V. I. Shematovich

4.3k total citations
150 papers, 2.7k citations indexed

About

V. I. Shematovich is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, V. I. Shematovich has authored 150 papers receiving a total of 2.7k indexed citations (citations by other indexed papers that have themselves been cited), including 142 papers in Astronomy and Astrophysics, 45 papers in Atmospheric Science and 8 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in V. I. Shematovich's work include Astro and Planetary Science (109 papers), Planetary Science and Exploration (55 papers) and Solar and Space Plasma Dynamics (51 papers). V. I. Shematovich is often cited by papers focused on Astro and Planetary Science (109 papers), Planetary Science and Exploration (55 papers) and Solar and Space Plasma Dynamics (51 papers). V. I. Shematovich collaborates with scholars based in Russia, Belgium and United States. V. I. Shematovich's co-authors include Д. В. Бисикало, Jean‐Claude Gérard, R. E. Johnson, B. Hubert, H. Lämmer, Eric Herbst, François Leblanc, Randall S. Johnson, B. Hubert and Bertrand Bonfond and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Geophysical Research Letters.

In The Last Decade

V. I. Shematovich

142 papers receiving 2.5k 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. I. Shematovich Russia 31 2.5k 683 249 244 216 150 2.7k
Laurence M. Trafton United States 30 2.4k 0.9× 767 1.1× 300 1.2× 241 1.0× 308 1.4× 151 2.8k
Jane L. Fox United States 35 3.1k 1.2× 693 1.0× 103 0.4× 289 1.2× 146 0.7× 107 3.4k
Olivier Witasse Netherlands 32 2.7k 1.1× 498 0.7× 183 0.7× 276 1.1× 146 0.7× 168 3.0k
Joseph Harrington United States 28 2.5k 1.0× 462 0.7× 115 0.5× 127 0.5× 227 1.1× 74 2.7k
R. Rodrigo Spain 27 1.8k 0.7× 831 1.2× 85 0.3× 167 0.7× 164 0.8× 78 2.0k
Д. В. Бисикало Russia 24 1.9k 0.8× 374 0.5× 194 0.8× 86 0.4× 59 0.3× 169 2.0k
J. J. López‐Moreno Spain 29 1.9k 0.8× 845 1.2× 102 0.4× 160 0.7× 166 0.8× 117 2.3k
T. E. Cravens United States 37 3.8k 1.5× 637 0.9× 520 2.1× 419 1.7× 153 0.7× 107 4.0k
R. E. Hartle United States 36 4.0k 1.6× 518 0.8× 861 3.5× 193 0.8× 115 0.5× 125 4.2k
Wing‐Huen Ip Taiwan 26 1.8k 0.7× 253 0.4× 261 1.0× 241 1.0× 114 0.5× 104 2.0k

Countries citing papers authored by V. I. Shematovich

Since Specialization
Citations

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

Fields of papers citing papers by V. I. Shematovich

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of V. I. Shematovich

This figure shows the co-authorship network connecting the top 25 collaborators of V. I. Shematovich. A scholar is included among the top collaborators of V. I. Shematovich 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. I. Shematovich. V. I. Shematovich 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.
Shematovich, V. I., et al.. (2023). Non-Thermal Nitric Oxide Formation in the Earth’s Polar Atmosphere. Atmosphere. 14(7). 1092–1092. 3 indexed citations
2.
Hughes, A. C. G., Michael Chaffin, E. J. Mierkiewicz, et al.. (2023). Advancing Our Understanding of Martian Proton Aurora Through a Coordinated Multi‐Model Comparison Campaign. Journal of Geophysical Research Space Physics. 128(10). 5 indexed citations
3.
Bhattacharyya, Dolon, J. T. Clarke, Majd Mayyasi, et al.. (2023). Evidence of Non‐Thermal Hydrogen in the Exosphere of Mars Resulting in Enhanced Water Loss. Journal of Geophysical Research Planets. 128(8). 7 indexed citations
4.
Жилкин, А. Г., et al.. (2023). Aeronomic Model of Hydrogen–Helium Upper Atmospheres of Hot Giant Exoplanets. Astronomy Reports. 67(12). 1329–1347. 2 indexed citations
5.
Shematovich, V. I., et al.. (2022). Nonthermal Atmospheric Losses for the Exoplanet GJ 3470b. Astronomy Reports. 66(12). 1254–1261. 1 indexed citations
6.
Бисикало, Д. В., et al.. (2020). Gas envelopes of exoplanets — hot Jupiters. Physics-Uspekhi. 64(8). 747–800. 12 indexed citations
7.
Shematovich, V. I. & M. Ya. Marov. (2017). Escape of planetary atmospheres: physical processes and numerical models. Physics-Uspekhi. 61(3). 217–246. 16 indexed citations
8.
Goldstein, J., Д. В. Бисикало, V. I. Shematovich, et al.. (2016). Analytical estimate for low‐altitude ENA emissivity. Journal of Geophysical Research Space Physics. 121(2). 1167–1191. 8 indexed citations
9.
Lucchetti, Alice, Christina Plainaki, G. Cremonese, et al.. (2015). Loss rates of Europa's exosphere. European Planetary Science Congress. 2 indexed citations
10.
Бисикало, Д. В., et al.. (2012). 3D gas dynamic simulation of the interaction between the ``hot Jupiter'' planet and its host star. 39. 196. 1 indexed citations
11.
Shematovich, V. I. & Takashi Abe. (2008). Kinetics of Suprathermal Atoms and Molecules in the Rarefied Planetary Atmospheres. AIP conference proceedings. 1047–1054. 11 indexed citations
12.
Shematovich, V. I., et al.. (2003). Supply of trans-Europa Neutral Torus by the Surface-bounded Atmosphere of Europa. AGU Fall Meeting Abstracts. 2003. 1 indexed citations
13.
Smith, H. T., et al.. (2003). 3-D Modeling of Saturn's Titan Generated Nitrogen Cloud. 35. 1 indexed citations
14.
Johnson, R. E., R. W. Carlson, F. Leblanc, & V. I. Shematovich. (2001). Radiolysis: Icy Satellite Atmospheres and Surface Aging. 33. 1 indexed citations
15.
Boyarchuk, K. A., A. V. Karelin, & V. I. Shematovich. (2000). On a Possible Mechanism for the Formation of Oxygen Atmospheres on Jupiter's Icy Satellites.. Solar System Research. 34(1). 12. 5 indexed citations
16.
Shematovich, V. I., D. S. Wiebe, & Б. М. Шустов. (1999). Chemical and dynamical evolution of protostellar clouds: Chemistry at early stages of collapse. 43(10). 645–656. 3 indexed citations
17.
Wiebe, D. S., V. I. Shematovich, & Б. М. Шустов. (1996). Chemical and dynamical evolution of protostellar clouds: Initial stages of collapse. 40(5). 639–652. 1 indexed citations
18.
Shematovich, V. I., Д. В. Бисикало, & Jean‐Claude Gérard. (1992). The thermospheric odd nitrogen photochemistry - Role of non thermal N(4S) atoms. Open Repository and Bibliography (University of Liège). 16 indexed citations
19.
Shematovich, V. I., Д. В. Бисикало, & M. Ya. Marov. (1991). Kinetic approach to the mathematical modelling of collisional physical and chemical processes in planetary atmospheres. 345–352. 1 indexed citations
20.
Shematovich, V. I., et al.. (1982). Stochastic modeling of uniformly expanding rarefied gases. Soviet physics. Doklady. 266. 573. 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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