Investigation of Umbral Dots with the New Vacuum Solar Telescope
Kaifan Ji, Xia Jiang, Song Feng, Yunfei Yang, Hui Deng, Feng Wang

TL;DR
This study investigates the properties of umbral dots in sunspots using high-resolution images and magnetic field data, revealing how their characteristics depend on magnetic field strength.
Contribution
It provides new insights into how umbral dot properties vary with magnetic field strength and distinguishes differences between central and peripheral UDs.
Findings
UD diameters and lifetimes increase with brightness
UD velocities are unaffected by brightness
UD properties depend on surrounding magnetic field strength
Abstract
Umbral dots (UDs) are small isolated brightenings observed in sunspot umbrae. They are convective phenomena existing inside umbrae. UDs are usually divided into central UDs (CUDs) and peripheral UDs (PUDs) according to their positions inside an umbra. Our purpose is to investigate UD properties and analyze their relationships, and further to find whether or not the properties depend on umbral magnetic field strengths. Thus, we selected high-resolution TiO images of four active regions (ARs) taken under the best seeing conditions with the \textit{New Vacuum Solar Telescope} in the Fuxian Solar Observatory of the Yunnan Astronomical Observatory, China. The four ARs (NOAA 11598, 11801, 12158, and 12178) include six sunspots. A total of 1220 CUDs and 603 PUDs were identified. Meanwhile, the radial component of the vector magnetic field of the sunspots taken with the \textit{Helioseismic and…
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