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19982008
most citedCompressible Turbulence in Galaxy Clusters: Physics and Stochastic Particle Re-acceleration

389 citations · 559 across the 9 of their papers we have counts for

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15 papers · 1 filter

astro-ph20082 cited

Grain Alignment and CMB Polarization Studies

A. Lazarian

Polarized microwave emission from dust is an important foreground that may contaminate polarized CMB studies unless carefully accounted for. Modeling of polarization from dust requ…

astro-ph20073 cited

Diffusion Processes in Turbulent Magnetic Fields

Alex Lazarian

We study of the effect of turbulence on diffusion processes within magnetized medium. While we exemplify our treatment with heat transfer processes, our results are quite general a…

astro-ph2007389 cited

Compressible Turbulence in Galaxy Clusters: Physics and Stochastic Particle Re-acceleration

G. Brunetti, A. Lazarian

We attempt to explain the non-thermal emission arising from galaxy clusters as a result of the re-acceleration of electrons by compressible turbulence induced by cluster mergers. I…

astro-ph20071 cited

Density Distribution of the Warm Ionized Medium

Alex S. Hill, Ronald J. Reynolds, Robert A. Benjamin +1

Observations of Halpha emission measures and pulsar dispersion measures at high Galactic latitude (|b| > 10 deg) provide information about the density and distribution of the diffu…

astro-ph200633 cited

Polarization from aligned atoms as a diagnostics of circumstellar, AGN and interstellar magnetic fields: II. Atoms with Hyperfine Structure

Huirong Yan, A. Lazarian

We show that atomic alignment presents a reliable way to study topology of astrophysical magnetic fields. The effect of atomic alignment arises from modulation of the relative popu…

astro-ph2005

MHD Turbulence: Properties of Alfven, Slow and Fast Modes

A. Lazarian, A. Beresnyak

We summarise basic properties of MHD turbulence. First, MHD turbulence is not so messy as it is believed. In fact, the notion of strong non-linear coupling of compressible and inco…