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Heating the solar wind by a magnetohydrodynamic turbulent energy cascade
ArticleAbstract: Solar wind plasma is known to cool down more slowly while it is blown away from the Sun than expectePalabras claves:MHD, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusObservation of inertial energy cascade in interplanetary space plasma
ArticleAbstract: Direct evidence for the presence of an inertial energy cascade, the most characteristic signature ofPalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Lepreti F., Luca Sorriso-Valvo, Noullez A., Pietropaolo E., Raffaele Marino, Veltri P.Fuentes:scopusScaling laws of turbulence and heating of fast solar wind: The role of density fluctuations
ArticleAbstract: Incompressible and isotropic magnetohydrodynamic turbulence in plasmas can be described by an exactPalabras claves:Autores:Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusThe energy cascade in solar wind MHD turbulence
Conference ObjectAbstract: Direct evidence for the presence of an inertial energy cascade, the most characteristic signature ofPalabras claves:magnetohydrodynamics, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusThe magnetohydrodynamic turbulent cascade in the ecliptic solar wind: Study of Ulysses data
ArticleAbstract: The occurrence of a nonlinear turbulent energy cascade in solar wind plasma has been recently establPalabras claves:magnetohydrodynamics, solar wind, TurbulenceAutores:Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele Marino, Veltri P.Fuentes:scopus