Predictability analysis and skillful scale verification of the Lightning Potential Index (LPI) in the COSMO-D2 high resolution ensemble system

Q2 Earth and Planetary Sciences
Michele Salmi, C. Marsigli, M. Dorninger
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引用次数: 1

Abstract

Abstract. During the last decade, the constant improvement in computational capacity led to the development of the first limited-area, kilometer-scale ensemble prediction systems (L-EPS). The COSMO-D2 EPS (now ICON-D2) was the operational L-EPS at the German weather service (DWD) and has a spatial resolution of around 2.2 km. This grid resolution allows large scale, deep convective processes such as thunderstorms or heavy showers to be handled explicitly, without any physical parametrization. Special parameters involving both clouds microphysics and large scale lifting – such as the Lightning Potential Index, or LPI – have also been developed in order to try to bring the forecasting of deep convection and therefore also of lightning activity to a new level of spatial accuracy. With such high resolution forecasts comes however also a higher error potential, at least for gridpoint-verification. The use of this high resolution setup in an ensemble prediction system might however bring huge benefits in terms of skill and predictability. This work is a preliminary attempt to apply innovative verification approaches such as the dispersion Fractions Skill Score (dFSS) and the ensemble-SAL (eSAL) to the LPI in the COSMO-D2 EPS. Aim of this work is to assess the relationship between the ensemble error and the ensemble dispersion at different spatial scales. For the summer months 2019, the COSMO-D2 EPS shows a general tendency to overestimate the predictability (underestimate the ensemble spread) of the lightning events, though the spread-error relationship varies greatly for different forecast lead times. With the help of the dFSS, one can also express this relationship in terms of skillful scales. On average, the system produces a useful forecast during the afternoon hours for horizontal scales of around 200 km. However, the ensemble members show an average horizontal dispersion that amounts to around half of that value, at more or less 100 km.
COSMO-D2高分辨率集合系统雷电势指数(LPI)的可预测性分析及熟练尺度验证
摘要在过去十年中,计算能力的不断提高导致了第一个有限区域,千米尺度的集合预测系统(L-EPS)的发展。cosmos - d2 EPS(现在的ICON-D2)是德国气象局(DWD)的运行L-EPS,空间分辨率约为2.2公里。这种网格分辨率允许在没有任何物理参数化的情况下,明确地处理雷暴或暴雨等大规模、深度对流过程。涉及云微物理和大尺度抬升的特殊参数——如闪电势指数(简称LPI)——也被开发出来,以尝试将深对流的预报以及闪电活动的预报提高到一个新的空间精度水平。然而,如此高分辨率的预测也带来了更高的误差潜力,至少对于网格点验证而言。然而,在集成预测系统中使用这种高分辨率设置可能会在技能和可预测性方面带来巨大的好处。这项工作是将创新的验证方法(如分散分数技能分数(dFSS)和集成sal (eSAL))应用于cosmos - d2 EPS中的LPI的初步尝试。本文研究了不同空间尺度下系综误差与系综色散之间的关系。对于2019年夏季,cosmos - d2 EPS显示出高估闪电事件可预测性(低估集合传播)的总体趋势,尽管不同预测提前期的传播误差关系差异很大。在dFSS的帮助下,人们也可以用技巧尺度来表达这种关系。平均而言,该系统在下午为200公里左右的水平范围提供有用的预报。然而,整体成员显示平均水平色散约为该值的一半,大约在100公里左右。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Advances in Science and Research
Advances in Science and Research Earth and Planetary Sciences-Geophysics
CiteScore
4.10
自引率
0.00%
发文量
13
审稿时长
22 weeks
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