Open AccessQuantification of the gravity wave forcing of the migrating diurnal tide in a gravity wave–resolving general circulation model
Author(s) -
Watanabe Shingo,
Miyahara Saburo
Publication year - 2009
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2008jd011218
Subject(s) - solstice , gravity wave , atmospheric sciences , atmospheric tide , forcing (mathematics) , thermosphere , tidal model , tidal waves , geology , climatology , mesosphere , atmospheric circulation , physics , latitude , gravitational wave , ionosphere , geophysics , oceanography , geodesy , stratosphere , astrophysics
The interaction of gravity waves (GWs) and the migrating diurnal tide are studied in a GW‐resolving general circulation model (GCM) by calculating the tidal components of zonal wind accelerations and equivalent Rayleigh friction due to tidal induced GW dissipation. Two 15‐day periods for perpetual equinoctial and solstice simulations are analyzed, which are performed with the Japanese Atmospheric General circulation model for Upper Atmosphere Research (JAGUAR) high‐resolution GCM. The model can directly simulate GWs with horizontal wavelengths greater than about 190 km, and, thus reproduce the general features of the mean winds and temperatures from the surface to the mesosphere and lower thermosphere (MLT). The amplitudes of the migrating diurnal tide are successfully simulated during both seasons, and the tidal winds affect the altitudes of GW dissipation in the low‐latitude MLT. The tidal component of GW forcing has maximal values of about 15 m s −1 d −1 near the maximal vertical shears of the tidal winds and generally works to shorten the vertical wavelength of the migrating diurnal tide. The phase relationship between the tidal winds and the tidal induced GW forcing is not exactly 90° out of phase, causing amplification/suppression of the tide. The GW forcing amplifies the migrating diurnal tide during the equinox, while during the solstice, it suppresses the tidal winds in the upper mesosphere of both hemispheres. This difference in behavior can be attributed to a seasonal variation of the mean zonal winds, because combination of the mean and tidal winds affects the altitudes of GW dissipation.