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

نویسندگان

چکیده

Evidence for the presence of ion cyclotron waves, driven by turbulence, at boundaries current sheet is reported in this paper. By exploiting full potential joint observations performed Parker Solar Probe and Metis coronagraph on board Orbiter, local measurements solar wind can be linked with large-scale structures corona. The results suggest that dynamics layers generates which turn creates a sufficiently strong temperature anisotropy to make solar-wind plasma unstable anisotropy-driven instabilities such as Alfv\'en ion-cyclotron, mirror-mode, firehose instabilities. study polarization state high-frequency magnetic fluctuations reveals waves are indeed present along sheet, thus linking topology remotely imaged coronal source regions wave bursts observed situ. may allow improvement state-of-the-art models based mechanism, providing new insights into processes involved heating.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2023

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/acb693