Correlation Function Analysis between Sunspot Cycle Amplitudes and Rise Times
文献类型：期刊论文
| 作者 | Du, Zhanle ; Wang, Huaning; Zhang, Liyun
|
| 刊名 | SOLAR PHYSICS
 |
| 出版日期 | 2009-03-01 |
| 卷号 | 255期号:1页码:179-185 |
| 关键词 | Sunspots, statistics Solar cycle, models |
| 英文摘要 | The running cross-correlation coefficient between solar-cycle amplitudes and rise times at a certain cycle lag is found to vary in time, when using the smoothed monthly-mean sunspot group numbers available for 1610 -aEuro parts per thousand 1995. It may be negative or positive for different periods of time. The Waldmeier effect (in which the rise times decrease with amplitude) is also found to be very weak for some cycles. This result represents an observational constraint on solar-dynamo models and can help us better understand the long-term evolution of solar activity. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000263649900013 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/7943]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Du, Zhanle,Wang, Huaning,Zhang, Liyun. Correlation Function Analysis between Sunspot Cycle Amplitudes and Rise Times[J]. SOLAR PHYSICS,2009,255(1):179-185. |
| APA | Du, Zhanle,Wang, Huaning,&Zhang, Liyun.(2009).Correlation Function Analysis between Sunspot Cycle Amplitudes and Rise Times.SOLAR PHYSICS,255(1),179-185. |
| MLA | Du, Zhanle,et al."Correlation Function Analysis between Sunspot Cycle Amplitudes and Rise Times".SOLAR PHYSICS 255.1(2009):179-185. |
入库方式： OAI收割
来源：国家天文台
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