Decay Length of Slow Magnetoacoustic Waves in the Solar Corona using SDO/AIA and SolO/EUI

arXiv:2607.25509 · astro-ph.SR · Submitted 2026-07-28 · Read on arXiv

R. L. Meadowcroft, N. Narang, D. Berghmans, M. Dominique, V. M. Nakariakov

astro-ph.SR

Submitted: 2026-07-28

Comments: Accepted for publication in Philosophical Transactions of the Royal Society A

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

Terminology

• Alignment — 5× in this paper · explained in 1 episode
• Royal Observatory of Belgium — 3× in this paper
• Atmospheric Imaging Assembly — 2× in this paper
• Active Regions — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Interactive Data Language — 1× in this paper
• Ministry of Education — 1× in this paper
• Sunspot-Oscillations Solar Orbiter Observing Plan — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

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?