Dominance of 2 Minute Oscillations near the Alfvén Surface

Dominance of 2 Minute Oscillations near the Alfvén Surface

Alfvén waves, considered one of the primary candidates for heating and accelerating the fast solar wind, are ubiquitous in spacecraft observations, yet their origin remains elusive. In this study, we analyze data from the first 19 encounters of the Parker Solar Probe and report the dominance of 2 mi...

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Bibliographic Details
Main Authors: Zesen Huang, Marco Velli, Chen Shi, Yingjie Zhu, B. D. G. Chandran, Trevor Bowen, Victor Réville, Jia Huang, Chuanpeng Hou, Nikos Sioulas, Mingzhe Liu, Marc Pulupa, Sheng Huang, Stuart D. Bale
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar wind
Fast solar wind
Alfvén waves
Interplanetary turbulence
Solar corona
Solar coronal heating
Online Access:https://doi.org/10.3847/2041-8213/ad9271
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https://doi.org/10.3847/2041-8213/ad9271

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