Abstract

Abstract. The quasi-biennial oscillation (QBO) of the zonal mean zonal wind is a dynamical phenomenon of the tropical middle atmosphere. Influences of the QBO can even be found at mid and high latitudes. It is widely accepted that the phase descent of alternating tropical easterlies and westerlies is driven by atmospheric waves of both global scale (equatorial wave modes like Kelvin, equatorial Rossby, Rossby-gravity, or inertia-gravity waves), as well as mesoscale gravity waves. However, the relative distribution of the different types of waves to the forcing of the QBO winds is highly uncertain. This is the case because until recently there were no high resolution long-term global measurements in the stratosphere. In our study we estimate Kelvin wave momentum flux and the contribution of zonal wind forcing by Kelvin waves based on space-time spectra determined from both Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) temperature measurements as well as temperatures from European Centre for Medium-Range Weather Forecasts (ECMWF) operational analyses. Peak values of total Kelvin wave zonal wind forcing found are about 0.2 m/s/day. There is good agreement between SABER and ECMWF results. Altitude-time cross sections are shown and the results are compared to the total wave forcing required to balance the background atmosphere. Sometimes Kelvin wave forcing is sufficient to explain almost the whole total wave forcing required for the momentum balance during the transition from QBO easterly to westerly winds. This is especially the case during the periods of strong westerly wind shear when the zonal wind is between −20 and 10 m/s at the equator in the altitude range 20 to 35 km. During other parts of the phases of strong westerly wind shear, however, the contribution of Kelvin waves can be comparably low and the missing wave forcing, which is often attributed to mesoscale gravity waves or intermediate scale waves, can be the by far dominant contribution of the QBO forcing. It is also found that seasonal variations of Kelvin wave accelerations could play an important role for the maintenance of the QBO westerly wind jets in the lower stratosphere.

Highlights

  • The tropics are an important region for the dynamics of the whole atmosphere

  • We carried out all analyses without subtracting the spectral background due to gravity waves, and we found that the results are almost unchanged for European Centre for Medium-Range Weather Forecasts (ECMWF)

  • For both SABER and ECMWF the accuracy of the k=1–6 momentum fluxes is in the 10% range if no vertical gradients are present

Read more

Summary

Introduction

The tropics are an important region for the dynamics of the whole atmosphere. Characteristic for the tropical region are enhanced solar heating and deep convective processes. This effect is too large to be neglected, and Dunkerton (1997) concluded that additional wave forcing by mesoscale gravity waves is required to compensate the vertical advection due to the residual mean upwelling so that the observed descent of QBO wind phases can still be explained This additional wave forcing was estimated to be about 2–4 times as strong as the forcing due to global scale equatorial wave modes (Dunkerton, 1997). First results for global scale equatorial wave modes have already been shown, for example, by Garcia et al (2005); Ern et al (2008, 2009) or Alexander et al (2008) These new sensors provide the high resolution data sets required for a better assessment of the different wave contributions to the total QBO forcing.

Theory of equatorial wave modes
Space-time spectral analysis
Zonal wind forcing by Kelvin waves
Kelvin wave temperature spectra
Kelvin wave momentum flux spectra
Wind acceleration terms derived from an ECMWF background atmosphere
Vertical smoothing of SABER temperature variances
Kelvin wave accelerations derived from SABER and ECMWF temperature variances
Comparison with previous estimates
Uncertainties of Kelvin wave momentum fluxes and zonal wind accelerations
Spectral artifacts and non-Kelvin wave contributions
Accuracy of the spectral background
Vertical oscillation of SABER temperature variances
Summary of error ranges
Uncertainties of ECMWF zonal mean meridional and vertical winds
Choice of the window length for the space-time spectral analysis
Findings
Summary and conclusions
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call