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.
Influence of Cosmic Repulsion and Magnetic Fields on Accretion Disks Rotating around Kerr Black Holes
2020158 citationsZdeněk Stuchlík, Martin Kološ et al.Universeprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of Jiří Kovář'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 Jiří Kovář with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Jiří Kovář more than expected).
This network shows the impact of papers produced by Jiří Kovář. 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 Jiří Kovář. The network helps show where Jiří Kovář may publish in the future.
Co-authorship network of co-authors of Jiří Kovář
This figure shows the co-authorship network connecting the top 25 collaborators of Jiří Kovář.
A scholar is included among the top collaborators of Jiří Kovář 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 Jiří Kovář. Jiří Kovář is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Stuchlík, Zdeněk, Martin Kološ, Jiří Kovář, Petr Slaný, & Arman Tursunov. (2020). Influence of Cosmic Repulsion and Magnetic Fields on Accretion Disks Rotating around Kerr Black Holes. Universe. 6(2). 26–26.158 indexed citations breakdown →
Karas, V., D. Kunneriath, Michal Zajaček, et al.. (2017). Plunging neutron stars as origin of organised magnetic field in galactic nuclei. Contributions of the Astronomical Observatory Skalnaté Pleso. 47(2). 124–132.2 indexed citations
9.
Kovář, Jiří, et al.. (2016). Virtual reality in context of Industry 4.0 proposed projects at Brno University of Technology.26 indexed citations
10.
Mouralová, Kateřina, et al.. (2016). Freeman-Tukey pseudoquasi-norm for evaluating the total height of profile Rt after WEDM.2 indexed citations
11.
Mouralová, Kateřina, et al.. (2016). Optimization of the cutting speed for Ti-6Al-4V using WEDM depending on quality of the machined surface.2 indexed citations
12.
Mouralová, Kateřina, Jiří Kovář, Radim Zahradníček, & Ondřej Man. (2016). Characterisation of 3D topography of the surface machined by finishing technologies of WEDM and grinding.2 indexed citations
13.
Kovář, Jiří, Zdeněk Stuchlík, & Petr Slaný. (2014). Pseudo-Newtonian gravitational potential of Schwarzschild black hole in the presence of quintessence. 133–141.
Karas, V., et al.. (2012). Regular and Chaotic Motion in General Relativity. Case of Magnetized Black Hole and a Massive Magnetic Dipole. AAS. 220.4 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.