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Cancellation analysis of current density in solar active region NOAA10019
ArticleAbstract: Solar flares are often associated with changes in the fine magnetic structure of the emitting activePalabras claves:Active regions, Photosphere, Solar flaresAutores:Briand C., Carbone V., De Vita G., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A.Fuentes:scopusDissipation measures in weakly collisional plasmas
ArticleAbstract: The physical foundations of the dissipation of energy and the associated heating in weakly collisionPalabras claves:magnetic reconnection, plasmas, solar wind, TurbulenceAutores:Cassak P.A., Christian L. Vásconez, Juno J.L., Liang H., Luca Sorriso-Valvo, Matthaeus W.H., Perrone D., Pezzi O., Roytershteyn V., Servidio S., TenBarge J.M.Fuentes:googlescopusDifferential 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: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: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: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:scopusNonlinear waves and instabilities leading to secondary reconnection in reconnection outflows
ArticleAbstract: Reconnection outflows have been under intense recent scrutiny, from in situ observations and from siPalabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Newman D.L., Olshevsky V., Pucci F., Servidio S.Fuentes:scopusSign 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:scopus