印度喜马拉雅地区两个地形不同地点的气溶胶光学特性及其辐射效应

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Archana Bawari , Jagdish Chandra Kuniyal , Sheetal Chaudhary , Renu Lata , Bimal Pande
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引用次数: 0

摘要

本研究利用地面测量研究了两个不同地区的气溶胶特征,Mohal-Kullu(31.9°N, 77.12°E;ksi - katarmal(29.64°N, 79.62°E;从2019年7月到2022年6月。Mohal的平均黑碳浓度为1.5±1.0 μ m−3,Katarmal的平均黑碳浓度为1.1±1.4 μ m−3。BC表现出强烈的季节变化,季风后(2.6±1.0 μ m−3)和季风前(1.8±0.5 μ m−3)季节最大。各季节的日变化均表现出明显的早晚高峰。季风前AOD500高(0.30±0.06 ~ 0.54±0.08),Ångström指数低(0.67±0.10 ~ 0.95±0.30),表明大颗粒占优势;季风后和冬季AOD500低(0.21±0.07 ~ 0.25±0.03),Ångström指数高(1.05±0.74 ~ 1.13±0.11),表明小颗粒占优势。卫星衍生(OMI和MAIAC)的AOD500与Mohal (MAIAC的R = 0.4639, OMI的R = 0.1402)和Katarmal (MAIAC的R = 0.3976, OMI的R = 0.2980)的地面测量值呈弱至中度相关。利用气溶胶和云的光学特性(OPAC)和Santa Barbara离散坐标辐射传输(SBDART)模式,发现短波气溶胶辐射强迫(SWARF)在大气表面和顶部为负,而在大气中为正,表明明显的地表冷却和大气变暖分别导致高升温速率。Mohal的年平均大气辐射强迫为27.36±6.00 Wm−2,Katarmal的年平均辐射强迫为21.87±7.26 Wm−2。这些发现可能会对规划空气污染策略和了解区域气候变化的影响产生影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Aerosol Optical Properties and its radiative effects over two topographically different locations of the Indian Himalayan Region
This study investigates aerosol characteristics using ground-based measurements at two distinct regions, Mohal-Kullu (31.9°N, 77.12°E; 1154 m amsl) and Kosi-Katarmal (29.64°N, 79.62°E; 1225 m amsl), from July 2019 to June 2022. The average Black Carbon (BC) concentrations were 1.5 ± 1.0 μg m−3 at Mohal and 1.1 ± 1.4 μg m−3 at Katarmal. BC showed strong seasonal variability, with maxima during post-monsoon (2.6 ± 1.0 μg m−3) and pre-monsoon (1.8 ± 0.5 μg m−3) seasons. The diurnal variation displayed distinct morning and evening peaks in all the seasons. High pre-monsoon AOD500 (0.30 ± 0.06 to 0.54 ± 0.08) and low values of Ångström exponent (0.67 ± 0.10 to 0.95 ± 0.30) indicated dominance of large particles, whereas lower AOD500 (0.21 ± 0.07 to 0.25 ± 0.03) in post-monsoon and winter, along with larger Ångström exponent (1.05 ± 0.74 to 1.13 ± 0.11), indicated smaller particles. Satellite-derived (OMI and MAIAC) AOD500 showed weak to moderate correlation with ground-based measurements at Mohal (R = 0.4639 for MAIAC, R = 0.1402 for OMI) and Katarmal (R = 0.3976 for MAIAC, R = 0.2980 for OMI). Using optical properties of aerosols and clouds (OPAC) and Santa Barbara discrete ordinate radiative transfer (SBDART) models, the short-wave aerosol radiative forcing (SWARF) was found negative at the surface and top of the atmosphere but positive in the atmosphere, suggesting significant surface cooling and atmospheric warming leading to high heating rates, respectively. Annual mean atmospheric radiative forcing was 27.36 ± 6.00 Wm−2 at Mohal and 21.87 ± 7.26 Wm−2 at Katarmal. These findings may have consequences for planning air pollution strategies and understanding the effects of regional climate change.
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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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