S. A. Markovskii

956 total citations
46 papers, 675 citations indexed

About

S. A. Markovskii is a scholar working on Astronomy and Astrophysics, Molecular Biology and Computational Mechanics. According to data from OpenAlex, S. A. Markovskii has authored 46 papers receiving a total of 675 indexed citations (citations by other indexed papers that have themselves been cited), including 45 papers in Astronomy and Astrophysics, 19 papers in Molecular Biology and 7 papers in Computational Mechanics. Recurrent topics in S. A. Markovskii's work include Solar and Space Plasma Dynamics (43 papers), Ionosphere and magnetosphere dynamics (40 papers) and Geomagnetism and Paleomagnetism Studies (19 papers). S. A. Markovskii is often cited by papers focused on Solar and Space Plasma Dynamics (43 papers), Ionosphere and magnetosphere dynamics (40 papers) and Geomagnetism and Paleomagnetism Studies (19 papers). S. A. Markovskii collaborates with scholars based in United States, Russia and United Kingdom. S. A. Markovskii's co-authors include Bernard J. Vasquez, Joseph V. Hollweg, C. W. Smith, Benjamin D. G. Chandran, Б. В. Сомов, Philip A. Isenberg, T. N. Parashar, J. V. Hollweg, Martin A. Lee and C. J. Farrugia and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Geophysical Research Letters.

In The Last Decade

S. A. Markovskii

43 papers receiving 655 citations

Peers

S. A. Markovskii

NHEP

Alfred Mallet United States

A. Dosch United States

Parisa Mostafavi United States

Andrea Verdini Italy

I. Ballai United Kingdom

Luca Franci United Kingdom

Emanuele Papini Italy

Masaru Nakanotani United States

Sanjoy Ghosh United States

R. Ratkiewicz Poland

Alfred Mallet United States

S. A. Markovskii

741 ×1.1

255 ×1.2

162 ×1.6

NHEP

52 ×1.1

17 ×0.7

Citations per year, relative to S. A. Markovskii S. A. Markovskii (= 1×) peers Alfred Mallet

Countries citing papers authored by S. A. Markovskii

Since Specialization

Citations

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

Fields of papers citing papers by S. A. Markovskii

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. A. Markovskii

This figure shows the co-authorship network connecting the top 25 collaborators of S. A. Markovskii. A scholar is included among the top collaborators of S. A. Markovskii 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 S. A. Markovskii. S. A. Markovskii 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

Markovskii, S. A. & Bernard J. Vasquez. (2025). Nonlinear evolution of the mirror instability in the solar wind plasma: Transition from humps to holes. Physics of Plasmas. 32(6).

Markovskii, S. A. & Bernard J. Vasquez. (2024). Ion Heating by a Fast Magnetosonic Turbulence in the Solar Corona. The Astrophysical Journal. 966(1). 1–1. 3 indexed citations

Markovskii, S. A. & Bernard J. Vasquez. (2023). Magnetic Helicity Associated with the Proton Temperature Anisotropy Instabilities in the Presence of an Imbalanced Solar Wind Turbulence. The Astrophysical Journal. 952(1). 16–16. 1 indexed citations

Markovskii, S. A. & Bernard J. Vasquez. (2022). Observational Analysis and Numerical Modeling of the Solar Wind Fluctuation Spectra during Intervals of Plasma Instability. The Astrophysical Journal. 941(1). 72–72. 2 indexed citations

Markovskii, S. A., Bernard J. Vasquez, & Benjamin D. G. Chandran. (2019). Proton Temperature-anisotropy Instability Coexisting with Ambient Turbulence in the Solar-wind Plasma. The Astrophysical Journal. 875(2). 125–125. 12 indexed citations

Markovskii, S. A., Benjamin D. G. Chandran, & Bernard J. Vasquez. (2018). Two-dimensional Nonlinear Simulations of Temperature-anisotropy Instabilities with a Proton-alpha Drift. The Astrophysical Journal. 856(2). 153–153. 7 indexed citations

Markovskii, S. A., Bernard J. Vasquez, & C. W. Smith. (2016). THE EFFECT OF ELECTRON THERMAL PRESSURE ON THE OBSERVED MAGNETIC HELICITY IN THE SOLAR WIND. The Astrophysical Journal. 833(2). 212–212. 7 indexed citations

Parashar, T. N., Bernard J. Vasquez, & S. A. Markovskii. (2014). The role of electron equation of state in heating partition of protons in a collisionless plasma. Physics of Plasmas. 21(2). 22301–22301. 16 indexed citations

Markovskii, S. A. & Bernard J. Vasquez. (2013). Magnetic helicity signature produced by cross-field 2D turbulence. AIP conference proceedings. 239–242.

10.

Chandran, Benjamin D. G., Philip A. Isenberg, Martin A. Lee, et al.. (2010). RESONANT INTERACTIONS BETWEEN PROTONS AND OBLIQUE ALFVÉN/ION-CYCLOTRON WAVES IN THE SOLAR CORONA AND SOLAR FLARES. The Astrophysical Journal. 722(1). 710–720. 20 indexed citations

11.

Markovskii, S. A., Bernard J. Vasquez, & Joseph V. Hollweg. (2009). PROTON HEATING BY NONLINEAR FIELD-ALIGNED ALFVÉN WAVES IN SOLAR CORONAL HOLES. The Astrophysical Journal. 695(2). 1413–1420. 25 indexed citations

12.

Markovskii, S. A., Bernard J. Vasquez, & C. W. Smith. (2008). Statistical Analysis of the High‐Frequency Spectral Break of the Solar Wind Turbulence at 1 AU. The Astrophysical Journal. 675(2). 1576–1583. 78 indexed citations

13.

Markovskii, S. A. & J. V. Hollweg. (2004). Radial evolution of intermittent heat flux in solar coronal holes. Nonlinear processes in geophysics. 11(4). 485–494. 8 indexed citations

14.

Markovskii, S. A.. (2003). Ion Heating Due to Plasma Microinstabilities in Coronal Holes and the Fast Solar Wind. AIP conference proceedings. 679. 307–310. 2 indexed citations

15.

Markovskii, S. A. & Joseph V. Hollweg. (2002). Parametric cross‐field current instability in solar coronal holes. Journal of Geophysical Research Atmospheres. 107(A10). 31 indexed citations

16.

Hollweg, Joseph V. & S. A. Markovskii. (2002). Cyclotron resonances of ions with obliquely propagating waves in coronal holes and the fast solar wind. Journal of Geophysical Research Atmospheres. 107(A6). 26 indexed citations

17.

Markovskii, S. A. & J. V. Hollweg. (2001). Ion Cyclotron Instabilities in Multicomponent Coronal Hole Plasma with Cross-Field Streaming Species. AGU Spring Meeting Abstracts. 2001. 1 indexed citations

18.

Vasquez, Bernard J., C. J. Farrugia, S. A. Markovskii, et al.. (2001). Nature of fluctuations on directional discontinuities inside a solar ejection: Wind and IMP 8 observations. Journal of Geophysical Research Atmospheres. 106(A12). 29283–29298. 11 indexed citations

19.

Markovskii, S. A., et al.. (2000). Disintegration of trans‐Alfvénic shocks due to variable viscosity and resistivity. Journal of Geophysical Research Atmospheres. 105(A6). 12705–12711. 4 indexed citations

20.

Markovskii, S. A.. (1999). Unsteady propagation of collisionless trans‐Alfvénic shocks at large timescales. Geophysical Research Letters. 26(7). 979–982. 2 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