activity
19972022
most citedDensity Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology

259 citations · 2.2k across the 40 of their papers we have counts for

collaborators

40 papers

physics.plasm-ph2022★ 3 cited

Simulating a pulsed power-driven plasma with ideal MHD

A. Beresnyak, A. L. Velikovich, J. L. Giuliani +4

We describe a simple practical numerical method for simulating plasma driven within a vacuum chamber by a pulsed power generator. Typically, in this type of simulation, the vacuum…

physics.plasm-ph2021★ 5 cited

Stable and unstable supersonic stagnation of an axisymmetric rotating magnetized plasma

Andrey Beresnyak, Alexander L. Velikovich, John L. Giuliani +1

The Naval Research Laboratory "Mag Noh problem", described in this paper, is a self-similar magnetized implosion flow, which contains a fast MHD outward propagating shock of consta…

physics.space-ph2020★ 6 cited

Major Scientific Challenges and Opportunities in Understanding Magnetic Reconnection and Related Explosive Phenomena in Solar and Heliospheric Plasmas

H. Ji, J. Karpen, A. Alt +105

Magnetic reconnection underlies many explosive phenomena in the heliosphere and in laboratory plasmas. The new research capabilities in theory/simulations, observations, and labora…

physics.plasm-ph2020★ 5 cited

Major Scientific Challenges and Opportunities in Understanding Magnetic Reconnection and Related Explosive Phenomena throughout the Universe

H. Ji, A. Alt, S. Antiochos +97

This white paper summarizes major scientific challenges and opportunities in understanding magnetic reconnection and related explosive phenomena as a fundamental plasma process.

astro-ph.GA2019★ 67 cited

MHD Turbulence

Andrey Beresnyak

We review the current status of research in MHD turbulence theory and numerical experiments and their applications to astrophysics and solar science. We introduce general tools for…

astro-ph.CO2015★ 75 cited

Self-similar energetics in large clusters of galaxies

Francesco Miniati, Andrey Beresnyak

Massive galaxy clusters are filled with a hot, turbulent and magnetized intra-cluster medium. Still forming under the action of gravitational instability, they grow in mass by accr…