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Heating 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:scopusClustering of polarity reversals of the geomagnetic field
ArticleAbstract: Often in nature the temporal distribution of inhomogeneous stochastic point processes can be modeledPalabras claves:Autores:Carbone V., Guerra I., Harabaglia P., Lepreti F., Luca Sorriso-Valvo, Vecchio A., Veltri P.Fuentes:scopusCancellation properties in Hall magnetohydrodynamics with a strong guide magnetic field
ArticleAbstract: We present a signed measure analysis of compressible Hall magnetohydrodynamic turbulence with an extPalabras claves:Autores:Carbone V., De Vita G., Dmitruk P., Luca Sorriso-Valvo, Martin L.N., Nigro G., Primavera L.Fuentes:scopusIntermittency and turbulence in a magnetically confined fusion plasma
ArticleAbstract: The intermittency of the magnetic turbulence in reversed field pinch plasmas was measured. The probaPalabras claves:Autores:Antoni V., Carbone V., Luca Sorriso-Valvo, Martines E., Veltri P.Fuentes:scopusIntermittency of magnetic turbulence in slow solar wind
Conference ObjectAbstract: We investigate the properties of intermittency of magnetic turbulence by using magnetic field data cPalabras claves:Isotropic turbulence, MagnetohydrodynamicAutores:Bruno R., Carbone V., Lepreti F., Luca Sorriso-ValvoFuentes:scopusIntermittent character of interplanetary magnetic field fluctuations
ArticleAbstract: Interplanetary magnetic field magnitude fluctuations are notoriously more intermittent than velocityPalabras claves:Autores:Bruno R., Carbone V., Chapman S., Hnat B., Luca Sorriso-Valvo, Noullez A.Fuentes:scopusMagnetic turbulence in space plasmas: Scale-dependent effects of anisotropy
ArticleAbstract: The presence of a background magnetic field induces anisotropy in magnetic turbulence. UnderstandingPalabras claves:Autores:André M., Bruno R., Carbone V., Luca Sorriso-Valvo, Perri S., Veltri P., Yordanova E.Fuentes:scopusObservations of magnetohydrodynamic turbulence in the 3D heliosphere
Conference ObjectAbstract: The solar wind is a high Reynolds' number plasma flow of solar origin that permeates the whole helioPalabras claves:Interplanetary space, Solar wind fields, Solar wind plasma, Waves and discontinuitiesAutores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusOn the origin of the strong intermittent nature of interplanetary magnetic field
Conference ObjectAbstract: We briefly discuss the strong intermittent nature of the interplanetary magnetic field, observing thPalabras claves:Interplanetary magnetic field, TurbulenceAutores:Bruno R., Carbone V., Luca Sorriso-ValvoFuentes:scopusOn the probability distribution function of small-scale interplanetary magnetic field fluctuations
ArticleAbstract: In spite of a large number of papers dedicated to the study of MHD turbulence in the solar wind therPalabras claves:Interplanetary physics (interplanetary magnetic fields), Space plasma physics (waves and instabilities)Autores:Bavassano B., Bruno R., Carbone V., Luca Sorriso-Valvo, Malara F., Primavera L., Veltri P.Fuentes:scopus