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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:scopusIntermittency in space plasma turbulence
Book PartAbstract: This chapter provides an overview on theoretical aspects and observational findings about intermittePalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Pietropaolo E.Fuentes:scopusSome aspects of waiting time statistics of interplanetary magnetic field fluctuations: Focusing on B<inf>S</inf>
Conference ObjectAbstract: Statistics associated with fluctuations of solar wind parameters shows a remarkable dependence on thPalabras claves:Alfvénic fluctuations, Coherent structures, Waiting time statisticsAutores: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: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: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:scopusObservations of magnetohydrodynamic turbulence in the 3D heliosphere
Conference ObjectAbstract: The solar wind is a high Reynolds' number plasma flow of solar origin that permeates the whole helioPalabras claves:Interplanetary space, Solar wind fields, Solar wind plasma, Waves and discontinuitiesAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusObservations of turbulence and anomalous scaling in the solar wind
ArticleAbstract: In situ observations collected in the past decades, at different heliocentric distances and coveringPalabras claves:MHD turbulence, scaling, solar windAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Noullez A., Raffaele Marino, Salem C.Fuentes:scopusObserving small scale Alfvénic turbulence around 0.2 AU
Conference ObjectAbstract: Recent results obtained from the analysis of interplanetary observations recorded by Helios 2 withinPalabras claves:Interplanetary space, MHD turbulence, solar windAutores:Bavassano B., Bruno R., Carbone V., Cattaneo M.B., D’Amicis R., Luca Sorriso-Valvo, Pietropaolo E.Fuentes:scopusOn the radial evolution of alfvénic turbulence in the solar wind
Conference ObjectAbstract: The observations at different solar distances and latitudes, collected in the past three decades, anPalabras claves:nonlinear dynamics, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Pietropaolo E.Fuentes:scopus