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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:scopusCompressive turbulent cascade and heating in the solar wind
Conference ObjectAbstract: A turbulent energy cascade has been recently identified in high-latitude solar wind data samples byPalabras claves:MHD turbulence, scaling, solar windAutores:Bruno R., Carbone V., Luca Sorriso-Valvo, Noullez A., Raffaele MarinoFuentes:scopusBuilding up Solar-wind-like 3D Uniform-intensity Magnetic Fields
ArticleAbstract: A numerical model representing a 3D turbulent constant-magnitude magnetic field B is described. AssuPalabras claves:Magnetic fields, solar wind, TurbulenceAutores:Bruno R., Luca Sorriso-Valvo, Malara F., Primavera L., Valentini F.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: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:scopusDissipation measures in weakly collisional plasmas
ArticleAbstract: The physical foundations of the dissipation of energy and the associated heating in weakly collisionPalabras claves:magnetic reconnection, plasmas, solar wind, TurbulenceAutores:Cassak P.A., Christian L. Vásconez, Juno J.L., Liang H., Luca Sorriso-Valvo, Matthaeus W.H., Perrone D., Pezzi O., Roytershteyn V., Servidio S., TenBarge J.M.Fuentes:googlescopusDifferential kinetic dynamics and heating of ions in the turbulent solar wind
ArticleAbstract: The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solarPalabras claves:plasma heating, solar wind, space missions, TurbulenceAutores:Brienza D., Bruno R., Consolini G., de Keyser J., De Marco R., Lavraud B., Luca Sorriso-Valvo, Marcucci M.F., Perrone D., Pezzi O., Retinò A., Salatti M., Servidio S., Stabile S., Vaivads A., Valentini F., Veltri P.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:scopus