Dependence of the Continuum Intensities on the Magnetic Fields at Different Evolution Phases of Sunspots
文献类型:期刊论文
作者 | Li, Qiaoling4,5; Zhang, Li4; Yan XL(闫晓理)2,3; Norton, Aimee A.1; Wang JC(王金成)2,3; Yang LH(杨丽恒)2,3; Xue ZK(薛志科)2,3; Kong DF(孔德芳)2,3 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2022-09-01 |
卷号 | 936期号:1 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ac83b3 |
产权排序 | 第3完成单位 |
文献子类 | Article |
英文摘要 | The relationship between the continuum intensities and magnetic fields for stable and decaying sunspots is analyzed using the scattered-light-corrected data from the Helioseismic and Magnetic Imager. From our analysis, the main differences between stable and decaying sunspots are as follows. In the continuum intensity range from 0.35I (qs) to 0.65I (qs), where I (qs) is the continuum intensity of the quiet solar surface, the relationship between continuum intensity and transverse magnetic field and the relationship between continuum intensity and inclination display a much higher scatter during the decaying phase of the sunspots. During and after the formation of the light bridge, the scatter plots show a bifurcation that indicates that the two umbrae separated by the light bridge have different thermodynamic properties. The continuum intensity of the umbra in a decaying sunspot is brighter than that of the stable sunspot, indicating that the temperatures in the umbra of decaying sunspots are higher. Furthermore, our results show that the mean continuum intensity of the umbra gradually increases during the decay of the sunspot, but the mean continuum intensity of the penumbra remains constant. Simultaneously, the vertical and transverse magnetic field strengths in the umbra gradually decrease, and the vertical magnetic field strengths in the penumbra gradually increase. The changes in the umbra occur earlier than the changes in the penumbra of the decaying sunspot, suggesting that the umbral and penumbral decay may be an interdependent process during the decay of the sunspot. |
学科主题 | 天文学 ; 太阳与太阳系 ; 太阳物理学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | EVERSHED FLOW ; DECAY ; TEMPERATURE ; SPECTROSCOPY ; SIMULATIONS |
资助项目 | National Key R&D program of China[2018YFA0404204] ; National Science Foundation of China (NSFC)[11873087] ; Yunnan Science Foundation for Distinguished Young Scholars[202001AV070004] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:000847188100001 |
资助机构 | National Key R&D program of China[2018YFA0404204] ; National Science Foundation of China (NSFC)[11873087] ; Yunnan Science Foundation for Distinguished Young Scholars[202001AV070004] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25550] |
专题 | 云南天文台_抚仙湖太阳观测站 |
通讯作者 | Li, Qiaoling |
作者单位 | 1.HEPL Solar Physics, Stanford University, Stanford, CA 94305, USA 2.Yunnan Key Laboratory of Solar Physics and Space Science, 650216, People's Republic of China; 3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 4.Department of Astronomy, Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, People's Republic of China; lizhang@ynu.edu.cn; 5.Department of Physics, Yunnan University, Kunming 650091, People's Republic of China; liqiaoling@ynu.edu.cn; |
推荐引用方式 GB/T 7714 | Li, Qiaoling,Zhang, Li,Yan XL,et al. Dependence of the Continuum Intensities on the Magnetic Fields at Different Evolution Phases of Sunspots[J]. ASTROPHYSICAL JOURNAL,2022,936(1). |
APA | Li, Qiaoling.,Zhang, Li.,Yan XL.,Norton, Aimee A..,Wang JC.,...&Kong DF.(2022).Dependence of the Continuum Intensities on the Magnetic Fields at Different Evolution Phases of Sunspots.ASTROPHYSICAL JOURNAL,936(1). |
MLA | Li, Qiaoling,et al."Dependence of the Continuum Intensities on the Magnetic Fields at Different Evolution Phases of Sunspots".ASTROPHYSICAL JOURNAL 936.1(2022). |
入库方式: OAI收割
来源:云南天文台
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