Forward Modeling Transient Brightenings and Microflares around an Active Region Observed with Hi-C
Adam R. Kobelski, David E. McKenzie

TL;DR
This study uses high-resolution EUV observations from Hi-C to analyze small-scale brightenings around active regions, revealing frequent, strand-like microflares likely caused by bursty reconnection, advancing understanding of coronal heating.
Contribution
It demonstrates that microflares are more frequent and involve smaller strands than previously observed, supporting bursty reconnection as a key energy release mechanism.
Findings
Microflares occur much more frequently than expected.
Events are likely made from strands about 100 km wide.
Multiple heating events per strand suggest impulsive heating processes.
Abstract
Small scale flare-like brightenings around active regions are among the smallest and most fundamental of energetic transient events in the corona, providing a testbed for models of heating and active region dynamics. In a previous study, we modeled a large collection of these microflares observed with Hinode/XRT using EBTEL and found that they required multiple heating events, but could not distinguish between multiple heating events on a single strand, or multiple strands each experiencing a single heating event. We present here a similar study, but with EUV data of Active Region 11520 from the High Resolution Coronal Imager (Hi-C) sounding rocket. Hi- C provides an order of magnitude improvement to the spatial resolution of XRT, and a cooler temperature sensitivity, which combine to provide significant improvements to our ability to detect and model microflare activity around active…
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.
