K. M. Kuzanyan

1.0k total citations
44 papers, 727 citations indexed

About

K. M. Kuzanyan is a scholar working on Astronomy and Astrophysics, Molecular Biology and Oceanography. According to data from OpenAlex, K. M. Kuzanyan has authored 44 papers receiving a total of 727 indexed citations (citations by other indexed papers that have themselves been cited), including 42 papers in Astronomy and Astrophysics, 32 papers in Molecular Biology and 3 papers in Oceanography. Recurrent topics in K. M. Kuzanyan's work include Solar and Space Plasma Dynamics (40 papers), Geomagnetism and Paleomagnetism Studies (32 papers) and Astro and Planetary Science (24 papers). K. M. Kuzanyan is often cited by papers focused on Solar and Space Plasma Dynamics (40 papers), Geomagnetism and Paleomagnetism Studies (32 papers) and Astro and Planetary Science (24 papers). K. M. Kuzanyan collaborates with scholars based in Russia, China and United Kingdom. K. M. Kuzanyan's co-authors include D. D. Sokoloff, C. A. Jones, Hongqi Zhang, Shudong Bao, D. Moss, N. Kleeorin, G. Belvedère, В. В. Пипин, I. Rogachevskii and A. M. Soward and has published in prestigious journals such as The Astrophysical Journal, Journal of Fluid Mechanics and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

K. M. Kuzanyan

42 papers receiving 694 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
K. M. Kuzanyan Russia 15 656 484 94 56 41 44 727
Mathieu Ossendrijver Germany 11 594 0.9× 468 1.0× 86 0.9× 60 1.1× 34 0.8× 25 707
C. Foullon United Kingdom 27 1.8k 2.7× 665 1.4× 73 0.8× 40 0.7× 50 1.2× 58 1.8k
D. A. Biesecker United States 21 1.9k 2.9× 368 0.8× 83 0.9× 64 1.1× 171 4.2× 49 2.0k
Patrick Antolin United Kingdom 29 2.0k 3.0× 543 1.1× 66 0.7× 63 1.1× 121 3.0× 78 2.0k
H. P. Jones United States 17 855 1.3× 200 0.4× 42 0.4× 55 1.0× 139 3.4× 56 914
Cooper Downs United States 23 1.3k 2.0× 285 0.6× 54 0.6× 41 0.7× 138 3.4× 70 1.3k
K. Petrovay Hungary 16 832 1.3× 249 0.5× 76 0.8× 56 1.0× 153 3.7× 44 885
Teresa Nieves‐Chinchilla United States 21 1.4k 2.1× 500 1.0× 41 0.4× 44 0.8× 73 1.8× 85 1.5k
Lidong Xia China 22 1.4k 2.1× 346 0.7× 30 0.3× 47 0.8× 90 2.2× 90 1.4k
I. V. Zimovets Russia 16 1.1k 1.7× 375 0.8× 33 0.4× 29 0.5× 46 1.1× 67 1.1k

Countries citing papers authored by K. M. Kuzanyan

Since Specialization
Citations

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

Fields of papers citing papers by K. M. Kuzanyan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by K. M. Kuzanyan. 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 K. M. Kuzanyan. The network helps show where K. M. Kuzanyan may publish in the future.

Co-authorship network of co-authors of K. M. Kuzanyan

This figure shows the co-authorship network connecting the top 25 collaborators of K. M. Kuzanyan. A scholar is included among the top collaborators of K. M. Kuzanyan 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 K. M. Kuzanyan. K. M. Kuzanyan 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.
Kleeorin, N., et al.. (2020). The mean tilt of sunspot bipolar regions: theory, simulations and comparison with observations. Monthly Notices of the Royal Astronomical Society. 495(1). 238–248. 10 indexed citations
2.
Zhang, Hongqi, et al.. (2016). On the Origin of Differences in Helicity Parameters Derived from Data of Two Solar Magnetographs. Solar Physics. 291(8). 2253–2267. 4 indexed citations
3.
Stepanov, Rodion, et al.. (2015). Current helicity and magnetic field anisotropy in solar active regions. Monthly Notices of the Royal Astronomical Society. 454(2). 1921–1930. 9 indexed citations
4.
Gao, Yu, Takashi Sakurai, H. Zhang, K. M. Kuzanyan, & D. D. Sokoloff. (2013). Statistical distribution of current helicity in solar active regions over the magnetic cycle. Monthly Notices of the Royal Astronomical Society. 433(2). 1648–1658. 1 indexed citations
5.
Пипин, В. В., H. Zhang, D. D. Sokoloff, K. M. Kuzanyan, & Yu Gao. (2013). The origin of the helicity hemispheric sign rule reversals in the mean-field solar-type dynamo. Monthly Notices of the Royal Astronomical Society. 435(3). 2581–2588. 12 indexed citations
6.
Jones, C. A., et al.. (2009). Linear theory of compressible convection in rapidly rotating spherical shells, using the anelastic approximation. Journal of Fluid Mechanics. 634. 291–319. 58 indexed citations
7.
Jones, C. A. & K. M. Kuzanyan. (2009). Compressible convection in the deep atmospheres of giant planets. Icarus. 204(1). 227–238. 85 indexed citations
8.
Kuzanyan, K. M., et al.. (2008). Predictions of the Magnitude of the Forthcoming Solar Cycles using Knowledge on the Solar Dynamo and Singular Spectrum Analysis. 12.
9.
Sokoloff, D. D., et al.. (2008). Current Helicity and Twist as Two Indicators of the Mirror Asymmetry of Solar Magnetic Fields. Solar Physics. 248(1). 17–28. 9 indexed citations
10.
Sokoloff, D. D., et al.. (2007). Magnetic and current helicities in solar dynamos. Advances in Space Research. 39(11). 1670–1673. 2 indexed citations
11.
Обридко, В. Н., D. D. Sokoloff, K. M. Kuzanyan, B. D. Shelting, & V. Zakharov. (2005). Solar cycle according to mean magnetic field data. Monthly Notices of the Royal Astronomical Society. 365(3). 827–832. 25 indexed citations
12.
Galitski, Victor, Dmitry D. Sokoloff, & K. M. Kuzanyan. (2005). A dynamo wave near the solar equator. Astronomy Reports. 49(4). 337–342. 8 indexed citations
13.
Kleeorin, N., et al.. (2003). Magnetic helicity evolution during the solar activity cycle: Observations and dynamo theory. Springer Link (Chiba Institute of Technology). 51 indexed citations
14.
Seehafer, N., M. Gellert, K. M. Kuzanyan, & В. В. Пипин. (2003). Helicity and the solar dynamo. Advances in Space Research. 32(10). 1819–1833. 13 indexed citations
15.
Zhang, Hongqi, Shudong Bao, & K. M. Kuzanyan. (2002). Twist of magnetic fields in solar active regions. Astronomy Reports. 46(5). 424–434. 14 indexed citations
16.
Belvedère, G., K. M. Kuzanyan, & D. D. Sokoloff. (2000). A two-dimensional asymptotic solution for a dynamo wave in the light of the solar internal rotation. Monthly Notices of the Royal Astronomical Society. 315(4). 778–790. 40 indexed citations
17.
Kuzanyan, K. M. & D. D. Sokoloff. (1999). The solar dynamo wave in Parker's migratory dynamo. Astronomical and Astrophysical Transactions. 18(1). 129–133. 1 indexed citations
18.
Kuzanyan, K. M. & D. D. Sokoloff. (1997). HALF-WIDTH OF A SOLAR DYNAMO WAVE IN PARKER'S MIGRATORY DYNAMO. Solar Physics. 173(1). 1–14. 20 indexed citations
19.
Kuzanyan, K. M. & D. D. Sokolov. (1996). A dynamo wave in a thin shell. Astronomy Reports. 40(3). 424–430. 7 indexed citations
20.
Kuzanyan, K. M. & D. D. Sokoloff. (1993). Parametric resonance in a thin disc dynamo. Astrophysics and Space Science. 208(2). 245–252. 6 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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