Origin of small-scale evaporation flows deep in the chromosphere during a solar flare
astro-ph.SR, physics.plasm-ph, physics.space-ph
Submitted: 2026-08-30
Updated: 2026-09-11
Comments: Accepted for publication in the Astrophysical Journal Letters (Issue: Sunrise III Early Science)
Code: https://github.com/han-uitenbroek/RH
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
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?