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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:googlescopusAnalysis of cancellation exponents in two-dimensional vlasov turbulence
ArticleAbstract: Statistical properties of plasma turbulence are investigated by means of two-dimensional Vlasov simuPalabras claves:Autores:Carbone V., De Vita G., Luca Sorriso-Valvo, Primavera L., Servidio S., Valentini F., Veltri P.Fuentes:scopusA statistical analysis of polarity reversals of the geomagnetic field
ArticleAbstract: We investigate the temporal distribution of polarity reversals of the geomagnetic field. In spite ofPalabras claves:Dynamo effect, Geomagnetism, Paleomagnetic measurementsAutores:Carbone V., Lepreti F., Luca Sorriso-Valvo, Nigro G., Stefani F., Vecchio A., Veltri P.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:scopusCancellations and structures in the solar photosphere: Signature of flares
Conference ObjectAbstract: The topological properties of the typical current structures in a turbulent magnetohydrodynamic flowPalabras claves:Autores:Abramenko V., Carbone V., Luca Sorriso-Valvo, Noullez A., Politano H., Pouquet A., Veltri P., Yurchyshyn V.Fuentes:scopusErratum: Multifractal scaling and intermittency in hybrid Vlasov-Maxwell simulations of plasma turbulence (Physics of Plasmas (2016) 23 (022307))
OtherAbstract:Palabras claves:Autores:Carbone F., Leonardis E., Luca Sorriso-Valvo, Servidio S., Valentini F., Veltri P.Fuentes:scopusErratum: On the occurrence of the third-order scaling in high-latitude solar wind (Astrophysical Journal (2012) 750 (41))
OtherAbstract:Palabras claves:Autores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Veltri P.Fuentes:scopusDifferential 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:scopusNature 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:scopus