Satellite constraint on the tropospheric ozone radiative effect

被引:36
作者
Rap, A. [1 ]
Richards, N. A. D. [1 ,2 ]
Forster, P. M. [1 ]
Monks, S. A. [1 ]
Arnold, S. R. [1 ]
Chipperfield, M. P. [1 ,2 ]
机构
[1] Univ Leeds, Sch Earth & Environm, Leeds, W Yorkshire, England
[2] Univ Leeds, Natl Ctr Earth Observat, Leeds, W Yorkshire, England
基金
英国自然环境研究理事会;
关键词
tropospheric ozone; radiative effect; radiative forcing; radiative kernel; BIOMASS BURNING EMISSIONS; ATMOSPHERIC CHEMISTRY; CLIMATE; MODEL; 21ST-CENTURY; TRANSPORT; VERSION; IMPACT; GASES;
D O I
10.1002/2015GL064037
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Tropospheric ozone directly affects the radiative balance of the Earth through interaction with shortwave and longwave radiation. Here we use measurements of tropospheric ozone from the Tropospheric Emission Spectrometer satellite instrument, together with chemical transport and radiative transfer models, to produce a first estimate of the stratospherically adjusted annual radiative effect (RE) of tropospheric ozone. We show that differences between modeled and observed ozone concentrations have little impact on the RE, indicating that our present-day tropospheric ozone RE estimate of 1.170.03Wm(-2) is robust. The RE normalized by column ozone decreased between the preindustrial and the present-day. Using a simulation with historical biomass burning and no anthropogenic emissions, we calculate a radiative forcing of 0.32Wm(-2) for tropospheric ozone, within the current best estimate range. We propose a radiative kernel approach as an efficient and accurate tool for calculating ozone REs in simulations with similar ozone abundances.
引用
收藏
页码:5074 / 5081
页数:8
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