Dynamical and thermal evolution of localized reconnecting current sheets under varying guide-fields in the solar corona
astro-ph.SR
Submitted: 2026-10-13
Updated: 2026-10-13
Comments: 19 pages, 15 figures, Accepted for publication in Astronomy and Astrophysics
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- A comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere
- The SOHO LASCO CME Catalog -- Version 2
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
- Finite-Element Asteroseismology I: Two-Dimensional Adiabatic Oscillations of Rapidly Rotating N=3 Polytropes
- Constraining the origin of magnetic white dwarfs
- EPRV Asteroseismology of the K dwarfs GJ 570 A and GJ 783 A with ESPRESSO. Empirical mode-amplitude scaling in tension with 3D convection simulations
- JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting