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A cloud-ozone data product from Aura OMI and MLS satellite measurements

机译:来自Aura OMI和MLS卫星测量的云臭氧数据产品

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摘要

Ozone within deep convective clouds is controlled by several factorsinvolving photochemical reactions and transport. Gas-phase photochemicalreactions and heterogeneous surface chemical reactions involving ice, waterparticles, and aerosols inside the clouds all contribute to the distributionand net production and loss of ozone. Ozone in clouds is also dependent onconvective transport that carries low-troposphere/boundary-layer ozone andozone precursors upward into the clouds. Characterizing ozone in thick cloudsis an important step for quantifying relationships of ozone with troposphericHO, OH production, and cloud microphysics/transportproperties. Although measuring ozone in deep convective clouds from eitheraircraft or balloon ozonesondes is largely impossible due to extrememeteorological conditions associated with these clouds, it is possible toestimate ozone in thick clouds using backscattered solar UV radiationmeasured by satellite instruments. Our study combines Aura Ozone MonitoringInstrument (OMI) and Microwave Limb Sounder (MLS) satellite measurements togenerate a new research product of monthly-mean ozone concentrations in deepconvective clouds between 30° S and 30° N for October 2004–April 2016.These measurements represent mean ozone concentration primarilyin the upper levels of thick clouds and reveal key features of cloud ozoneincluding: persistent low ozone concentrations in the tropical Pacific of ∼ 10 ppbv or less; concentrations of up to 60 pphv or greaterover landmass regions of South America, southern Africa, Australia, andIndia/east Asia; connections with tropical ENSO events; andintraseasonal/Madden–Julian oscillation variability. Analysis of OMI aerosolmeasurements suggests a cause and effect relation between boundary-layerpollution and elevated ozone inside thick clouds over landmass regionsincluding southern Africa and India/east Asia.
机译:深对流云层中的臭氧受涉及光化学反应和传输的几个因素控制。气相光化学反应和涉及冰,水颗粒和云内气溶胶的非均质表面化学反应都有助于臭氧的分布,净产生和损失。云中的臭氧还取决于对流传输,对流传输会将低对流层/边界层臭氧和臭氧前体向上带入云中。表征厚云中的臭氧是量化臭氧与对流层HO,OH的产生以及云的微观物理/传输特性之间关系的重要步骤。尽管由于与这些云相关的极端气象条件,在很大程度上不可能从飞机或气球臭氧探空仪测量深对流云中的臭氧,但仍可以使用卫星仪器测量的反向散射太阳紫外线辐射来估算厚云中的臭氧。我们的研究结合了Aura臭氧监测仪器(OMI)和微波肢体探测仪(MLS)的卫星测量结果,以产生2004年10月至2016年4月介于30°S和30°N之间的深对流云中月平均臭氧浓度的新研究产品。平均臭氧浓度主要集中在厚云层的上层,并显示出云层臭氧的主要特征,包括:热带太平洋地区臭氧的持续低浓度,约为10〜ppppv或更低。南美,南部非洲,澳大利亚和印度/东亚的陆地区域浓度最高可达60 pphv或更高;与热带ENSO事件的联系;季节内/马登-朱利安振荡变异性。对OMI气溶胶测量的分析表明,边界层污染与包括南非和印度/东亚在内的陆地区域上厚云内部的臭氧升高之间存在因果关系。

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