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Generation of Turbulence in Colliding Reconnection Jets
ArticleAbstract: The collision of magnetic reconnection jets is studied by means of a three-dimensional numerical simPalabras claves:magnetic reconnection, methods: numerical, TurbulenceAutores:Chasapis A., Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Matthaeus W.H., Newman D.L., Olshevsky V., Pucci F., Servidio S.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:googlescopusSign singularity and flares in solar active region NOAA 11158
ArticleAbstract: Solar Active Region NOAA 11158 has hosted a number of strong flares, including one X2.2 event. The cPalabras claves:Sun: flares, Sun: magnetic fields, turbulence Supporting material: animationAutores:Carbone V., De Vita G., Fisher G.H., Kazachenko M.D., Krucker S., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A., Welsch B.T.Fuentes:scopusREVISITING 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: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:scopusProton-Proton Collisions in the Turbulent Solar Wind: Hybrid Boltzmann-Maxwell Simulations
ArticleAbstract: The mechanism of heating for hot, dilute, and turbulent plasmas represents a long-standing problem iPalabras claves:Autores:Luca Sorriso-Valvo, Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P.Fuentes:scopus