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20202026
most citedFast degradation of the circular flare ribbon on 2014 August 24

13 citations · 23 across the 13 of their papers we have counts for

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15 papers · 1 filter

astro-ph.SR2026

Quadrupole White-light Sources in an X1.2 Flare Observed by ASO-S/LST/WST and SDO/HMI

Zhichen Jing, Ying Li, Dechao Song +2

We present observations of an X1.2 white-light flare on 2023 January 6, which exhibits a rare quadrupolar white-light source configuration. This event was observed by the White-lig…

astro-ph.SR2026

The Lyman-alpha Emission in Solar Flares. II. A Statistical Study on Its Relationship with the White-light plus Soft X-ray Emission

De-Chao Song, Ying Li, Qiao Li +1

The hydrogen \lya\ line and the white-light (WL) continuum are two key diagnostics of energy transport in the lower atmosphere during solar flares, yet their relationship remains p…

astro-ph.SR2025

The M- and X-class White-light Flares in Super Active Region NOAA 13664/13697 Observed by ASO-S/LST/WST

Zhichen Jing, Ying Li, Jingwei Li +1

Solar white-light flares (WLFs) have been observed since 1859, but their occurrence rate is not yet fully understood. The physical properties of WLFs in super active regions (SARs)…

astro-ph.SR2025

Sun-as-a-star Analysis of the Solar Eruption Source Region Using Ha Spectroscopic Observations of CHASE

Xiaofeng Liu, Yijun Hou, Ying Li +6

Sun-as-a-star analyses serve as a bridge for comparative studies on solar and stellar activities. To investigate the typical Sun-as-a-star Ha temporal spectral characteristics in s…

astro-ph.SR2025

Understanding the Lyα Emission Observed by the Solar Disk Imager Aboard the Advanced Space-based Solar Observatory

Yiliang Li, Ping Zhang, Zhengyuan Tian +12

The H I Lyman-alpha (Ly) emission, with a wavelength of 1216 Å, is the brightest solar ultraviolet (UV) line. However, comprehensive observations of the Ly emission line acro…

astro-ph.SR2025★ 9 cited

Unveiling Spatiotemporal Properties of the Quasi-periodic Pulsations in the Balmer Continuum at 3600 Å in an X-class Solar White-light Flare

De-Chao Song, Marie Dominique, Ivan Zimovets +11

Quasi-periodic pulsations (QPPs) in the Balmer continuum of solar white-light flares (WLFs) are rarely reported, and accurately pinpointing the spatial source of flaring QPPs remai…

astro-ph.SR2024★ 1 cited

Improving image quality of the Solar Disk Imager (SDI) of the Lyman-alpha Solar Telescope (LST) onboard the ASO-S mission

Hui Liu, Hui Li, Sizhong Zou +11

The in-flight calibration and performance of the Solar Disk Imager (SDI), which is a pivotal instrument of the Lyman-alpha Solar Telescope (LST) onboard the Advanced Space-based So…

astro-ph.SR2024

Various Features of the X-class White-light Flares in Super Active Region NOAA 13664

Ying Li, Xiaofeng Liu, Zhichen Jing +8

Super active region NOAA 13664 produced 12 X-class flares (including the largest one, an occulted X8.7 flare, in solar cycle 25 so far) during 2024 May 8-15 and 11 of them are iden…

astro-ph.SR2024

Inflight Performance and Calibrations of the Lyman-alpha Solar Telescope on board the Advanced Space-based Solar Observatory

Bo Chen, Li Feng, Guang Zhang +40

The Lyman-alpha Solar Telescope (LST) on board the Advanced Space-based Solar Observatory (ASO-S) is the first payload to image the full solar disk and the solar corona in both whi…

astro-ph.SR2024

Asymmetric Hard X-ray Radiation of Two Ribbons in a Thermal-Dominated C-Class Flare

Guanglu Shi, Li Feng, Jun Chen +9

The asymmetry in hard X-ray (HXR) emission at the footpoints (FPs) of flare loops is a ubiquitous feature closely associated with nonthermal electron transport. We analyze the asym…

astro-ph.SR2024

Association between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence

Jianchao Xue, Li Feng, Hui Li +31

Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here we present two failed prominence eru…

astro-ph.SR2024

Spectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese H Solar Explorer (CHASE)

Qiao Li, Ying Li, Yang Su +27

Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (say X- and M-class flares). Here we report a small C2.3 white…

astro-ph.SR2024

The White-light Emissions in Two X-class Flares Observed by ASO-S and CHASE

Ying Li, Zhichen Jing, De-Chao Song +9

The white-light continuum emissions in solar flares (i.e., white-light flares) are usually observed on the solar disk but, in a few cases, off the limb. Here we present on-disk as…

astro-ph.SR2024

A Statistical Study of Solar White-Light Flares Observed by the White-light Solar Telescope of the Lyman-alpha Solar Telescope on the Advanced Space-based Solar Observatory (ASO-S/LST/WST) at 360 nm

Zhichen Jing, Ying Li, Li Feng +26

Solar white-light flares (WLFs) are those accompanied by brightenings in the optical continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of the L…

astro-ph.SR2020★ 13 cited

Fast degradation of the circular flare ribbon on 2014 August 24

Q. M. Zhang, S. H. Yang, T. Li +2

The separation and elongation motions of solar flare ribbons have extensively been investigated. The degradation and disappearance of ribbons have rarely been explored. In this pap…