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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:scopusComparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause
ArticleAbstract: The properties of turbulence observed within the plasma originating from the magnetosheath and the mPalabras claves:MHD, plasmas, solar wind, TurbulenceAutores:Christian L. Vásconez, Federico Fraternale, Luca Sorriso-Valvo, Paulina Quijia, Perri S., Raffaele Marino, Stawarz J.E., 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: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: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:scopusDensity fluctuations associated with turbulence and waves: First observations by Solar Orbiter
ArticleAbstract: Aims. The aim of this work is to demonstrate that the probe-to-spacecraft potential measured by RPWPalabras claves:solar wind, Turbulence, WavesAutores:Angelini V., Bale S.D., Chust T., Edberg N.J.T., Eriksson A.I., Evans V., Graham D.B., Horbury T.S., Johansson E.P.G., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Lorfèvre E., Luca Sorriso-Valvo, Maksimovic M., O'brien H., Plettemeier D., Souček J., Steinvall K., Steller M., Štverák , Trávníček P., Vaivads A., Vecchio A.Fuentes:scopusEditorial: Advances in Space Plasma Turbulence: Theory and Observations
OtherAbstract:Palabras claves:dissipation processes, in situ observations, magnetic reconnection, Numerical simulations, plasma turbulenceAutores:Hellinger P., Luca Sorriso-Valvo, Perri S., Tenerani A.Fuentes:scopusEditorial: New challenges in space plasma physics: Open questions and future mission concepts
OtherAbstract:Palabras claves:dissipation processes, in situ observations, magnetic reconnection, Numerical simulations, plasma turbulence, space physicsAutores:Chen C.H.K., Luca Sorriso-Valvo, Retinò A., Verscharen D.Fuentes:scopusHelios 2 observations of solar wind turbulence decay in the inner heliosphere
ArticleAbstract: Aims. A linear scaling of the mixed third-order moment of the magnetohydrodynamic (MHD) fluctuationsPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Bruno R., D,Aamicis R., Foldes R., Lévêque E., Luca Sorriso-Valvo, Raffaele Marino, Telloni D., Yordanova E.Fuentes:scopus