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太阳总辐照的演化特征分析
Alternative TitleEvolution Character Analysis of Total Solar Irradiance
向南彬1,2
Source Publication天文学报(Acta Astronomica Sinica)
2013-05
Volume54Issue:3Pages:219-228
DOI10.15940/j.cnki.0001-5245.2013.03.002
ClassificationP182
Contribution Rank第1完成单位
Indexed ByCSCD ; 核心
Keyword太阳:活动 太阳:黑子
Abstract

太阳总辐照在23和24太阳活动周的显著周期分别为35 d和26 d,进而推断太阳的准旋转周期在23和24太阳活动周也分别为35 d和26 d太阳总辐照在24周极小期的值可能与蒙德极小期的值相近.在一个太阳旋转周到几个月的时间尺度上,太阳黑子是引起太阳总辐照变化的主要原因,但不是唯一的原因;在几天到一个太阳旋转周的时间尺度上,太阳总辐照的变化与MgⅡ特征指数是不相关的.

Other Abstract

The significant periods of total solar irradiance are 35 days and 26 days in solar cycle 23 and 24, respectively. It is inferred that the solar quasi-rotation periods are 35 days and 26 days in solar cycle 23 and 24, respectively. The value of total solar irradiance in solar cycle 24 minimum should be close to the value of Maunder minimum. On short time scales, sunspots should be the main reason to cause variations of total solar irradiance on the scale of one solar rotation cycle to several months, but not the unique one, and the variations of total solar irradiance are not related with the Mg II index on the scale of a few days to one solar rotation cycle.

Funding Project国家自然科学基金项目[10921303] ; 国家自然科学基金项目[10583032] ; 973项目[2011CB811406] ; 973项目[2012CB957801]
Funding Organization国家自然科学基金项目[10921303, 10583032] ; 973项目[2011CB811406, 2012CB957801]
Language中文
Subject Area天文学 ; 太阳与太阳系
MOST Discipline Catalogue理学 ; 理学::天文学
ISSN0001-5245
Archive Date2013-08-20
CSCD IDCSCD:4870950
Citation statistics
Cited Times:2[CSCD]   [CSCD Record]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6495
Collection太阳物理研究组
Affiliation1.中国科学院云南天文台, 昆明, 650011
2.中国科学院大学, 北京, 100049
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
向南彬. 太阳总辐照的演化特征分析[J]. 天文学报(Acta Astronomica Sinica),2013,54(3):219-228.
APA 向南彬.(2013).太阳总辐照的演化特征分析.天文学报(Acta Astronomica Sinica),54(3),219-228.
MLA 向南彬."太阳总辐照的演化特征分析".天文学报(Acta Astronomica Sinica) 54.3(2013):219-228.
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