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Cancellation 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:scopusKINETIC ALFVÉN WAVE GENERATION by LARGE-SCALE PHASE MIXING
ArticleAbstract: One view of the solar wind turbulence is that the observed highly anisotropic fluctuations at spatiaPalabras claves:lasmas, solar wind, Sun: corona, WavesAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Pucci F., Servidio S., Valentini F.Fuentes:googlescopusTwo-fluid numerical simulations of turbulence inside Kelvin-Helmholtz vortices: Intermittency and reconnecting current sheets
ArticleAbstract: The turbulence developing inside Kelvin-Helmholtz vortices has been studied using a two-fluid numeriPalabras claves:Autores:Califano F., Chasapis A., Henri P., Luca Sorriso-Valvo, Retinò A., Rezeau L., Rossi C., Servidio S., Valentini F.Fuentes: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:scopus