activity
19972025
most citedA turbulence-driven model for heating and acceleration of the fast wind in coronal holes

234 citations · 1.3k across the 36 of their papers we have counts for

collaborators

34 papers

physics.space-ph2025

Turbulence in the terrestrial magnetosheath: space-time correlation using the Magnetospheric Multiscale mission

Francesco Pecora, William H. Matthaeus, Antonella Greco +4

Spatiotemporal correlation of magnetic field fluctuations is investigated using the Magnetospheric Multiscale mission in the terrestrial magnetosheath. The first observation of the…

physics.plasm-ph2025

The Energy Cascade Rate in Supersonic Magnetohydrodynamic Turbulence

Gonzalo Javier Alvarez, Pablo Dmitruk, Branislav Rabatin +2

Three-dimensional direct numerical simulations (DNS) are implemented to investigate the energy cascade rate in compressible isothermal magnetohydrodynamic (MHD) turbulence. Utilizi…

physics.plasm-ph2023

Energization of charged test particles in magnetohydrodynamic fields: waves vs turbulence picture

F. Pugliese, M. Brodiano, N. Andrés +1

Direct numerical simulations of 3D compressible MHD turbulence were performed in order to study the relation between waves modes and coherent structures and the consequent energiza…

physics.space-ph2022

The essential role of multi-point measurements in investigations of turbulence, three-dimensional structure, and dynamics: the solar wind beyond single scale and the Taylor Hypothesis

W. H. Matthaeus, S. Adhikari, R. Bandyopadhyay +49

Space plasmas are three-dimensional dynamic entities. Except under very special circumstances, their structure in space and their behavior in time are not related in any simple way…

physics.plasm-ph2022★ 4 cited

Effect of the electronic pressure on the energy and magnetic moment of charged test particles in turbulent electromagnetic fields

B. Balzarini, F. Pugliese, P. Dmitruk

In this work we perform direct numerical simulations of three-dimensional magnetohydrodynamics with a background magnetic field, representing solar wind plasma, and introduce test…

astro-ph.SR2022★ 18 cited

A Statistical Study of the Compressible Energy Cascade Rate in Solar Wind Turbulence: Parker Solar Probe Observations

Maia Brodiano, Pablo Dmitruk, Nahuel Andrés

We investigated incompressible and compressible magnetohydrodynamic (MHD) energy cascade rates in the solar wind at different heliocentric distances. We used in situ magnetic field…