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Two types of coronal bright points their characteristics, and evolution

  • Isroil Sattarov (a1), Nina V. Karachik (a2), Chori T. Sherdanov (a3), Azlarxon M. Tillaboev (a1) and Alexei A. Pevtsov (a2)...

Abstract

Using maximum brightness of coronal bright point's (CBP) as a criterion, we separate them on two categories: dim CBPs, associated with areas of a quiet Sun, and bright CBPs, associated with an active Sun. This study reports on characteristics of two types of CBPs and their evolution.

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References

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Golub, L., Krieger, A. S., & Vaiana, G. S. 1975, Solar Phys., 42, 131
McIntosh, S. W. & Gurman, J. B. 2005, Solar Phys., 228, 285
Sattarov, I., Pevtsov, A. A., Karachik, N. V., Sherdanov, C. T., & Tillaboev, A. M. 2010, Solar Phys., 262, 321
Sattarov, I., Pevtsov, A. A., Karachik, N. V., & Sherdanov, C. T. 2007, Adv. Sp. Res. 39, 1777
Sattarov, I., Pevtsov, A. A., Karachik, N. V., & Sattarova, B. J. 2005a, ASP Conf. Ser., 346, 363
Sattarov, I., Pevtsov, A. A., Karachik, N. V., & Sattarova, B. J. 2005b, ASP Conf. Ser., 346, 395
Sattarov, I., Pevtsov, A. A., Hojaev, A. S., & Sherdonov, C. T. 2002, Astrophys. J., 564, 1042
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