Automatic Method for Identifying Photospheric Bright Points and Granules Observed by Sunrise
Mohsen Javaherian, Hossein Safari, Ali Amiri, Shervin Ziaei

TL;DR
This paper presents an automated method using image segmentation and machine learning to identify and analyze photospheric bright points and granules from UV solar observations, revealing their size, brightness, and velocity characteristics.
Contribution
The study introduces a novel automated approach combining region growing, mean shift segmentation, Zernike moments, and SVM classification for photospheric feature detection.
Findings
Power-law size distribution of BPs with slope -1.5
Granule sizes peak at about 0.5 arcsec^2
Mean filling factors: BPs 0.01, granules 0.51
Abstract
In this study, we propose methods for the automatic detection of photospheric features (bright points and granules) from ultra-violet (UV) radiation, using a feature-based classifier. The methods use quiet-Sun observations at 214 nm and 525 nm images taken by Sunrise on 9 June 2009. The function of region growing and mean shift procedure are applied to segment the bright points (BPs) and granules, respectively. Zernike moments of each region are computed. The Zernike moments of BPs, granules, and other features are distinctive enough to be separated using a support vector machine (SVM) classifier. The size distribution of BPs can be fitted with a power-law slope -1.5. The peak value of granule sizes is found to be about 0.5 arcsec^2. The mean value of the filling factor of BPs is 0.01, and for granules it is 0.51. There is a critical scale for granules so that small granules with sizes…
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.
