Vyas Brij Mohan, Gogoi Mukunda M, Jose Subin
Department of Physics, Pacific College of Basic & Applied Sciences, Pacific University, Udaipur, 313 024, India.
Space Physics Laboratory, Vikram Sarabhai Space Centre, Indian Space Research Organization, Trivandrum, 695 022, India.
Environ Sci Pollut Res Int. 2021 May;28(18):22864-22877. doi: 10.1007/s11356-020-12300-y. Epub 2021 Jan 11.
Continuous and multi-year (2008-2012) measurements of black carbon (BC) mass concentrations (M), carried out from the semiarid tropical site Udaipur (24.6° N, 74° E, 580 m a.s.l.) near the western Indian desert, are analyzed for their region-specific features. M varied over a wide range during the period of study, with the hourly mean values occurring as low as 0.09 to as high as 49.1 μg m, with the multi-year average ~ 4.5 ± 2.6 μg m. Annual variations showed the highest concentrations during November and December (winter seasonal mean = 7.4 ± 3.3 μg m) and the lowest in the monsoon months of July and August (monsoon seasonal mean = 2.5 ± 2.2 μg m). M showed significant inverse relationship with the planetary boundary layer height (ρ ~ - 0.50) as well as ventilation coefficient (ρ ~ - 0.72). Alike aforesaid atmospheric dynamic parameters, T, WS, and RH also possessed statistically significant negative correlations with monthly M. Enhancement in annual as well as diurnal amplitude in M during deficient monsoon years relative to excessive monsoon years have given marked indication of BC sink mechanism due to precipitation. Roles of long-range regional air pollutant transport also have been identified. Identical and consistent seasonal variation in percentage contribution of M with PM (varying from 2.6 to 9.1%) and absorption Angstrom exponent (α, monthly mean values varying from 0.77 ± 0.04 to 1.16 ± 0.08) gives evidence of substantial amount of enhanced anthropogenic source activities of fossil fuel incomplete combustion in post-monsoon and winter period.
对印度西部沙漠附近半干旱热带地区乌代布尔(北纬24.6°,东经74°,海拔580米)在2008 - 2012年期间进行的连续多年的黑碳(BC)质量浓度(M)测量数据进行了区域特征分析。在研究期间,M的变化范围很广,每小时平均值低至0.09微克/立方米,高至49.1微克/立方米,多年平均值约为4.5±2.6微克/立方米。年度变化显示,11月和12月浓度最高(冬季季节平均值 = 7.4±3.3微克/立方米),7月和8月季风月份浓度最低(季风季节平均值 = 2.5±2.2微克/立方米)。M与行星边界层高度(ρ约为 - 0.50)以及通风系数(ρ约为 - 0.72)呈显著负相关。与上述大气动力学参数一样,温度(T)、风速(WS)和相对湿度(RH)与月度M也具有统计学上的显著负相关。相对于季风过剩年份,季风不足年份M的年度和日变化幅度增大,这明显表明降水导致了黑碳汇机制。还确定了远距离区域空气污染物传输的作用。M在PM中的贡献百分比(从2.6%到9.1%不等)以及吸收埃指数(α,月平均值从0.77±0.04到1.16±0.08不等)呈现相同且一致的季节性变化,这证明在季风后和冬季期间,化石燃料不完全燃烧的人为源活动大量增加。