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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:scopusOne-point statistics and intermittency of induced electric field in the solar wind
ArticleAbstract: The interplanetary induced electric field e = v × b is studied, using solar-wind time series. The prPalabras claves:Autores:Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusIntermittency in the solar wind turbulence through probability distribution functions of fluctuations
ArticleAbstract: Intermittency in fluid turbulence can be emphasized through the analysis of Probability DistributionPalabras claves:Autores:Bruno R., Carbone V., Consolini G., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusPhase-synchronization, energy cascade, and intermittency in solar-wind turbulence
ArticleAbstract: The energy cascade in solar wind magnetic turbulence is investigated using MESSENGER data in the innPalabras claves:Autores:Bruno R., Carbone V., Korth H., Luca Sorriso-Valvo, Perri S., Vecchio A., Zurbuchen T.H.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:scopusScaling laws in plasma turbulence
ReviewAbstract:Palabras claves:Autores:Antoni V., Bruno R., Carbone V., Lepreti F., Luca Sorriso-Valvo, 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