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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: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:scopus