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Substructure of quiet sun bright points

Published online by Cambridge University Press:  26 August 2011

Aleksandra Andic ,
Jongchul Chae  and
Phillip R. Goode
Aleksandra Andic
Affiliation:
BBSO, 40386 N. Shore Ln.Big Bear City, CA-92314, USA email: aandic@bbso.njit.edu
Jongchul Chae
Affiliation:
Astronomy Program, Department of Physics and Astronomy, Seoul National UniversitySeoul 151-741, Korea email: jcchae@snu.ac.kr
Phillip R. Goode
Affiliation:
BBSO, 40386 N. Shore Ln.Big Bear City, CA-92314, USA email: aandic@bbso.njit.edu
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Abstract

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Since photospheric bright points (BPs) were first observed, there has been a question as to how are they structured. Are they just single flux tubes or a bundle of the flux-tubes? Surface photometry of the quiet Sun (QS) has achieved resolution close to 0.1″ with the New Solar Telescope at Big Bear Solar Observatory. This resolution allowed us to detect a richer spectrum of BPs in the QS. The smallest BPs we observed with TiO 705.68 nm were 0.13″, and we were able to resolve individual components in some of the BPs clusters and ribbons observed in the QS, showing that they are composed of the individual BPs. Average size of observed BPs was 0.22″.

Keywords

Photospherebright points
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 339 - 342
Copyright
Copyright © International Astronomical Union 2011

References

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