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scopus(5)
First polar observations of the fast solar wind with the Metis Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration
ArticleAbstract: Context. The fast solar wind is known to emanate from polar coronal holes. Aims. This Letter reportsPalabras claves:magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: UV radiationAutores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Capuano G.E., De Leo Y., Deppo V.D., D’Amicis R., Fineschi S., Giordano S., Grimani C., Heinzel P., Jerse G., Landini F., Liberatore A., Luca Sorriso-Valvo, Moses J.D., Naletto G., Nicolini G., Pancrazzi M., Perrone D., Raffaele Marino, Romoli M., Russano G., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Uslenghi M., Vai M., Zank G.P., Zhao L.L.Fuentes:scopusDoes Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?
ArticleAbstract: Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries ofPalabras claves:Autores:Adhikari L., Andretta V., Antonucci E., Bruno R., Burtovoi A., Carbone F., De Leo Y., Deppo V.D., D’Amicis R., Fineschi S., Giordano S., Grimani C., Heinzel P., Jerse G., Landini F., Liberatore A., Luca Sorriso-Valvo, Moses J.D., Naletto G., Nicolini G., Pancrazzi M., Perrone D., Raffaele Marino, Romoli M., Sasso C., Slemer A., Spadaro D., Stangalini M., Susino R., Telloni D., Teriaca L., Verscharen D., Zank G.P., Zhao L.L., Zimbardo G.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: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:scopusSudden depletion of Alfvénic turbulence in the rarefaction region of corotating solar wind high-speed streams at 1 AU: Possible solar origin?
ArticleAbstract: A canonical description of a corotating solar wind high-speed stream in terms of velocity profile woPalabras claves:magnetohydrodynamics (MHD), solar wind, Sun: corona, Sun: magnetic fields, TurbulenceAutores:Bruno R., Carnevale G., Pietropaolo E., Raffaele Marino, Raines J.M.Fuentes:scopus