Abstract

The response of the period of the quasi‐biennial oscillation (QBO) to increases in tropical upwelling are considered using a one‐dimensional model. We find that the imposition of the annual cycle in tropical upwelling creates substantial variability in the period of the QBO. The annual cycle creates synchronisation regions in the wave forcing space, within which the QBO period locks onto an integer multiple of the annual forcing period. Outside of these regions, the QBO period undergoes discrete jumps as it attempts to find a stable relationship with the oscillator forcing. The resulting set of QBO periods can be either discrete or broad‐banded, depending on the intrinsic period of the QBO.We use the same model to study the evolution of the QBO period as the strength of tropical upwelling increases, as would be expected in a warmer climate. The QBO period lengthens and migrates closer towards 36‐ and 48‐month locking regions as upwelling increases. The QBO period does not vary continuously with increased upwelling, however, but instead transitions through a series of two‐ and three‐cycles before becoming locked to the annual cycle. Finally, some observational evidence for the cyclical behaviour of the QBO periods in the real atmosphere is presented.

Highlights

  • The quasi-biennial oscillation (QBO) is the dominant mode of variability in the equatorial stratosphere (Baldwin et al, 2001)

  • In the context of increasing tropical upwelling, we investigate the evolution of the QBO period and suggest the possibility that the QBO period may adjust toward a 36-month period in a warming climate

  • Because of the tendency of the QBO to stay in a synchronised state with the annual cycle, the upwelling has to become quite strong before the period of a QBO in a frequency-locked regime

Read more

Summary

Introduction

The quasi-biennial oscillation (QBO) is the dominant mode of variability in the equatorial stratosphere (Baldwin et al, 2001). The oscillation arises as the result of a wave–mean flow interaction between the background stratospheric winds and a wide variety of tropospheric equatorial waves (Lindzen and Holton, 1968; Holton and Lindzen, 1972). As these waves propagate vertically through the stratosphere, they dissipate and deposit momentum into the mean flow. Certain combinations of waves can create different zonal accelerations in height that change as the mean flow evolves, allowing for the creation of an oscillation in the zonal wind (Plumb, 1977)

Methods
Results
Conclusion
Full Text
Paper version not known

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

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.