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Colliding Alfvénic wave packets in magnetohydrodynamics, Hall and kinetic simulations
ArticleAbstract: The analysis of the Parker-Moffatt problem, recently revisited in Pezzi et al. (Astrophys. J., vol.Palabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusBuilding 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:scopusAnalysis of cancellation exponents in two-dimensional vlasov turbulence
ArticleAbstract: Statistical properties of plasma turbulence are investigated by means of two-dimensional Vlasov simuPalabras claves:Autores:Carbone V., De Vita G., Luca Sorriso-Valvo, Primavera L., Servidio S., Valentini F., Veltri P.Fuentes:scopusA New Journey Around (and Around) the Sun
ArticleAbstract:Palabras claves:Autores:Raffaele Marino, Telloni D., Valentini F.Fuentes:scopusFrom Alfvén waves to kinetic Alfvén waves in an inhomogeneous equilibrium structure
ArticleAbstract: Kinetic Alfvén waves are believed to primary form fluctuations in a hydromagnetic turbulence at scalPalabras claves:Alfvén waves, Hall MHD, kinetic Alfvén waves, kinetic plasma simulations, solar coronaAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Pezzi O., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusElectron 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:scopusEnergetic particle transport in the presence of magnetic turbulence: Influence of spectral extension and intermittency
ArticleAbstract: The transport of energetic particles in the presence of magnetic turbulence is an important but unsoPalabras claves:diffusion, Magnetic fields, methods: numerical, solar windAutores:Luca Sorriso-Valvo, Malara F., Perri S., Pucci F., Valentini F., Zimbardo G.Fuentes:scopusErratum: Multifractal scaling and intermittency in hybrid Vlasov-Maxwell simulations of plasma turbulence (Physics of Plasmas (2016) 23 (022307))
OtherAbstract:Palabras claves:Autores:Carbone F., Leonardis E., Luca Sorriso-Valvo, Servidio S., Valentini F., Veltri P.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:scopusNature of Electrostatic Fluctuations in the Terrestrial Magnetosheath
ArticleAbstract: The high cadence plasma, electric, and magnetic field measurements by the Magnetospheric MultiScalePalabras claves:Autores:Luca Sorriso-Valvo, Perri S., Perrone D., Roberts O.W., Settino A., Valentini F., Veltri P., Yordanova E.Fuentes:scopus