Manifestations of bright points observed in G-band and Ca II H by Hinode/SOT
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/18/i=10/a=125/pdf
Reference80 articles.
1. TURBULENT DIFFUSION IN THE PHOTOSPHERE AS DERIVED FROM PHOTOSPHERIC BRIGHT POINT MOTION
2. STATISTICAL DISTRIBUTION OF SIZE AND LIFETIME OF BRIGHT POINTS OBSERVED WITH THE NEW SOLAR TELESCOPE
3. THE SPATIAL AND TEMPORAL DEPENDENCE OF CORONAL HEATING BY ALFVÉN WAVE TURBULENCE
4. Magnetic properties of G-band bright points in a sunspot moat
5. On the Relation of G‐Band Bright Points to the Photospheric Magnetic Field
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1. Using Bright Point Shapes to Constrain Wave Heating of the Solar Corona: Predictions for DKIST;The Astrophysical Journal;2024-03-01
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3. Similarity measurement tracking and properties evolution of photospheric bright point groups in the quiet Sun and active region;Monthly Notices of the Royal Astronomical Society;2023-08-21
4. Research on Multiwavelength Isolated Bright Points Based on Deep Learning;The Astrophysical Journal;2021-04-01
5. Morphological Classification of G-band Bright Points Based on Deep Learning;The Astrophysical Journal;2019-12-16
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