太阳辐射量测量 太阳辐射量测量
1Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, 80303 USA.
概括
自1978年以来的太阳辐射量测量揭示了太阳周期的变化,并有助于了解气候影响. 现代仪器的目标是以气候驱动的准确度来检测长期太阳能趋势.
科学领域:
- 地球和太空科学 地球和太空科学
- 太阳物理 太阳物理
- 气候科学 气候科学
背景情况:
- 太阳是地球气候系统的主要能源.
- 自1978年以来,太阳辐射已经从太空中精确测量,覆盖了多个太阳周期.
- 了解太阳的变化对于气候建模和预测长期趋势至关重要.
研究的目的:
- 详细介绍太空太阳辐射仪器的功能和方法.
- 总结太阳辐射量测量和不同时间尺度上的变化.
- 讨论太阳辐射监测的未来方向和气候驱动的要求.
主要方法:
- 自1978年以来,一直在太空中测量太阳总辐射量 (TSI).
- 自1979年至2003年以来的光谱分辨率辐射量测量 (紫外线,近紫外线到近红外线).
- 对更长时间的太阳活动代理和模型的分析.
主要成果:
- 总太阳辐射 (TSI) 显示了短期 (天) 和太阳周期相关的变化 (~0.1%).
- 对光谱辐射的测量显示了太阳周期的变化.
- 现代仪器正在接近气候驱动的准确度来检测长期太阳能趋势.
结论:
- 从太空进行的测量提供了关于太阳辐射变量的准确数据.
- 太阳的变化影响了地球的气候系统在不同的时间尺度.
- 持续,精确的测量对于了解太阳对气候的影响至关重要.
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