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Simulation of regional dust and its effect on photochemistry in the Mexico City area during MILAGRO experiment

机译:在MILAGRO实验中模拟墨西哥城地区的区域尘埃及其对光化学的影响

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摘要

Dust particles have important effects on solar radiation, climate, and photochemistry in the troposphere. Dust events were observed from March 16 to 20, 2006 in the Mexico City (MC) area during the MILAGRO (Megacity Initiative: Local and Global Research Observations) field experiment. In order to study the effects of dust aerosols on total aerosol mass concentrations and photochemistry, a regional chemical/ dynamical model (Weather Research and Forecasting Chemical model version 3 - WRF/Chem-v3) was used in this study, and a dust module was implemented in the model. Analysis of model and observational data suggests that the large area of coastal dry lands to the northeast of MC is an important source of dust particles for the entire MC area. The simulations of both PM2.5 (total particle mass with radius less than 2.5 um) and PM_10 (total particle mass with radius less than 10 (im) concentrations are more consistent with observations than the results of the model without the dust module. During this dust period (March 16-20, 2006), the simulated dust aerosol mass accounts for about 70% of the total PM10 aerosol mass concentrations, with a strong diurnal variation. The results also suggest that dust aerosols have important effects on actinic fluxes and therefore photochemistry, especially on hydroxyl radical (OH) and ozone (O_3) concentrations, in the MC area and the surrounding region. The dust particles decrease the photochemical production of OH, with a maximum reduction of 60% in the dust source region (northeast of the MC area). Near the city area, the reduction of OH concentrations is about 5-20%. The strongest effects on O_3 concentrations are near MC, where the maximum reduction of O_3 is about 10 ppbv. In the dust source region, O_3 concentrations are reduced by about 3-5 ppbv.
机译:尘埃颗粒对对流层的太阳辐射,气候和光化学具有重要影响。 2006年3月16日至20日,在MILAGRO(大城市倡议:本地和全球研究观察)实地实验期间,在墨西哥城(MC)地区观测到沙尘事件。为了研究粉尘气溶胶对总气溶胶质量浓度和光化学的影响,本研究使用区域化学/动力学模型(天气研究和预报化学模型版本3-WRF / Chem-v3),并使用粉尘模块在模型中实施。对模型和观测数据的分析表明,MC东北部的大片沿海干旱地区是整个MC区域重要的尘埃颗粒来源。与没有粉尘模块的模型结果相比,PM2.5(半径小于2.5微米的总粒子质量)和PM_10(半径小于10(im)的浓度总粒子)的仿真与观测结果更加一致。在这段粉尘时期(2006年3月16日至20日),模拟的粉尘气溶胶质量约占PM10气溶胶总浓度的70%,且昼夜变化很大,结果还表明粉尘气溶胶对光化通量和因此,MC区域及其周围区域的光化学反应,尤其是羟基自由基(OH)和臭氧(O_3)的浓度。尘埃颗粒降低了OH的光化学生成,在粉尘源区域最大降低了60%(东北)在市区附近,OH浓度的降低约为5-20%。对O_3浓度的影响最大的是在MC附近,其中O_3的最大降低约为10 ppbv。在欧尔斯地区,O_3浓度降低了约3-5 ppbv。

著录项

  • 来源
    《Atmospheric environment》 |2011年第15期|p.2549-2558|共10页
  • 作者单位

    Department of Earth and Science, York University, Toronto, Canada,National Center for Atmospheric Research, Boulder, CO, USA;

    National Center for Atmospheric Research, Boulder, CO, USA;

    National Center for Atmospheric Research, Boulder, CO, USA;

    Molina Center for the Energy and the Environment, La Jolla, CA, USA;

    National Center for Atmospheric Research, Boulder, CO, USA;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    dust; wrf/chem; photochemistry; mexico city;

    机译:灰尘;wrf / chem;光化学;墨西哥城;

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