HR: 16:00h
AN: SA34A-01 [Abstracts]
TI: Nonmigrating Diurnal Tidal Variability in Mesopause Region Winds: TIDI, TIME-GCM and GSWM
Comparisons
AU: Oberheide, J
EM: joberh@uni-wuppertal.de
AF: Physics Department
Wuppertal University, Gauss Strasse 20, Wuppertal, D-42097
Germany
AU: * Hagan, M E
EM: hagan@ucar.edu
AF: National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
United States
AU: Wu, Q
EM: qwu@ucar.edu
AF: National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
United States
AU: Ortland, D A
EM: ortland@nwra.com
AF: NorthWest Research Associates, 14508 NE 20th Street, Bellevue, WA 98007-3713
United States
AU: Killeen, T L
EM: killeen@ucar.edu
AF: National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
United States
AU: Roble, R G
EM: roble@ucar.edu
AF: National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
United States
AU: Niciejewski, R
EM: niciejew@umich.edu
AF: University of Michigan, Space Physics Research Laboratory
2455 Hayward, Ann Arbor, MI 48109-2143
United States
AU: Skinner, W
EM: wskinner@umich.edu
AF: University of Michigan, Space Physics Research Laboratory
2455 Hayward, Ann Arbor, MI 48109-2143
United States
AB:
We compare nonmigrating diurnal wind estimates determined from measurements made by the TIMED Doppler Inteferometer (TIDI)
instrument on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite with predictions from the NCAR
Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM) and the Global-Scale Wave Model
(GSWM). The models account for two different nonmigrating tidal sources. The GSWM includes tropospheric latent heat release
associate with deep tropical convection, while the TIME-GCM includes nonlinear interactions between quasi-stationary
planetary waves and migrating tides. The model and measurement comparisons suggest that both sources are important to the
interpretation of the TIDI tidal winds. We contrast the true model tidal results with estimates that we determine from the
subsets of model wind predictions that represent what TIDI would observe if it flew through the model atmospheres. These
contrasts allow us to quantify the sampling issues associated determining tidal signatures from the slowly precessing TIMED
TIDI satellite data.
DE: 3332 Mesospheric dynamics
DE: 3334 Middle atmosphere dynamics (0341, 0342)
DE: 3384 Waves and tides
SC: SPA-Aeronomy [SA]
MN: 2004 AGU Fall Meeting