Characterizing the Umbral Magnetic Knots of $\delta$-Sunspots
A. A. Norton, P. J. Levens, K. J. Knizhnik, M. G. Linton, Y. Liu

TL;DR
This study introduces the degree of delta (Doδ) to quantify magnetic flux participation in delta sunspots, revealing their dynamic properties, formation mechanisms, and strong association with flare activity.
Contribution
The paper presents a new metric, Doδ, to analyze delta sunspot magnetic knots, providing insights into their formation, dynamics, and relation to flare energy, based on extensive observational data.
Findings
Delta regions are active as delta-spots 55% of the time with high flux participation.
Delta-spots exhibit significantly higher flux, emergence rate, rotation, and flare energy than beta-spots.
Most delta-spots are formed by single flux emergence events and show diverse formation mechanisms.
Abstract
Delta ()-spots are active regions (ARs) in which positive and negative umbrae share a penumbra. They are known to be the source of strong flares. We introduce a new quantity, the degree of (Do), to measure the fraction of umbral flux participating in the -configuration and to isolate the dynamics of the magnetic knot, i.e. adjacent umbrae in the -configuration. Using Helioseismic and Magnetic Imager data, we analyze 19 -spots and 11 -spots in detail, and 120 -spots in less detail. We find that -regions are not in a -configuration for the entire time but spend 55 of their observed time as -spots with an average, maximum Do of 72. Compared to -spots, -spots have 2.6 the maximum umbral flux, 1.9 the flux emergence rate, 2.6 the rotation, and…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
