Prasad Subramanian

1.4k total citations
40 papers, 831 citations indexed

About

Prasad Subramanian is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Molecular Biology. According to data from OpenAlex, Prasad Subramanian has authored 40 papers receiving a total of 831 indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 8 papers in Nuclear and High Energy Physics and 4 papers in Molecular Biology. Recurrent topics in Prasad Subramanian's work include Solar and Space Plasma Dynamics (31 papers), Ionosphere and magnetosphere dynamics (22 papers) and Stellar, planetary, and galactic studies (12 papers). Prasad Subramanian is often cited by papers focused on Solar and Space Plasma Dynamics (31 papers), Ionosphere and magnetosphere dynamics (22 papers) and Stellar, planetary, and galactic studies (12 papers). Prasad Subramanian collaborates with scholars based in India, United States and Japan. Prasad Subramanian's co-authors include A. Vourlidas, R. A. Howard, K. P. Dere, S. T. Wu, A. H. Wang, Peter A. Becker, P. Janardhan, A. Lara, Iver H. Cairns and P. K. Manoharan and has published in prestigious journals such as Physical Review Letters, Journal of Geophysical Research Atmospheres and The Astrophysical Journal.

In The Last Decade

Prasad Subramanian

36 papers receiving 806 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Prasad Subramanian India 14 808 112 104 40 35 40 831
B. Jurcevich United States 3 729 0.9× 160 1.4× 51 0.5× 43 1.1× 25 0.7× 8 754
K.‐L. Klein France 22 1.0k 1.3× 123 1.1× 88 0.8× 98 2.5× 19 0.5× 53 1.1k
I. V. Zimovets Russia 16 1.1k 1.4× 375 3.3× 66 0.6× 46 1.1× 33 0.9× 67 1.1k
Andrea Verdini Italy 18 896 1.1× 317 2.8× 94 0.9× 45 1.1× 30 0.9× 45 913
F. Fárník Czechia 17 622 0.8× 126 1.1× 38 0.4× 46 1.1× 34 1.0× 42 636
S. J. Tappin United Kingdom 23 1.4k 1.7× 262 2.3× 54 0.5× 58 1.4× 70 2.0× 57 1.4k
Xianzhi Ao United States 11 453 0.6× 67 0.6× 78 0.8× 55 1.4× 15 0.4× 50 481
C. A. de Koning United States 16 679 0.8× 176 1.6× 30 0.3× 55 1.4× 27 0.8× 33 692
E. G. Kupriyanova Russia 13 712 0.9× 234 2.1× 50 0.5× 20 0.5× 41 1.2× 28 718
Pankaj Kumar United States 19 948 1.2× 267 2.4× 36 0.3× 58 1.4× 27 0.8× 50 968

Countries citing papers authored by Prasad Subramanian

Since Specialization
Citations

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

Fields of papers citing papers by Prasad Subramanian

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Prasad Subramanian

This figure shows the co-authorship network connecting the top 25 collaborators of Prasad Subramanian. A scholar is included among the top collaborators of Prasad Subramanian 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 Prasad Subramanian. Prasad Subramanian 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.
Subramanian, Prasad, et al.. (2025). Turbulent Power: A Discriminator Between Sheaths and CMEs. Solar Physics. 300(4). 1 indexed citations
2.
Subramanian, Prasad, et al.. (2021). Turbulent Proton Heating Rate in the Solar Wind from 5–45 R . The Astrophysical Journal. 914(2). 137–137. 11 indexed citations
3.
Subramanian, Prasad, et al.. (2019). Automated Detection of Solar Radio Bursts Using a Statistical Method. Solar Physics. 294(8). 12 indexed citations
4.
Subramanian, Prasad, et al.. (2018). Energetics of small electron acceleration episodes in the solar corona from radio noise storm observations. Monthly Notices of the Royal Astronomical Society. 479(2). 1603–1611. 8 indexed citations
5.
Subramanian, Prasad, et al.. (2017). Small electron acceleration episodes in the solar corona. Monthly Notices of the Royal Astronomical Society. 471(1). 89–99. 13 indexed citations
6.
Ramesh, R., et al.. (2016). Amplitude of solar wind density turbulence from 10 to 45 R. Journal of Geophysical Research Space Physics. 121(12). 8 indexed citations
7.
Mohanty, P. K., K. P. Arunbabu, T. Aziz, et al.. (2016). Transient Weakening of Earth’s Magnetic Shield Probed by a Cosmic Ray Burst. Physical Review Letters. 117(17). 171101–171101. 13 indexed citations
8.
Bhaskar, Ankush, Prasad Subramanian, & Geeta Vichare. (2016). RELATIVE CONTRIBUTION OF THE MAGNETIC FIELD BARRIER AND SOLAR WIND SPEED IN ICME-ASSOCIATED FORBUSH DECREASES. The Astrophysical Journal. 828(2). 104–104. 23 indexed citations
9.
Arunbabu, K. P., H. M. Antia, S. R. Dugad, et al.. (2015). How are Forbush decreases related to interplanetary magnetic field enhancements?. Springer Link (Chiba Institute of Technology). 28 indexed citations
10.
Subramanian, Prasad, et al.. (2015). Coronal turbulence and the angular broadening of radio sources – the role of the structure function. Monthly Notices of the Royal Astronomical Society. 447(4). 3486–3497. 13 indexed citations
12.
Arunbabu, K. P., H. M. Antia, S. R. Dugad, et al.. (2013). High-rigidity Forbush decreases: due to CMEs or shocks?. Springer Link (Chiba Institute of Technology). 26 indexed citations
13.
Lara, A., et al.. (2011). Velocity profile of interplanetary coronal mass ejections beyond 1 AU. Journal of Geophysical Research Atmospheres. 116(A12). n/a–n/a. 7 indexed citations
14.
Subramanian, Prasad, H. M. Antia, S. R. Dugad, et al.. (2008). Forbush decreases and turbulence levels at coronal mass ejection fronts. Springer Link (Chiba Institute of Technology). 35 indexed citations
15.
Subramanian, Prasad & A. Vourlidas. (2007). Energetics of solar coronal mass ejections. Springer Link (Chiba Institute of Technology). 26 indexed citations
16.
Becker, Peter A. & Prasad Subramanian. (2005). Restrictions on the Physical Prescription for the Viscosity in Advection‐dominated Accretion Disks. The Astrophysical Journal. 622(1). 520–530. 10 indexed citations
17.
Subramanian, Prasad & A. Vourlidas. (2004). Energetics of Coronal Mass Ejections. Proceedings of the International Astronomical Union. 2004(IAUS226). 314–315. 1 indexed citations
18.
Gopal‐Krishna, Prasad Subramanian, Paul J. Wiita, & Peter A. Becker. (2001). Are the hotspots of radio galaxies the sites of in situacceleration of relativistic particles?. Springer Link (Chiba Institute of Technology). 7 indexed citations
19.
Subramanian, Prasad, et al.. (1999). Relativistic Outflows from Advection-dominated Accretion Disks around Black Holes. AAS. 194. 369–370. 1 indexed citations
20.
Subramanian, Prasad, Peter A. Becker, & Demosthenes Kazanas. (1999). Formation of Relativistic Outflows in Shearing Black Hole Accretion Coronae. The Astrophysical Journal. 523(1). 203–222. 12 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026