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Building up Solar-wind-like 3D Uniform-intensity Magnetic Fields
ArticleAbstract: A numerical model representing a 3D turbulent constant-magnitude magnetic field B is described. AssuPalabras claves:Magnetic fields, solar wind, TurbulenceAutores:Bruno R., Luca Sorriso-Valvo, Malara F., Primavera L., Valentini F.Fuentes:scopusDifferential kinetic dynamics and heating of ions in the turbulent solar wind
ArticleAbstract: The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solarPalabras claves:plasma heating, solar wind, space missions, TurbulenceAutores:Brienza D., Bruno R., Consolini G., de Keyser J., De Marco R., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Perrone D., Pezzi O., Retinò A., Salatti M., Servidio S., Stabile S., Vaivads A., Valentini F., Veltri P.Fuentes:scopusElectron Heating by Kinetic Alfvén Waves in Coronal Loop Turbulence
ArticleAbstract: A test-particle model describing the energization of electrons in a turbulent plasma is presented. PPalabras claves:acceleration of particles, Sun: corona, Turbulence, WavesAutores:Luca Sorriso-Valvo, Malara F., Nigro G., Valentini F.Fuentes:scopusKINETIC ALFVÉN WAVE GENERATION by LARGE-SCALE PHASE MIXING
ArticleAbstract: One view of the solar wind turbulence is that the observed highly anisotropic fluctuations at spatiaPalabras claves:lasmas, solar wind, Sun: corona, WavesAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusTransition to kinetic turbulence at proton scales driven by large-amplitude kinetic Alfvén fluctuations
ArticleAbstract: Space plasmas are dominated by the presence of large-amplitude waves, large-scale inhomogeneities, kPalabras claves:Interplanetary medium, plasmas, Turbulence, WavesAutores:Christian L. Vásconez, Malara F., Pezzi O., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusTwo-fluid numerical simulations of turbulence inside Kelvin-Helmholtz vortices: Intermittency and reconnecting current sheets
ArticleAbstract: The turbulence developing inside Kelvin-Helmholtz vortices has been studied using a two-fluid numeriPalabras claves:Autores:Califano F., Chasapis A., Henri P., Luca Sorriso-Valvo, Retinò A., Rezeau L., Rossi C., Servidio S., Valentini F.Fuentes:scopusVlasov simulations of kinetic Alfvén waves at proton kinetic scales
ArticleAbstract: Kinetic Alfvén waves represent an important subject in space plasma physics, since they are thoughtPalabras claves:Autores:Camporeale E., Christian L. Vásconez, Valentini F., Veltri P.Fuentes:googlescopusREVISITING A CLASSIC: The PARKER-MOFFATT PROBLEM
ArticleAbstract: The interaction of two colliding Alfvén wave packets is described here by means of magnetohydrodynamPalabras claves:magnetohydrodynamics (MHD), plasmas, solar windAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusLocal and global properties of energy transfer in models of plasma turbulence
ArticleAbstract: The nature of the turbulent energy transfer rate is studied using direct numerical simulations of wePalabras claves:plasma nonlinear phenomena, Plasma Simulation, Space plasma physicsAutores:Christian L. Vásconez, Laveder D., Luca Sorriso-Valvo, Mininni P.D., Perrone D., Raffaele Marino, Servidio S., Valentini F.Fuentes:scopusLocal energy transfer rate and kinetic processes: The fate of turbulent energy in two-dimensional hybrid Vlasov-Maxwell numerical simulations
ArticleAbstract: The nature of the cross-scale connections between the inertial-range turbulent energy cascade and thPalabras claves:plasma nonlinear phenomena, Plasma Simulation, Space plasma physicsAutores:Luca Sorriso-Valvo, Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P., Zouganelis I.Fuentes:scopus