Large-scale solar cycle features of solar photospheric magnetic field | |
Song, W. B. | |
刊名 | Advances in Space Research |
2007 | |
卷号 | 39期号:11页码:1749-1752 |
关键词 | solar cycle photosphere solar magnetic field dynamo model flux |
ISSN号 | 0273-1177 |
通讯作者 | 北京8701信箱 |
英文摘要 | It is well accepted that the solar cycle originates from a magnetohydrodynamics dynamo deep inside the Sun. Many dynamo models have long been proposed based on a lot of observational constraints. In this paper, using 342 NSO/Kitt Peak solar synoptic charts we study the solar cycle phases in different solar latitudinal zones to set further constraints. Our results can be summarized as follows: (1) The variability of solar polar regions' area has a correlation with total unsigned magnetic flux in advance of 5 years. (2) The high-latitude region mainly appears unipolar in the whole solar cycle and its flux peak time lags sunspot cycle for 3 years. (3) For the activity belt, it is not surprised that its phase be the same as sunspot's. (4) The flux peak time of the low-latitude region shifts forward with an average gradient of 32.2 day/deg. These typical characteristics may provide some hints for constructing an actual solar dynamo. |
学科主题 | 空间物理 |
收录类别 | SCI |
原文出处 | http://www.sciencedirect.com/science?_ob=MImg&_imagekey=B6V3S-4MY6GF0-5-9&_cdi=5738&_user=1999492&_orig=search&_coverDate=12%2F31%2F2007&_sk=999609988&view=c&wchp=dGLbVzW-zSkzk&md5=f7b8a2b6c113e79255d4d759f46ecc68&ie=/sdarticle.pdf |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://ir.cssar.ac.cn/handle/122/1075] |
专题 | 国家空间科学中心_空间科学部 |
推荐引用方式 GB/T 7714 | Song, W. B.. Large-scale solar cycle features of solar photospheric magnetic field[J]. Advances in Space Research,2007,39(11):1749-1752. |
APA | Song, W. B..(2007).Large-scale solar cycle features of solar photospheric magnetic field.Advances in Space Research,39(11),1749-1752. |
MLA | Song, W. B.."Large-scale solar cycle features of solar photospheric magnetic field".Advances in Space Research 39.11(2007):1749-1752. |
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