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Monthly Notices of the Royal Astronomical Society(2)
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scopus(5)
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:scopusEnergetic particle transport in the presence of magnetic turbulence: Influence of spectral extension and intermittency
ArticleAbstract: The transport of energetic particles in the presence of magnetic turbulence is an important but unsoPalabras claves:diffusion, Magnetic fields, methods: numerical, solar windAutores:Luca Sorriso-Valvo, Malara F., Perri S., Pucci F., Valentini F., Zimbardo G.Fuentes:scopusOn the Statistical Properties of Turbulent Energy Transfer Rate in the Inner Heliosphere
ArticleAbstract: The transfer of energy from large to small scales in solar wind turbulence is an important ingbkp_rePalabras claves:Intermittency, solar wind, TurbulenceAutores:Bruno R., Carbone F., Greco A., Luca Sorriso-Valvo, Perri S., Raffaele MarinoFuentes:scopusSELF-CONSISTENT CASTAING DISTRIBUTION OF SOLAR WIND TURBULENT FLUCTUATIONS
ArticleAbstract: The intermittent behavior of solar wind turbulent fluctuations has often been investigated through tPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Carbone V., Lijoi L., Luca Sorriso-Valvo, Perri S., Raffaele MarinoFuentes:scopusStudy of two interacting interplanetary coronal mass ejections encountered by Solar Orbiter during its first perihelion passage: Observations and modeling
ArticleAbstract: Context. Solar Orbiter, the new-generation mission dedicated to solar and heliospheric exploration,Palabras claves:magnetohydrodynamics (MHD), solar wind, Solar-terrestrial relations, Sun: coronal mass ejections (CMEs), Sun: evolution, Sun: heliosphereAutores:Adhikari L., Angelini V., Antonucci E., Bruno R., Carbone F., Chust T., Davies E.E., De Marco R., D’Amicis R., Evans V., Fineschi S., Giordano S., Gómez-Herrero R., Hietala H., Horbury T.S., Ivanovski S.L., Jagarlamudi V.K., Khotyaintsev Y.V., Kretzschmar M., Laker R., Liang H., Luca Sorriso-Valvo, Maksimovic M., Mancuso S., Messerotti M., Möstl C., Müller D., Nakanotani M., O'brien H., Perri S., Perrone D., Raffaele Marino, Reiss M.A., Rodríguez-Pacheco J., Romoli M., Scolini C., Souček J., Stangalini M., Steinvall K., Susino R., Telloni D., Vecchio A., Weiss A.J., Wimmer-Schweingruber R.F., Winslow R.M., Woodham L.D., Zank G.P., Zhao L.L., Zouganelis I.Fuentes:scopus