Reconstruction of solar irradiance variations in cycle 23: Is solar surface magnetism the cause?

被引：227

作者：

Krivova, NA ^{[1
]}

Solanki, SK

Fligge, A

Unruh, YC

机构：

[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany

[2] ETH Zentrum, Inst Astron, CH-8092 Zurich, Switzerland

[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, England

来源：

ASTRONOMY & ASTROPHYSICS | 2003年 / 399卷 / 01期

关键词：

solar-terrestrial relations; Sun : activity; Sun : faculae; Sun : magnetic fields; sunspots;

D O I：

10.1051/0004-6361:20030029

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A model of solar irradiance variations is presented which is based on the assumption that solar surface magnetism is responsible for all total irradiance changes on time scales of days to years. A time series of daily magnetograms and empirical models of the thermal structure of magnetic features (sunspots, faculae) are combined to reconstruct total (and spectral) irradiance from 1996 to 2002. Comparisons with observational data reveal an excellent correspondence, although the model only contains a single free parameter. This provides strong support for the hypothesis that solar irradiance variations are caused by changes in the amount and distribution of magnetic flux at the solar surface.

引用

页码：L1 / L4

页数：4

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