activity
20112026
most citedObservations of Turbulent Magnetic Reconnection Within a Solar Current Sheet

151 citations · 541 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2026

Revisiting Approaches to Stellar White-Light Flare Energy Based on Spatiotemporally Resolved Solar Observations

Yingjie Cai, Yijun Hou, Ting Li +5

Accurately estimating the bolometric energy of solar and stellar white-light flares (WLFs) is crucial for understanding their physical nature and impact on surrounding planets. How…

astro-ph.SR2023

Spectral Features of the Solar Transition Region and Chromospheric Lines at Flare Ribbons Observed with IRIS

Lingfang Wang, Ying Li, Qiao Li +2

We report on the spectral features of the Si IV 1402.77 Å, C II 1334.53 Å, and Mg II h or k lines, formed in the layers from the transition region to the chromosphere, in three two…

astro-ph.SR2022★ 5 cited

The Lyman- Emission in a C1.4 Solar Flare Observed by the Extreme Ultraviolet Imager aboard Solar Orbiter

Ying Li, Qiao Li, De-Chao Song +7

The hydrogen Lyman- (H {\sc i} Ly) emission during solar flares has rarely been studied in spatially resolved images and its physical origin has not been fully understood. In…

astro-ph.SR2021

Revisiting the Spectral Features of Ellerman Bombs and UV Bursts. I. Radiative Hydrodynamic Simulations

Jie Hong, Ying Li, M. D. Ding +1

Ellerman bombs (EBs) and UV bursts are both small-scale solar activities that occur in active regions. They are now believed to form at different heights in the lower atmosphere. I…

astro-ph.SR2020★ 7 cited

Radiative Hydrodynamic Simulations of the Spectral Characteristics of Solar White-light Flares

Yu-Tong Yang, Jie Hong, Ying Li +2

As one of the most violent activities in the solar atmosphere, white-light flares (WLFs) are generally known for their enhanced white-light (or continuum) emission, which primarily…

astro-ph.SR2020★ 3 cited

Non-LTE Calculations of the Mg I 12.32 m Line in a Flaring Atmosphere

Jie Hong, Xianyong Bai, Ying Li +2

The infrared Mg I lines near 12 microns are a pair of emission lines which are magnetically sensitive and have been used to measure solar magnetic fields. Here we calculate the res…