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Compressive turbulent cascade and heating in the solar wind
Conference ObjectAbstract: A turbulent energy cascade has been recently identified in high-latitude solar wind data samples byPalabras claves:MHD turbulence, scaling, solar windAutores:Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusCancellations and structures in the solar photosphere: Signature of flares
Conference ObjectAbstract: The topological properties of the typical current structures in a turbulent magnetohydrodynamic flowPalabras claves:Autores:Abramenko V., Carbone V., Luca Sorriso-Valvo, Noullez A., Politano H., Pouquet A., Veltri P., Yurchyshyn V.Fuentes:scopusHeating 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: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:scopusIntermittent character of interplanetary magnetic field fluctuations
ArticleAbstract: Interplanetary magnetic field magnitude fluctuations are notoriously more intermittent than velocityPalabras claves:Autores:Bruno R., Carbone V., Chapman S., Hnat B., Luca Sorriso-Valvo, Noullez A.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:scopusRecent insights in solar wind MHD turbulence
Conference ObjectAbstract: In this short review we report about recent findings related to two fundamental points in the studyPalabras claves:MHD turbulence, scaling, solar windAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Noullez A., Pietropaolo E., Raffaele MarinoFuentes:scopusSorriso-Valvo et al. Reply:
ArticleAbstract: A Reply to the Comment by M.A. Forman, C.W. Smith, and B.J. Vasquez. © 2010 The American Physical SoPalabras claves:Autores:Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele Marino, Veltri P.Fuentes: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