Author
Listed:
- Xinping Zhou
(Sichuan Normal University)
- Yuandeng Shen
(Chinese Academy of Sciences)
- Ding Yuan
(Harbin Institute of Technology
Chinese Academy of Sciences)
- Rony Keppens
(Department of Mathematics, KU Leuven)
- Xiaozhou Zhao
(Department of Mathematics, KU Leuven)
- Libo Fu
(Harbin Institute of Technology
Chinese Academy of Sciences)
- Zehao Tang
(Chinese Academy of Sciences)
- Jiaoyang Wang
(Harbin Institute of Technology
Chinese Academy of Sciences)
- Chengrui Zhou
(Chinese Academy of Sciences)
Abstract
Electromagnetic wave lensing, a common physical phenomenon recognized in visible light for centuries, finds extensive applications in manipulating light in optical systems such as telescopes and cameras. Magnetohydrodynamic wave is a common perturbation phenomenon in the corona. By using high spatio-temporal resolution observations from the Solar Dynamics Observatory, here, we report the observation of a magnetohydrodynamic wave lensing in the highly ionized and magnetized coronal plasma, where quasi-periodic wavefronts emanated from a flare converged at a specific point after traversing a coronal hole. The entire process resembles an electromagnetic wave lensing from the source to the focus. Meanwhile, the magnetohydrodynamic wave lensing is well reproduced through a magnetohydrodynamic numerical simulation with full spatio-temporal resolution. We further investigate potential applications for coronal seismology, as the lensing process encodes information on the Alfvén speed, in conjunction with favorable geometric and density variations.
Suggested Citation
Xinping Zhou & Yuandeng Shen & Ding Yuan & Rony Keppens & Xiaozhou Zhao & Libo Fu & Zehao Tang & Jiaoyang Wang & Chengrui Zhou, 2024.
"Resolved magnetohydrodynamic wave lensing in the solar corona,"
Nature Communications, Nature, vol. 15(1), pages 1-11, December.
Handle:
RePEc:nat:natcom:v:15:y:2024:i:1:d:10.1038_s41467-024-46846-z
DOI: 10.1038/s41467-024-46846-z
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