Wild Martin, Hakuba Maria Z, Folini Doris, Dörig-Ott Patricia, Schär Christoph, Kato Seiji, Long Charles N
1Institute for Atmospheric and Climate Science, ETH Zurich, 8001 Zurich, Switzerland.
2Department of Atmospheric Sciences, Colorado State University, Ft Collins, CO 80523 USA.
Clim Dyn. 2019;52(7):4787-4812. doi: 10.1007/s00382-018-4413-y. Epub 2018 Aug 21.
In recent studies we quantified the global mean Earth energy balance based on direct observations from surface and space. Here we infer complementary reference estimates for its components specifically under cloud-free conditions. While the clear-sky fluxes at the top of atmosphere (TOA) are accurately known from satellite measurements, the corresponding fluxes at the Earth's surface are not equally well established, as they cannot be directly measured from space. This is also evident in 38 global climate models from CMIP5, which are shown to greatly vary in their clear-sky surface radiation budgets. To better constrain the latter, we established new clear-sky reference climatologies of surface downward shortwave and longwave radiative fluxes from worldwide distributed Baseline Surface Radiation Network sites. 33 out of the 38 CMIP5 models overestimate the clear-sky downward shortwave reference climatologies, whereas both substantial overestimations and underestimations are found in the longwave counterparts in some of the models. From the bias structure of the CMIP5 models we infer best estimates for the global mean surface downward clear-sky shortwave and longwave radiation, at 247 and 314 Wm, respectively. With a global mean surface albedo of 13.5% and net shortwave clear-sky flux of 287 Wm at the TOA this results in a global mean clear-sky surface and atmospheric shortwave absorption of 214 and 73 Wm, respectively. From the newly-established diagrams of the global energy balance under clear-sky and all-sky conditions, we quantify the cloud radiative effects not only at the TOA, but also within the atmosphere and at the surface.
在最近的研究中,我们基于地表和太空的直接观测数据对全球平均地球能量平衡进行了量化。在此,我们特别推断了在无云条件下其各组成部分的补充参考估计值。虽然卫星测量能准确得知大气顶层(TOA)的晴空通量,但地球表面的相应通量却没有同样明确的确立,因为无法从太空直接测量。这在CMIP5的38个全球气候模型中也很明显,这些模型的晴空地表辐射收支差异很大。为了更好地约束后者,我们根据全球分布的基线地表辐射网络站点建立了新的晴空地表向下短波和长波辐射通量参考气候学。CMIP5的38个模型中有33个高估了晴空向下短波参考气候学,而在一些模型的长波对应部分则发现了大量的高估和低估情况。根据CMIP5模型的偏差结构,我们推断出全球平均地表向下晴空短波和长波辐射的最佳估计值,分别为247和314 W/m²。由于全球平均地表反照率为13.5%,TOA处净晴空短波通量为287 W/m²,这导致全球平均晴空地表和大气短波吸收分别为214和73 W/m²。根据新建立的晴空和全天空条件下的全球能量平衡图,我们不仅量化了TOA处的云辐射效应,还量化了大气中和地表的云辐射效应。