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20032009
most citedStrong Anisotropic MHD Turbulence with Cross Helicity

123 citations · 262 across the 7 of their papers we have counts for

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16 papers

astro-ph.SR200929 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.SR20096 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-ph200843 cited

Weakly Turbulent MHD Waves in Compressible Low-Beta Plasmas

Benjamin D. G. Chandran

In this Letter, weak turbulence theory is used to investigate interactions among Alfven waves and fast and slow magnetosonic waves in collisionless low-beta plasmas. The wave kinet…

astro-ph20087 cited

Parker/buoyancy instabilities with anisotropic thermal conduction, cosmic rays, and arbitrary magnetic field strength

Timothy J. Dennis, Benjamin D. G. Chandran

We report the results of a local stability analysis for a magnetized, gravitationally stratified plasma containing cosmic rays. We account for cosmic-ray diffusion and thermal cond…

astro-ph200824 cited

Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conduction

Yann Rasera, Benjamin Chandran

In clusters of galaxies, the specific entropy of intracluster plasma increases outwards. Nevertheless, a number of recent studies have shown that the intracluster medium is subject…

astro-ph2008123 cited

Strong Anisotropic MHD Turbulence with Cross Helicity

Benjamin D. G. Chandran

This paper proposes a new phenomenology for strong incompressible MHD turbulence with nonzero cross helicity. This phenomenology is then developed into a quantitative Fokker-Planck…