105 citations · 269 across the 11 of their papers we have counts for
11 papers
Secondary Electron-Only Reconnection Driven by Large Scale Ion-Coupled Reconnection and Electron Kelvin-Helmholtz Instabilities in Hybrid Simulations of Solar Wind Turbulence
Joaquín Espinoza-Troni, Giuseppe Arrò, Francesco Califano +2
Electron-only reconnection (EREC) is a magnetic reconnection regime occurring within subion-scale current sheets (CSs), exhibiting only electron jets, without any ion outflows. ERE…
Impact of solar wind turbulence on a planetary bow shock
E. Behar, F. Pucci, C. Simon Wedlund +4
Over the past decades, near-Earth spacecraft observations have provided insights into the physics of the bow shock, suggesting that solar wind intrinsic turbulence influences the b…
Large Scale Linear Magnetic Holes with Magnetic Mirror Properties in Hybrid Simulations of Solar Wind Turbulence
Giuseppe Arrò, Francesco Califano, Francesco Pucci +2
Magnetic holes (MHs) are coherent magnetic field dips whose size ranges from fluid to kinetic scale, ubiquitously observed in the heliosphere and in planetary environments. Despite…
On the Cascade-Dissipation Balance in Astrophysical Plasmas
Davide Manzini, Fouad Sahraoui, Francesco Califano
The differential heating of electrons and ions by turbulence in weakly collisional magnetized plasmas and the scales at which such energy dissipation is most effective are still de…
Comparative simulations of Kelvin-Helmholtz induced magnetic reconnection at the Earth's magnetospheric flanks
Silvia Ferro, Matteo Faganello, Francesco Califano +1
This study presents three-dimensional (3D) resistive Hall-magnetohydrodynamic simulations of the Kelvin-Helmholtz instability (KHI) dynamics at Earth's magnetospheric flanks during…
Subion Scale Turbulence Driven by Magnetic Reconnection
Davide Manzini, Fouad Sahraoui, Francesco Califano
The interplay between plasma turbulence and magnetic reconnection remains an unsettled question in astrophysical and laboratory plasmas. Here we report the first observational evid…
Local cascade and dissipation in incompressible Hall magnetohydrodynamic turbulence: the Coarse-Graining approach
Davide Manzini, Fouad Sahraoui, Francesco Califano +1
We derive the coarse-graining (CG) equations of incompressible Hall Magnetohydrodynamics (HMHD) turbulence to investigate the {\it local (in space)} energy cascade rate as a functi…
[Plasma 2020 Decadal] Disentangling the Spatiotemporal Structure of Turbulence Using Multi-Spacecraft Data
J. M. TenBarge, O. Alexandrova, S. Boldyrev +26
This white paper submitted for 2020 Decadal Assessment of Plasma Science concerns the importance of multi-spacecraft missions to address fundamental questions concerning plasma tur…
Coherent structures and spectral energy transfer in turbulent plasma: a space-filter approach
Enrico Camporeale, Luca Sorriso-Valvo, Francesco Califano +1
Plasma turbulence at scales of the order of the ion inertial length is mediated by several mechanisms, including linear wave damping, magnetic reconnection, formation and dissipati…
Plasma turbulence at ion scales: a comparison between PIC and Eulerian hybrid-kinetic approaches
S. S. Cerri, L. Franci, F. Califano +2
Kinetic-range turbulence in magnetized plasmas and, in particular, in the context of solar-wind turbulence has been extensively investigated over the past decades via numerical sim…
Proton Kinetic Effects in Vlasov and Solar Wind Turbulence
S. Servidio, K. T. Osman, F. Valentini +5
Kinetic plasma processes have been investigated in the framework of solar wind turbulence, employing Hybrid Vlasov-Maxwell (HVM) simulations. The dependency of proton temperature a…