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The Magnetic Origin of Solar Campfires View all abstracts by submitter

Navdeep Panesar   Submitted: 2021-11-18 10:47

Solar campfires are fine-scale heating events, recently observed by Extreme Ultraviolet Imager (EUI) on board Solar Orbiter. Here we use EUI 174 images, together with EUV images from Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA), and line-of-sight magnetograms from SDO/Helioseismic and Magnetic Imager (HMI) to investigate the magnetic origin of 52 randomly selected campfires in the quiet solar corona. We find that (i) the campfires are rooted at the edges of photospheric magnetic network lanes; (ii) most of the campfires reside above the neutral line between majority-polarity magnetic flux patch and a merging minority-polarity flux patch, with a flux cancelation rate of ~1018 Mx hr-1; (iii) some of the campfires occur repeatedly from the same neutral line; (iv) in the large majority of instances, campfires are preceded by a cool-plasma structure, analogous to minifilaments in coronal jets; and (v) although many campfires have "complex" structure, most campfires resemble small-scale jets, dots, or loops. Thus, "campfire" is a general term that includes different types of small-scale solar dynamic features. They contain sufficient magnetic energy (~1026-1027 erg) to heat the solar atmosphere locally to 0.5-2.5 MK. Their lifetimes range from about 1 minute to over 1 hr, with most of the campfires having a lifetime of <10 minutes. The average lengths and widths of the campfires are 5400 2500 km and 1600 640 km, respectively. Our observations suggest that (a) the presence of magnetic flux ropes may be ubiquitous in the solar atmosphere and not limited to coronal jets and larger-scale eruptions that make CMEs, and (b) magnetic flux cancelation is the fundamental process for the formation and triggering of most campfires.

Authors: Panesar, Navdeep K.,Tiwari, Sanjiv K.; Berghmans, David; Cheung, Mark C. M; Mueller, Daniel; Auchere, Frederic; and Zhukov, Andrei
Projects: SDO-AIA,SDO-HMI,SO/EUI

Publication Status: Published in ApJ Leetters
Last Modified: 2021-11-20 20:07
Go to main E-Print page  Implications of spicule activity on coronal loop heating and catastrophic cooling  On the evolution of a sub-C class flare: a showcase for the capabilities of the revamped Catania Solar Telescope  Edit Entry  Download Preprint  Delete Entry 

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