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G. Rottman 《Space Science Reviews》2006,125(1-4):39-51
The Sun’s electromagnetic radiation powers our solar system. In the case of the Earth it heats the lands and ocean, maintains
our atmosphere, generates clouds, and cycles water. For other planets and minor bodies, similar and appropriate physical processes
occur, also powered by the Sun. The Sun varies on all time scales and a precise knowledge of the Sun's irradiance and its
variation is essential to our understanding of environments and physical conditions throughout our solar system. Measurements
of solar irradiance and its variation can only be made from space, and almost thirty years of observation have now established
that the total solar irradiance (TSI) varies by only 0.1 to 0.3%, while certain portions of the solar spectrum, the ultraviolet
for example, vary by orders of magnitude more. This paper provides an overview of TSI observations and of spectral irradiance
observations from the ultraviolet to the near infrared. 相似文献
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Space Science Reviews - 相似文献
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The Solar Stellar Irradiance Comparison Experiment (SOLSTICE) is one of ten instruments on the Upper Atmosphere Research Satellite (UARS) — one of two instruments measuring the solar ultraviolet irradiance. The instrument is a three channel spectrometer covering the spectral range 120 to 420nm with a spectral resolution of approximately 0.2nm. It has been successfully operating since October 1991, and has now provided more than eight years of data, extending from near the peak of solar cycle 22, through solar minimum and into the new cycle. The data provide time series that display solar variations over time scales from a few days up to the 11-year solar cycle. Quantitative estimates of amplitudes of both rotational modulation and the solar cycle variation in the 1991–1999 epoch are given for the UV spectrum between 119 and 300nm. 相似文献
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