Analysis of Different Solar Spectral Irradiance Reconstructions and Their Impact on Solar Heating Rates

被引:16
|
作者
Thuillier, G. [1 ]
Melo, S. M. L. [2 ,3 ]
Lean, J. [4 ]
Krivova, N. A. [5 ]
Bolduc, C. [6 ]
Fomichev, V. I. [7 ]
Charbonneau, P. [6 ]
Shapiro, A. I. [8 ]
Schmutz, W. [8 ]
Bolsee, D. [9 ]
机构
[1] LATMOS CNRS, F-78280 Guyancourt, France
[2] Univ Toronto, Dept Phys, Toronto, ON, Canada
[3] Canadian Space Agcy, St Hubert, PQ J3Y 8Y9, Canada
[4] Naval Res Lab, Div Space Sci, Washington, DC 20375 USA
[5] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
[6] Univ Montreal, Dept Phys, Montreal, PQ H2C 3J7, Canada
[7] York Univ, Dept Earth & Space Sci & Engn, Toronto, ON M3J 1P3, Canada
[8] PMOD WRC, Davos, Switzerland
[9] Inst Aeron Spatiale, B-1180 Uccle, Belgium
基金
瑞士国家科学基金会;
关键词
Solar spectral irradiance model; Reconstruction; MIDDLE ATMOSPHERE; MODEL; EVOLUTION; PARAMETERIZATION; VARIABILITY; DEPENDENCE; SOLSTICE; ENERGY; CYCLE;
D O I
10.1007/s11207-013-0381-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Proper numerical simulation of the Earth's climate change requires reliable knowledge of solar irradiance and its variability on different time scales, as well as the wavelength dependence of this variability. As new measurements of the solar spectral irradiance have become available, so too have new reconstructions of historical solar irradiance variations, based on different approaches. However, these various solar spectral irradiance reconstructions have not yet been compared in detail to quantify differences in their absolute values, variability, and implications for climate and atmospheric studies. In this paper we quantitatively compare five different reconstructions of solar spectral irradiance changes during the past four centuries, in order to document and analyze their differences. The impact on atmosphere and climate studies is discussed in terms of the calculation of short wave solar heating rates.
引用
收藏
页码:1115 / 1142
页数:28
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