Count-based spectral component imaging (CCI) of solar flares in X-rays

arXiv:2609.17178 · astro-ph.SR, astro-ph.IM · Submitted 2026-09-15 · Read on arXiv

astro-ph.SR, astro-ph.IM

Submitted: 2026-09-15

Updated: 2026-09-15

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

Terminology

• Spectral Component Imaging — 7× in this paper
• Differential Emission Measure — 4× in this paper
• Hard X-ray Imager — 2× in this paper
• Inverse Problem — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• EMMA — 1× in this paper · explained in 2 episodes
• Reuven Ramaty High-Energy Solar Spectroscopic Imager — 1× in this paper

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?