activity
20072026
most citedIncompressive Energy Transfer in the Earth's Magnetosheath: Magnetospheric Multiscale Observations

56 citations · 110 across the 6 of their papers we have counts for

collaborators

6 papers

physics.plasm-ph2026

Collimation of diamagnetic laser-driven plasma outflows by an ambient magnetic-pressure gradient

Yigeng Tian, Chung Hei Leung, Arijit Bose +3

We present magnetohydrodynamic simulations of laser driven plasma outflows propagating along an externally applied poloidal magnetic field, designed to mimic coronal open-field pla…

physics.plasm-ph2024★ 1 cited

Scale Separation Effects on Simulations of Plasma Turbulence

Jago Edyvean, Tulasi N. Parashar, Tom Simpson +7

Understanding plasma turbulence requires a synthesis of experiments, observations, theory, and simulations. In the case of kinetic plasmas such as the solar wind, the lack of colli…

physics.plasm-ph2023

Scale Filtering Analysis of Kinetic Reconnection and its Associated Turbulence

Subash Adhikari, Yan Yang, William H. Matthaeus +3

Previously, using an incompressible von Kármán-Howarth formalism, the behavior of cross-scale energy transfer in magnetic reconnection and turbulence was found to be essentially id…

physics.plasm-ph2023

Effective Viscosity, Resistivity, and Reynolds Number in Weakly Collisional Plasma Turbulence

Yan Yang, William H. Matthaeus, Sean Oughton +6

We examine dissipation and energy conversion in weakly collisional plasma turbulence, employing in situ observations from the Magnetospheric Multiscale (MMS) mission and kinetic Pa…

physics.space-ph2018★ 56 cited

Incompressive Energy Transfer in the Earth's Magnetosheath: Magnetospheric Multiscale Observations

Riddhi Bandyopadhyay, A. Chasapis, R. Chhiber +14

Using observational data from the \emph{Magnetospheric Multiscale} (MMS) Mission in the Earth's magnetosheath, we estimate the energy cascade rate using different techniques within…

astro-ph2007★ 53 cited

From Solar and Stellar Flares to Coronal Heating: Theory and Observations of How Magnetic Reconnection Regulates Coronal Conditions

P. A. Cassak, D. J. Mullan, M. A. Shay

There is currently no explanation of why the corona has the temperature and density it has. We present a model which explains how the dynamics of magnetic reconnection regulates th…