Characterising motion types of G-band bright points in the quiet Sun
Yun-Fei Yang, Hui-Xue Qu, Kai-Fan Ji, Song Feng, Hui Deng, Jia-Ben Lin, and Feng Wang

TL;DR
This study classifies G-band bright point motions in the quiet Sun into straight, rotary, and erratic types, revealing distinct velocities and diffusive behaviors using high-resolution Hinode/SOT data.
Contribution
It introduces an automatic tracking method and a new categorization of GBP motions based on an index, providing detailed velocity and diffusion characteristics for each motion type.
Findings
Straight motion GBPs have higher, constant velocities.
Diffusive processes vary: ballistic, super, and sub diffusion.
Motion directions are homogeneous and isotropic.
Abstract
We study the motions of G band bright points (GBPs) in the quiet Sun to obtain the characteristics of different motion types. A high resolution image sequence taken with the Hinode/Solar Optical Telescope (SOT) is used, and GBPs are automatically tracked by segmenting 3D evolutional structures in a space time cube. After putting the GBPs that do not move during their lifetimes aside, the non stationary GBPs are categorized into three types based on an index of motion type. Most GBPs that move in straight or nearly straight lines are categorized into a straight motion type, a few moving in rotary paths into a rotary motion, and the others fall into a motion type we called erratic. The mean horizontal velocity is 2.18 km/s, 1.63 km/s and 1.33 km/s for straight, erratic and rotary motion type, respectively. We find that a GBP drifts at a higher and constant velocity during its whole life…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
