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20232026
most citedMeridional flow in the solar polar caps revealed by magnetic field observation and simulation

11 citations · 28 across the 26 of their papers we have counts for

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astro-ph.SR2024

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops

Leping Li, Hongqiang Song, Yijun Hou +11

Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…

astro-ph.SR2024★ 10 cited

Long-term variation of the solar polar magnetic fields at different latitudes

Shuhong Yang, Jie Jiang, Zifan Wang +10

The polar magnetic fields of the Sun play an important role in governing solar activity and powering fast solar wind. However, because our view of the Sun is limited in the eclipti…

astro-ph.SR2024

Statistics of Solar White-Light Flares I: Optimization of Identification Methods and Application

Yingjie Cai, Yijun Hou, Ting Li +1

White-light flares (WLFs) are energetic activity in stellar atmosphere. However, the observed solar WLF is relatively rare compared to stellar WLFs or solar flares observed at othe…

astro-ph.SR2024★ 11 cited

Meridional flow in the solar polar caps revealed by magnetic field observation and simulation

Shuhong Yang, Jie Jiang, Zifan Wang +10

As a large-scale motion on the Sun, the meridional flow plays an important role in determining magnetic structure and strength and solar cycle. However, the meridional flow near th…

astro-ph.SR2024

The Solar Origin of an Intense Geomagnetic Storm on 2023 December 1st: Successive Slipping and Eruption of Multiple Magnetic Flux Ropes

Zheng Sun, Ting Li, Yijun Hou +12

The solar eruption that occurred on 2023 November 28 (SOL2023-11-28) triggered an intense geomagnetic storm on Earth on 2023 December 1. The associated Earth's auroras manifested a…

astro-ph.SR2024

Formation and Evolution of Transient Prominence Bubbles Driven by Erupting Mini-filaments

Yilin Guo, Yijun Hou, Ting Li +6

Prominence bubbles, the dark arch-shaped "voids" below quiescent prominences, are generally believed to be caused by the interaction between the prominences and the slowly-emerging…

astro-ph.SR2024

Negative-energy waves in the vertical threads of a solar prominence

Jincheng Wang, Dong Li, Chuan Li +5

Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination due to their thread-like features and dynamic behaviors. Utilizing data from the New V…

astro-ph.SR2024

Survey of Magnetic Field Parameters Associated With Large Solar Flares

Ting Li, Yanfang Zheng, Xuefeng Li +4

Until now, how the magnetic fields in M/X-class flaring active regions (ARs) differ from C-class flaring ARs remains unclear. Here, we calculate the key magnetic field parameters w…

astro-ph.SR2024

Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event

Liheng Yang, Xiaoli Yan, Zhike Xue +5

Previous studies have revealed that solar coronal jets triggered by the eruption of mini-filaments (MFs) conform to the famous magnetic-breakout mechanism. In such scenario, a brea…