Observational estimation of radiative feedback to surface air temperature over Northern High Latitudes

被引:15
|
作者
Hwang, Jiwon [1 ]
Choi, Yong-Sang [1 ,2 ]
Kim, WonMoo [3 ]
Su, Hui [2 ]
Jiang, Jonathan H. [2 ]
机构
[1] Ewha Womans Univ, Dept Atmospher Sci & Engn, Engineer B 353, 52 Ewhayeodae Gil, Seoul 03760, South Korea
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] APEC Climate Ctr, Climate Predict Dept, Busan, South Korea
基金
美国国家航空航天局;
关键词
Local radiative feedback; High-latitude climate feedback; Radiative kernel; Observational estimates of feedback; CLIMATE FEEDBACKS; POLAR AMPLIFICATION; SEA-ICE; KERNEL TECHNIQUE; ALBEDO FEEDBACK; ARCTIC CLIMATE; SENSITIVITY; CLOUDS; VARIABILITY; AQUAPLANET;
D O I
10.1007/s00382-017-3629-6
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
The high-latitude climate system contains complicated, but largely veiled physical feedback processes. Climate predictions remain uncertain, especially for the Northern High Latitudes (NHL; north of 60 degrees N), and observational constraint on climate modeling is vital. This study estimates local radiative feedbacks for NHL based on the CERES/Terra satellite observations during March 2000-November 2014. The local shortwave (SW) and longwave (LW) radiative feedback parameters are calculated from linear regression of radiative fluxes at the top of the atmosphere on surface air temperatures. These parameters are estimated by the de-seasonalization and 12-month moving average of the radiative fluxes over NHL. The estimated magnitudes of the SW and the LW radiative feedbacks in NHL are 1.88 +/- 0.73 and 2.38 +/- 0.59 W m(-2) K-1, respectively. The parameters are further decomposed into individual feedback components associated with surface albedo, water vapor, lapse rate, and clouds, as a product of the change in climate variables from ERA-Interim reanalysis estimates and their pre-calculated radiative kernels. The results reveal the significant role of clouds in reducing the surface albedo feedback (1.13 +/- 0.44 W m(-2) K-1 in the cloud-free condition, and 0.49 +/- 0.30 W m(-2) K-1 in the all-sky condition), while the lapse rate feedback is predominant in LW radiation (1.33 +/- 0.18 W m(-2) K-1). However, a large portion of the local SW and LW radiative feedbacks were not simply explained by the sum of these individual feedbacks.
引用
收藏
页码:615 / 628
页数:14
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