Resolved magnetohydrodynamic wave lensing in the solar corona
Xinping Zhou,
Yuandeng Shen (),
Ding Yuan (),
Rony Keppens,
Xiaozhou Zhao,
Libo Fu,
Zehao Tang,
Jiaoyang Wang and
Chengrui Zhou
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Xinping Zhou: Sichuan Normal University
Yuandeng Shen: Chinese Academy of Sciences
Ding Yuan: Harbin Institute of Technology
Rony Keppens: Department of Mathematics, KU Leuven
Xiaozhou Zhao: Department of Mathematics, KU Leuven
Libo Fu: Harbin Institute of Technology
Zehao Tang: Chinese Academy of Sciences
Jiaoyang Wang: Harbin Institute of Technology
Chengrui Zhou: Chinese Academy of Sciences
Nature Communications, 2024, vol. 15, issue 1, 1-11
Abstract:
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.
Date: 2024
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DOI: 10.1038/s41467-024-46846-z
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