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A simple model for the solar cycle
ArticleAbstract: A simple nonlinear model which describes the 11 -year solar cycle can be derived from the usual α -Palabras claves:Autores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Pontieri A., Vecchio A.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:scopusCancellation analysis of current density in solar active region NOAA10019
ArticleAbstract: Solar flares are often associated with changes in the fine magnetic structure of the emitting activePalabras claves:Active regions, Photosphere, Solar flaresAutores:Briand C., Carbone V., De Vita G., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A.Fuentes: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:scopusErratum: On the occurrence of the third-order scaling in high-latitude solar wind (Astrophysical Journal (2012) 750 (41))
OtherAbstract:Palabras claves:Autores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Veltri P.Fuentes:scopusMultipoint observation of anisotropy and intermittency in solar-wind turbulence
ArticleAbstract: Using high-resolution magnetic-field Cluster observations, we have investigated the magnetic-field aPalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Perri S., Yordanova E.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:scopusOn the origin of the strong intermittent nature of interplanetary magnetic field
Conference ObjectAbstract: We briefly discuss the strong intermittent nature of the interplanetary magnetic field, observing thPalabras claves:Interplanetary magnetic field, TurbulenceAutores:Bruno R., Carbone V., Luca Sorriso-ValvoFuentes: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 scaling properties of anisotropy of interplanetary magnetic turbulent fluctuations
ArticleAbstract: The anisotropic character of interplanetary magnetic-field turbulence has been studied through the aPalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Yordanova E.Fuentes:scopus