAS-F/SPIRIT telescope-coronagraph. Annales Geophysicae. 26(10). 3007–3016. 13 indexed citations
12.
Berghmans, D., J.‐F. Hochedez, A. BenMoussa, et al.. (2005). Space Weather with ESA's PROBA2 Mission. ESASP. 592. 685. 1 indexed citations
13.
Grechnev, V. V., I. M. Chertok, V. A. Slemzin, et al.. (2005). CORONAS‐F/SPIRIT EUV observations of October–November 2003 solar eruptive events in combination with SOHO/EIT data. Journal of Geophysical Research Atmospheres. 110(A9). 26 indexed citations
14.
Pertsov, A. A., et al.. (2003). High resolution temporal and spatial dynamics of solar flares from the spirit MGXII 8,42A spectral images of the Sun.. ESASP. 535. 239–241. 1 indexed citations
15.
Zhitnik, I. A., Sergey Kuzin, A. P. Ignat’ev, et al.. (2003). Results of XUV full sun imaging spectroscopy for eruptive and transient events by the spirit spectroheliograph on the CORONAS-F mission. Advances in Space Research. 32(12). 2573–2577. 5 indexed citations
16.
Kuzin, Sergey, A. P. Ignat’ev, A. V. Mitrofanov, et al.. (2002). EUV observations of solar corona in the SPIRIT experiment on board the CORONAS-F satellite. 34. 2119. 1 indexed citations
17.
Zhitnik, I. A., J. P. Delaboudinière, S. V. Kuzin, et al.. (2002). SPIRIT X-ray telescope/spectroheliometer results. elib (German Aerospace Center). 2. 915–918. 19 indexed citations
18.
Обридко, В. Н., et al.. (2000). Analyses and modelling of coronal holes observed by CORONAS-1. I. Morphology and magnetic field configuration. Astronomical and Astrophysical Transactions. 18(6). 819–828. 8 indexed citations
19.
Kolachevsky, N., Sergey Kuzin, A. V. Mitrofanov, et al.. (1998). Manufacture and testing of x-ray optical elements for the TEREK-C and RES-C instruments on the CORONAS-I mission. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 6 indexed citations
20.
Sobel'man, Igor I, I. A. Zhitnik, A. P. Ignat’ev, et al.. (1996). X-ray spectroscopy of the Sun in the 0.84-30.4 nm band in the TEREK-K and RES-K experiments on the KORONAS-I satellite. 22(4). 539–554. 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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