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The Dispersion of Silver Iodide Particles from Ground-Based Generators

机译:地基发生器中碘化银颗粒的扩散

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A numerical modeling study has been conducted to explore the ability of the Weather Research and Forecasting (WRF) model-based large-eddy simulation (LES) with 100-m grid spacing to reproduce silver iodide (AgI) particle dispersion by comparing the model results with measurements made on 16 February 2011 over the Medicine Bow Mountains in Wyoming. Xue et al.'s recently developed AgI cloud-seeding parameterization was applied in this study to simulate AgI release from ground-based generators. Qualitative and quantitative comparisons between the LES results and observed AgI concentrations were conducted. Analyses of turbulent kinetic energy (TKE) features within the planetary boundary layer (PBL) and comparisons between the 100-m LES and simulations with 500-m grid spacing were performed as well. The results showed the following: 1) Despite the moist bias close to the ground and above 4 km AGL, the LES with 100-m grid spacing captured the essential environmental conditions except for a slightly more stable PBL relative to the observed soundings. 2) Wind shear is the dominant TKE production mechanism in wintertime PBL over complex terrain and generates a PBL of about 1000-m depth. The terrain-induced turbulent eddies are primarily responsible for the vertical dispersion of AgI particles. 3) The LES-simulated AgI plumes were shallow and narrow, in agreement with observations. The LES overestimated AgI concentrations close to the ground, which is consistent with the higher static stability in the model than is observed. 4) Non-LES simulations using PBL schemes had difficulty in capturing the shear-dominant turbulent PBL structure over complex terrain in wintertime. Therefore, LES of wintertime orographic clouds with grid spacing close to 500 m or finer are recommended
机译:进行了数值建模研究,以通过比较模型结果来探索基于气象研究和预报(WRF)模型的大涡模拟(LES)的网格间距为100-m的能力来再现碘化银(AgI)颗粒的分散性于2011年2月16日在怀俄明州的梅德弓山进行了测量。 Xue等人最近开发的AgI云播种参数化技术在本研究中用于模拟地面发电机产生的AgI释放。 LES结果与观察到的AgI浓度之间进行了定性和定量比较。还对行星边界层(PBL)内的湍动能(TKE)特征进行了分析,并对100 m LES和500 m网格间距的模拟进行了比较。结果表明:1)尽管靠近地面且在AGL高于4 km处存在潮湿偏见,但网格间距为100 m的LES捕获了必要的环境条件,但相对于观测到的测深线而言,PBL略稳定。 2)风切变是冬季复杂地形上PBL的主要TKE产生机制,并产生约1000 m深度的PBL。地形引起的湍流是造成AgI颗粒垂直分散的主要原因。 3)LES模拟的AgI羽流浅而窄,与观察结果一致。 LES高估了接近地面的AgI浓度,这与模型中观察到的静态稳定性更高有关。 4)使用PBL方案进行的非LES模拟难以捕获冬季复杂地形上以剪切力为主的湍流PBL结构。因此,建议使用网格间距接近500 m或更细的冬季地形云LES

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