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Article
Open AccessAutomatic Solar Flare Detection Using the Solar Disk Imager Onboard the ASO-S Mission
We present an automated solar flare detection software tool to automatically process solar observed images, detect and track solar flares, and finally compile an event catalog. It can identify and track flares...
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Article
Open AccessSpectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese H \(\alpha \) Solar Explorer (CHASE)
Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (X- and M-class flares). Here, we report a small C2.3 white-light flare (SOL2022-12-20T04:1...
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Article
Open AccessA 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
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 Lyman-alpha Solar Telescope (LST)...
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Article
The Advanced Space-Based Solar Observatory (ASO-S)
The Advanced Space-based Solar Observatory (ASO-S) was successfully launched at 23:43 UT on 8 October 2022. Here we describe the final technical status of the whole mission right before the launch, including the ...
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Article
Microwave diagnostics of magnetic field strengths in solar flaring loops
We have performed microwave diagnostics of the magnetic field strengths in solar flaring loops based on the theory of gyrosynchrotron emission. From Nobeyama Radioheliograph observations of three flare events ...
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Article
The bi-directional moving structures in a coronal bright point
We report the bi-directional moving structures in a coronal bright point (CBP) on 2015 July 14. It is observed by the Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO). This CBP has a li...
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Article
Open AccessObserving the release of twist by magnetic reconnection in a solar filament eruption
Magnetic reconnection is a fundamental process of topology change and energy release, taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory. However, observational eviden...
