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20212026
most citedResolved magnetohydrodynamic wave lensing in the solar corona

26 citations · 60 across the 7 of their papers we have counts for

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astro-ph.SR2026

Phase-drifting with emitting plasma temperature in the quasi-periodic pulsations of an X-class solar flare

Libo Fu, Valery M. Nakariakov, Ding Yuan +3

Recent multi-wavelength observations of solar flares have provided new constraints on the physical origin of quasi-periodic pulsations (QPPs). In an X-class flare, we detect a shor…

astro-ph.SR2026

Chromospheric resonator model for sunspot revealed by multi-height observation of umbral wave

Kartika Sangal, A. K. Srivastava, Libo Fu +3

Sunspots are transient, magnetically intense features that host oscillations linked to magnetohydrodynamic (MHD) waves. These waves may contribute to plasma heating and drive mass…

astro-ph.SR2025★ 12 cited

Exploring the origin of multi-periodic pulsations during a white-light flare

Dong Li, Ding Yuan, Jingye Yan +9

We explored the quasi-periodic pulsations (QPPs) at multiple periods during an X4.0 flare on 2024 May 10 (SOL2024-05-10T06:27), which occurred in the complex active region of NOAA…

astro-ph.SR2024★ 26 cited

Resolved magnetohydrodynamic wave lensing in the solar corona

Xinping Zhou, Yuandeng Shen, Ding Yuan +6

Electromagnetic wave lensing, a common physical phenomenon recognized in visible light for centuries, finds extensive applications in manipulating light in optical systems such as…

astro-ph.SR2023★ 17 cited

30-min Decayless Kink Oscillations in a Very Long Bundle of Solar Coronal Plasma Loops

Sihui Zhong, Valery M. Nakariakov, Yuhu Miao +2

The energy balance in the corona of the Sun is the key to the long-standing coronal heating dilemma, which could be potentially revealed by observational studies of decayless kink…

astro-ph.SR2022

Inter-Correlation Between Sunspot Oscillations and Their Internal Structures

Libo Fu, Zizhan Zhu, Ding Yuan +3

Three- and five-minute oscillations are commonly found in any sunspot. As they are modulated by the internal thermal and magnetic structures of a sunspot, therehence, they could be…