84 citations · 103 across the 9 of their papers we have counts for
11 papers
Statistics of Solar Filament Mass based on CHASE Sun-as-a-star Spectroscopic Observations
T. Y. Xie, Z. H. Zhao, X. Cheng +5
Filaments are cool and dense plasmas suspended in the hot corona of the Sun and other stars. Accurately estimating their masses is of great significance for understanding subsequen…
A Modern ConvNet for Solar Filament Detection
J. R. Hu, Q. Hao, Z. Zheng +3
Automated solar filament detection using deep learning faces several challenges. Semantic segmentation of solar filaments is a complicated multiscale feature extraction task with l…
Explainable AI for Solar Flare Prediction: Quantitative Magnetic Field Analysis of Model-Focused Regions
Z. Zheng, Q. Hao, C. Li +4
Solar flares are intense energy release events in the solar atmosphere that may pose significant space weather hazards, which makes developing reliable prediction models essential.…
Inversion of CHASE H Spectral Line during Solar Flares Based on RADYN Dataset via Deep Learning
W. Xu, Q. Hao, Z. Zheng +6
Solar flares represent one of the most intense forms of solar activity. Understanding the evolution of physical parameters in the solar atmosphere during flares is key to studying…
Sun-as-a-star Study of an X-class Solar Flare with Spectroscopic Observations of CHASE
Y. L. Ma, Q. H. Lao, X. Cheng +5
Sun-as-a-star spectroscopic characteristics of solar flares can be used as a benchmark for the detection and analyses of stellar flares. Here, we study the Sun-as-a-star properties…
Developing an Automated Detection, Tracking and Analysis Method for Solar Filaments Observed by CHASE via Machine Learning
Z. Zheng, Q. Hao, Y. Qiu +3
Studies on the dynamics of solar filaments have significant implications for understanding their formation, evolution, and eruption, which are of great importance for space weather…
Formation of a long filament through the connection of two filament segments observed by CHASE
H. T. Li, X. Cheng, Y. W. Ni +5
We present imaging and spectroscopic diagnostics of a long filament during its formation with the observations from the Chinese H Solar Explorer and Solar Dynamics Observatory.…
Sequential Remote Brightenings and Co-spatial Fast Downflows during Two Successive Flares
B. T. Wang, X. Cheng, C. Li +2
Remote brightenings often appear at outskirts of source active regions of solar eruptive events, nevertheless, their origin remains to be ascertained. In this study, we report imag…
Grow-up of a Filament Channel by Intermittent Small-scale Magnetic Reconnection
H. T. Li, X. Cheng, J. H. Guo +5
Filament channel (FC), a plasma volume where the magnetic field is primarily aligned with the polarity inversion line, is believed to be the pre-eruptive configuration of coronal m…
What determine Solar Flares Producing Interplanetary Type III Radio Bursts?
Y. K. Kou, Z. C. Jing, X. Cheng +4
Energetic electrons accelerated by solar flares often give rise to type III radio bursts at a broad waveband and even interplanetary type III bursts (IT3) if the wavelength extends…
Tracking the Evolution of A Coherent Magnetic Flux Rope Continuously from the Inner to the Outer Corona
X. Cheng, M. D. Ding, Y. Guo +6
The magnetic flux rope (MFR) is believed to be the underlying magnetic structure of coronal mass ejections (CMEs). However, it remains unclear how an MFR evolves into and forms the…