Mostrando 6 resultados de: 6
Filtros aplicados
Área temáticas
Cuerpos y fenómenos celestes específicos(3)
Magnetismo(2)
Astronomía y ciencias afines(1)
Matemáticas(1)
Mecánica clásica(1)
Erratum: 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: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:scopusREVISITING A CLASSIC: The PARKER-MOFFATT PROBLEM
ArticleAbstract: The interaction of two colliding Alfvén wave packets is described here by means of magnetohydrodynamPalabras claves:magnetohydrodynamics (MHD), plasmas, solar windAutores:Christian L. Vásconez, Malara F., Matthaeus W.H., Parashar T.N., Pezzi O., Servidio S., Valentini F., Veltri P., Yang Y.Fuentes:googlescopusRadial evolution of the intermittency of density fluctuations in the fast solar wind
ArticleAbstract: We study the radial evolution of the intermittency of density fluctuations in the fast solar wind. TPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, WavesAutores:Bruno R., Carbone V., D’Amicis R., Luca Sorriso-Valvo, Malara F., Pietropaolo E., Primavera L., Telloni D., Veltri P.Fuentes:scopusProton-Proton Collisions in the Turbulent Solar Wind: Hybrid Boltzmann-Maxwell Simulations
ArticleAbstract: The mechanism of heating for hot, dilute, and turbulent plasmas represents a long-standing problem iPalabras claves:Autores:Luca Sorriso-Valvo, Perrone D., Pezzi O., Servidio S., Valentini F., Veltri P.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:scopus