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NO_x production by lightning in Hector: First airborne measurements during SCOUT-O3/ACTIVE

机译:赫克托尔闪电产生的NO_x:SCOUT-O3 / ACTIVE期间的首次空中测量

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During the SCOUT-O3/ACTIVE field phase in November??" December 2005, airborne in situ measurements were performed inside and in the vicinity of thunderstorms over northern Australia with several research aircraft (German Falcon, Russian M55 Geophysica, and British Dornier-228. Here a case study from 19 November is presented in detail on the basis of airborne trace gas measurements (NO, NO_y, CO, O_3) and stroke measurements from the German LIghtning Location NETwork (LINET), set up in the vicinity of Darwin during the field campaign. The anvil outflow from three different types of thunderstorms was probed by the Falcon aircraft: (1) a continental thunderstorm developing in a tropical airmass near Darwin, (2) a mesoscale convective system (MCS), known as Hector, developing within the tropical maritime continent (Tiwi Islands), and (3) a continental thunderstorm developing in a subtropical airmass ~200 km south of Darwin. For the first time detailed measurements of NO were performed in the Hector outflow. The highest NO mixing ratios were observed in Hector with peaks up to 7 nmol mol~(−1) in the main anvil outflow at ~11.5??"12.5 km altitude. The mean NO_x (Combining double low lineNO+NO_2) mixing ratios during these penetrations (~100 km width) varied between 2.2 and 2.5 nmol mol~(−1). The NO_x contribution from the boundary layer (BL), transported upward with the convection, to total anvil-NO_x was found to be minor (<10%). On the basis of Falcon measurements, the mass flux of lightning-produced NO_x (LNO_x) in the well-developed Hector system was estimated to 0.6??"0.7 kg(N) s ~(−1). The highest average stroke rate of the probed thunderstorms was observed in the Hector system with 0.2 strokes s ~(−1) (here only strokes with peak currents ≥10 kA contributing to LNO_x were considered). The LNO_x mass flux and the stroke rate were combined to estimate the LNO_x production rate in the different thunderstorm types. For a better comparison with other studies, LINET strokes were scaled with Lightning Imaging Sensor (LIS) flashes. The LNO_x production rate per LIS flash was estimated to 4.1??"4.8 kg(N) for the well-developed Hector system, and to 5.4 and 1.7 kg(N) for the continental thunderstorms developing in subtropical and tropical airmasses, respectively. If we assume, that these different types of thunderstorms are typical thunderstorms globally (LIS flash rate ~44 s ~(−1)), the annual global LNO_x production rate based on Hector would be ~5.7??"6.6 Tg(N) a ~(−1) and based on the continental thunderstorms developing in subtropical and tropical airmasses ~7.6 and ~2.4 Tg(N) a ~(−1), respectively. The latter thunderstorm type produced much less LNO_x per flash compared to the subtropical and Hector thunderstorms, which may be caused by the shorter mean flash component length observed in this storm. It is suggested that the vertical wind shear influences the horizontal extension of the charged layers, which seems to play an important role for the flash lengths that may originate. In addition, the horizontal dimension of the anvil outflow and the cell organisation within the thunderstorm system are probably important parameters influencing flash length and hence LNO_x production per flash.
机译:在2005年11月的11月的SCOUT-O3 / ACTIVE野外试验阶段——2005年12月,澳大利亚北部的雷暴内部和附近进行了机载原位测量,并使用了几架研究飞机(德国的“猎鹰”,俄罗斯的M55 地球物理学报和英国的 Dornier-228 。这里根据空气中的痕量气体测量值(NO,NO_y,CO,O_3)详细介绍了11月19日的案例研究野战期间在达尔文附近建立的德国闪电定位网络(LINET)进行了最大的行程和冲程测量,猎鹰飞机探查了三种不同类型的雷暴的砧座流出情况:(1)达尔文附近的热带气团,(2)在热带海洋大陆(提维群岛)内发展的中尺度对流系统(MCS),称为赫克托(Hector),以及(3)在达尔文以南约200公里的亚热带气团中发生的大陆性雷暴。首次详细测量N O在赫克托流出中进行。在Hector观察到最高的NO混合比,在〜11.5?“ 12.5 km的高度,主砧流出的峰值达到7 nmol mol〜(-1)。在此期间,平均NO_x(混合双低线NO + NO_2)混合比这些穿透(〜100 km的宽度)在2.2至2.5 nmol mol〜(-1)之间变化。边界层(BL)的NO_x随对流向上传输,对总砧座NO_x的贡献很小(< 10%)。根据猎鹰的测量,在发达的赫克托系统中,闪电产生的NO_x(LNO_x)的质量通量估计为0.6≤“ 0.7 kg(N)s〜(-1)。在Hector系统中观察到探测到的雷暴的最高平均冲程速率为0.2冲程s〜(-1)(此处仅考虑峰值电流≥10kA的冲程对LNO_x的影响)。将LNO_x质量通量和冲程速率结合起来,以估计不同雷暴类型中的LNO_x生产率。为了与其他研究更好地比较,使用闪电成像传感器(LIS)闪光灯对LINET笔划进行了缩放。对于发达的赫克托系统,每个LIS闪现的LNO_x生产率估计为4.1≤4.8kg(N),对于在亚热带和热带气团中发生的大陆雷暴,分别为5.4和1.7 kg(N)。我们假设,这些不同类型的雷暴是全球典型的雷暴(LIS闪速〜44 s〜(-1)),基于赫克托尔的全球年度LNO_x生产率为〜5.7 ??“ 6.6 Tg(N)a〜 (−1)并基于在亚热带和热带气团中分别产生的大陆性雷暴〜7.6和〜2.4 Tg(N)a〜(-1)。与亚热带和赫克托雷暴相比,后一种雷暴类型每次闪光产生的LNO_x少得多,这可能是由于在该风暴中观察到的平均闪光分量长度较短所致。建议垂直风切变影响带电层的水平延伸,这似乎对可能产生的闪光长度起重要作用。另外,砧座流出物的水平尺寸和雷暴系统内的细胞组织可能是影响闪光长度并因此影响每次闪光产生LNO_x的重要参数。

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