Benjamin D. G. Chandran

6.9k citations
93 papers · 2.5k indexed · h-index 27

Benjamin D. G. Chandran

86 papers receiving 2.3k citations

Peers

Benjamin D. G. Chandran
Comparison fields: 5 of 37
  • Astronomy and Astrophysics 2.5k
  • Nuclear and High Energy Physics 514
  • Molecular Biology 556
  • Computational Mechanics 125
  • Instrumentation 19
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Citations per year

Countries citing papers authored by Benjamin D. G. Chandran

Since Specialization
Citations

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

Fields of papers citing papers by Benjamin D. G. Chandran

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside Benjamin D. G. Chandran, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with Benjamin D. G. Chandran Line = papers co-authored together Benjamin D. G. Chandran links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20252
2 20250
3 20254
4 20241
5 202419
6 202410
7 202320
8 202318
9 202243
10 202229
11 202235
12 202123
13 202182
14 202125
15 20213
16 20216
17
Advances in Fluid Modeling of the Solar Wind. Part 1: Electron and Anisotropic Proton Temperatures from the Collisionless Dissipation of Alfven Wave Turbulence
20111
18
Plasma Physics in Clusters of Galaxies
20090
19
Scattering of energetic particles by anisotropic magnetohydrodynamic turbulence with a Goldreich-Sridhar power spectrum in the quasilinear approximation
20001
20
Nonlinear Turbulent Dynamos and the Origin of the Galactic Magnetic Field
19971

About Benjamin D. G. Chandran

Benjamin D. G. Chandran is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atmospheric Science, having authored 93 papers that have together received 2.5k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (83 papers), Ionosphere and magnetosphere dynamics (63 papers), Astro and Planetary Science (26 papers), Geomagnetism and Paleomagnetism Studies (19 papers), Astrophysics and Star Formation Studies (15 papers), Stellar, planetary, and galactic studies (14 papers), Magnetic confinement fusion research (12 papers) and Galaxies: Formation, Evolution, Phenomena (7 papers). The work is most often cited by research in Astronomy and Astrophysics (2.5k citations), Nuclear and High Energy Physics (514 citations) and Molecular Biology (556 citations). Benjamin D. G. Chandran has collaborated with scholars based in United States, United Kingdom and France. Frequent co-authors include Eliot Quataert, S. C. Cowley, S. D. Bale, Timothy J. Dennis, Joseph V. Hollweg, Alfred Mallet, Daniel Verscharen, Jean C. Perez, K. Germaschewski and B. N. Rogers. Their work appears in journals such as Physical Review Letters, Journal of Geophysical Research Atmospheres and The Astrophysical Journal.

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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