Department of Earth and Planetary Sciences, Weizmann Institute of Science, 76100 Rehovot, Israel.
Max-Planck-Institut fur Meteorologie, D-20146 Hamburg, Germany.
Proc Natl Acad Sci U S A. 2023 Jan 31;120(5):e2208778120. doi: 10.1073/pnas.2208778120. Epub 2023 Jan 27.
Clouds are one of the most influential components of Earth's climate system. Specifically, the midlatitude clouds play a vital role in shaping Earth's albedo. This study investigates the connection between baroclinic activity, which dominates the midlatitude climate, and cloud-albedo and how it relates to Earth's existing hemispheric albedo symmetry. We show that baroclinic activity and cloud-albedo are highly correlated. By using Lagrangian tracking of cyclones and anticyclones and analyzing their individual cloud properties at different vertical levels, we explain why their cloud-albedo increases monotonically with intensity. We find that while for anticyclones, the relation between strength and cloudiness is mostly linear, for cyclones, in which clouds are more prevalent, the relation saturates with strength. Using the cloud-albedo strength relationships and the climatology of baroclinic activity, we demonstrate that the observed hemispheric difference in cloud-albedo is well explained by the difference in the population of cyclones and anticyclones, which counter-balances the difference in clear-sky albedo. Finally, we discuss the robustness of the hemispheric albedo symmetry in the future climate. Seemingly, the symmetry should break, as the northern hemisphere's storm track response differs from that of the southern hemisphere due to Arctic amplification. However, we show that the saturation of the cloud response to storm intensity implies that the increase in the skewness of the southern hemisphere storm distribution toward strong storms will decrease future cloud-albedo in the southern hemisphere. This complex response explains how albedo symmetry might persist even with the predicted asymmetric hemispheric change in baroclinicity under climate change.
云是地球气候系统中最具影响力的组成部分之一。具体来说,中纬度云在塑造地球反照率方面起着至关重要的作用。本研究调查了主导中纬度气候的斜压活动与云反照率之间的关系,以及它与地球现有的半球反照率对称性的关系。我们表明,斜压活动和云反照率高度相关。通过对气旋和反气旋进行拉格朗日跟踪,并分析它们在不同垂直高度的个别云特性,我们解释了为什么它们的云反照率随强度单调增加。我们发现,虽然对于反气旋,强度与云量之间的关系主要是线性的,但对于云量更为普遍的气旋,这种关系随强度而饱和。利用云反照率强度关系和斜压活动的气候学,我们表明,观测到的半球间云反照率差异很好地解释了气旋和反气旋数量的差异,这平衡了晴空反照率的差异。最后,我们讨论了未来气候中半球反照率对称性的稳健性。由于北极放大,北半球的风暴轨迹响应似乎与南半球不同,因此对称性似乎会被打破。然而,我们表明,云对风暴强度的响应饱和意味着,南半球风暴分布对强风暴的偏度增加将减少未来南半球的云反照率。这种复杂的响应解释了为什么即使在气候变化下,预计斜压性的不对称性半球变化下,反照率对称性仍可能持续。