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An assessment of the polar HO_x photochemical budget based on 2003 Summit Greenland field observations

机译:根据2003年格陵兰峰会实地观测,对极性HO_x光化学预算进行了评估

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An interpretative modeling analysis is conducted to simulate the diurnal variations in OH and HO_2 + RO_2 observed at Summit, Greenland in 2003. The main goal is to assess the HO_x budget and to quantify the impact of snow emissions on ambient HO_x as well as on CH_2O and H_2O_2.This analysis is based on composite diurnal profiles of HO_x precursors recorded during a 3-day period (July 7-9), which were generally compatible with values reported in earlier studies. The model simulations can reproduce the observed diurnal variation in HO_2 + RO_2 when they are constrained by observations of H_2O_2 and CH_2O. By contrast, model predictions of OH were about factor of 2 higher than the observed values. Modeling analysis of H_2O_2 suggests that its distinct diurnal variation is likely controlled by snow emissions and loss by deposition and/or scavenging. Similarly, deposition and/or scavenging sinks are needed to reproduce the observed diel profile in CH_2O. This study suggests that for the Summit 2003 period snow emissions contribute ~25% of the total CH_2O production, while photochemical oxidation of hydrocarbon appears to be the dominant source. A budget assessment of HO_x radicals shows that primary production from O(~1D) + H_2O and photolysis of snow emitted precursors (i.e., H_2O_2 and CH_2O) are the largest primary HO_x sources at Summit, contributing 41% and 40%, respectively. The snow contribution to the HO_x budget is mostly in the form of emissions of H_2O_2. The dominant HO_x sink involves the HO2 + HO2 reaction forming H_2O_2, followed by its deposition to snow. These results differ from those previously reported for the South Pole (SP), in that primary production of HO_x was shown to be largely driven by both the photolysis of CH_2O and H_2O_2 emissions (46%) with smaller contributions coming from the oxidation of CH_4 and the O(~1D) + H_2O reaction (i.e., 27% each). In sharp contrast to the findings at Summit in 2003, due to the much higher levels of NO_x, the SP HO_x sinks are dominated by HO_x-NO_x reactions, leading to the formation and deposition of HNO_3 and HO_2NO_2. Thus, a comparison between SP and Summit studies suggests that snow emissions appear to play a prominent role in controlling primary HO_x production in both environments. However, as regards to maintaining highly elevated levels of OH, the two environments differ substantially. At Summit the elevated rate for primary production of HO_x is most important; whereas, at SP it is the rapid recycling of the more prevalent HO_2 radical, through reaction with NO, back to OH that is primarily responsible.
机译:进行了解释性建模分析,以模拟2003年在格陵兰萨米特峰观察到的OH和HO_2 + RO_2的昼夜变化。主要目标是评估HO_x预算并量化雪排放对环境HO_x和CH_2O的影响和H_2O_2。此分析基于3天(7月7日至9日)期间记录的HO_x前体的复合日廓线,通常与早期研究中报道的值相符。当通过观察H_2O_2和CH_2O约束时,模型模拟可以重现HO_2 + RO_2的日变化。相反,OH的模型预测值比观测值高约2倍。对H_2O_2的模型分析表明,其明显的昼夜变化很可能受积雪排放和沉积和/或清除造成的损失控制。类似地,需要沉积和/或清除沉来重现CH_2O中观察到的diel轮廓。这项研究表明,在2003年峰会期间,雪的排放量约占CH_2O总产量的25%,而碳氢化合物的光化学氧化似乎是主要来源。 HO_x自由基的预算评估表明,O(〜1D)+ H_2O的初级生产以及雪释放的前体(即H_2O_2和CH_2O)的光解是Summit上最大的HO_x初级来源,分别占41%和40%。降雪对HO_x预算的贡献主要是H_2O_2的排放。占优势的HO_x吸收体参与形成H_2O_2的HO2 + HO2反应,然后沉积到雪中。这些结果与先前针对南极(SP)报道的结果不同,因为表明HO_x的主要产生主要受CH_2O和H_2O_2排放物的光解作用(46%)的驱动,而CH_4和CH2的氧化作用较小。 O(〜1D)+ H_2O反应(即每个反应的27%)。与2003年Summit的调查结果形成鲜明对比的是,由于NO_x含量高得多,SP HO_x汇主要由HO_x-NO_x反应控制,从而导致HNO_3和HO_2NO_2的形成和沉积。因此,SP和Summit研究之间的比较表明,在两种环境中,降雪似乎在控制主要HO_x产生中起着重要作用。然而,关于维持高度升高的OH水平,两种环境有很大不同。在Summit峰会上,HO_x初级生产速率的提高是最重要的;而在SP处,更主要的原因是通过与NO反应将更普遍的HO_2自由基快速循环回OH。

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