Inter-correlation between Sunspot Oscillations and Their Internal Structures
Inter-correlation between Sunspot Oscillations and Their Internal Structures作者机构:Institute of Space Science and Applied TechnologyHarbin Institute of TechnologyShenzhen 518055China Faculty of Information Engineering and AutomationKunming University of Science and TechnologyKunming 650500China Institute of Solar-Terrestrial Physics SB RASLermontov st.126a664033IrkutskRussia
出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))
年 卷 期:2022年第22卷第11期
页 面:97-106页
核心收录:
学科分类:07[理学] 070401[理学-天体物理] 0704[理学-天文学]
基 金:supported by the National Natural Science Foundation of China(NSFC,Grant Nos.12173012 and 12111530078) the Shenzhen Technology project(GXWD20201230155427003-20200804151658001) supported by the Joint Funds of the NSFC(U1931107)
主 题:(Sun:)sunspots Sun:oscillations methods:data analysis
摘 要:Three-and five-minute oscillations are commonly observed in any *** they are modulated by the internal thermal and magnetic structures of a sunspot,they could be used as an effective tool for researching sunspot *** this paper,we investigate the properties of oscillations in sunspot groups with varying sizes and magnetic fields,and aim to establish the relationships between sunspot oscillations and its internal structure *** selected three groups of the unipolar sunspot with approximately axial-symmetric magnetic field and calculated their Fourier spectra based on the ultraviolet/extreme ultraviolet emission intensity variations recorded by the Solar Dynamics Observatory/Atmospheric Imaging *** found that the distribution of three-minute oscillation is defined by the joint effect of diverging magnetic field and the stratification of the sunspot *** distribution could be modified by any invading magnetic structures in the *** contrast,the five-minute oscillations are more prominent in small spots,implying that five-minute oscillation is very closely connected with umbral dynamics.