Estimating the radiative forcing of carbonaceous aerosols over California based on satellite and ground observations

被引:29
作者
Xu, Yangyang [1 ]
Bahadur, Ranjit [1 ]
Zhao, Chun [2 ]
Leung, L. Ruby [2 ]
机构
[1] Univ Calif San Diego, Scripps Inst Oceanog, La Jolla, CA 92013 USA
[2] Pacific NW Natl Lab, Atmospher Sci & Global Change Div, Richland, WA 99352 USA
基金
美国国家科学基金会;
关键词
BLACK CARBON; LIGHT-ABSORPTION; BROWN CARBON; OPTICAL-PROPERTIES; EMISSION FACTORS; ORGANIC-CARBON; CLIMATE; CLOUDS; MODEL; PARTICLES;
D O I
10.1002/jgrd.50835
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Carbonaceous aerosols have the potential to impact climate directly through absorption of incoming solar radiation and indirectly by affecting cloud and precipitation. Recent modeling studies have made great efforts to simulate both the spatial and temporal distributions of carbonaceous aerosol's optical properties and radiative forcing. This study makes the first observationally constrained assessment of the direct radiative forcing of carbonaceous aerosols over California. By exploiting multiple observations (including ground sites and satellites), we constructed the distribution of aerosol optical depths and aerosol absorption optical depths (AAOD) over California for a 10 year period (2000-2010). We partitioned the total solar absorption into individual contributions from elemental carbon (EC), organic carbon (OC), and dust aerosols, using a newly developed scheme. Our results show that AAOD due to carbonaceous aerosols (EC and OC) at 440 nm was 50%-200% larger than natural dust, with EC contributing the bulk (70%-90%). Observationally constrained EC absorption agrees reasonably well with estimates from global and regional chemical transport models, but the models underestimate the OC AAOD by at least 50%. We estimated that the top of the atmosphere (TOA) forcing from carbonaceous aerosols was 0.7 W/m2 and the TOA forcing due to OC was close to zero. The atmospheric heating of carbonaceous aerosol was 2.2-2.9 W/m 2, of which EC contributed about 80-90%. We estimated the atmospheric heating of OC at 0.1-0.4 W/m2, larger than model simulations. EC reduction over the last two decades may have caused a surface brightening of 1.5-3.5 W/m2. Key Points The solar absorption was partitioned into contributions from EC, OC and dust. Observed and modeled EC AAOD agrees but models underestimate OC AAOD by 50%. TOA warming of carbonaceous aerosols is 0.7 W/m2 and that of OC is near zero. ©2013. American Geophysical Union. All Rights Reserved.
引用
收藏
页码:11148 / 11160
页数:13
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