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Differential 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:scopusThe Solar Orbiter Science Activity Plan: Translating solar and heliospheric physics questions into action
ArticleAbstract: Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, fromPalabras claves:Methods: observational, Space vehicles: instruments, Sun: generalAutores:Abbo L., Alexandrova O., Anastasiadis A., Andretta V., Antonucci E., Appourchaux T., Aran A., Arge C.N., Auchère F., Aulanier G., Baker D., Bale S.D., Battaglia M., Bellot Rubio L., Bemporad A., Berghmans D., Berthomier M., Bocchialini K., Bonnin X., Brun A.S., Bruno R., Buchlin E., Büchner J., Bucik R., Carcaboso F., Carr R., Carrasco-Blázquez I., Cecconi B., Cernuda I., Chen C.H.K., Chitta L.P., Chust T., Dalmasse K., De Groof A., De Marco R., Deppo V.D., Dolei S., Dolla L., Dudok De Wit T., D’Amicis R., Eastwood J.P., Espinosa Lara F., Etesi L., Fedorov A., Félix-Redondo F., Fineschi S., Fleck B., Fludra A., Fontaine D., Fox N.J., Gandorfer A., Genot V., Georgoulis M.K., Gilbert H.R., Gissot S., Giunta A., Gizon L., Gómez-Herrero R., Gontikakis C., Graham G., Green L., Grundy T., Haberreiter M., Harra L.K., Hassler D.M., Hirzberger J., Ho G.C., Horbury T.S., Howard R.A., Hurford G., Innes D., Issautier K., James A.W., Janitzek N., Janvier M., Jeffrey N., Jenkins J., Khotyaintsev Y.V., Klein K.L., Kontar E.P., Kontogiannis I., Krafft C., Krasnoselskikh V., Krucker S., Lefort J., Luca Sorriso-Valvo, Maksimovic M., Müller D., Nieves-Chinchilla T., Osuna P., Owen C.J., Rodríguez-Pacheco J., Romoli M., Sanchez L., Solanki S.K., St Cyr O.C., Van Driel-Gesztelyi L., Walsh A.P., Watson C., Williams D.R., 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