We provide the first characterization of diurnal and semidiurnal thermal tides in temperature from 30 to 110 km in the winter season (May through August) at McMurdo (77.8°S, 166.7°E), Antarctica. The observations were made with an Fe Boltzmann temperature lidar in 2011 and 2012. Over 330 h of winter data are compiled into a composite day of temperature perturbations that significantly reduce the incoherent wave effects while preserving the coherent tidal signatures. Both diurnal and semidiurnal tides have small amplitudes (less than 3 K) below 100 km with vertical wavelengths of~29 and~23 km, respectively. A new finding of this study is the fast growth of diurnal and semidiurnal tidal amplitudes above 100 km to at least 15 K near 110 km, exceeding that of the freely propagating tides originating from the lower atmosphere. Such fast growth exists for all Kp index cases and diurnal amplitude increases to 15-30 K at 110 km with larger Kp indices corresponding to larger tidal amplitudes and faster growth rates. The slopes of diurnal tidal phases become steeper above 100 km, and the tidal phases barely change with altitude from 100 to 106 km. The tidal growth behavior is reproduced in the Whole Atmosphere Model (WAM) with phases comparable to the observations but magnitudes significantly underestimated. WAM compares reasonably well with the observations below 100 km. The observed significant amplitude increases and phase structure changes suggest additional tidal sources near or above 100 km, which deserve future investigation.
IntroductionAtmospheric tides are global-scale oscillations in pressure, density, temperature, and wind fields for which the periods are harmonics of a solar day. They can be classified as migrating (Sun-synchronous) and nonmigrating (non-Sun-synchronous) tides according to their horizontal phase velocities, i.e., migrating tides follow the motion of the Sun. The driving forces of migrating tides are mainly periodic absorption of solar radiation in the atmosphere, and those for nonmigrating tides are mainly latent heat release in the tropical region [Hagan and Forbes, 2002;Zhang et al., 2010aZhang et al., , 2010b and nonlinear interactions between planetary waves and migrating tides [Angelats i Coll and Forbes, 2002;Hagan and Roble, 2001;Murphy et al., 2009]. Tides can obtain large amplitudes in the middle and upper atmosphere, where they modulate ionospheric variability via the E region dynamo effect [Forbes et al., 2000;Forbes et al., 2008], enhance vertical atmosphere coupling [Forbes et al., 2000;Immel et al., 2006], and cause instabilities by inducing significant temperature gradients and wind shears [Hecht et al., 1997;Liu et al., 2004]. Tides affect the propagation of gravity waves (GWs) [Walterscheid, 1981;Lu et al., 2009] and modulate GW momentum fluxes [Fritts and Vincent, 1987;Espy et al., 2004;Liu et al., 2013]. Tides also impact the vertical transport of atmospheric constituents and thereby the total solar heating in the upper part of the middle atmosphere [Smith et al., ...