activity
20222025
most citedThe Chinese Hα Solar Explorer (CHASE) mission: An overview

152 citations · 251 across the 11 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.SR2025

Two-stage primary acceleration in filament initial eruption under a fan-spine magnetic configuration

Haitang Li, Ke Yu, Chang Zhou +6

Understaning the filament rising process is crucial for unveiling the triggering mechanisms of the coronal mass ejections and forecasting the space weather. In this paper, we prese…

astro-ph.SR2025

Two-Stage Nature of a Solar Flare with Parallel and Semi-Circular Ribbons

Ruifei Huang, Hao Ning, Ze Zhong +6

Flare ribbons with parallel and circular morphologies are typically associated with different magnetic reconnection models, and the simultaneous observation of both types in a sing…

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★ 3 cited

The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field

Ye Qiu, Yang Guo, Mingde Ding +3

Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms. Particularly, some geom…

astro-ph.SR2025★ 7 cited

Observational Study of Recurrent Jets: Evolution of Magnetic Flux, Current, and Helicity

Chang Zhou, Yang Guo, Guoyin Chen +2

We observed three recurrent blowout jets in an active regio with Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory (SDO). Using Helioseismic Magnetic Imager…

astro-ph.SR2025

Radio dimming associated with filament eruptions in the meter and decimeter wavebands

Zhenyong Hou, Hui Tian, Jingye Yan +12

Filament eruptions are considered to be a common phenomenon on the Sun and other stars, yet they are rarely directly imaged in the meter and decimeter wavebands. Using imaging data…