北印度洋上空活性痕量气体的海气交换回顾

IF 1.3 4区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY
Mansi Gupta, Nidhi Tripathi, T G Malik, L K Sahu
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引用次数: 0

摘要

在地球大气层中,温室气体(GHGs)和活性痕量气体是化学与气候相互作用的重要组成部分。这些痕量气体来自陆地和海洋区域的自然和人为排放源。海气交换是控制几种重要痕量气体在偏远海洋区域分布的主要过程。虽然海洋-大气界面覆盖了地球表面的约 70%,但在有限的海洋区域,反应性痕量气体的定量海气交换是通过估算得出的。痕量气体的产生和海气交换受界面两侧的物理条件和海洋生物地球化学的控制。北印度洋(NIO)有强烈的季节性季风和强烈的热带气旋。北印度洋由阿拉伯海和孟加拉湾组成,是世界上生物生产力最高的海洋之一,也是阿拉伯海溶解氧浓度最高的最低含氧区(OMZ)的所在地。因此,NIO 为研究活性痕量气体的海气交换过程提供了一个独特的系统。迄今为止,对痕量气体海气交换的研究大多集中在大西洋和太平洋,而对北印度洋的研究非常有限,报告的主要是 CH4、CO2 和 N2O。虽然近年来取得了一些进展,但对非甲烷碳氢化合物(NMHCs)、含氧、含硫和含卤烃等活性痕量气体的海气交换研究仍然很少。本文探讨了目前对北印度洋非甲烷碳氢化合物、二甲基硫化物 (DMS)、含氧挥发性有机化合物 (OVOC)、卤代碳化物、一氧化碳 (CO) 和臭氧 (O3) 等活性痕量气体的海气交换过程和通量的认识。本综述概述了有关北印度洋上空痕量气体海气交换的研究,以及用于估算气体海气通量的常用参数化方法。通过各种现场和模拟研究,总结了北印度洋上空乙烯(3-10.35 微摩尔米-2 d-1)、异戊二烯(0.215-0.172 微摩尔米-2 d-1)、乙醛(-6.75-11.35 微摩尔米-2 d-1)、丙酮(-9-9 微摩尔米-2 d-1)、二甲基亚砜(0.03-41.4 微摩尔米-2 d-1)和一氧化碳(1.4-5.4 微摩尔米-2 d-1)的通量范围。论文论述了北印度洋在活性痕量气体的产生和交换方面的重要性、知识差距和未来的科学范围。此外,论文还强调有必要对海洋活性痕量气体循环及其对北印度洋区域大气化学的影响进行多学科研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

A review on air–sea exchange of reactive trace gases over the northern Indian Ocean

A review on air–sea exchange of reactive trace gases over the northern Indian Ocean

In the Earth’s atmosphere, greenhouse gases (GHGs) and reactive trace gases are essential components of chemistry–climate interactions. These trace gases are emitted from both natural and anthropogenic sources over terrestrial and marine regions. Air–sea exchange is the dominant process controlling the distribution of several important trace gases over remote marine regions. Although the ocean–atmosphere interface covers ~70% of the Earth’s surface, the quantitative air–sea exchange of reactive trace gases is estimated over the limited oceanic regions. The production and air–sea exchange of trace gases are controlled by physical conditions at both sides of the interface and ocean biogeochemistry. The northern Indian Ocean (NIO) experiences strong seasonal monsoon winds and intense tropical cyclones. Consisting of the Arabian Sea and the Bay of Bengal, it is one of the most biologically productive regimes of the world ocean and home to the intense oxygen minimum zone (OMZ) of the Arabian Sea with dissolved oxygen concentrations. Thus, the NIO offers a unique system to investigate the air–sea exchange processes of reactive trace gases. So far, most of the studies of air–sea exchange of trace gases is focused on the Atlantic and Pacific Oceans, while studies over the northern Indian Ocean are very limited and reported mainly for CH4, CO2 and N2O. Although progress has been made in recent years, studies of air–sea exchange of reactive trace gases such as non-methane hydrocarbon (NMHCs), oxygen-, sulfur- and halogen-containing hydrocarbons remain scarce. This paper addresses the current understanding of air–sea exchange processes and fluxes of reactive trace gases, including NMHCs, dimethyl sulfide (DMS), oxygenated volatile organic compounds (OVOCs), halocarbons, carbon monoxide (CO) and ozone (O3) in the northern Indian Ocean. This review summarizes the studies on the air–sea exchange of trace gases over the northern Indian Ocean and common parametrization approaches used to estimate the air–sea flux of gases. Flux range for ethene (3–10.35 µmol m–2 d–1), isoprene (0.215–0.172 µmol m–2 d–1), acetaldehyde (–6.75–11.35 µmol m–2 d–1), acetone (–9–9 µmol m–2 d–1), DMS (0.03–41.4 µmol m–2 d–1) and CO (1.4–5.4 µmol m–2 d–1) over the NIO were summarized from various in-situ and modelling studies. The paper addresses the importance of the northern Indian Ocean apropos the production and exchange of reactive trace gases, the knowledge gaps and the future scientific scope. Additionally, it emphasizes the need for a multidisciplinary study of oceanic reactive trace gas cycling and its impact on regional atmospheric chemistry over the northern Indian Ocean.

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来源期刊
Journal of Earth System Science
Journal of Earth System Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
3.20
自引率
5.30%
发文量
226
期刊介绍: The Journal of Earth System Science, an International Journal, was earlier a part of the Proceedings of the Indian Academy of Sciences – Section A begun in 1934, and later split in 1978 into theme journals. This journal was published as Proceedings – Earth and Planetary Sciences since 1978, and in 2005 was renamed ‘Journal of Earth System Science’. The journal is highly inter-disciplinary and publishes scholarly research – new data, ideas, and conceptual advances – in Earth System Science. The focus is on the evolution of the Earth as a system: manuscripts describing changes of anthropogenic origin in a limited region are not considered unless they go beyond describing the changes to include an analysis of earth-system processes. The journal''s scope includes the solid earth (geosphere), the atmosphere, the hydrosphere (including cryosphere), and the biosphere; it also addresses related aspects of planetary and space sciences. Contributions pertaining to the Indian sub- continent and the surrounding Indian-Ocean region are particularly welcome. Given that a large number of manuscripts report either observations or model results for a limited domain, manuscripts intended for publication in JESS are expected to fulfill at least one of the following three criteria. The data should be of relevance and should be of statistically significant size and from a region from where such data are sparse. If the data are from a well-sampled region, the data size should be considerable and advance our knowledge of the region. A model study is carried out to explain observations reported either in the same manuscript or in the literature. The analysis, whether of data or with models, is novel and the inferences advance the current knowledge.
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