Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode

Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode

Low- m inertial modes have been recently discovered in the Sun’s high-latitude regions. In this study, we characterize the observational properties of the m = 1 mode by analyzing time–distance subsurface flow maps. Synoptic flow maps, constructed from daily subsurface flow maps using a tracking rate...

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Bibliographic Details
Main Authors: Boyang Ding, Junwei Zhao, Ruizhu Chen, Matthias Waidele, Sushant S. Mahajan, Oana Vesa
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar interior
Solar oscillations
Helioseismology
Solar rotation
Online Access:https://doi.org/10.3847/1538-4357/ade980
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