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researcher

B. Chandran

87 papers hereh-index 416.3k citations184 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author11
  • first author16
  • middle author36
  • last author17

Across the 80 of 87 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR42
  • physics.space-ph18
  • astro-ph16
  • physics.plasm-ph7
  • astro-ph.HE4
same name
  • B. Chandran — 17 papers, h 7
  • B. Chandran — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002025
most citedPerpendicular Ion Heating by Low-Frequency Alfven-Wave Turbulence in the Solar Wind

326 citations · 4.6k across the 86 of their papers we have counts for

collaborators
Showing 2014 · physics.space-phShow all

3 papers · 2 filters

physics.space-ph2014★ 34 cited

A Modified Version of Taylor's Hypothesis for Solar Probe Plus Observations

Kristopher G. Klein, Jean C. Perez, Daniel Verscharen +2

The Solar Probe Plus (SPP) spacecraft will explore the near-Sun environment, reaching heliocentric distances less than 10R⊙​. Near Earth, spacecraft measurements of fluctu…

physics.space-ph2014★ 32 cited

Deceleration of Alpha Particles in the Solar Wind by Instabilities and the Rotational Force: Implications for Heating, Azimuthal Flow, and the Parker Spiral Magnetic Field

Daniel Verscharen, Benjamin D. G. Chandran, Sofiane Bourouaine +1

Protons and alpha particles in the fast solar wind are only weakly collisional and exhibit a number of non-equilibrium features, including relative drifts between particle species.…

physics.space-ph2014★ 12 cited

Magnetohydrodynamic Slow Mode with Drifting He++: Implications for Coronal Seismology and the Solar Wind

Joseph V. Hollweg, Daniel Verscharen, Benjamin D. G. Chandran

The MHD slow mode wave has application to coronal seismology, MHD turbulence, and the solar wind where it can be produced by parametric instabilities. We consider analytically how…

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