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scopus(18)
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: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: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: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:scopusIntermittency in the solar wind turbulence through probability distribution functions of fluctuations
ArticleAbstract: Intermittency in fluid turbulence can be emphasized through the analysis of Probability DistributionPalabras claves:Autores:Bruno R., Carbone V., Consolini G., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusPersistence of small-scale anisotropy of magnetic turbulence as observed in the solar wind
ArticleAbstract: The anisotropy of magnetohydrodynamic turbulence is investigated by using solar wind data from the HPalabras claves:Autores:Bruno R., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusUnified scaling law for waiting times between seismic events
ArticleAbstract: The statistical properties of seismic time series, including both sequences of aftershocks, and pattPalabras claves:Autores:Carbone V., Guerra I., Harabaglia P., Luca Sorriso-ValvoFuentes: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:scopus