Active region

In solar physics and observation, an active region is a temporary feature in the Sun's atmosphere characterized by a strong and complex magnetic field. They are often associated with sunspots and are commonly the source of violent eruptions such as coronal mass ejections and solar flares.[1] The number and location of active regions on the solar disk at any given time is dependent on the solar cycle.[2][3][4][5][6]

  1. ^ Zell, Holly (20 April 2015). "Active Regions on the Sun". NASA. Retrieved 18 July 2021.
  2. ^ Warren, Harry P.; Winebarger, Amy R.; Brooks, David H. (10 November 2012). "A Systematic Survey of High-Temperature Emission in Solar Active Regions". The Astrophysical Journal. 759 (2): 141. arXiv:1204.3220. Bibcode:2012ApJ...759..141W. doi:10.1088/0004-637X/759/2/141. S2CID 119117669.
  3. ^ Del Zanna, G. (October 2013). "The multi-thermal emission in solar active regions". Astronomy & Astrophysics. 558: A73. Bibcode:2013A&A...558A..73D. doi:10.1051/0004-6361/201321653.
  4. ^ Basu, Sarbani; Antia, H. M.; Bogart, Richard S. (August 2004). "Ring-Diagram Analysis of the Structure of Solar Active Regions". The Astrophysical Journal. 610 (2): 1157–1168. Bibcode:2004ApJ...610.1157B. doi:10.1086/421843.
  5. ^ Hagino, Masaoki; Sakurai, Takashi (25 October 2004). "Latitude Variation of Helicity in Solar Active Regions". Publications of the Astronomical Society of Japan. 56 (5): 831–843. doi:10.1093/pasj/56.5.831.
  6. ^ Zhang, Jie; Wang, Yuming; Liu, Yang (10 November 2010). "Statistical Properties of Solar Active Regions Obtained from an Automatic Detection System and the Computational Biases". The Astrophysical Journal. 723 (2): 1006–1018. Bibcode:2010ApJ...723.1006Z. doi:10.1088/0004-637X/723/2/1006. S2CID 122852367.