Extreme Ultraviolet Microflashes at Plume Bases: A Candidate for Powering the Corona and Solar Wind?

arXiv:2606.17361 · astro-ph.SR · Submitted 2026-06-15 · Read on arXiv

Navdeep K. Panesar, Sanjiv K. Tiwari, Meng Jin, Ayla Weitz, Ronald L. Moore, V. Aparna, Alphonse Sterling

astro-ph.SR

Submitted: 2026-06-15

Comments: 21 pages, 12 Figures

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

Terminology

• Active Regions — 3× in this paper · explained in 1 episode
• Core — 2× in this paper · explained in 2 episodes
• Solar Dynamics Observatory — 2× in this paper
• Adam — 1× in this paper · explained in 2 episodes
• Extreme Ultravoilet Imager — 1× in this paper
• Potential Field Source Surface — 1× in this paper

Sources

• Co-existence of longitudinal and transverse oscillations in polar plumes observed with Solar Orbiter/EUI

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