Analysis of X1.3 Flare Events in the Solar Active Region AR 12975
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Hans Publishers
Reference28 articles.
1. Stability of the coronal magnetic field around large confined and eruptive solar flares
2. Numerical MHD simulations of solar flares and their associated small-scale structures
3. The Link between Nonthermal Velocity and Free Magnetic Energy in Solar Flares
4. What Are the Causes of Super Activity of Solar Active Regions?
5. Study of Reconnection Dynamics and Plasma Relaxation in MHD Simulation of a Solar Flare
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