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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:scopusHelios 2 observations of solar wind turbulence decay in the inner heliosphere
ArticleAbstract: Aims. A linear scaling of the mixed third-order moment of the magnetohydrodynamic (MHD) fluctuationsPalabras claves:magnetohydrodynamics (MHD), solar wind, TurbulenceAutores:Bruno R., D,Aamicis R., Foldes R., Lévêque E., Luca Sorriso-Valvo, Raffaele Marino, Telloni D., Yordanova E.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:scopusStatistical analysis of field-aligned alfvénic turbulence and intermittency in fast solar wind
ArticleAbstract: The statistical properties of fast Alfvénic solar wind turbulence have been analyzed by means of empPalabras claves:Scaling laws, solar wind, TurbulenceAutores:Adhikari L., Bruno R., Carbone F., Luca Sorriso-Valvo, Telloni D., Zank G.P., Zhao L.L.Fuentes:scopusStatistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations
ArticleAbstract: Context. The recently released spacecraft potential measured by the RPW instrument on board Solar OrPalabras claves:plasmas, solar wind, Turbulence, WavesAutores:Angelini V., Bale S.D., Bruno R., Carbone F., Christian L. Vásconez, Chust T., D’Amicis R., Edberg N.J.T., Eriksson A.I., Evans V., Graham D.B., Horbury T.S., Johansson E.P.G., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Lorfèvre E., Luca Sorriso-Valvo, Maksimovic M., O'brien H., Plettemeier D., Souček J., Steinvall K., Steller M., Štverák , Telloni D., Trávníček P., Vaivads A., Vecchio A., Yordanova E.Fuentes:googlescopusThe 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