Identifiers
-
name variant
Benjamin D. G. Chandran
0.60 · backfill
Papers (40)
-
Cyclotron breaking: a mechanism for parallel ion cyclotron waves to heat the fast solar wind
astro-ph.SR · 2026 · author #2
-
Stochastic proton heating by kinetic-Alfv\'en-wave turbulence in moderately high-$\beta$ plasmas
physics.plasm-ph · 2018 · author #2
-
Parametric Instability, Inverse Cascade, and the $1/f$ Range of Solar-Wind Turbulence
physics.space-ph · 2017 · author #1
-
Heating of Accretion-Disk Coronae and Jets by General Relativistic MHD Turbulence
astro-ph.HE · 2017 · author #1
-
On the Conservation of Cross Helicity and Wave Action in Solar-Wind Models with Non-WKB Alfven Wave Reflection
astro-ph.SR · 2015 · author #1
-
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
physics.space-ph · 2014 · author #2
-
Stochastic Acceleration of Electrons by Fast Magnetosonic Waves in Solar Flares: the Effects of Anisotropy in Velocity andWavenumber Space
astro-ph.SR · 2014 · author #2
-
Magnetohydrodynamic Slow Mode with Drifting He$^{++}$: Implications for Coronal Seismology and the Solar Wind
physics.space-ph · 2014 · author #3
-
Intermittency and Alignment in Strong RMHD Turbulence
astro-ph.SR · 2014 · author #1
-
Acceleration of Relativistic Electrons by MHD Turbulence: Implications for Non-thermal Emission from Black Hole Accretion Disks
astro-ph.HE · 2014 · author #3
-
Limits on Alpha Particle Temperature Anisotropy and Differential Flow from Kinetic Instabilities: Solar Wind Observations
astro-ph.SR · 2013 · author #3
-
Perpendicular Ion Heating by Reduced Magnetohydrodynamic Turbulence
astro-ph.SR · 2013 · author #3
-
Direct Numerical Simulations of Reflection-Driven, Reduced MHD Turbulence from the Sun to the Alfven Critical Point
astro-ph.SR · 2013 · author #2
-
Observational Test of Stochastic Heating in Low-$\beta$ Fast Solar Wind Streams
astro-ph.SR · 2013 · author #2
-
Instabilities Driven by the Drift and Temperature Anisotropy of Alpha Particles in the Solar Wind
physics.space-ph · 2013 · author #3
-
The Efficiency of Second-Order Fermi Acceleration by Weakly Compressible MHD Turbulence
astro-ph.SR · 2013 · author #3
-
A Parallel-Propagating Alfv\'enic Ion-Beam Instability in the High-Beta Solar Wind
physics.space-ph · 2013 · author #3
-
The Dispersion Relations and Instability Thresholds of Oblique Plasma Modes in the Presence of an Ion Beam
physics.space-ph · 2012 · author #2
-
Resonance Broadening and Heating of Charged Particles in Magnetohydrodynamic Turbulence
astro-ph.SR · 2012 · author #4
-
Incorporating Kinetic Physics into a Two-Fluid Solar-Wind Model with Temperature Anisotropy and Low-Frequency Alfven-Wave Turbulence
astro-ph.SR · 2011 · author #1
-
Alfven Wave Turbulence and Perpendicular Ion Temperatures in Coronal Holes
astro-ph.SR · 2010 · author #1
-
Perpendicular Ion Heating by Low-Frequency Alfven-Wave Turbulence in the Solar Wind
astro-ph.SR · 2010 · author #1
-
Alfven Wave Reflection and Turbulent Heating in the Solar Wind from 1 Solar Radius to 1 AU: an Analytical Treatment
astro-ph.SR · 2009 · author #1
-
Constraining Low-Frequency Alfvenic Turbulence in the Solar Wind Using Density Fluctuation Measurements
astro-ph.SR · 2009 · author #1
-
The Turbulent Heating Rate in Strong MHD Turbulence with Nonzero Cross Helicity
astro-ph.SR · 2009 · author #1
-
Weakly Turbulent MHD Waves in Compressible Low-Beta Plasmas
astro-ph · 2008 · author #1
-
Parker/buoyancy instabilities with anisotropic thermal conduction, cosmic rays, and arbitrary magnetic field strength
astro-ph · 2008 · author #2
-
Strong Anisotropic MHD Turbulence with Cross Helicity
astro-ph · 2008 · author #1
-
Convection and AGN Feedback in Clusters of Galaxies
astro-ph · 2007 · author #1
-
Weak compressible magnetohydrodynamic turbulence in the solar corona
astro-ph · 2005 · author #1
-
AGN-driven convection in galaxy-cluster plasmas
astro-ph · 2005 · author #1
-
Stochastic relativistic shock-surfing acceleration
astro-ph · 2004 · author #1
-
Convection in galaxy-cluster plasmas driven by active galactic nuclei and cosmic-ray buoyancy
astro-ph · 2004 · author #1
-
Acceleration of energetic particles by large-scale compressible magnetohydrodynamic turbulence
astro-ph · 2003 · author #1
-
Particle acceleration by slow modes in strong compressible MHD turbulence, with application to solar flares
astro-ph · 2003 · author #1
-
A review of the theory of incompressible MHD turbulence
astro-ph · 2003 · author #1
-
Thermal conduction and particle transport in strong MHD turbulence, with application to galaxy-cluster plasmas
astro-ph · 2003 · author #1
-
The divergence of neighboring magnetic field lines and fast-particle diffusion in strong magnetohydrodynamic turbulence, with application to thermal conduction in galaxy clusters
astro-ph · 2003 · author #2
-
Rayleigh-Taylor stability of a strong vertical magnetic field at the Galactic center confined by a disk threaded with horizontal magnetic field
astro-ph · 2000 · author #1
-
Scattering of energetic particles by anisotropic magnetohydrodynamic turbulence with a Goldreich-Sridhar power spectrum
astro-ph · 2000 · author #1
Mentions
-
2605.25117
#2 · arxiv_oai · confidence 0.70
Benjamin D. G. Chandran
-
1212.5192
#2 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
1204.0155
#4 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
1110.3029
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
1006.3473
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
1001.2069
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0911.1068
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0908.0757
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0905.3382
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0810.5360
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0809.0718
#2 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0801.4903
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran
-
0707.2351
#1 · backfill · confidence 0.70
Benjamin D. G. Chandran