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Clustering of polarity reversals of the geomagnetic field
ArticleAbstract: Often in nature the temporal distribution of inhomogeneous stochastic point processes can be modeledPalabras claves:Autores:Carbone V., Guerra I., Harabaglia P., Lepreti F., Luca Sorriso-Valvo, Vecchio A., Veltri P.Fuentes:scopusA possible link between turbulence and plasma heating
ArticleAbstract: Numerical simulations and experimental results have shown that the formation of current sheets in spPalabras claves:Autores:Dimmock A.P., Kilpua E., Luca Sorriso-Valvo, Vörös Z., Yordanova E.Fuentes: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:scopusArbitrary-order Hilbert Spectral Analysis and Intermittency in Solar Wind Density Fluctuations
ArticleAbstract: The properties of inertial- and kinetic-range solar wind turbulence have been investigated with thePalabras claves:plasmas, solar wind, TurbulenceAutores:Alberti T., Carbone F., Chen C.H.K., Lepreti F., Luca Sorriso-Valvo, Nemecek Z., Šafránková J.Fuentes:scopusEnergetic particle transport in the presence of magnetic turbulence: Influence of spectral extension and intermittency
ArticleAbstract: The transport of energetic particles in the presence of magnetic turbulence is an important but unsoPalabras claves:diffusion, Magnetic fields, methods: numerical, solar windAutores:Luca Sorriso-Valvo, Malara F., Perri S., Pucci F., Valentini F., Zimbardo G.Fuentes:scopusEvolution of turbulence in the Kelvin–Helmholtz instability in the terrestrial magnetopause
ArticleAbstract: The dynamics occurring at the terrestrial magnetopause are investigated by using Geotail and THEMISPalabras claves:Intermittency, Kelvin–Helmholtz instability, Magnetosheath, TurbulenceAutores:Di Mare F., Hasegawa H., Luca Sorriso-Valvo, Malara F., Retinò A.Fuentes:scopusNon-gaussian probability distribution functions in two-dimensional magnetohydrodynamic turbulence
ArticleAbstract: Intermittency in MHD turbulence has been analyzed using high-resolution 2D numerical simulations. WePalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Politano H., Pouquet A., Veltri P.Fuentes:scopusNonlinear waves and instabilities leading to secondary reconnection in reconnection outflows
ArticleAbstract: Reconnection outflows have been under intense recent scrutiny, from in situ observations and from siPalabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Goldman M.V., Lapenta G., Luca Sorriso-Valvo, Newman D.L., Olshevsky V., Pucci F., Servidio S.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:scopusMagnetic turbulence in space plasmas: Scale-dependent effects of anisotropy
ArticleAbstract: The presence of a background magnetic field induces anisotropy in magnetic turbulence. UnderstandingPalabras claves:Autores:André M., Bruno R., Carbone V., Luca Sorriso-Valvo, Perri S., Veltri P., Yordanova E.Fuentes:scopus