NAOC Open IR  > 太阳物理研究部
Three super active regions in the descending phase of solar cycle 23
Zhang, HQ; Bao, XM; Zhang, Y; Liu, JH; Bao, SD; Deng, YY; Li, W; Chen, J; Dun, JP; Su, JT; Guo, J; Wang, XF; Hu, KL; Lin, GH; Wang, DG
2003-12-01
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
Volume3Issue:6Pages:491-494
AbstractWe analyze the magnetic configurations of three super active regions, NOAA 10484, 10486 and 10488, observed by the Huairou Multi-Channel Solar Telescope (MCST) from 2003 October 18 to November 4. Many energetic phenomena, such as flares (including a X-28 flare) and coronal mass ejections (CMEs), occurred during this period. We think that strong shear and fast emergence of magnetic flux are the main causes of these events. The question is also of great interest why these dramatic eruptions occurred so close together in the descending phase of the solar cycle.
KeywordSun : Activity Sun : Flares Sun : Magnetic Fields
Indexed BySCI
Language英语
WOS IDWOS:000187404500001
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8425
Collection太阳物理研究部
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Zhang, HQ,Bao, XM,Zhang, Y,et al. Three super active regions in the descending phase of solar cycle 23[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2003,3(6):491-494.
APA Zhang, HQ.,Bao, XM.,Zhang, Y.,Liu, JH.,Bao, SD.,...&Wang, DG.(2003).Three super active regions in the descending phase of solar cycle 23.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,3(6),491-494.
MLA Zhang, HQ,et al."Three super active regions in the descending phase of solar cycle 23".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 3.6(2003):491-494.
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