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Comparing 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:scopusHeating the solar wind by a magnetohydrodynamic turbulent energy cascade
ArticleAbstract: Solar wind plasma is known to cool down more slowly while it is blown away from the Sun than expectePalabras claves:MHD, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes: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:scopusObserving Mesospheric Turbulence With Specular Meteor Radars: A Novel Method for Estimating Second-Order Statistics of Wind Velocity
ArticleAbstract: There are few observational techniques for measuring the distribution of kinetic energy within the mPalabras claves:Correlation function, Mesosphere, Structure function, Turbulence, WindAutores:Avsarkisov V., Charuvil H., Chau J.L., Clahsen M., Raffaele Marino, Urco J.M., Vierinen J., Volz R.Fuentes:scopusOn the Statistical Properties of Turbulent Energy Transfer Rate in the Inner Heliosphere
ArticleAbstract: The transfer of energy from large to small scales in solar wind turbulence is an important ingbkp_rePalabras claves:Intermittency, solar wind, TurbulenceAutores:Bruno R., Carbone F., Greco A., Luca Sorriso-Valvo, Perri S., Raffaele MarinoFuentes:scopusScaling laws for the energy transfer in space plasma turbulence
ReviewAbstract: One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-linear tranPalabras claves:Energy transfer, Heliosphere, magnetohydrodynamics, Scaling laws, solar wind, Space plasmas, Sun, Turbulence, WavesAutores:Luca Sorriso-Valvo, Raffaele MarinoFuentes:scopusSELF-CONSISTENT CASTAING DISTRIBUTION OF SOLAR WIND TURBULENT FLUCTUATIONS
ArticleAbstract: The intermittent behavior of solar wind turbulent fluctuations has often been investigated through tPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Carbone V., Lijoi L., Luca Sorriso-Valvo, Perri S., Raffaele MarinoFuentes:scopusSudden depletion of Alfvénic turbulence in the rarefaction region of corotating solar wind high-speed streams at 1 AU: Possible solar origin?
ArticleAbstract: A canonical description of a corotating solar wind high-speed stream in terms of velocity profile woPalabras claves:magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: magnetic fields, TurbulenceAutores:Bruno R., Carnevale G., Pietropaolo E., Raffaele Marino, Raines J.M.Fuentes:scopusThe energy cascade in solar wind MHD turbulence
Conference ObjectAbstract: Direct evidence for the presence of an inertial energy cascade, the most characteristic signature ofPalabras claves:magnetohydrodynamics, solar wind, TurbulenceAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusThe low-frequency break observed in the slow solar wind magnetic spectra
ArticleAbstract: Fluctuations of solar wind magnetic field and plasma parameters exhibit a typical turbulence power sPalabras claves:Magnetic fields, plasmas, solar wind, Sun: heliosphere, Turbulence, WavesAutores:Bruno R., De Marco R., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Telloni D.Fuentes:scopus