Limits to solar cycle predictability: Cross-equatorial flux plumes
文献类型：期刊论文
| 作者 | Cameron, R. H.1; Dasi-Espuig, M.1; Jiang, J.2 ; Isik, E.3; Schmitt, D.1; Schuessler, M.1
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| 刊名 | ASTRONOMY & ASTROPHYSICS
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| 出版日期 | 2013-09-01 |
| 卷号 | 557 |
| 关键词 | Sun: surface magnetism |
| 英文摘要 | Context. Within the Babcock-Leighton framework for the solar dynamo, the strength of a cycle is expected to depend on the strength of the dipole moment or net hemispheric flux during the preceding minimum, which depends on how much flux was present in each hemisphere at the start of the previous cycle and how much net magnetic flux was transported across the equator during the cycle. Some of this transport is associated with the random walk of magnetic flux tubes subject to granular and supergranular buffeting, some of it is due to the advection caused by systematic cross-equatorial flows such as those associated with the inflows into active regions, and some crosses the equator during the emergence process. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000325211900137 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6028]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | 1.Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China 3.Istanbul Kultur Univ, Fac Sci & Letters, Dept Phys, TR-34156 Istanbul, Turkey |
| 推荐引用方式 GB/T 7714 | Cameron, R. H.,Dasi-Espuig, M.,Jiang, J.,et al. Limits to solar cycle predictability: Cross-equatorial flux plumes[J]. ASTRONOMY & ASTROPHYSICS,2013,557. |
| APA | Cameron, R. H.,Dasi-Espuig, M.,Jiang, J.,Isik, E.,Schmitt, D.,&Schuessler, M..(2013).Limits to solar cycle predictability: Cross-equatorial flux plumes.ASTRONOMY & ASTROPHYSICS,557. |
| MLA | Cameron, R. H.,et al."Limits to solar cycle predictability: Cross-equatorial flux plumes".ASTRONOMY & ASTROPHYSICS 557(2013). |
入库方式： OAI收割
来源：国家天文台
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