Indian institute of Tropical Meteorology, Ministry of Earth Sciences, Pune, India.
Savitribai Phule Pune University, Pune, India.
Environ Sci Pollut Res Int. 2021 Jul;28(26):35266-35277. doi: 10.1007/s11356-021-13163-7. Epub 2021 Mar 5.
The temporal variability of the planetary boundary layer height (PBLH) over Mahabaleshwar was studied for a period of 1 year from 1 December 2015 to 30 November 2016 using microwave radiometer (MWR) observations. The PBLH over Mahabaleshwar was found to be the highest during the pre-monsoon (March-May) season and lowest during the winter (December-February) season. The seasonal mean of PBLH was estimated to be 339±88 m during winter, 485±70 m during pre-monsoon, 99±153 m during monsoon, and 438±24 m during post-monsoon season. Frequency distribution analysis of PBLH during pre-monsoon season revealed that the formation of turbulence internal boundary layer (TIBL) is evident. In contrast, cold and moist air mass during the monsoon season enhances the wind shear with lower buoyancy term which results in lowering of PBLH. The comparison of PBLH between MWR and radiosonde observations shows a good correlation (r = 0.66, p=0.001). The growth rate was observed to be 388 m/h during pre-monsoon, 206 m/h during winter, 57 m/h during monsoon, and 167 m/h during post-monsoon season. The seasonal mean concentration of PM was found to be 42.3±4.6 μg/mduring winter, 33.4±8.7 μg/m during pre-monsoon, 6.6±2.2 μg/m during monsoon, and 26.1±1.7 μg/mduring post-monsoon season. The effect of higher loading of scattering-type aerosol (dust particle) was also investigated as a case study. The analysis reveals the inverse relationship between the PBL height variability and the particulate loading indicating the importance of aerosol direct effect. Analysis of the ventilation coefficient (Vc) revealed that the dissipation potential was higher (1736 m/s) during pre-monsoon season as compared to (1191 m/s, 455m/s, and 1580 m/s) winter, monsoon, and post-monsoon seasons.
利用微波辐射计(MWR)观测,对马哈拉施特拉邦(Mahabaleshwar)的行星边界层高度(PBLH)的时间变化进行了为期一年的研究,从 2015 年 12 月 1 日至 2016 年 11 月 30 日。结果表明,马哈拉施特拉邦的 PBLH 在季风前(3 月至 5 月)季节最高,在冬季(12 月至 2 月)最低。冬季 PBLH 的季节平均估计值为 339±88 m,季风前为 485±70 m,季风期间为 99±153 m,季风后为 438±24 m。对季风前季节 PBLH 的频率分布分析表明,湍流内部边界层(TIBL)的形成是明显的。相比之下,季风季节寒冷潮湿的气团增强了风切变,而浮力项较低,导致 PBLH 降低。MWR 和无线电探空仪观测结果的 PBLH 比较显示出良好的相关性(r=0.66,p=0.001)。观测到的生长率在季风前为 388 m/h,冬季为 206 m/h,季风期间为 57 m/h,季风后为 167 m/h。冬季 PM 的平均浓度为 42.3±4.6μg/m,季风前为 33.4±8.7μg/m,季风期间为 6.6±2.2μg/m,季风后为 26.1±1.7μg/m。作为案例研究,还研究了散射型气溶胶(灰尘颗粒)较高负荷的影响。分析表明,PBL 高度变化与颗粒负荷之间存在反比关系,这表明气溶胶直接效应的重要性。通风系数(Vc)的分析表明,在季风前季节,消散潜力较高(1736 m/s),而在冬季(1191 m/s、455 m/s 和 1580 m/s)、季风和季风后季节则较低。