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Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?

Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the joint observations performed by Parker Solar Probe and the Metis coronagraph on board Solar Orbiter, local measurem...

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Principais autores: Daniele Telloni, Gary P. Zank, Laxman Adhikari, Lingling Zhao, Roberto Susino, Ester Antonucci, Silvano Fineschi, Marco Stangalini, Catia Grimani, Luca Sorriso-Valvo, Daniel Verscharen, Raffaele Marino, Silvio Giordano, Raffaella D’Amicis, Denise Perrone, Francesco Carbone, Alessandro Liberatore, Roberto Bruno, Gaetano Zimbardo, Marco Romoli, Vincenzo Andretta, Vania Da Deppo, Petr Heinzel, John D. Moses, Giampiero Naletto, Gianalfredo Nicolini, Daniele Spadaro, Luca Teriaca, Aleksandr Burtovoi, Yara De Leo, Giovanna Jerse, Federico Landini, Maurizio Pancrazzi, Clementina Sasso, Alessandra Slemer
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Assuntos:
Magnetohydrodynamics
Interplanetary turbulence
Alfven waves
Solar corona
Solar coronal heating
Coronagraphic imaging
Acceso en liña:https://doi.org/10.3847/1538-4357/acb693
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