Dominance of Bursty over Steady Heating of the 4--8 MK Coronal Plasma in a Solar Active Region: Quantification using Maps of Minimum, Maximum, and Average Brightness

TL;DR

This study introduces a method to distinguish between bursty and steady heating in solar active region plasma by analyzing brightness maps over various timescales, revealing that most heating occurs in short bursts less than 30 minutes.

Contribution

The paper presents a novel approach using brightness maps and multiple timescales to quantify the dominance of bursty heating over steady heating in solar active regions.

Findings

Less than 5% of luminosity is from steady heating over 24 hours.

Up to 33% of luminosity is from steady heating over 30 minutes.

Most heating occurs in bursts shorter than 30 minutes.

Abstract

A challenge in characterizing active region (AR) coronal heating is in separating transient (bursty) loop heating from the diffuse background (steady) heating. We present a method of quantifying coronal heating's bursty and steady components in ARs, applying it to FeXVIII (hot94) emission of an AR observed by SDO/AIA. The maximum, minimum, and average brightness values for each pixel, over a 24 hour period, yield a maximum-brightness map, a minimum-brightness map, and an average-brightness map of the AR. Running sets of such three maps come from repeating this process for each time step of running windows of 20, 16, 12, 8, 5, 3, 1 and 0.5 hours. From each running window's set of three maps, we obtain the AR's three corresponding luminosity light curves. We find: (1) The time-averaged ratio of minimum-brightness-map luminosity to average-brightness-map luminosity increases as the time window decreases, and the time-averaged ratio of maximum-brightness-map luminosity to average-brightness-map luminosity decreases as the window decreases. (2) For the 24-hour window, the minimum-brightness map's luminosity is 5% of the average-brightness map's luminosity, indicating that at most 5% of the AR's hot94 luminosity is from heating that is steady for 24 hours. (3) This upper limit on the fraction of the hot94 luminosity from steady heating increases to 33% for the 30-minute running window. This requires that the heating of the 4--8 MK plasma in this AR is mostly in bursts lasting less than 30 minutes: at most a third of the heating is steady for 30 minutes.