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Article(4)
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Astronomy and Astrophysics(1)
Astrophysical Journal(1)
Astrophysical Journal Letters(1)
New Journal of Physics(1)
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:scopusElectron 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: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:scopusTransition to kinetic turbulence at proton scales driven by large-amplitude kinetic Alfvén fluctuations
ArticleAbstract: Space plasmas are dominated by the presence of large-amplitude waves, large-scale inhomogeneities, kPalabras claves:Interplanetary medium, plasmas, Turbulence, WavesAutores:Christian L. Vásconez, Malara F., Pezzi O., Pucci F., Servidio S., Valentini F.Fuentes:googlescopus