A. K. Kulkarni

1.5k total citations
16 papers, 921 citations indexed

About

A. K. Kulkarni is a scholar working on Astronomy and Astrophysics, Geophysics and Biomedical Engineering. According to data from OpenAlex, A. K. Kulkarni has authored 16 papers receiving a total of 921 indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 3 papers in Geophysics and 3 papers in Biomedical Engineering. Recurrent topics in A. K. Kulkarni's work include Astrophysical Phenomena and Observations (11 papers), Astrophysics and Star Formation Studies (9 papers) and Stellar, planetary, and galactic studies (9 papers). A. K. Kulkarni is often cited by papers focused on Astrophysical Phenomena and Observations (11 papers), Astrophysics and Star Formation Studies (9 papers) and Stellar, planetary, and galactic studies (9 papers). A. K. Kulkarni collaborates with scholars based in United States, France and Canada. A. K. Kulkarni's co-authors include Robert F. Penna, Ramesh Narayan, Aleksander Sądowski, M. M. Romanova, M. M. Romanova, Jeffrey E. McClintock, Shane W. Davis, Yucong Zhu, Min Long and J.‐F. Donati and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Advances in Space Research.

In The Last Decade

A. K. Kulkarni

16 papers receiving 858 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. K. Kulkarni United States 12 901 295 119 54 28 16 921
Shigenobu Hirose Japan 15 914 1.0× 339 1.1× 77 0.6× 55 1.0× 15 0.5× 39 941
Mami Machida Japan 15 621 0.7× 269 0.9× 55 0.5× 26 0.5× 37 1.3× 45 640
L. K. Townsley United States 6 441 0.5× 188 0.6× 49 0.4× 39 0.7× 20 0.7× 10 446
Agnieszka Janiuk Poland 19 846 0.9× 318 1.1× 76 0.6× 35 0.6× 23 0.8× 60 873
F. K. Baganoff United States 13 664 0.7× 306 1.0× 81 0.7× 39 0.7× 12 0.4× 29 675
Robert Popham United States 13 1.2k 1.4× 395 1.3× 141 1.2× 26 0.5× 38 1.4× 16 1.3k
Keigo Fukumura United States 13 636 0.7× 278 0.9× 51 0.4× 76 1.4× 22 0.8× 30 653
T. Viehmann Germany 12 565 0.6× 168 0.6× 47 0.4× 56 1.0× 25 0.9× 20 582
M. Böck Germany 13 721 0.8× 327 1.1× 56 0.5× 88 1.6× 8 0.3× 16 728
J. E. Pringle United Kingdom 12 707 0.8× 320 1.1× 31 0.3× 49 0.9× 11 0.4× 15 724

Countries citing papers authored by A. K. Kulkarni

Since Specialization
Citations

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

Fields of papers citing papers by A. K. Kulkarni

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. K. Kulkarni

This figure shows the co-authorship network connecting the top 25 collaborators of A. K. Kulkarni. A scholar is included among the top collaborators of A. K. Kulkarni 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 A. K. Kulkarni. A. K. Kulkarni is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

16 of 16 papers shown
1.
Penna, Robert F., A. K. Kulkarni, & Ramesh Narayan. (2013). A new equilibrium torus solution and GRMHD initial conditions. Springer Link (Chiba Institute of Technology). 48 indexed citations
2.
Kulkarni, A. K. & M. M. Romanova. (2013). Analytical hotspot shapes and magnetospheric radius from 3D simulations of magnetospheric accretion. Monthly Notices of the Royal Astronomical Society. 433(4). 3048–3061. 60 indexed citations
3.
Narayan, Ramesh, Aleksander Sądowski, Robert F. Penna, & A. K. Kulkarni. (2012). GRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Outflows and Convection. arXiv (Cornell University). 1 indexed citations
4.
Penna, Robert F., Aleksander Sądowski, A. K. Kulkarni, & Ramesh Narayan. (2012). The Shakura-Sunyaev viscosity prescription with variable α (r). Monthly Notices of the Royal Astronomical Society. 428(3). 2255–2274. 56 indexed citations
5.
Zhu, Yucong, Shane W. Davis, Ramesh Narayan, et al.. (2012). The eye of the storm: light from the inner plunging region of black hole accretion discs. Monthly Notices of the Royal Astronomical Society. 424(4). 2504–2521. 63 indexed citations
6.
Narayan, Ramesh, Aleksander Sądowski, Robert F. Penna, & A. K. Kulkarni. (2012). GRMHD simulations of magnetized advection-dominated accretion on a non-spinning black hole: role of outflows. Monthly Notices of the Royal Astronomical Society. 426(4). 3241–3259. 326 indexed citations
7.
Kulkarni, A. K., Robert F. Penna, Roman V. Shcherbakov, et al.. (2011). Measuring black hole spin by the continuum-fitting method: effect of deviations from the Novikov-Thorne disc model. Monthly Notices of the Royal Astronomical Society. 414(2). 1183–1194. 70 indexed citations
8.
Long, Min, M. M. Romanova, A. K. Kulkarni, & J.‐F. Donati. (2011). Global 3D simulations of disc accretion on to the classical T Tauri star BP Tauri. Monthly Notices of the Royal Astronomical Society. 413(2). 1061–1071. 26 indexed citations
9.
Romanova, M. M., Min Long, Frederick K. Lamb, A. K. Kulkarni, & J.‐F. Donati. (2010). Global 3D simulations of disc accretion on to the classical T Tauri star V2129 Oph. Monthly Notices of the Royal Astronomical Society. 411(2). 915–928. 41 indexed citations
10.
Romanova, M. M. & A. K. Kulkarni. (2009). Discovery of drifting high-frequency quasi-periodic oscillations in global simulations of magnetic boundary layers. Monthly Notices of the Royal Astronomical Society. 398(3). 1105–1116. 13 indexed citations
11.
Kulkarni, A. K. & M. M. Romanova. (2009). Possible quasi-periodic oscillations from unstable accretion: 3D magnetohydrodynamic simulations. Monthly Notices of the Royal Astronomical Society. 398(2). 701–714. 29 indexed citations
12.
Romanova, M. M., A. K. Kulkarni, Min Long, et al.. (2008). Modeling of Disk-Star Interaction: Different Regimes of Accretion and Variability. AIP conference proceedings. 87–94. 3 indexed citations
13.
Kulkarni, A. K. & M. M. Romanova. (2008). Accretion to magnetized stars through the Rayleigh–Taylor instability: global 3D simulations. Monthly Notices of the Royal Astronomical Society. 386(2). 673–687. 144 indexed citations
14.
Lovelace, R. V. E., A. K. Kulkarni, & M. M. Romanova. (2007). Torsional Magnetic Oscillations in Type I X‐Ray Bursts. The Astrophysical Journal. 656(1). 393–398. 7 indexed citations
15.
Romanova, M. M., A. K. Kulkarni, Min Long, et al.. (2006). 2D and 3D MHD simulations of disk accretion by rotating magnetized stars: Search for variability. Advances in Space Research. 38(12). 2887–2892. 7 indexed citations
16.
Kulkarni, A. K. & M. M. Romanova. (2005). Variability Profiles of Millisecond X‐Ray Pulsars: Results of Pseudo‐Newtonian Three‐dimensional Magnetohydrodynamic Simulations. The Astrophysical Journal. 633(1). 349–357. 27 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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