首页> 外文期刊>Surveys in Geophysics: An International Review Journal of Geophysics and Planetary Sciences >Understanding and Measuring Earth's Energy Budget: From Fourier, Humboldt, and Tyndall to CERES and Beyond
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Understanding and Measuring Earth's Energy Budget: From Fourier, Humboldt, and Tyndall to CERES and Beyond

机译:理解和衡量地球的能源预算:从傅里叶,洪堡和廷德尔到CERES甚至更远

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摘要

This historical perspective on the determination of Earth's energy fluxes, beginning with the classical description of climate, outlines the establishment of the basic physics of the Earth climate system in the nineteenth century. After recalling the early twentieth century ground-based attempts to determine the Earth's energy budget, I review the growing contributions of observations from space to quantifying these exchanges. In particular, space observations have shown that variations of solar luminosity have been extremely small (of order 0.1%) over past decades and probably past centuries and that they play practically no role in present-day climate variations or variations that may be expected in coming decades. Overall geographical structure, diurnal and seasonal cycles, and some of the interannual and interdecadal variations of Earth's energy exchanges with the Sun and space are now quite well determined, but much remains to be done regarding, on the one hand, fluxes at the surface and, on the other hand, variations of clouds. Improvements are essential if scientific assessment of anthropogenic climate change risk is to keep up with the changes themselves.
机译:从确定气候的经典角度出发,这种关于确定地球能量通量的历史观点概述了19世纪地球气候系统的基本物理学的建立。在回顾20世纪初基于地面的确定地球能源预算的尝试之后,我回顾了太空观测对量化这些交换的日益增长的贡献。特别是,太空观测表明,过去几十年甚至可能是几个世纪以来,太阳光度的变化非常小(大约为0.1%),并且它们在当今的气候变化或未来可能发生的变化中几乎不起作用。几十年。总体地理结构,昼夜和季节周期,以及地球与太阳和空间交换能量的年际和年代际变化现在已经很确定了,但一方面,关于表面和地面通量的通量还有很多工作要做。另一方面,云的变化。如果要对人为气候变化风险进行科学评估以适应变化本身,则必须进行改进。

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