Mostrando 10 resultados de: 19
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scopus(19)
A possible truncated-Lévy-flight statistics recovered from interplanetary solar-wind velocity and magnetic-field fluctuations
ArticleAbstract: Interplanetary solar-wind fluctuations have been studied in the inner heliosphere and within the MHDPalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusCoordinated study on solar wind turbulence during the venus-express, ACE and ulysses alignment of August 2007
Conference ObjectAbstract: At the end of August 2007, Venus, Earth and Ulysses were aligned within a few degrees. This unusualPalabras claves:MHD turbulence, solar wind, Space plasma physicsAutores:Baumjohann W., Bavassano B., Biernat H., Bruno R., Carbone V., Cattaneo M.B., D’Amicis R., Jankovičová D., Kovács P., Luca Sorriso-Valvo, Milillo A., Mura A., Orsini S., Rucker H., Veltri P., Vörös Z., Zhang T.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 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 probability distribution function of small-scale interplanetary magnetic field fluctuations
ArticleAbstract: In spite of a large number of papers dedicated to the study of MHD turbulence in the solar wind therPalabras claves:Interplanetary physics (interplanetary magnetic fields), Space plasma physics (waves and instabilities)Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Malara F., Primavera L., Veltri P.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:scopusOn the role of coherent and stochastic fluctuations in the evolving solar wind MHD turbulence: Intermittency
Conference ObjectAbstract: One of the most interesting findings about solar wind turbulence is the intermittent character of itPalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopus