Improving the performance of solar flare prediction using active longitudes information
文献类型：期刊论文
| 作者 | Huang, X.1 ; Zhang, L.1,2; Wang, H.1; Li, L.1
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| 刊名 | ASTRONOMY & ASTROPHYSICS
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| 出版日期 | 2013 |
| 卷号 | 549 |
| 关键词 | Sun: flares Sun: activity Sun: magnetic topology |
| 英文摘要 | Context. Solar flare prediction models normally depend on properties of active regions, such as sunspot area, McIntosh classifications, Mount Wilson classifications, and various measures of the magnetic field. Nevertheless, the positional information of active regions has not been used. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000313745000127 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6019]  |
| 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, Peoples R China 2.Univ Oulu, Dept Phys, Oulu, Finland |
| 推荐引用方式 GB/T 7714 | Huang, X.,Zhang, L.,Wang, H.,et al. Improving the performance of solar flare prediction using active longitudes information[J]. ASTRONOMY & ASTROPHYSICS,2013,549. |
| APA | Huang, X.,Zhang, L.,Wang, H.,&Li, L..(2013).Improving the performance of solar flare prediction using active longitudes information.ASTRONOMY & ASTROPHYSICS,549. |
| MLA | Huang, X.,et al."Improving the performance of solar flare prediction using active longitudes information".ASTRONOMY & ASTROPHYSICS 549(2013). |
入库方式： OAI收割
来源：国家天文台
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