activity
20182026
most citedA Statistical Study of the Magnetic Imprints of X-Class Solar Flares

9 citations · 19 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Unprecedent fast winking of solar flares triggered by bursty magnetic reconnection

Ting Li, Xuchun Duan, Yijun Hou +13

Flare ribbons form as a result of energy deposition associated with particles accelerated in low layers of the solar atmosphere. The fine-scale structures of flare ribbons, also ca…

astro-ph.EP2026

Positive YORP effect induced by lateral heat conduction in a crater

Zehua Qi, Yining Zhang, Hailiang Li +2

The YORP effect plays an important role in the spin evolution of asteroids. Although craters are ubiquitous surface features, their influence on YORP torque has received limited at…

astro-ph.EP2025★ 1 cited

A High-Precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multi-Layer Internal Structure Models

Kai Huang, Yongzhang Yang, Yuhao Chen +2

China is planing to launch the Tianwen-4 mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space explorat…

astro-ph.SR2025

A Statistical Analysis of Magnetic Parameters in Solar Source Regions of Halo-CMEs with and without SEP events

Xuchun Duan, Ting Li, Yijun Hou +5

Large SEPs can cause adverse space weather hazard to humans technology and such events are especially associated with halo coronal mass ejections (CMEs). But in turn, a significant…

astro-ph.EP2025★ 2 cited

Shape index of Yarkovsky effect on irregularly shaped asteroids

Yining Zhang, Yang-Bo Xu, Zehua Qi +2

The Yarkovsky effect on real asteroids is complicated to calculate either by analytical or numerical methods, since they are generally irregular in shape. We propose an index to pr…

astro-ph.SR2025

Quasiperiodic Slow-Propagating EUV "Wave" Trains After the Filament Eruption

Yining Zhang, Ting Li, Weilin Teng +6

The eruption of the filament/flux rope generates the coronal perturbations, which further form EUV waves. There are two types of EUV waves, including fast-mode magnetosonic waves a…

astro-ph.SR2025

Quasiperiodic Super-Alfvenic Slippage Along Flare Ribbons Observed by the Interface Region Imaging Spectrograph

Yining Zhang, Ting Li, Yijun Hou +3

The apparent slipping motion of flare loops is regarded as a key feature of the 3D magnetic reconnection in the solar flares. The slippage with a super-Alfvénic speed could be defi…

astro-ph.SR2024

Quasi-periodic oscillations of flare loops and slipping motion of ribbon substructures during a C-class flare

Yining Zhang, Ting Li, Jing Ye

Quasi-periodic oscillations in solar flaring emission have been observed over the past few decades. To date, the underpinning processes resulting in the quasi-periodic oscillations…

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

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.SR2022★ 7 cited

Two-dimensional modeling of the tearing-mode-governed magnetic reconnection in the large-scale current sheet above the two-ribbon flare

Yining Zhang, Jing Ye, Zhixing Mei +2

We attempt to model magnetic reconnection during the two-ribbon flare in the gravitationally stratified solar atmosphere with the Lundquist number of using 2D simulations.…

astro-ph.SR2018★ 9 cited

A Statistical Study of the Magnetic Imprints of X-Class Solar Flares

Zekun Lu, Weiguang Cao, Gaoxiang Jin +3

Magnetic imprints, the rapid and irreversible evolution of photospheric magnetic fields as a feedback from flares in the corona, have been confirmed by many previous studies. These…