Magnetic Reconnection Process in Partially Ionized Fluids: Insights from the Solar Chromosphere

arXiv:2607.28447 · astro-ph.SR · Submitted 2026-07-30 · Read on arXiv

Adrian R. Montañez-Lobo, Fabio D. Lora-Clavijo

astro-ph.SR

Submitted: 2026-07-30

Comments: 34 pages, 14 figures. Accepted for publication in Solar Physics

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

Terminology

• Accuracy — 2× in this paper · explained in 1 episode
• Consistency — 2× in this paper · explained in 3 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Active Regions — 1× in this paper · explained in 1 episode
• Ambipolar Diffusion — 1× in this paper · explained in 1 episode
• Dynamical regimes — 1× in this paper · explained in 2 episodes
• Interface Region Imaging Spectrograph — 1× in this paper

Sources

• The Interface Region Imaging Spectrograph (IRIS)
• Two-fluid Modeling of Acoustic Wave Propagation in Gravitationally Stratified Isothermal Media
• Coalescence Instability in Chromospheric Partially Ionised Plasmas
• A Family of ESDIRK Integration Methods

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