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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:scopusRadial evolution of the intermittency of density fluctuations in the fast solar wind
ArticleAbstract: We study the radial evolution of the intermittency of density fluctuations in the fast solar wind. TPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, WavesAutores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Malara F., Pietropaolo E., Primavera L., Telloni D., Veltri P.Fuentes:scopus