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sunstotalirradiancereconstructionbasedonmultiplesolarindices
Zhao Juan2; Han Yanben1
刊名sciencechinaphysicsmechanicsastronomy
2012
卷号55期号:1页码:179
ISSN号1674-7348
英文摘要In order to uncover a possible influence on the Earth's climate, we need a much longer time series, i.e., the total solar irradiance (TSI) which is also an interesting issue in its own right in solar physics. By comparing different solar indices associated with TSI during the period 1979 to 2009, several empirical models in the TSI are presented. We verify that the reconstruction model based on the three variables: sunspot number, sunspot area, and solar 10.7 cm radio flux, is the best one. As demonstrated by model calculations, the history of TSI was reconstructed back to 1947 based on 3-indices and to 1874 based on 2-indices, respectively. The reason that the reduced irradiance on the trough during 2006 to 2009 lasts long may be due to the about 85-year cycle of solar activity, which modulates the intensity of the 11-year cycle (Schwabe cycles), possesses a considerable potential to produce an effective reducing, and holds on a steadily lower level of irradiance.
资助项目[National Natural Science Foundation of China] ; [Excellent Scientists Training Program of Beijing]
语种英语
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/48039]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.北京师范大学
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Zhao Juan,Han Yanben. sunstotalirradiancereconstructionbasedonmultiplesolarindices[J]. sciencechinaphysicsmechanicsastronomy,2012,55(1):179.
APA Zhao Juan,&Han Yanben.(2012).sunstotalirradiancereconstructionbasedonmultiplesolarindices.sciencechinaphysicsmechanicsastronomy,55(1),179.
MLA Zhao Juan,et al."sunstotalirradiancereconstructionbasedonmultiplesolarindices".sciencechinaphysicsmechanicsastronomy 55.1(2012):179.
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