4.10
Climatology of Wave Breaking and Mixing in the Northern Hemisphere Summer Stratosphere
Richard E. Wagner, Texas A&M Univ., College Station, TX; and K. P. Bowman
The cause of large zonal ozone variations observed by POAM II (Polar Ozone and Aerosol Measurement II) in the Northern Hemisphere summer stratosphere between 55°N-65°N and ~20-30 km is investigated using the United Kingdom Meteorological Office stratospheric data set. This study tests the hypothesis from Hoppel et al. [1999] that breaking of westward-propagating planetary waves in the induces substantial meridional transport which is responsible for the observed ozone variance.
EP-flux vectors calculated from the UKMO data show that wave activity propagates vertically from source regions in the lower troposphere into the stratosphere during the NH summer. In the region of maximum ozone variance (RMV), the EP-flux divergence is clearly nonzero, which means the zonal-mean zonal flow is forced by waves in this region. Close examination of the individual zonal wavenumber contributions to the climatological monthly-mean EP-flux divergence shows that contributions by zonal wavenumbers 1-5 generally account for over 90% of the forcing of the zonal-mean flow in the lower half of the RMV from June to August. In the upper half of the RMV, planetary waves 1-3 dominate the forcing in June and July, but waves 1-5 appear to be able to penetrate to all RMV levels in August.
The forcing of the zonal-mean flow in the RMV is shown to be driven primarily by dissipation of waves that are breaking at critical levels in the region. Power spectra show power in westward-propagating waves 1-5 with phase speeds equal to the zonal-mean flow at all RMV levels. Therefore, breaking waves in the RMV are westward-propagating waves 1-5.
EP flux divergence, meridional mixing (transport), and ozone variance in the RMV are all shown to decrease from June to July and increase in August in a similar fashion. This trend is also mirrored specifically in the amplitudes of zonal waves 1-5, further connecting the meridional transport (which induces the ozone variance in the RMV) to the breaking of westward-propagating planetary-scale waves 1-3 and medium-scale waves 4-5 in the RMV, lending credibility to the hypothesis in Hoppel et al. [1999].
Session 4, Continued
Tuesday, 11 January 2000, 2:15 PM-4:45 PM
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