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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 and coherent structures in the solar wind
ArticleAbstract: The interplanetary medium is characterized by a very high Reynolds number and is pervaded by fluctuaPalabras claves:Interplanetary magnetic fields, Interplanetary physics, Space plasma physics, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-ValvoFuentes: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:scopus