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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

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Showing 2009Show all

6 papers · 1 filter

astro-ph.SR2009★ 1 cited

Resonant Interactions Between Protons and Oblique Alfvén/Ion-Cyclotron Waves

Peera Pongkitiwanichakul, Benjamin D. G. Chandran, Philip A. Isenberg +1

Resonant interactions between ions and Alfvén/ion-cyclotron (A/IC) waves may play an important role in the heating and acceleration of the fast solar wind. Although such interactio…

astro-ph.SR2009★ 148 cited

Alfven Wave Reflection and Turbulent Heating in the Solar Wind from 1 Solar Radius to 1 AU: an Analytical Treatment

Benjamin D. G. Chandran, Joseph V. Hollweg

We study the propagation, reflection, and turbulent dissipation of Alfven waves in coronal holes and the solar wind. We start with the Heinemann-Olbert equations, which describe no…

astro-ph.SR2009★ 99 cited

Constraining Low-Frequency Alfvenic Turbulence in the Solar Wind Using Density Fluctuation Measurements

Benjamin D. G. Chandran, Eliot Quataert, Gregory G. Howes +2

One proposed mechanism for heating the solar wind, from close to the sun to beyond 10 AU, invokes low-frequency, oblique, Alfven-wave turbulence. Because small-scale oblique Alfven…

astro-ph.SR2009★ 29 cited

The Turbulent Heating Rate in Strong MHD Turbulence with Nonzero Cross Helicity

Benjamin D. G. Chandran, Eliot Quataert, Gregory G. Howes +2

Different results for the cascade power in strong, incompressible MHD turbulence with nonzero cross helicity appear in the literature. In this paper, we discuss the conditions unde…

astro-ph.SR2009★ 6 cited

Scale dependent alignment between velocity and magnetic field fluctuations in the solar wind and comparisons to Boldyrev's phenomenological theory

J. J. Podesta, A. Bhattacharjee, B. D. G. Chandran +2

(Abridged abstract) A theory of incompressible MHD turbulence recently developed by Boldyrev predicts the existence of a scale dependent angle of alignment between velocity and mag…

astro-ph.HE2009★ 61 cited

Buoyancy Instabilities in Galaxy Clusters: Convection Due to Adiabatic Cosmic Rays and Anisotropic Thermal Conduction

P. Sharma, B. D. G. Chandran, E. Quataert +1

Using a linear stability analysis and two and three-dimensional nonlinear simulations, we study the physics of buoyancy instabilities in a combined thermal and relativistic (cosmic…