Automated detection and tracking of solar magnetic bright points

25Citations
Citations of this article
10Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Magnetic bright points (MBPs) in the internetwork are among the smallest objects in the solar photosphere and appear bright against the ambient environment. An algorithm is presented that can be used for the automated detection of the MBPs in the spatial and temporal domains. The algorithm works by mapping the lanes through intensity thresholding. A compass search, combined with a study of the intensity gradient across the detected objects, allows the disentanglement of MBPs from bright pixels within the granules. Object growing is implemented to account for any pixels that might have been removed when mapping the lanes. The images are stabilized by locating long-lived objects that may have been missed due to variable light levels and seeing quality. Tests of the algorithm, employing data taken with the Swedish Solar Telescope, reveal that ≈90 per cent of MBPs within a 75 × 75 arcsec2 field of view are detected. © 2009 The Authors. Journal compilation © 2009 RAS.

Cite

CITATION STYLE

APA

Crockett, P. J., Jess, D. B., Mathioudakis, M., & Keenan, F. P. (2009). Automated detection and tracking of solar magnetic bright points. Monthly Notices of the Royal Astronomical Society, 397(4), 1852–1861. https://doi.org/10.1111/j.1365-2966.2009.15083.x

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free