改进青藏高原中部土壤上臭氧快速沉积的模型表征†。

IF 2.8 Q3 ENVIRONMENTAL SCIENCES
Chong Zhang, Jianshu Wang, Yingjie Zhang, Wanyun Xu, Gen Zhang, Guofang Miao, Jiacheng Zhou, Hui Yu, Weixiong Zhao, Weili Lin, Ling Kang, Xuhui Cai, Hongsheng Zhang and Chunxiang Ye
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引用次数: 0

摘要

臭氧土壤沉积在低植被覆盖的土地上的臭氧总沉积量中占很大一部分,并扰乱了区域和全球范围内的臭氧预算。臭氧土壤沉积模型与观测结果之间存在巨大差异,因此需要不断努力提高机械理解和模型表述能力。观测裸露土壤上的臭氧沉积直接满足了这一要求。在此,我们利用空气动力梯度法对青藏高原裸露土壤上的臭氧沉积进行了实地观测。结果表明,臭氧最高沉积速度的日平均值为 0.49 ± 0.11 (1 sd) cm s-1(2019 年 5 月 1 日至 7 月 10 日),午后臭氧沉积速度的小时最大值为 0.73 ± 0.67 cm s-1。如此快速的臭氧沉积主要归因于极低的土壤阻力(Rsoil),而中低的土壤粘土含量、干燥的条件以及中央热量区强烈的太阳辐射又进一步调节了这一阻力。根据我们的验证,在新开发的斯特拉方案中对 Rsoil 进行参数化是有效的。在加入我们的观测结果后,更新的方案得到了进一步完善,比斯特拉方案更好地体现了 Rsoil 的变化。因此,我们鼓励进行更多的验证,希望能改进斯特拉方案。最后,Stella 方案和我们的更新方案都比当前模型中过于简化的方案显示出巨大优势,为了更好地表示臭氧土壤沉积及其变化,应更认真地加以考虑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Improving model representation of rapid ozone deposition over soil in the central Tibetan Plateau†

Improving model representation of rapid ozone deposition over soil in the central Tibetan Plateau†

Ozone soil deposition contributes a major part to the total deposition of ozone on land covered by low vegetation and perturbs the ozone budget on both regional and global scales. Large model-observation divergences in ozone soil deposition require continuous efforts to improve the mechanical understanding and model representation. Observation of ozone deposition over bare soil directly meets the requirement. Here, we performed field observation of ozone deposition over bare soil first available in the Tibetan Plateau (TP) using the aerodynamic gradient method. A top ozone deposition velocity with a daily mean of 0.49 ± 0.11 (1 sd) cm s−1 (1 May to 10 July 2019) and an hourly mean maximum across the diel pattern of 0.73 ± 0.67 cm s−1 in the afternoon were recorded. Such rapid ozone deposition was mainly attributed to extremely low soil resistance (Rsoil), which was further regulated by median low soil clay content, dry conditions, and strong solar radiation in the central TP. Parameterization of Rsoil in the newly developed Stella scheme was demonstrated to be effective according to our verification. An updated scheme was further attained with the inclusion of our observation and better represents the Rsoil variability than the Stella scheme. More verification is therefore encouraged and hopefully to improve the Stella scheme. Finally, both the Stella scheme and our updated scheme showed great advantages over the oversimplified scheme in current models and should be considered more seriously for the sake of better representation of ozone soil deposition and its variability.

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