TL;DR
This paper introduces ASDA, an automated algorithm for detecting solar atmospheric swirls, demonstrating its effectiveness on synthetic and observational data, and analyzing swirl properties and detection challenges.
Contribution
The paper presents a novel automated swirl detection algorithm (ASDA) and applies it to both simulated and observational solar data, revealing new insights into swirl characteristics.
Findings
ASDA effectively detects swirls in noisy synthetic data.
Approximately 162,000 swirls are identified in the solar photosphere.
Detection accuracy depends on data resolution and noise levels.
Abstract
Swirling motions in the solar atmosphere have been widely observed in recent years and suggested to play a key role in channeling energy from the photosphere into the corona. Here, we present a newly-developed Automated Swirl Detection Algorithm (ASDA) and discuss its applications. ASDA is found to be very proficient at detecting swirls in a variety of synthetic data with various levels of noise, implying our subsequent scientific results are astute. Applying ASDA to photospheric observations with a spatial resolution of 39.2 km sampled by the Solar Optical Telescope (SOT) on-board Hinode, suggests a total number of swirls in the photosphere, with an average radius and rotating speed of km and km s, respectively. Comparisons between swirls detected in Bifrost numerical MHD simulations and both ground-based and space-borne observations, suggest…
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