HR: 08:20h
AN: A11E-02 INVITED [Abstracts]
TI: The Transfer of the Solar Signal From the Stratosphere to the Troposphere: Northern Winter
AU: * Matthes, K
EM: kmatthes@ucar.edu
AF: Freie Universitaet Berlin,
Institut fuer Meteorologie, Carl-Heinrich-Becker-Weg 6-10, Berlin, 12165
Germany
AU: * Matthes, K
EM: kmatthes@ucar.edu
AF: National Center for Atmospheric Research, 1850 Table Mesa Drive, Boulder, CO 80305
United States
AB:
The atmospheric response to the solar cycle has been previously investigated with the Freie Universitaet Berlin Climate
Middle Atmosphere Model (FUB-CMAM) using prescribed spectral solar UV and ozone changes as well as prescribed equatorial,
QBO-like winds. The solar signal is transferred from the upper to the lower stratosphere through a modulation of the polar
night jet and the Brewer-Dobson circulation. The interaction between QBO and solar signal are comparable to estimates from
observations.
These model experiments are further investigated here to show the transfer of the solar signal from the lower stratosphere to
the troposphere and down to the surface during northern hemisphere winter. During October and November, the model response
is concentrated in the stratosphere. However, during December and January there is a significant response in tropospheric
circulation which decays in February. Analysis focuses on the transition from the early winter stratospheric-dominated signal
to the mid-winter tropospheric-dominated signal. The results show that the stratosphere has an important effect on
tropospheric changes through a stratospheric-tropospheric circulation regime that develops in December and January and
disappears in February.
The Brewer-Dobson circulation provides the link between low and high latitude changes as well as between upper and lower
stratospheric changes. Dynamical heating in the tropical lower stratosphere induces circulation changes (changes in
tropopause height, static stability, convection and precipitation) in the tropical troposphere and down to the surface. These
effects are identified as indirect effects from the stratosphere mainly because the sea surface temperatures are identical
in the solar maximum and minimum experiment. The tropospheric changes confirm results from other simplified model studies as
well as results from observations.
DE: 3334 Middle atmosphere dynamics (0341, 0342)
DE: 3362 Stratosphere/troposphere interactions
DE: 1610 Atmosphere (0315, 0325)
DE: 1620 Climate dynamics (3309)
DE: 1650 Solar variability
SC: Atmospheric Sciences [A]
MN: 2004 AGU Fall Meeting