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Seasonal variation of non-migrating semidiurnal tide in the polar MLT region in a general circulation model
Affiliation:1. Nanotechnology and Catalysis Research Center (NANOCAT), University of Malaya, 50603 Kuala Lumpur, Malaysia;2. Physics Department, Faculty of Science, University of Sidi-Bel-Abbes, 22000, Algeria;3. School of Physics, Universiti Sains Malaysia, 11800 Penang, Malaysia;4. College of Medicine, Al Iraqia University, 1556 Baghdad, Iraq;5. Institute of Nano Electronic Engineering, University Malaysia Perlis, 01000 Kangar, Perlis, Malaysia;6. Department of Physics, Renewable Energy Laboratory, University of Tabuk, P.O. Box 741, Tabuk 71491, Saudi Arabia;7. Center for Advanced Materials, University of Houston, Houston, TX 77204-5004, USA
Abstract:Behavior of semidiurnal tides in the north and south polar MLT regions simulated by Middle Atmosphere Circulation Model at Kyushu University is described. Summertime enhancement of westward propagating semidiurnal tide with zonal wavenumber s=1 is found, which is consistent with the observed result at the South Pole (Ann. Geophys. 16 (1998) 828). Additional numerical simulations show that the non-migrating semidiurnal tide is mainly generated by the nonlinear interactions between stationary planetary waves with zonal wavenumber s=1 and the migrating semidiurnal tide in the stratosphere and mesosphere as suggested by Forbes et al. (Geophys. Res. Lett. 22(23) (1995) 3247).
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