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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:scopusMultiscale views of an Alfvénic slow solar wind: 3D velocity distribution functions observed by the Proton-Alpha Sensor of Solar Orbiter
ArticleAbstract: Context. The Alfvénic slow solar wind is of particular interest, as it is often characterized by intPalabras claves:plasmas, solar wind, TurbulenceAutores:Allegrini F., André N., Angelini V., Bale S.D., Barthe A., Berthomier M., Bruno R., D’Amicis R., Evans V., Fedorov A., Fortunato V., Fruit G., Genot V., Horbury T.S., Kasper J.C., Khataria D., Kieokaew R., Lavraud B., Livi S., Louarn P., Luca Sorriso-Valvo, Maksimovic M., Mele G., O'brien H., Owen C.J., Penou E., Plotnikov I., Prech L., Raines J.M., Réville V., Rouillard A.P., Verscharen D.Fuentes:scopusICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter
ArticleAbstract: The primary scientific goal of ICARUS (Investigation of Coronal AcceleRation and heating of solar wiPalabras claves:Heliophysics, Solar atmosphere, solar wind, Space missionAutores:Agapitov O., Balat-Pichelin M., Bale S.D., Balikhin M., Baumjohann W., Berthomier M., Bruno R., Cranmer S.R., de Pontieu B., Dudok De Wit T., Eastwood J., Erdelyi R., Ergun R., Fedorov A., Fedun V., Ganushkina N., Greco A., Harra L.K., Henri P., Horbury T.S., Hudson H., Kasper J., Khotyaintsev Y.V., Krasnoselskikh V., Kretzschmar M., Krucker S., Kucharek H., Langevin Y., Lavraud B., Lebreton J.P., Lepri S., Liemohn M., Louarn P., Luca Sorriso-Valvo, Maksimovic M., Meneses D.d.S., Moebius E., Mozer F., Nemecek Z., Panasenco O., Retinò A., Šafránková J., Scudder J., Servidio S., Souček J., Szabo A., Tsurutani B.T., Vaivads A., Vekstein G., Velli M.C., Vörös Z., Walker S., Zaqarashvili T., Zimbardo G.Fuentes:scopus