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First Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source
ArticleAbstract: Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagatPalabras claves:Interplanetary medium, magnetohydrodynamics (MHD), methods: data analysis, solar wind, Sun: general, TurbulenceAutores:André N., Angelini V., Bruno R., Coco I., De Marco R., D’Amicis R., Evans V., Fedorov A., Genot V., Horbury T.S., Jagarlamudi V.K., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Marcucci M.F., Matteini L., Müller D., O'brien H., Owen C.J., Panasenco O., Perrone D., Pezzi O., Rouillard A.P., Telloni D., Tenerani A., Velli M.C., Verscharen D., Woodham L.D., Zouganelis I.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:scopusInvestigating Alfvénic Turbulence in Fast and Slow Solar Wind Streams
ArticleAbstract: Solar wind turbulence dominated by large-amplitude Alfvénic fluctuations, mainly propagating away frPalabras claves:Interplanetary medium, Magnetic Field, methods: data analysis, solar wind, TurbulenceAutores:Bruno R., De Marco R., D’Amicis R., Luca Sorriso-Valvo, Perrone D., Telloni D., Velli M.C.Fuentes: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:scopusThe low-frequency break observed in the slow solar wind magnetic spectra
ArticleAbstract: Fluctuations of solar wind magnetic field and plasma parameters exhibit a typical turbulence power sPalabras claves:Magnetic fields, plasmas, solar wind, Sun: heliosphere, Turbulence, WavesAutores:Bruno R., De Marco R., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Telloni D.Fuentes:scopus