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

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astro-ph.SR2025

Multiwavelength spectroscopic observations of a quiescent prominence

Jianchao Xue, Ping Zhang, Jean-Claude Vial +5

In this paper we focus on the analysis of the multiwavelength spectroscopic observations of a quiescent prominence. The spectral and geometrical parameters in the prominence were d…

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★ 1 cited

Parameter effects on the total intensity of H I Lyα line for a modelled coronal mass ejection and its driven shock

Beili Ying, Guanglu Shi, Li Feng +5

The combination of the H I Lyα (121.6 nm) line formation mechanism with ultraviolet (UV) Lyα and white-light (WL) observations provides an effective method for determining the elec…