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Clustering 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:scopusColliding Alfvénic wave packets in magnetohydrodynamics, Hall and kinetic simulations
ArticleAbstract: The analysis of the Parker-Moffatt problem, recently revisited in Pezzi et al. (Astrophys. J., vol.Palabras claves:Astrophysical Plasmas, Plasma Simulation, Space plasma physicsAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusNature of Electrostatic Fluctuations in the Terrestrial Magnetosheath
ArticleAbstract: The high cadence plasma, electric, and magnetic field measurements by the Magnetospheric MultiScalePalabras claves:Autores:Luca Sorriso-Valvo, Perri S., Perrone D., Roberts O.W., Settino A., Valentini F., Veltri P., Yordanova E.Fuentes:scopusNon-gaussian probability distribution functions in two-dimensional magnetohydrodynamic turbulence
ArticleAbstract: Intermittency in MHD turbulence has been analyzed using high-resolution 2D numerical simulations. WePalabras claves:Autores:Carbone V., Luca Sorriso-Valvo, Politano H., Pouquet A., Veltri P.Fuentes: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: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:scopusTurbulence-Driven Ion Beams in the Magnetospheric Kelvin-Helmholtz Instability
ArticleAbstract: The description of the local turbulent energy transfer and the high-resolution ion distributions meaPalabras claves:Autores:Burch J.L., Carbone V., Catapano F., Coburn J.T., Di Mare F., Federico Fraternale, Giles B.L., Greco A., Khotyaintsev Y.V., Le Contel O., Luca Sorriso-Valvo, Malara F., Moore T.E., Panebianco V., Perri S., Perrone D., Pezzi O., Raffaele Marino, Retinò A., Roberts O.W., Russell C.T., Torbert R.B., Valentini F., Veltri P.Fuentes:scopusSmall-scale anisotropy in the solar wind
Conference ObjectAbstract: We investigate small-scale anisotropy of the interplanetary magnetic field (IMF) fluctuations in thePalabras claves:Autores:André M., Bruno R., Carbone V., Khotyaintsev Y.V., Luca Sorriso-Valvo, Perri S., Veltri P., Yordanova E.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 turbulent spectra and role of hall effect: A case study
Conference ObjectAbstract: Turbulent fluctuations within solar wind spectrum follows nearly Kolmogorov's power law spectrum f-5Palabras claves:ESA, LaTeX, MacrosAutores:Alexandrova O., Carbone V., Luca Sorriso-Valvo, Veltri P.Fuentes:scopus