Revisiting Approaches to Stellar White-Light Flare Energy Based on Spatiotemporally Resolved Solar Observations

arXiv:2606.15913 · astro-ph.SR · Submitted 2026-06-14 · Read on arXiv

Yingjie Cai, Yijun Hou, Ting Li, Ying Li, Mingde Ding, Dechao Song, Changwen Zeng, Jifeng Liu

astro-ph.SR

Submitted: 2026-06-14

Comments: 13 pages, 5 figures, accepted for publication in ApJL

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Scaling Laws — 7× in this paper · explained in 4 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Atmospheric Imaging Assembly — 1× in this paper
• Calibration — 1× in this paper · explained in 7 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Helioseismic and Magnetic Imager — 1× in this paper
• Solar Dynamics Observatory — 1× in this paper

Sources

• Magnetic Evolution of Highly-Sheared Region in Active Region 13842 Producing Large X9.0 Flare

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