1.7k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR28 papers
- National Research CouncilLK21 papers
- University of CalabriaIT20 papers
- Swedish Institute of Space PhysicsSE19 papers
- KTH Royal Institute of TechnologySE18 papers
- Gran Sasso Science InstituteIT12 papers
- Institute for Space Astrophysics and PlanetologyIT12 papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoIT12 papers
- Agenzia Spaziale ItalianaIT11 papers
- École PolytechniqueFR11 papers
- Imperial College LondonGB11 papers
- National Institute for AstrophysicsIT11 papers
16 papers · 1 filter
Transport of electrons in tangled magnetic fields
Daniel Verscharen, Natasha Jeffrey, Anton Artemyev +6
Cosmic magnetic fields are typically inhomogeneous and often highly tangled due to large-scale plasma flows, turbulence, and instabilities. If the variations in the magnetic field…
Turbulent dynamo in the terrestrial magnetosheath
Zoltán Vörös, Owen Wyn Roberts, Yasuhito Narita +10
Dynamo action refers to energy exchange processes through which magnetic fields are generated at the expense of kinetic energy of the plasma flows. Dynamos can generate magnetic fi…
Extent of the Magnetotail of Venus From the Solar Orbiter, Parker Solar Probe and BepiColombo Flybys
Niklas J. T. Edberg, David J. Andrews, J. Jordi Boldú +20
We analyze data from multiple flybys by the Solar Orbiter, BepiColombo, and Parker Solar Probe (PSP) missions to study the interaction between Venus' plasma environment and the sol…
Temperature anisotropy instabilities driven by intermittent velocity shears in the solar wind
Simon Opie, Daniel Verscharen, Christopher H. K. Chen +5
Where and under what conditions the transfer of energy between electromagnetic fields and particles takes place in the solar wind remains an open question. We investigate the condi…
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…
Evaluation of scale-dependent kurtosis with HelioSwarm
Francesco Pecora, Francesco Pucci, Francesco Malara +4
Plasma turbulence involves complex, nonlinear interactions of electromagnetic fields and charged particles across multiple scales. Studying these phenomena in space plasmas, like t…
Higher-Order Analysis of Three-Dimensional Anisotropy in Imbalanced Alfvénic Turbulence
Nikos Sioulas, Themistocles Zikopoulos, Chen Shi +10
We analyze in-situ observations of imbalanced solar wind turbulence to evaluate MHD turbulence models grounded in "Critical Balance" (CB) and "Scale-Dependent Dynamic Alignment" (S…
Three-dimensional modelling of the shock-turbulence interaction
Domenico Trotta, Oreste Pezzi, David Burgess +12
The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We s…
Helios 2 observations of solar wind turbulence decay in the inner heliosphere
Luca Sorriso-Valvo, Raffaele Marino, Foldes Raffaello +5
The linear scaling of the mixed third-order moment of the magnetohydrodynamic fluctuations is used to estimate the energy transfer rate of the turbulent cascade in the expanding so…
Turbulence, intermittency and cross-scale energy transfer in an interplanetary coronal mass ejection
Roque Márquez Rodríguez, Luca Sorriso-Valvo, Emiliya Yordanova
Solar wind measurements carried out by NASA's Wind spacecraft before, during and after the passing of an interplanetary coronal mass ejection (ICME) detected on 12-14 September 201…
Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations
F. Carbone, L. Sorriso-Valvo, Yu. V. Khotyaintsev +27
The recently released spacecraft potential measured by the RPW instrument on-board Solar Orbiter has been used to estimate the solar wind electron density in the inner heliosphere.…
Local and global properties of energy transfer in models of plasma turbulence
Christian L. Vásconez, Denise Perrone, Raffaele Marino +5
The nature of the turbulent energy transfer rate is studied using direct numerical simulations of weakly collisional space plasmas. This is done comparing results obtained from hyb…
Kelvin-Helmholtz instability at proton scales with an exact kinetic equilibrium
A. Settino, F. Malara, O. Pezzi +3
The Kelvin-Helmholtz instability is a ubiquitous physical process in ordinary fluids and plasmas, frequently observed also in space environments. In this paper, kinetic effects at…
Sign singularity of the local energy transfer in space plasma turbulence
Luca Sorriso-Valvo, Gaetano De Vita, Federico Fraternale +18
In weakly collisional space plasmas, the turbulent cascade provides most of the energy that is dissipated at small scales by various kinetic processes. Understanding the characteri…
In-situ observation of Hall Magnetohydrodynamic Cascade in Space Plasma
Riddhi Bandyopadhyay, Luca Sorriso-Valvo, Alexandros Chasapis +13
We present estimates of the turbulent energy cascade rate, derived from a Hall-MHD third-order law. We compute the contribution from the Hall term and the MHD term to the energy fl…
On the deviation from Maxwellian of the ion velocity distribution functions in the turbulent magnetosheath
Silvia Perri, D. Perrone, E. Yordanova +20
The degree of deviation from the thermodynamic equilibrium in the ion velocity distribution functions (VDFs), measured by the Magnetospheric Multiscale (MMS) mission in the Earth's…