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Development of a regional lightning nitrogen oxide parameterization for the weather and research forecast chemistry model.

机译:为天气和研究预报化学模型开发区域闪电氮氧化物参数化。

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摘要

Nitrogen oxides (NOx) produced by lightning (LNOx) play an important role in atmospheric chemistry, including the formation of tropospheric ozone (O3). Chemical transport models such as the Weather Research and Forecasting (WRF-Chem) model can simulate some aspects of ozone chemistry related to anthropogenic pollution, but to produce accurate O3 concentrations, it is important to accurately specify the LNO x. WRF-Chem currently only includes lightning and the production of the resulting NOx when run at cloud scale resolution. These cloud scale parameterizations are based on previous studies that have shown that lightning flash rate is strongly correlated with radar-derived storm height, updraft strength, the vertical flux of ice, and other storm parameters. We describe a new way to parameterize lightning occurrence and the formation of LNOx when WRF-Chem is run at the regional scale (e.g., 36 or 12 km grid spacing).;We present a comparison of three regional scale lightning parameterizations during NASA's Intercontinental Chemical and Transport Experiment (INTEX-A, 2004). Two of the parameterizations use previously reported relations between lightning flash rate and radar-derived storm top height. We have developed the third parameterization which uses a relationship between convective precipitation, depth of the mixed phase layer, and flash rate. We investigated each lightning parameterization in the WRF-Chem model. After comparing them at 36 km and 12 km grid spacing for six different summer days during 2004, we found that our parameterization, called LCLIPER (Lightning Climatology and Persistence), produces total lightning (IC+CG) results that generally are comparable to "observations" of NLDN' total lightning. Two other parameterizations, Futyan and Del Genio (FDG) (2007) and Yoshida et al. (2009) were compared with LCLIPER. Since both parameterizations use a relationship with radar echo top and total lightning, they both produced similar results.;Contingency table statistics, domain wide total flash counts and mean flash rate of coinciding observations and model lightning are presented to help determine which parameterization is superior. Results show that FDG and the Yoshida et al. (2009) schemes underestimated flash rate at 36 km grid spacing, and overestimated them at 12 km. LCLIPER also overall underestimates flash rate, but to a lesser extent. LCLIPER is the focus of the study since it provided the best results.;The predicted flash rates and a NOx production term determine the two dimensional pattern of LNOx. The LNOx then is vertically distributed using our previously calculated climatological vertical distributions of lightning sources measured by the Lightning Detection and Ranging (LDAR) network at Kennedy Space Center that are functions of storm top. Warm season vertical distributions of lightning sources and flashes are presented using data from the Lightning Detection and Ranging (LDAR) network at Kennedy Space Center, FL. We emphasize the percentage of sources/flashes at each level compared to the vertical total and present the distributions as a function of storm top above ground level (AGL). The vertical profiles of sources and flashes are compared with each other and with those from previous studies. Results indicate that storms with tops higher than ∼10 km AGL often have a bimodal or multiple peak distribution of percentage sources and flashes. However, distributions for storms with tops lower than ∼10 km AGL exhibit only a single dominant peak. Temporal variations in the vertical distributions of flash percentages are examined for four clusters of storms occurring on different days. Results reveal considerable storm-to-storm and intra-storm variability. However, two similarities are observed between the four cases: (1) Maximum flash density (flashes km-3) occurs as the maximum storm top is reached, and (2) As the storms increase in intensity, both maximum flash density and flash percentage increase in altitude, and then both decrease in altitude as the storms decay.;When compared to aircraft measurements during the INTEX-A field campaign, results of WRF-Chem LNOx indicated that the addition of lightning improved values of upper tropospheric NOx, but underestimated the values when considering the mean of the entire flight. At 12 km grid spacing, WRF-Chem without lightning predicted 61 pptv NOx in the layer between 7--9 km, while 248 pptv NOx was observed during the 12 July 2004 INTEX-A flight. WRF-Chem with the addition of lightning from LCLIPER increased NOx in this layer to 220 pptv. When the model produced lightning, LNOx was overestimated throughout the atmospheric column. Results indicate that radar derived echo tops may be underestimated causing the incorrect vertical distribution method to be selected.
机译:闪电(LNOx)产生的氮氧化物(NOx)在大气化学中起重要作用,包括形成对流层臭氧(O3)。诸如天气研究与预报(WRF-Chem)模型之类的化学迁移模型可以模拟与人为污染相关的臭氧化学的某些方面,但是要产生准确的O3浓度,准确指定LNO x至关重要。目前,WRF-Chem仅包括闪电和以云级分辨率运行时生成的NOx。这些云规模参数化基于先前的研究,这些研究表明,雷闪速率与雷达衍生的风暴高度,上升气流强度,冰的垂直通量以及其他风暴参数密切相关。我们描述了一种在WRF-Chem在区域范围内运行时(例如36或12 km网格间距)对闪电发生和LNOx形成进行参数化的新方法。我们在NASA洲际化学过程中对三种区域规模闪电参数化进行了比较和运输实验(INTEX-A,2004年)。其中两个参数设置使用了先前报道的雷击闪速与雷达衍生风暴顶高度之间的关系。我们开发了第三种参数化方法,该方法利用对流降水,混合相层的深度和闪蒸速率之间的关系。我们研究了WRF-Chem模型中的每个闪电参数设置。在2004年的六个不同的夏日比较它们在36 km和12 km网格间距处的位置之后,我们发现称为LCLIPER(闪电气候和持久性)的参数设置产生的总闪电(IC + CG)结果通常与“观测”相当NLDN”的总闪电。另外两个参数化,Futyan和Del Genio(FDG)(2007)和Yoshida等人。 (2009)与LCLIPER进行了比较。由于这两个参数化都使用与雷达回波顶部和总闪电的关系,因此它们都产生相似的结果。列联表统计,全域总闪光计数以及一致观测值和模型闪电的平均闪光率有助于确定哪个参数化效果更好。结果表明,FDG和吉田等人。 (2009年)的方案低估了36 km网格间距下的闪速,而高估了12 km网格上的闪速。 LCLIPER还总体上低估了闪速,但程度较低。 LCLIPER是研究的重点,因为它提供了最佳的结果。预测的闪速和NOx生成项决定了LNOx的二维模式。然后,使用我们先前计算的闪电源的气候垂直分布来垂直分布LNOx,该分布是由肯尼迪航天中心的雷电探测与测距(LDAR)网络测量的,是风暴顶的功能。佛罗里达州肯尼迪航天中心的雷电探测与测距(LDAR)网络的数据显示了暖季垂直方向的雷源和闪光分布。我们强调了每个级别的源/闪光相对于垂直总数的百分比,并给出了与地面风暴顶(AGL)有关的分布。将光源和闪光的垂直剖面相互比较,并与以前的研究进行比较。结果表明,顶部高于AGL约10 km的风暴通常具有双峰或多峰百分比分布的源和闪光。但是,AGL低于10 km的风暴的分布只表现出一个主峰。针对在不同日期发生的四场暴风雨,检查了闪光百分比的垂直分布的时间变化。结果显示,暴风雨之间和暴风雨中的变化很大。但是,在这四种情况之间观察到两个相似之处:(1)当达到最大风暴顶时会出现最大闪光密度(闪光km-3),并且(2)随着风暴强度的增加,最大闪光密度和闪光百分比当与暴风雨衰减有关时,高度会升高,然后两者都会降低。;与INTEX-A野战期间的飞机测量相比,WRF-Chem LNOx的结果表明,增加对流层NOx的闪电值有所改善,但被低估了考虑整个飞行平均值时的值。在12 km的网格间距处,WRF-Chem在没有闪电的情况下预测在7--9 km之间的层中有61 pptv NOx,而在2004年7月12日的INTEX-A飞行中观测到248 pptv NOx。 WRF-Chem加上LCLIPER的闪电,使该层的NOx增至220 pptv。当模型产生闪电时,整个大气柱中的LNOx都被高估了。结果表明,雷达得出的回波顶部可能被低估,从而导致选择了错误的垂直分布方法。

著录项

  • 作者

    Hansen, Amanda E.;

  • 作者单位

    The Florida State University.;

  • 授予单位 The Florida State University.;
  • 学科 Atmospheric Chemistry.;Meteorology.
  • 学位 Ph.D.
  • 年度 2012
  • 页码 120 p.
  • 总页数 120
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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