activity
20202026
most citedTurbulent Heating between 0.2 and 1 au: A Numerical Study

33 citations · 34 across the 3 of their papers we have counts for

collaborators

5 papers

physics.plasm-ph2026★ 1 cited

Rugged magneto-hydrodynamic invariants in weakly collisional plasma turbulence: Two-dimensional hybrid simulation results

Petr Hellinger, Victor Montagud-Camps

Aims. We investigated plasma turbulence in the context of solar wind. We concentrated on properties of ideal second-order magneto-hydrodynamic (MHD) and Hall MHD invariants. Method…

physics.space-ph2026★ 33 cited

Turbulent Heating between 0.2 and 1 au: A Numerical Study

Victor Montagud-Camps, Roland Grappin, Andrea Verdini

The heating of the solar wind is a key to understand its dynamics and acceleration process. The observed radial decrease of proton temperature in the solar wind is slow compared to…

astro-ph.SR2022

Ion-scale transition of plasma turbulence: Pressure-strain effect

Petr Hellinger, Victor Montagud-Camps, Luca Franci +4

We investigate properties of solar wind-like plasma turbulence using direct numerical simulations. We analyze the transition from large, magnetohydrodynamic (MHD) scales to the ion…

physics.plasm-ph2021

Spectral transfer and Kármán-Howarth-Monin equations for compressible Hall magnetohydrodynamics

Petr Hellinger, Emanuele Papini, Andrea Verdini +4

We derive two new forms of the Kármán-Howarth-Monin equation for decaying compressible Hall magnetohydrodynamic (MHD) turbulence. We test them on results of a weakly-compressible,…

astro-ph.SR2020

Comparing turbulent cascades and heating vs spectral anisotropy in solar wind via direct simulations

Victor Montagud-Camps, Roland Grappin, Andrea Verdini

In a previous work (MGV18), we showed numerically that the turbulent cascade generated by quasi-2D structures (with wave vectors mostly-perpendicular to the mean magnetic field) is…