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不同大气O水平下,一维模型和三维模型计算得到的臭氧柱深度与甲烷寿命之间的比较。

Comparison between ozone column depths and methane lifetimes computed by one- and three-dimensional models at different atmospheric O levels.

作者信息

Ji A, Kasting J F, Cooke G J, Marsh D R, Tsigaridis K

机构信息

Department of Geosciences, Penn State University, University Park, PA 16802, USA.

School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK.

出版信息

R Soc Open Sci. 2023 May 3;10(5):230056. doi: 10.1098/rsos.230056. eCollection 2023 May.

Abstract

Recently, Cooke . (Cooke . 2022 , 211165. (doi:10.1098/rsos.211165)) used a three-dimensional coupled chemistry-climate model (WACCM6) to calculate ozone column depths at varied atmospheric O levels. They argued that previous one-dimensional (1-D) photochemical model studies, e.g. Segura . (Segura . 2003 , 689-708. (doi:10.1089/153110703322736024)), may have overestimated the ozone column depth at low pO, and hence also overestimated the lifetime of methane. We have compared new simulations from an updated version of the Segura . model with those from WACCM6, together with some results from a second three-dimensional model. The discrepancy in ozone column depths is probably due to multiple interacting parameters, including HO in the upper troposphere, lower boundary conditions, vertical and meridional transport rates, and different chemical mechanisms, especially the treatment of O photolysis in the Schumann-Runge (SR) bands (175-205 nm). The discrepancy in tropospheric OH concentrations and methane lifetime between WACCM6 and the 1-D model at low pO is reduced when absorption from CO and HO in this wavelength region is included in WACCM6. Including scattering in the SR bands may further reduce this difference. Resolving these issues can be accomplished by developing an accurate parametrization for O photolysis in the SR bands and then repeating these calculations in the various models.

摘要

最近,库克(库克,2022年,211165。(doi:10.1098/rsos.211165))使用三维化学-气候耦合模型(WACCM6)来计算不同大气氧水平下的臭氧柱深度。他们认为,之前的一维(1-D)光化学模型研究,例如塞古拉(塞古拉,2003年,689 - 708。(doi:10.1089/153110703322736024)),可能在低氧分压下高估了臭氧柱深度,因此也高估了甲烷的寿命。我们将塞古拉模型更新版本的新模拟结果与WACCM6的结果进行了比较,同时还比较了另一个三维模型的一些结果。臭氧柱深度的差异可能是由于多个相互作用的参数导致的,包括对流层上部的羟基自由基、下边界条件、垂直和经向传输速率以及不同的化学机制,特别是舒曼-龙格(SR)波段(175 - 205纳米)中氧光解的处理方式。当WACCM6中包含该波长区域一氧化碳和羟基自由基的吸收时,WACCM6与一维模型在低氧分压下对流层羟基自由基浓度和甲烷寿命的差异会减小。在SR波段中考虑散射可能会进一步减小这种差异。通过为SR波段中的氧光解开发精确的参数化方法,然后在各种模型中重复这些计算,可以解决这些问题。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ddc6/10154922/39f0b4d7c400/rsos230056f01.jpg

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