Spatiotemporal characteristics and driving factors of global planetary albedo: an analysis using the Geodetector method

被引:4
|
作者
Lv, Mingzhu [1 ]
Song, Yan [1 ]
Li, Xijia [2 ]
Wang, Mengsi [1 ]
Qu, Ying [1 ]
机构
[1] Northeast Normal Univ, Sch Geog Sci, Key Lab Geog Proc & Ecol Secur Changbai Mt, Minist Educ, Changchun, Peoples R China
[2] Jilin Jianzhu Univ, Sch Geomat & Prospecting Engn, Changchun, Peoples R China
基金
中国国家自然科学基金;
关键词
ENERGY SYSTEM CERES; CLIMATE; CLOUDS; FEEDBACK;
D O I
10.1007/s00704-021-03858-9
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
As an important parameter of the Earth's energy budget, the planetary albedo of Earth varies with the dynamics of atmospheric and surface variables. In this study, we investigated the spatiotemporal characteristics and driving factors of the global planetary albedo using the Clouds and the Earth's Radiant Energy System (CERES) Energy Balanced and Filled (EBAF) dataset and the Geodetector method. The results revealed that the planetary albedo can be decomposed into atmospheric and surface contributions, and the planetary albedo in the middle and low latitudes was predominantly affected by the atmospheric contribution. The global planetary albedo and the atmospheric and surface contributions exhibited decreasing trends of - 0.0020, - 0.0015, and - 0.0004/decade from 2001 to 2018, respectively, which were closely related to the variations of atmospheric and surface variables. The cloud fraction was the driving factor of the atmospheric contribution in the middle and low latitudes, and its influence was further enhanced by the aerosol optical thickness (AOT), ice water path (IWP), and liquid water path (LWP). The snow/ice coverage and normalized difference vegetation index (NDVI) were the driving factors of the surface contribution in the snow/ice-covered and vegetated areas, respectively. The interaction relationships between the surface variables were mainly bi-enhanced and nonlinearly enhanced. These results provide useful information about the driving factors of the planetary albedo and are benefit for improving the parametrization of the planetary albedo.
引用
收藏
页码:737 / 752
页数:16
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