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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/102107


    題名: A statistical study of the subsurface structure and eruptivity of solar active regions
    作者: 林佳賢;Lin, C.-H.
    貢獻者: 地球科學學院太空科學與工程學系
    關鍵詞: Adiabatic flow;Astrobiology;Astronomy;Astronomy and Astrophysics;Astrophysics;Astrophysics and Astroparticles;Corona;Correlation;Correlation coefficient;Cosmology;Disturbances;Flares;Kinetic energy;Magnetic fields;Observations and Techniques;Original Article;Physics;Samples;Solar physics;Space and Planetary Science;Space Exploration and Astronautics;Space Sciences (including Extraterrestrial Physics;Statistical analysis;Statistical methods;Sun;Trends
    日期: 2014-01-01
    上傳時間: 2026-04-23 11:03:02 (UTC+8)
    出版者: Springer Netherlands;Dordrecht: Springer Science and Business Media LLC
    摘要: 摘要: A statistical study of 77 solar active regions (ARs) is conducted to investigate the existence of identifiable correlations between the subsurface structural disturbances and the activity level of the active regions. The disturbances examined in this study are 〈| δΓ 1 / Γ 1 |〉, 〈| δc 2 / c 2 |〉, and 〈| δc 2 / c 2 − δΓ 1 / Γ 1 |〉, where Γ 1 and c are the thermodynamic properties of first adiabatic index and sound speed modified by magnetic field, respectively. The averages are over three depth layers: 0.975–0.98 R ⊙ , 0.98–0.99 R ⊙ and 0.99–0.995 R ⊙ to represent the structural disturbances in that layer. The level of the surface magnetic activity is measured by the Magnetic Activity Index (MAI) of active region and the relative and absolute MAI differences (rdMAI and dMAI) between the active and quiet regions. The eruptivity of each active region is quantified by its Flare Index, total number of coronal mass ejections (CMEs), and total kinetic energy of the CMEs. The existence and level of the correlations are evaluated by scatter plots and correlation coefficients. No definitive correlation can be claimed from the results. While a weak positive trend is visible between dMAI and 〈| δΓ 1 / Γ 1 |〉 and 〈| δc 2 / c 2 |〉 in the layer 0.975–0.98 R ⊙ , their correlation levels, being approximately 0.6, are not sufficiently high to justify the correlation. Some subsurface disturbances are seen to increase with eruptivity indices among ARs with high eruptivity. The statistical significance of such trend, however, cannot be ascertained due to the small number of very eruptive ARs in our sample.
    其他題名: Astrophys Space Sci
    出版者: Dordrecht: Springer Science and Business Media LLC
    出版日期: 2014-08-01
    出處: Astrophysics and Space Science, 2014-08, Vol.352 (2), p.361-371
    資源來源: Springer Nature Link Journals
    版權: The Author(s) 2014
    版權: Springer Science+Business Media Dordrecht 2014
    識別號: ISSN: 0004-640X
    識別號: ISSN: 1572-946X
    識別號: EISSN: 1572-946X
    識別號: DOI: 10.1007/s10509-014-1931-x
    顯示於類別:[太空科學與工程學系] 期刊論文

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