The Solar Irradiance Spectrum at Solar Activity Minimum Between Solar Cycles 23 and 24

被引：32

作者：

Thuillier, G. ^{[1
]}

Bolsee, D. ^{[2
]}

Schmidtke, G. ^{[3
]}

Foujols, T. ^{[1
]}

Nikutowski, B. ^{[3
,4
]}

Shapiro, A. I. ^{[5
]}

Brunner, R. ^{[3
]}

Weber, M. ^{[6
]}

Erhardt, C. ^{[3
]}

Herse, M. ^{[1
]}

Gillotay, D. ^{[2
]}

Peetermans, W. ^{[2
]}

Decuyper, W. ^{[2
]}

Pereira, N. ^{[2
]}

Haberreiter, M. ^{[5
]}

Mandel, H. ^{[7
]}

Schmutz, W. ^{[5
]}

机构：

[1] LATMOS CNRS, F-78280 Guyancourt, France

[2] Inst Aeron Spatiale Belgique, B-1180 Brussels, Belgium

[3] Fraunhofer Inst Phys Measuring Tech, D-79110 Freiburg, Germany

[4] Univ Leipzig, Inst Meteorol, D-04103 Leipzig, Germany

[5] World Radiat Ctr, Phys Meteorol Observ Davos, CH-7260 Davos, Switzerland

[6] Univ Bremen FB1, Inst Environm Phys IUP, D-28359 Bremen, Germany

[7] Landessternwarte Konigstuhl, Heidelberg, Germany

来源：

SOLAR PHYSICS | 2014年 / 289卷 / 06期

基金：

瑞士国家科学基金会;

关键词：

Solar spectrum; Solar minimum; Space Station; SolACES; SOLSPEC; SEMIEMPIRICAL MODELS; INSTRUMENT; ATMOSPHERE; SPECTROMETERS; CALIBRATION; OBJECTIVES; ONBOARD; INDEX; ISS;

D O I：

10.1007/s11207-013-0461-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

On 7 February 2008, the SOLAR payload was placed onboard the International Space Station. It is composed of three instruments, two spectrometers and a radiometer. The two spectrometers allow us to cover the 16 -aEuro parts per thousand 2900 nm spectral range. In this article, we first briefly present the instrumentation, its calibration and its performance in orbit. Second, the solar spectrum measured during the transition between Solar Cycles 23 to 24 at the time of the minimum is shown and compared with other data sets. Its accuracy is estimated as a function of wavelength and the solar atmosphere brightness-temperature is calculated and compared with those derived from two theoretical models.

引用

页码：1931 / 1958

页数：28

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