Abstract

Abstract. A new parameterization of the lightning-produced NOx has been developed for cloud-resolving models. This parameterization is based on the unique characteristics of identifying which convective cells are capable of producing lightning based on a vertical velocity threshold and estimating the lightning flash rate in each convective cell from the non-precipitation and precipitation ice mass flux product. Further, the source location is filamentary instead of volumetric as in most previous parameterizations. This parameterization has been tested on the 10 July 1996 Stratospheric-Tropospheric Experiment: Radiation, Aerosols and Ozone (STERAO) storm. Comparisons of the simulated flash rate and NO mixing ratio (control experiment) with observations at different locations and stages of the storm show good agreement. An individual flash produces on average 121±41 moles of NO (7.3±2.5×1025 molecules NO) for the simulated high cloud base, high shear storm that is dominated by intra-cloud flash activity. Sensitivity tests have been performed to study the impact of the flash rate, the cloud-to-ground flash ratio, the flash length, the spatial distribution of the NO molecules, and the production rate per flash on the NO concentration and distribution. Results show a strong impact from the flash rate, the spatial placement of the lightning-NOx source and the number of moles produced per flash. On the other hand, the simulations show almost no impact from the different cloud-to-ground (CG) ratios and the lightning-NOx production rates per CG flash used as input to the model.

Highlights

  • Lightning flashes are considered to be a major source for nitrogen oxides (NOx=NO+NO2) in the upper troposphere

  • The models that predicted the lower lightning-produced NOx (LNOx) production rates are the ones using explicit electrical schemes, which placed the lightning-produced NO source in a small volume along the simulated lightning flash and reproduced the observed peaks and flux quite well for this storm

  • Comparison between optical radiation detected by NASA Optical Transcient Detector (OTD) and VHF radiaton recorded by interferometeric mapper (ITF) for one passage over the STERAOA domain (9 July 1996) showed consistent observations between OTD and ITF (Defer et al, 2006), suggesting that a flash sensed by OTD corresponds to a flash sensed by ITF

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Summary

Introduction

Lightning flashes are considered to be a major source for nitrogen oxides (NOx=NO+NO2) in the upper troposphere. The CG flash rate is derived either from the depth of the layer from the freezing level to the cloud top height (Price and Rind, 1992; Pickering et al, 1998; Fehr et al, 2004) or deduced from global observations (Wang and Prinn, 2000). The models that predicted the lower LNOx production rates are the ones using explicit electrical schemes, which placed the lightning-produced NO source in a small volume along the simulated lightning flash (filamentary) and reproduced the observed peaks and flux quite well for this storm.

Description of the lightning-produced NOx parameterization
The WRF model
The 10 July 1996 STERAO storm
Initialization
Results
Sensitivity analyses
Total flash rate
Cloud-to-ground flash rate
Altitude of the upper and lower modes for the bimodal distribution
Flash length
Short duration flashes
Production of NO per flash
Findings
Conclusions
Full Text
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