G. Kowal

3.7k total citations
55 papers, 1.2k citations indexed

About

G. Kowal is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Molecular Biology. According to data from OpenAlex, G. Kowal has authored 55 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 54 papers in Astronomy and Astrophysics, 23 papers in Nuclear and High Energy Physics and 4 papers in Molecular Biology. Recurrent topics in G. Kowal's work include Solar and Space Plasma Dynamics (41 papers), Astrophysics and Star Formation Studies (24 papers) and Ionosphere and magnetosphere dynamics (16 papers). G. Kowal is often cited by papers focused on Solar and Space Plasma Dynamics (41 papers), Astrophysics and Star Formation Studies (24 papers) and Ionosphere and magnetosphere dynamics (16 papers). G. Kowal collaborates with scholars based in Brazil, United States and Poland. G. Kowal's co-authors include A. Lazarian, D. Falceta-Gonçalves, E. M. de Gouveia Dal Pino, Ethan T. Vishniac, K. Otmianowska‐Mazur, M. Hanasz, H. Lesch, Blakesley Burkhart, Snežana Stanimirović and Huirong Yan and has published in prestigious journals such as Physical Review Letters, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

G. Kowal

51 papers receiving 1.2k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
G. Kowal Brazil 18 1.2k 426 97 52 39 55 1.2k
T. N. Larosa United States 14 999 0.8× 356 0.8× 91 0.9× 22 0.4× 26 0.7× 29 1.0k
Allard Jan van Marle Belgium 20 1.0k 0.9× 288 0.7× 33 0.3× 23 0.4× 44 1.1× 44 1.1k
John R. Dickel United States 20 1.3k 1.1× 817 1.9× 27 0.3× 47 0.9× 24 0.6× 103 1.3k
R. Kothes Canada 19 1.3k 1.1× 909 2.1× 16 0.2× 27 0.5× 32 0.8× 74 1.4k
N. P. M. Kuin United Kingdom 18 1.1k 0.9× 337 0.8× 39 0.4× 14 0.3× 56 1.4× 110 1.1k
H. J. Fahr Germany 20 1.3k 1.1× 171 0.4× 51 0.5× 137 2.6× 19 0.5× 107 1.4k
R. L. Mutel United States 18 830 0.7× 388 0.9× 19 0.2× 39 0.8× 76 1.9× 73 895
R. S. Roger Canada 17 877 0.7× 453 1.1× 28 0.3× 38 0.7× 39 1.0× 68 925
Simone Landi Italy 24 1.4k 1.2× 284 0.7× 348 3.6× 83 1.6× 92 2.4× 60 1.5k
G. Dumas France 15 900 0.8× 142 0.3× 41 0.4× 34 0.7× 10 0.3× 29 927

Countries citing papers authored by G. Kowal

Since Specialization
Citations

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

Fields of papers citing papers by G. Kowal

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of G. Kowal

This figure shows the co-authorship network connecting the top 25 collaborators of G. Kowal. A scholar is included among the top collaborators of G. Kowal 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 G. Kowal. G. Kowal 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.
Pino, E. M. de Gouveia Dal, et al.. (2023). Particle Acceleration by Magnetic Reconnection in Relativistic Jets: The Transition from Small to Large Scales. The Astrophysical Journal. 952(2). 168–168. 7 indexed citations
2.
Kowal, G., et al.. (2021). Generation and effects of electromotive force in turbulent stochastic reconnection. Physics of Plasmas. 28(6). 2 indexed citations
3.
Kowal, G. & D. Falceta-Gonçalves. (2021). Colliding-Wind Binaries as a Source of TeV Cosmic Rays. Frontiers in Astronomy and Space Sciences. 8. 2 indexed citations
4.
Rosswog, Stephan, et al.. (2020). Consequences of Jet-Ejecta Interaction in Neutron Star Mergers. Proceedings of the International Astronomical Union. 16(S363). 245–249. 2 indexed citations
5.
Pino, E. M. de Gouveia Dal, et al.. (2018). Particle acceleration and the origin of the very high energy emission around black holes and relativistic jets. arXiv (Cornell University). 1 indexed citations
6.
Vishniac, Ethan T., et al.. (2018). Stochastic Reconnection for Large Magnetic Prandtl Numbers. The Astrophysical Journal. 860(1). 52–52. 9 indexed citations
7.
Nakwacki, M. S., G. Kowal, R. Santos-Lima, E. M. de Gouveia Dal Pino, & D. Falceta-Gonçalves. (2015). Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society. 455(4). 3702–3723. 5 indexed citations
8.
Santos-Lima, R., E. M. de Gouveia Dal Pino, G. Kowal, et al.. (2014). Magnetic Field Amplification and Evolution in Turbulent Collisionless Magnetohydrodynamics: An Application to the Intracluster Medium. Repositorio Digital Institucional de la Universidad de Buenos Aires (Universidad de Buenos Aires). 46 indexed citations
9.
Kowal, G., E. M. de Gouveia Dal Pino, & A. Lazarian. (2012). Particle Acceleration in Turbulence and Weakly Stochastic Reconnection. Physical Review Letters. 108(24). 241102–241102. 79 indexed citations
10.
Nakwacki, M. S., E. M. de Gouveia Dal Pino, G. Kowal, & R. Santos-Lima. (2012). The role of pressure anisotropy in the turbulent intracluster medium. Journal of Physics Conference Series. 370. 12043–12043. 3 indexed citations
11.
Montmerle, T., et al.. (2010). IAU volume 6 issue S271 Cover and Front matter. Proceedings of the International Astronomical Union. 6(S271). f1–f19. 1 indexed citations
12.
Pino, E. M. de Gouveia Dal, et al.. (2010). Removal of magnetic flux from self-gravitating clouds due turbulent reconnection. EGU General Assembly Conference Abstracts. 8924. 1 indexed citations
13.
Kowal, G. & A. Lazarian. (2010). VELOCITY FIELD OF COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE: WAVELET DECOMPOSITION AND MODE SCALINGS. The Astrophysical Journal. 720(1). 742–756. 109 indexed citations
14.
Kowal, G., et al.. (2009). Reconnection in weakly stochastic B-fields in 2D. 9 indexed citations
15.
Otmianowska‐Mazur, K., et al.. (2009). Formation of gaseous arms in barred galaxies with dynamically important magnetic field: 3D MHD simulations. Astronomy and Astrophysics. 498(2). L21–L24. 7 indexed citations
16.
Hanasz, M., K. Otmianowska‐Mazur, G. Kowal, & H. Lesch. (2009). Cosmic-ray-driven dynamo in galactic disks. Astronomy and Astrophysics. 498(2). 335–346. 37 indexed citations
17.
Falceta-Gonçalves, D., A. Lazarian, & G. Kowal. (2008). Studies of Regular and Random Magnetic Fields in the ISM: Statistics of Polarization Vectors and the Chandrasekhar‐Fermi Technique. The Astrophysical Journal. 679(1). 537–551. 131 indexed citations
18.
Kowal, G., K. Otmianowska‐Mazur, & M. Hanasz. (2006). Dynamo coefficients in Parker unstable disks with cosmic rays and shear. Astronomy and Astrophysics. 445(3). 915–929. 18 indexed citations
19.
Selwa, M., K. Murawski, & G. Kowal. (2004). Three-dimensional numerical simulations of impulsively generated MHD waves in solar coronal loops. Astronomy and Astrophysics. 422(3). 1067–1072. 18 indexed citations
20.
Kowal, G., M. Hanasz, & K. Otmianowska‐Mazur. (2003). Resistive MHD simulations of the Parker instability in galactic disks. Astronomy and Astrophysics. 404(2). 533–543. 9 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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