Quiet Sun mini-CMEs activated by supergranular flows
D.E. Innes, A. Genetelli, R. Attie, H.E. Potts

TL;DR
This study investigates small eruptions in the quiet Sun, revealing they are triggered by supergranular flows and are similar to mini-CMEs, with a high occurrence rate and associated wave phenomena.
Contribution
It demonstrates that small-scale eruptions in the quiet Sun are activated by supergranular flows and provides an estimate of their occurrence rate and characteristics.
Findings
Eruptions occur at supergranular cell junctions.
Approximately 1400 events per day across the Sun.
One-third of eruptions are associated with waves.
Abstract
Context: The atmosphere of the quiet Sun is controlled by photospheric flows sweeping up concentrations of mixed polarity magnetic field. Along supergranule boundaries and junctions, there is a strong correlation between magnetic flux and bright chromospheric and transition region emission. Aim: The aim is to investigate the relationship between photospheric flows and small flare-like brightenings seen in Extreme Ultraviolet images. Method: We describe observations of small eruptions seen in quiet Sun images taken with the Extreme UltraViolet Imager (EUVI) on STEREO. The photospheric flows during the eruption build-up phase are investigated by tracking granules in high resolution MDI continuum images. Results: Eruptions with characteristics of small coronal mass ejections (CMEs) occur at the junctions of supergranular cells. The eruptions produce brightening at the onset site,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
