Abstract

Abstract. A numerical study of mountain waves in the Upper Troposphere and Lower Stratosphere (UTLS) is presented for two Intensive Observational Periods (IOPs) of the Terrain-induced Rotor Experiment (T-REX). The simulations use the Weather Research and Forecasting (WRF) model and a microscale model that is driven by the finest WRF nest. During IOP8, the simulation results reveal presence of perturbations with short wavelengths in zones of strong vertical wind shear in the UTLS that cause a reversal of momentum fluxes. The spectral properties of these perturbations and the attendant vertical profiles of heat and momentum fluxes show strong divergence near the tropopause indicating that they are generated by shear instability along shear lines locally induced by the primary mountain wave originating from the lower troposphere. This is further confirmed by results of an idealized simulation initialized with the temperature and wind profiles obtained from the microscale model. For IOP6, we analyze distributions of O3 and CO observed in aircraft measurements. They show small scale fluctuations with amplitudes and phases that vary along the path of the flight. Detailed comparisons between these fluctuations and the observed vertical velocity show that the behavior of these short fluctuations is due not only to the vertical motion, but also to the local mean vertical gradients where the waves evolve, which are modulated by larger variations. The microscale model simulation results show favorable agreement with in situ radiosonde and aircraft observations. The high vertical resolution offered by the microscale model is found to be critical for resolution of smaller scale processes such as formation of inversion layer associated with trapped lee waves in the troposphere, and propagating mountain waves in the lower stratosphere.

Highlights

  • The extended region consisting of the bulk of the upper troposphere and lower stratosphere (UTLS) represents a significant challenge for numerical prediction

  • Observations as well as high resolution idealized simulations have shown that waves above over-shooting moist convection may cause small scale mixing in the UTLS through local turbulence and instabilities that can be triggered during gravity wave breaking events (e.g. Wang, 2003; Moustaoui et al, 2004; Lane and Sharman, 2006)

  • We examine some characteristics of mountain wave dynamics in the UTLS region that were observed during the Terrain-induced Rotor Experiment (T-REX)

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Summary

Introduction

The extended region consisting of the bulk of the upper troposphere and lower stratosphere (UTLS) represents a significant challenge for numerical prediction. Mahalov et al.: A numerical study of mountain waves of the UTLS region This low vertical grid spacing in UTLS used in NWP models prevents the resolution of small scale dynamical processes such as wave breaking and secondary wave generation near the tropopause and in the lower stratosphere that are associated with vertically propagating mountain waves. Kirkwood et al (2010) used radar observations and WRF model simulations to study turbulence associated with mountain waves over Northern Scandinavia They found that WRF can accurately match the vertical wind signatures at the radar site. We present results from high-resolution numerical simulations ( x = 1 km and 180 vertical levels) of two T-REX Intense Observing Periods (IOP8 and IOP6), which shed new light on dynamical process in UTLS that lead to secondary generation of smallscale fluctuations induced by shear instability there (IOP8).

T-REX field campaign
IOP 8 observations
WRF simulations
Microscale model
Comparison between simulations and observations
Simulation results
Characteristics of short fluctuations
Generation mechanism
Variations in the amplitudes of O3 and CO
Variations in the phases of O3 and CO
The role of the vertical gradients
Conclusions
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