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Paper: Large-scale Structures in Distribution of Coronal Bright Points
Volume: 346, Large-scale Structures and their Role in Solar Activity
Page: 363
Authors: Sattarov, I.; Pevtsov, A.; Karachik, N.; Sattarova, B.
Abstract: We use an automatic procedure to find coronal bright points (BPs) in EIT 195Å data observed in 1996 near deep minimum of solar activity. Identifying BPs as bright features with EUV flux above 80 DN/s and diameter about 2.6 — 58 arcsec, we find about 463±22 BPs per solar disk. We also uncover small intensity fluctuations of diffuse corona surrounding the BPs. The intensity fluctuations correlate with BP brightness: increase in brightness of BPs causes increase in coronal intensity.
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