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Effects of Ozone Isotopologue Formation on the Clumped-Isotope Composition of Atmospheric O2
Journal of Geophysical Research: Atmospheres ( IF 3.8 ) Pub Date : 2021-07-07 , DOI: 10.1029/2021jd034770
Laurence Y. Yeung 1 , Lee T. Murray 2 , Asmita Banerjee 1 , Xin Tie 2 , Yuzhen Yan 1 , Elliot L. Atlas 3 , Sue M. Schauffler 4 , Kristie A. Boering 5
Affiliation  

Tropospheric 18O18O is an emerging proxy for past tropospheric ozone and free-tropospheric temperatures. The basis of these applications is the idea that isotope-exchange reactions in the atmosphere drive 18O18O abundances toward isotopic equilibrium. However, previous work used an offline box-model framework to explain the 18O18O budget, approximating the interplay of atmospheric chemistry and transport. This approach, while convenient, has poorly characterized uncertainties. To investigate these uncertainties, and to broaden the applicability of the 18O18O proxy, we developed a scheme to simulate atmospheric 18O18O abundances (quantified as ∆36 values) online within the GEOS-Chem chemical transport model. These results are compared to both new and previously published atmospheric observations from the surface to 33 km. Simulations using a simplified O2 isotopic equilibration scheme within GEOS-Chem show quantitative agreement with measurements only in the middle stratosphere; modeled ∆36 values are too high elsewhere. Investigations using a comprehensive model of the O-O2-O3 isotopic photochemical system and proof-of-principle experiments suggest that the simple equilibration scheme omits an important pressure dependence to ∆36 values: the anomalously efficient titration of 18O18O to form ozone. Incorporating these effects into the online ∆36 calculation scheme in GEOS-Chem yields quantitative agreement for all available observations. While this previously unidentified bias affects the atmospheric budget of 18O18O in O2, the modeled change in the mean tropospheric ∆36 value since 1850 CE is only slightly altered; it is still quantitatively consistent with the ice-core ∆36 record, implying that the tropospheric ozone burden increased less than 40% over the twentieth century.

中文翻译:

臭氧同位素体的形成对大气O2聚集同位素组成的影响

对流层18 O 18 O 是过去对流层臭氧和自由对流层温度的新兴代表。这些应用的基础是大气中的同位素交换反应将18 O 18 O 丰度推向同位素平衡的想法。然而,之前的工作使用离线盒模型框架来解释18 O 18 O 预算,近似大气化学和传输的相互作用。这种方法虽然方便,但不确定性的特征很差。为了研究这些不确定性,并扩大18 O 18 O 代理的适用性,我们开发了一种模拟大气18O 18 O 丰度(量化为 ∆ 36值)在 GEOS-Chem 化学传输模型中在线。这些结果与新的和以前发表的从地表到 33 公里的大气观测结果进行了比较。在 GEOS-Chem 中使用简化的 O 2同位素平衡方案进行的模拟显示,与仅在平流层中部的测量结果一致;模拟的 ∆ 36值在其他地方太高了。使用 OO 2 -O 3同位素光化学系统的综合模型和原理验证实验进行的研究表明,简单的平衡方案忽略了对 Δ 36的重要压力依赖性值:异常有效的18 O 18 O滴定以形成臭氧。将这些影响纳入GEOS-Chem 中的在线 Δ 36计算方案,可以为所有可用的观察结果产生定量一致性。虽然这种先前未识别的偏差影响了O 218 O 18 O的大气收支,但自 1850 CE 以来平均对流层 Δ 36值的模拟变化仅略有改变;它仍然是与冰芯Δ定量一致36的记录,这意味着对流层臭氧负担在二十世纪增加了不到40%。
更新日期:2021-07-20
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