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Astrophysical Journal(2)
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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: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:scopusEvolution of turbulence in the Kelvin–Helmholtz instability in the terrestrial magnetopause
ArticleAbstract: The dynamics occurring at the terrestrial magnetopause are investigated by using Geotail and THEMISPalabras claves:Intermittency, Kelvin–Helmholtz instability, Magnetosheath, TurbulenceAutores:Di Mare F., Hasegawa H., Luca Sorriso-Valvo, Malara F., Retinò A.Fuentes:scopusTransition 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:googlescopusProperties of Turbulence in the Reconnection Exhaust: Numerical Simulations Compared with Observations
ArticleAbstract: The properties of the turbulence that develops in the outflows of magnetic reconnection have been inPalabras claves:magnetic reconnection, methods: numerical, TurbulenceAutores:Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Malara F., Matthaeus W.H., Newman D.L., Olshevsky V., Pucci F., Servidio S.Fuentes:scopus