activity
20162026
most citedSolar Magnetic Flux Rope Eruption Simulated by a Data-Driven Magnetohydrodynamic Model

63 citations · 66 across the 14 of their papers we have counts for

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Showing astro-ph.SRShow all

18 papers · 1 filter

astro-ph.SR2026

Kinematic Relationship Between Solar Extreme Ultraviolet Waves and Type II Metric Radio Bursts

Ramesh Chandra, Apoorv Dashora, P. F. Chen +1

Solar extreme-ultraviolet (EUV) waves are large-scale disturbances that manifest as bright wavefronts, often during coronal mass ejections (CMEs). According to the magnetic field l…

astro-ph.SR2026

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…

astro-ph.SR2026

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.…

astro-ph.SR2026

A Compact, Ultra-High Resolution VIPA Spectrograph for Solar Spectroscopic Observations: Astrocomb Characterization and First Light

Yutao Wang, Xiaoming Zhu, Xiaoli Yan +4

We present a compact, high spectral resolution prototype spectrograph based on a Virtually Imaged Phased Array (VIPA), which is designed for solar spectral observations. This fiber…

astro-ph.SR2026

An Improved HDBSCAN-based Detection and Tracking Method for Solar Active Regions in Magnetograms

C. X. Shi, Q. Hao, P. F. Chen +1

Solar active regions (ARs) are the primary source of solar eruptions and space weather. Accurate detection and tracking of ARs is crucial for understanding their evolution and pred…

astro-ph.SR2026

On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage

Jinhan Guo, Y. Guo, H. Wu +9

Observations show that many solar eruptions remain confined within strong overlying magnetic fields, forming a so-called magnetic cage. While confinement by poloidal overlying fiel…