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Does 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: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