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Electron 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: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:googlescopusRadial evolution of the intermittency of density fluctuations in the fast solar wind
ArticleAbstract: We study the radial evolution of the intermittency of density fluctuations in the fast solar wind. TPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, WavesAutores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Malara F., Pietropaolo E., Primavera L., Telloni D., Veltri P.Fuentes:scopusProperties 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