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Coherent Structures and Spectral Energy Transfer in Turbulent Plasma: A Space-Filter Approach
ArticleAbstract: Plasma turbulence at scales of the order of the ion inertial length is mediated by several mechanismPalabras claves:Autores:Califano F., Camporeale E., Luca Sorriso-Valvo, Retinò 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:scopusFast algorithm for a three-dimensional synthetic model of intermittent turbulence
ArticleAbstract: Synthetic turbulence models are useful tools that provide realistic representations of turbulence, nPalabras claves:Autores:Di Mare F., Luca Sorriso-Valvo, Malara F., Nigro G.Fuentes:scopusErratum: Comparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stab319)
OtherAbstract: The original version of this manuscript included some portions of text from the first submitted versPalabras claves:Autores:Christian L. Vásconez, Federico Fraternale, Luca Sorriso-Valvo, Paulina Quijia, Perri S., Raffaele Marino, Stawarz J.E., Yordanova E.Fuentes:scopusIntermittency in space plasma turbulence
Book PartAbstract: This chapter provides an overview on theoretical aspects and observational findings about intermittePalabras claves:Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Pietropaolo 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:scopusSmall-scale energy cascade of the solar wind turbulence
ArticleAbstract: Magnetic fluctuations in the solar wind are distributed according to Kolmogorov's power law f_5/3 bePalabras claves:MHD, solar wind, TurbulenceAutores:Alexandrova O., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopusSolar wind turbulence and the role of ion instabilities
ReviewAbstract: Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In additionPalabras claves:Ion instabilities, Kinetic scales, plasma turbulence, solar windAutores:Alexandrova O., Bale S.D., Chen C.H.K., Horbury T.S., Luca Sorriso-ValvoFuentes:scopusStatistical properties of dissipation bursts within turbulence: Solar flares and geomagnetic activity
Conference ObjectAbstract: We investigate some statistical properties of the solar soft X-ray flux and of the Auroral ElectrojePalabras claves:Geomagnetic activity, MHD turbulence, Solar flaresAutores:Carbone V., Giuliani P., Lepreti F., Luca Sorriso-Valvo, 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:scopus