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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