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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: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:googlescopusEnergetic 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: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:googlescopus