摘要
沙尘天气过程研究中,起沙过程是沙尘传输和沉降的基础,沙尘模式中的起沙参数化方案决定了能否准确模拟和预报沙尘天气。试验观测和数值模拟是研究起沙过程的重要途径。基于风蚀起沙的物理机制,总结了起沙机制和起沙特征的研究成果,介绍了风蚀起沙的主要影响因子,回顾了起沙关键参数(临界起沙摩擦速度(u_t)或临界起沙风速(U_t)、水平跃移沙尘通量(Q)和起沙通量(F))的试验观测及其沙尘模式应用中的参数化方案,并讨论了不同起沙参数化方案的应用与校验。同时,针对目前研究中存在的问题和今后可能的研究方向提出建议。
Dust emission generated by wind erosion is a basic process before the transport and deposition of dust particles.Parameterization of dust emission flux is important for accurate simulation and prediction of dust events.Field observation and numerical simulation are two approaches to understand the complex process of dust emission.Great progress has been made on the characteristics and mechanism of dust emission during dust storm events.This review introduces the major factors influencing dust emission,and summarizes the calculation methods of several key parameters of dust emission,including the threshold friction velocity u t,threshold wind speed U_t,streamwise saltation flux Q,and(vertical) dust emission flux F,from perspectives of both observation and parameterization.The paper also discusses the improvement,application,and validation of different dust emission schemes in dust models.Existing problems and future research directions are elaborated as well.
出处
《气象学报》
CAS
CSCD
北大核心
2014年第5期987-1000,共14页
Acta Meteorologica Sinica
基金
国家重点基础研究发展规划项目(2010CB428501)
财政部/科技部公益性行业(气象)科研专项(GYHY201006014)
高等学校博士学科点专项科研基金项目(20110001130010)
国家自然科学基金项目(41075005)
关键词
风蚀起沙
沙尘天气
试验观测
参数化方案
Dust emission by wind erosion
Dust storm
Experimental observation
Parameterization