activity
20082026
most citedEnergy transfer, pressure tensor and heating of kinetic plasma

183 citations · 1.7k across the 55 of their papers we have counts for

collaborators
Showing 2023Show all

8 papers · 1 filter

astro-ph.SR2023

Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by {\it Parker Solar Probe}

Panisara Thepthong, Peera Pongkitiwanichakul, David Ruffolo +4

Alfvénicity is a well-known property, common in the solar wind, characterized by a high correlation between magnetic and velocity fluctuations. Data from the Parker Solar Probe (PS…

physics.plasm-ph2023

Statistics of Turbulence in the Solar Wind. I. What is the Reynolds Number of the Solar Wind?

Daniel Wrench, Tulasi N. Parashar, Sean Oughton +2

The Reynolds number, Re, is an important quantity for describing a turbulent flow. It tells us about the bandwidth over which energy can cascade from large scales to smaller ones,…

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…

astro-ph.CO2023

Power spectrum estimation methods on intracluster medium surface brightness fluctuations

Mark Bishop, Yvette Perrott, Tulasi Parashar +1

Accurate estimation of galaxy cluster masses is a central problem in cosmology. Turbulence is believed to introduce significant deviations from the hydrostatic mass estimates. Esti…

astro-ph.CO2023

Probing the evolution of galaxy clusters using SZ effect and non-thermal emission: first results from A1413

Mohini Pachchigar, Yvette Perrott, Tulasi Parashar

Mass is the most fundamental property of galaxy clusters. However, measuring it is still a challenge. Calibrating mass from intracluster medium observables such as the Sunyaev-Zel'…

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.plasm-ph2023

Statistics of Pressure Fluctuations in Turbulent Kinetic Plasmas

Subash Adhikari, William H. Matthaeus, Tulasi N. Parashar +2

In this study we explore the statistics of pressure fluctuations in kinetic collisionless turbulence. A 2.5D kinetic particle-in-cell (PIC) simulation of decaying turbulence is use…

physics.plasm-ph2023

Effect of a guide field on the turbulence like properties of magnetic reconnection

Subash Adhikari, Michael A. Shay, Tulasi N. Parashar +4

The effect of an external guide field on the turbulence-like properties of magnetic reconnection is studied using five different 2.5D kinetic particle-in-cell (PIC) simulations. Th…