机构:
CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
CAS, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Li, K. J.
[1
,2
]
Feng, W.
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机构:
Kunming Univ Sci & Technol, Res Ctr Anal & Measurement, Kunming 650093, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Feng, W.
[3
]
Xu, J. C.
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h-index: 0
机构:
CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
CAS, Grad Sch, Beijing 100863, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Xu, J. C.
[1
,4
]
Gao, P. X.
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机构:
CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Gao, P. X.
[1
]
Yang, L. H.
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h-index: 0
机构:
CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
CAS, Grad Sch, Beijing 100863, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Yang, L. H.
[1
,4
]
Liang, H. F.
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机构:
Yunnan Normal Univ, Dept Phys, Kunming 650093, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Liang, H. F.
[5
]
Zhan, L. S.
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机构:
Jingdezhen Ceram Inst, Jingdezhen 333001, Jiangxi, Peoples R ChinaCAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
Zhan, L. S.
[6
]
机构:
[1] CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
[2] CAS, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
[3] Kunming Univ Sci & Technol, Res Ctr Anal & Measurement, Kunming 650093, Peoples R China
[4] CAS, Grad Sch, Beijing 100863, Peoples R China
[5] Yunnan Normal Univ, Dept Phys, Kunming 650093, Peoples R China
[6] Jingdezhen Ceram Inst, Jingdezhen 333001, Jiangxi, Peoples R China
In order to probe the mechanism of variations of the solar constant on the inter-solar-cycle scale, the total solar irradiance (TSI; the so-called solar constant) in the time interval of 1978 November 7 to 2010 September 20 is decomposed into three components through empirical mode decomposition and time-frequency analyses. The first component is the rotation signal, counting up to 42.31% of the total variation of TSI, which is understood to be mainly caused by large magnetic structures, including sunspot groups. The second is an annual-variation signal, counting up to 15.17% of the total variation, the origin of which is not known at this point in time. Finally, the third is the inter-solar-cycle signal, counting up to 42.52%, which is inferred to be caused by the network magnetic elements in quiet regions, whose magnetic flux ranges from (4.27-38.01) x 10(19) Mx.