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WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?
Xiang NB(向南彬)1,2,3; Kong DF(孔德芳)1,2; Xiang, NB (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊ASTRONOMICAL JOURNAL
2015-12
卷号150期号:6
DOI10.1088/0004-6256/150/6/171
产权排序第1完成单位
收录类别SCI
关键词Sun: Activity Sun: General Sun: Magnetic Fields
摘要The Physikalisch Meteorologisches Observatorium Davos total solar irradiance (TSI), Active Cavity Radiometer Irradiance Monitoring TSI, and Royal Meteorological Institute of Belgium TSI are three typical TSI composites. Magnetic Plage Strength Index (MPSI) and Mount Wilson Sunspot Index (MWSI) should indicate the weak and strong magnetic field activity on the solar full disk, respectively. Cross-correlation (CC) analysis of MWSI with three TSI composites shows that TSI should be weakly correlated with MWSI, and not be in phase with MWSI at timescales of solar cycles. The wavelet coherence (WTC) and partial wavelet coherence (PWC) of TSI with MWSI indicate that the inter-solar-cycle variation of TSI is also not related to solar strong magnetic field activity, which is represented by MWSI. However, CC analysis of MPSI with three TSI composites indicates that TSI should be moderately correlated and accurately in phase with MPSI at timescales of solar cycles, and that the statistical. significance. test indicates that the correlation coefficient of three TSI composites with MPSI is statistically significantly higher than that of three TSI composites with MWSI. Furthermore, the cross wavelet transform (XWT) and WTC of TSI with MPSI show that the TSI is highly related and actually in phase with MPSI at a timescale of a solar cycle as well. Consequently, the CC analysis, XWT, and WTC indicate that the solar weak magnetic activity on the full disk, which is represented by MPSI, dominates the inter-solar-cycle variation of TSI.
项目资助者National Natural Science Foundation of China(11273057,11221063) ; 973 programs(2012CB957801,2011CB811406) ; Chinese Academy of Sciences ; NASA ; ONR ; NSF ; Mount Wilson Institute
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-6256
URL查看原文
归档日期2015-11-10
WOS记录号WOS:000366588600006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]MOUNT-WILSON ; WAVELET TRANSFORM ; ACTIVITY INDEXES ; MAGNETIC-FIELDS ; POLAR FACULAE ; VARIABILITY ; RECONSTRUCTION ; CLIMATE ; TREND ; MAGNETOGRAMS
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被引频次:10[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9389
专题太阳物理研究组
通讯作者Xiang, NB (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
2.University of Chinese Academy of Sciences, Beijing 100049, China
3.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China
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Xiang NB,Kong DF,Xiang, NB . WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?[J]. ASTRONOMICAL JOURNAL,2015,150(6).
APA Xiang NB,Kong DF,&Xiang, NB .(2015).WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?.ASTRONOMICAL JOURNAL,150(6).
MLA Xiang NB,et al."WHAT CAUSES THE INTER-SOLAR-CYCLE VARIATION OF TOTAL SOLAR IRRADIANCE?".ASTRONOMICAL JOURNAL 150.6(2015).
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