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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: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:scopusPOD analysis of photospheric velocity field: Solar oscillations and granulation
Conference ObjectAbstract: The spatio-temporal dynamics of the solar photosphere is studied by performing a Proper Orthogonal DPalabras claves:Autores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Straus T., Vecchio A., Veltri P.Fuentes:scopusScaling laws and coherent structures in the solar wind
ArticleAbstract: The interplanetary medium is characterized by a very high Reynolds number and is pervaded by fluctuaPalabras claves:Interplanetary magnetic fields, Interplanetary physics, Space plasma physics, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., D’Amicis R., Luca Sorriso-ValvoFuentes:scopusSign singularity and flares in solar active region NOAA 11158
ArticleAbstract: Solar Active Region NOAA 11158 has hosted a number of strong flares, including one X2.2 event. The cPalabras claves:Sun: flares, Sun: magnetic fields, turbulence Supporting material: animationAutores:Carbone V., De Vita G., Fisher G.H., Kazachenko M.D., Krucker S., Lepreti F., Luca Sorriso-Valvo, Primavera L., Servidio S., Vecchio A., Welsch B.T.Fuentes:scopusRadial evolution of solar wind intermittency in the inner heliosphere
ArticleAbstract: We analyzed intermittency in the solar wind, as observed on the ecliptic plane, looking at magneticPalabras claves:Coherent structures, Intermittency, Interplanetary fluctuations, Stochastic F1Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopus