Friday, 13 June 2003: 11:45 AM
Stratospheric influence on the troposphere by planetary wave reflection
Statistical and dynamic diagnostics are combined to study the
formation of reflecting surfaces in the Northern Hemisphere
stratosphere and their impact on tropospheric waves. A time-lagged
singular value decomposition analysis is applied to daily tropospheric
and stratospheric height fields recomposed for a single zonal
wavenumber. This approach shows time lags at which the covariance
between the two fields is maximized and isolates the leading coupled
modes between the two fields. A wave geometry diagnostic for wave
propagation characteristics which separates the index of reflection
into vertical and meridional components is used to diagnose the
occurrence of reflecting surfaces. Results from the two types of
diagnostics show evidence of reflection for waves of zonal wavenumber
1 during high-winter (January to March, JFM), and not during fall
(September to November). Due to large interannual variability during
JFM, reflection does not occur during all winter seasons between 1979
-2002, but occurs frequently enough to give a maximum relationship
between tropospheric and stratospheric wave 1 fields when the
stratosphere is leading by a few days. Both diagnostics, however,
show much clearer evidence for reflection and its effect on the
troposphere, when we separate the data corresponding to months/seasons
with reflective and non-reflective basic states. The analysis of the
basic states shows the formation of one characteristic configuration
of the stratospheric jet which reflects waves back into the
troposphere - when the polar nigh jet peaks in the high latitude
mid-stratosphere. This configuration is related to the formation of a
reflecting surface for vertical propagation at around 5 hPa as a
result of the vertical curvature and a clear meridional
waveguide in the lower to middle stratosphere, that channels the
reflected wave activity to the high latitude troposphere. The
effect of the reflected waves on the tropospheric circulation will
also be discussed.
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