Mikhail Malkov

2.7k total citations · 1 hit paper
64 papers, 1.8k citations indexed

About

Mikhail Malkov is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, Mikhail Malkov has authored 64 papers receiving a total of 1.8k indexed citations (citations by other indexed papers that have themselves been cited), including 53 papers in Nuclear and High Energy Physics, 51 papers in Astronomy and Astrophysics and 6 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in Mikhail Malkov's work include Solar and Space Plasma Dynamics (32 papers), Astrophysics and Cosmic Phenomena (31 papers) and Gamma-ray bursts and supernovae (25 papers). Mikhail Malkov is often cited by papers focused on Solar and Space Plasma Dynamics (32 papers), Astrophysics and Cosmic Phenomena (31 papers) and Gamma-ray bursts and supernovae (25 papers). Mikhail Malkov collaborates with scholars based in United States, Germany and Russia. Mikhail Malkov's co-authors include P. H. Diamond, L. O’C. Drury, R. Z. Sagdeev, A. I. Smolyakov, H. J. Völk, M. N. Rosenbluth, I. V. Moskalenko, F. Aharonian, C. Holland and T. S. Hahm and has published in prestigious journals such as Physical Review Letters, Nature Communications and The Astrophysical Journal.

In The Last Decade

Mikhail Malkov

61 papers receiving 1.7k citations

Hit Papers

Nonlinear theory of diffusive acceleration of particles b... 2001 2026 2009 2017 2001 100 200 300 400
What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

  1. Nonlinear theory of diffusive acceleration of particles by shock waves
    2001 473 citations Mikhail Malkov, L. O’C. Drury profile →

Peers

Mikhail Malkov
S-I Itoh Japan
P. N. Guzdar United States
M. Ottaviani France
C. Mercier France
W. Horton United States
S. Vincena United States
E. Schwarz Germany
A. M. Bykov Russia
Shane W. Davis United States
Fritz J. Swenson United States
S-I Itoh Japan
Mikhail Malkov
Citations per year, relative to Mikhail Malkov Mikhail Malkov (= 1×) peers S-I Itoh

Countries citing papers authored by Mikhail Malkov

Since Specialization
Citations

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

Fields of papers citing papers by Mikhail Malkov

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Mikhail Malkov. 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 Mikhail Malkov. The network helps show where Mikhail Malkov may publish in the future.

Co-authorship network of co-authors of Mikhail Malkov

This figure shows the co-authorship network connecting the top 25 collaborators of Mikhail Malkov. A scholar is included among the top collaborators of Mikhail Malkov 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 Mikhail Malkov. Mikhail Malkov 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.
Malkov, Mikhail, J. Giacalone, & Fan Guo. (2024). Flat Spectra of Energetic Particles in Interplanetary Shock Precursors. The Astrophysical Journal. 973(1). 27–27. 1 indexed citations
2.
Malkov, Mikhail & I. V. Moskalenko. (2022). On the Origin of Observed Cosmic-Ray Spectrum Below 100 TV. The Astrophysical Journal. 933(1). 78–78. 13 indexed citations
3.
Malkov, Mikhail & Martin Lemoine. (2022). Particle Acceleration in Colliding Flows: Binary Star Winds and Other Double-Shock Structures. arXiv (Cornell University). 4 indexed citations
4.
Liseykina, T. V., et al.. (2020). Electron energization in quasi-parallel shocks. Astronomy and Astrophysics. 642. A47–A47. 3 indexed citations
5.
Malkov, Mikhail, P. H. Diamond, R. Z. Sagdeev, F. Aharonian, & I. V. Moskalenko. (2013). ANALYTIC SOLUTION FOR SELF-REGULATED COLLECTIVE ESCAPE OF COSMIC RAYS FROM THEIR ACCELERATION SITES. The Astrophysical Journal. 768(1). 73–73. 72 indexed citations
6.
Bykov, A. M., et al.. (2013). Collisionless Shocks in Partly Ionized Plasma with Cosmic Rays: Microphysics of Non-thermal Components. Space Science Reviews. 178(2-4). 599–632. 14 indexed citations
7.
Malkov, Mikhail, P. H. Diamond, & R. Z. Sagdeev. (2012). Proton-Helium Spectral Anomaly as a Signature of Cosmic Ray Accelerator. Physical Review Letters. 108(8). 81104–81104. 40 indexed citations
8.
Malkov, Mikhail, P. H. Diamond, L. O’C. Drury, & R. Z. Sagdeev. (2012). Angular distribution of energetic particles scattered by strongly anisotropic MHD turbulence: Understanding Milagro/IceCube results. AIP conference proceedings. 190–198. 1 indexed citations
9.
Malkov, Mikhail, P. H. Diamond, & R. Z. Sagdeev. (2011). Mechanism for spectral break in cosmic ray proton spectrum of supernova remnant W44. Nature Communications. 2(1). 194–194. 58 indexed citations
10.
Malkov, Mikhail, P. H. Diamond, L. O’C. Drury, & R. Z. Sagdeev. (2010). Probing nearby cosmic-ray accelerators and interstellar medium turbulence with MILAGRO hot spots. eScholarship (California Digital Library). 32 indexed citations
11.
Malkov, Mikhail, P. H. Diamond, Xianzhi Ao, & G. P. Zank. (2009). Wave Dynamics and Particle Acceleration in Shock Precursors. AIP conference proceedings. 66–73. 1 indexed citations
12.
Moskalenko, I. V., T. A. Porter, Mikhail Malkov, & P. H. Diamond. (2008). Hadronic Gamma Rays from Supernova Remnants. International Cosmic Ray Conference. 2. 763–766. 1 indexed citations
13.
Malkov, Mikhail, et al.. (2002). On the possible reason for nondetection of TeV protons in supernova remnants. eScholarship (California Digital Library). 11 indexed citations
14.
Malkov, Mikhail, P. H. Diamond, & A. I. Smolyakov. (2001). On the stability of drift wave spectra with respect to zonal flow excitation. Physics of Plasmas. 8(5). 1553–1558. 30 indexed citations
15.
Malkov, Mikhail & H. J. Voêlk. (1995). Theory of ion injection at shocks.. A&A. 300. 605. 12 indexed citations
16.
Malkov, Mikhail, A. A. Galeev, & H. J. Völk. (1995). Electrostatic Shocks Driven by Accelerated Electrons. ICRC. 3. 273.
17.
Malkov, Mikhail, et al.. (1991). High amplitude magnetosonic waves in the upstream region of the cometary bow-shock.. A&A. 243(2). 546–552. 3 indexed citations
18.
Kennel, C. F., Mikhail Malkov, R. Z. Sagdeev, V. D. Shapiro, & Alexander V. Khrabrov. (1988). Alfvén shock wave trains with a dispersion. ZhETF Pisma Redaktsiiu. 48. 75. 3 indexed citations
19.
Malkov, Mikhail, et al.. (1985). Lower hybrid drift instability and reconnection of magnetic lines of force. 11. 1096–1105. 1 indexed citations
20.
Malkov, Mikhail. (1982). Quasilinear theory of plasma waves in a large-amplitude monochromatic wave. 8. 495–500. 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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