2019冠状病毒病大流行期间气溶胶对印度南部地表臭氧的影响:基于地面和卫星观测以及模式模拟的多仪器方法

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2021-01-01 DOI:10.1016/j.jastp.2020.105491
Raja Obul Reddy Kalluri, Balakrishnaiah Gugamsetty, Chakradhar Rao Tandule, Rama Gopal Kotalo, Lokeswara Reddy Thotli, Ramakrishna Reddy Rajuru, Surya Nagi Reddy Palle
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引用次数: 12

摘要

世界卫生组织(世卫组织)宣布2019年冠状病毒病(COVID-19)为全球大流行。这导致包括印度在内的全球许多国家在不同阶段实施封锁。在本研究中,我们利用现场观测和模式模拟,在印度南部Anantapur半干旱地区,报告了在封锁前(2020年3月01日至24日(PLD))、封锁第一阶段(2020年3月25日至4月14日(LDP1))和封锁第二阶段(2020年4月15日至5月3日(LDP2))的晴朗天气下气溶胶对地表臭氧的影响。在研究期间,利用臭氧分析仪、MICROTOPS太阳光度计、臭氧计、Aethalometer和净辐射计收集了地表臭氧(O3)、气溶胶光学深度(AOD)、黑碳质量浓度(BC)、总柱状臭氧(TCO)、太阳辐射(SR)和紫外线辐射(UV-A)数据。O3和BC的日变化在3个阶段表现出相反的趋势。在LDP1期间,臭氧浓度(44.8±5.2 ppbv)比PLD期间(40.5±6.0 ppbv)高出约10.7%,这主要是由于NOx排放量的空前减少导致NO对O3的滴定率降低。LDP1期间地表区域的显著增加与对流层紫外可见(TUV)模式观测到的光解频率(j (O1D))基本一致。结果表明,在三个封城阶段,AOD的明显的光谱和时间变化主要是由于不同的气溶胶源。LDP2期间AOD的增加可以从西亚地区和印度中部带来大量的矿物粉尘和烟雾气溶胶,这与混合单粒子拉格朗日积分轨迹(HYSPLIT)气团回射轨迹和中分辨率成像光谱仪(MODIS)在测量地点的火数分析基本一致。总体而言,在LDP1期间,半干旱区BC浓度(~8.4%)和AOD(10.8%)急剧下降,与PLD相对应。光谱aod反演的柱状气溶胶粒径分布在三个阶段均服从幂律加单峰分布。吸收埃指数(AAE)分析显示,在测量地点的封锁期间,生物质燃烧活动对BC的主要贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Impact of aerosols on surface ozone during COVID-19 pandemic in southern India: A multi-instrumental approach from ground and satellite observations, and model simulations

The World Health Organization (WHO) declared the coronavirus disease of 2019 (COVID-19) as a pandemic due to its widespread global infection. This has resulted in lockdown under different phases in many nations, including India, around the globe. In the present study, we report the impact of aerosols on surface ozone in the context of pre-lockdown (01st - 24th March 2020 (PLD)), lockdown phase1 (25th March to 14th April 2020 (LDP1)), and lockdown phase 2 (15th April to 03rd May 2020 (LDP2)) on clear days at a semi-arid site, Anantapur in southern India using both in situ observations and model simulations. Collocated measurements of surface ozone (O3), aerosol optical depth (AOD), black carbon mass concentration (BC), total columnar ozone (TCO), solar radiation (SR), and ultraviolet radiation (UV-A) data were collected using an Ozone analyzer, MICROTOPS sunphotometer, Ozonometer, Aethalometer, and net radiometer during the study period. The diurnal variations of O3 and BC exhibited an opposite trend during three phases. The concentrations of ozone were ~10.7% higher during LDP1 (44.8 ± 5.2 ppbv) than the PLD (40.5 ± 6.0 ppbv), which mainly due to an unprecedented reduction in NOx emissions leading to a lower O3 titration by NO. The prominent increase in the surface zone during LDP1 is reasonably consistent with the observed photolysis frequencies (j (O1D)) through Tropospheric Ultraviolet and Visible (TUV) model. The results show that a pronounced spectral and temporal variability in the AOD during three lockdown phases is mainly due to distinct aerosol sources. The increase in AOD during LDP2 due to long-range transport can bring large amounts of mineral dust and smoke aerosols from the west Asian region and central India, and which is reasonably consistent with the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) air mass back trajectories and Moderate Resolution Imaging Spectroradiometer (MODIS) fire counts analysis over the measurement location. Overall, a drastic reduction in BC concentration (~8.4%) and AOD (10.8%) were observed in the semi-arid area during LDP1 with correspondence to PLD. The columnar aerosol size distributions retrieved from the spectral AODs followed power-law plus unimodal during three phases. The absorption angstrom exponent (AAE) analysis reveals a predominant contribution to the BC from biomass burning activities during the lockdown period over the measurement location.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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