Modeling solar cycles 15 to 21 using a flux transport dynamo
文献类型：期刊论文
| 作者 | Jiang, J.1 ; Cameron, R. H.2; Schmitt, D.2; Isik, E.3
|
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2013-05-01 |
| 卷号 | 553 |
| 关键词 | magnetohydrodynamics (MHD) Sun: dynamo Sun: surface magnetism |
| 英文摘要 | Context. The Sun's polar fields and open flux around the time of activity minima have been considered to be strongly correlated with the strength of the subsequent maximum of solar activity. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000319858700128 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6005]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China 2.Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany 3.Istanbul Kultur Univ, Fac Sci & Letters, Dept Phys, TR-34156 Istanbul, Turkey |
| 推荐引用方式 GB/T 7714 | Jiang, J.,Cameron, R. H.,Schmitt, D.,et al. Modeling solar cycles 15 to 21 using a flux transport dynamo[J]. ASTRONOMY & ASTROPHYSICS,2013,553. |
| APA | Jiang, J.,Cameron, R. H.,Schmitt, D.,&Isik, E..(2013).Modeling solar cycles 15 to 21 using a flux transport dynamo.ASTRONOMY & ASTROPHYSICS,553. |
| MLA | Jiang, J.,et al."Modeling solar cycles 15 to 21 using a flux transport dynamo".ASTRONOMY & ASTROPHYSICS 553(2013). |
入库方式： OAI收割
来源：国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。