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scopus(6)
Chaotic advection and particle pairs diffusion in a low-dimensional truncation of two-dimensional magnetohydrodynamics
ArticleAbstract: The chaotic advection of fluid particle pairs is investigated though a low-order model of two-dimensPalabras claves:Autores:Carbone F., Luca Sorriso-Valvo, Telloni D., Zank G.P.Fuentes:scopusDoes Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?
ArticleAbstract: Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries ofPalabras claves:Autores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Carbone F., De Leo Y., Deppo V.D., D’Amicis R., Fineschi S., Giordano S., Grimani C., Heinzel P., Jerse G., Landini F., Liberatore A., Luca Sorriso-Valvo, Moses J.D., Naletto G., Nicolini G., Pancrazzi M., Perrone D., Raffaele Marino, Romoli M., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Verscharen D., Zank G.P., Zhao L.L., Zimbardo G.Fuentes:scopusLocal dimensionality and inverse persistence analysis of atmospheric turbulence in the stable boundary layer
ArticleAbstract: The dynamics across different scales in the stable atmospheric boundary layer has been investigatedPalabras claves:Autores:Alberti T., Carbone F., Consolini G., Faranda D., Luca Sorriso-Valvo, Telloni D.Fuentes:scopusIon Cyclotron Waves in Field-aligned Solar Wind Turbulence
ArticleAbstract: The nature of the solar wind parallel fluctuations is investigated in this Letter by using magneticPalabras claves:Autores:Bruno R., Carbone F., Luca Sorriso-Valvo, Mancuso S., Telloni D., Zank G.P.Fuentes:scopusTransition to turbulence in a five-mode Galerkin truncation of two-dimensional magnetohydrodynamics
ArticleAbstract: The chaotic dynamics of a low-order Galerkin truncation of the two-dimensional magnetohydrodynamic sPalabras claves:Autores:Carbone F., Luca Sorriso-Valvo, Telloni D., Zank G.P.Fuentes:scopusThe low-frequency break observed in the slow solar wind magnetic spectra
ArticleAbstract: Fluctuations of solar wind magnetic field and plasma parameters exhibit a typical turbulence power sPalabras claves:Magnetic fields, plasmas, solar wind, Sun: heliosphere, Turbulence, WavesAutores:Bruno R., De Marco R., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Telloni D.Fuentes:scopus