TY - JOUR
T1 - Winter temperature tides from 30 to 110 km at McMurdo (77.8°s, 166.7°E), Antarctica
T2 - Lidar observations and comparisons with WAM
AU - Fong, Weichun
AU - Lu, Xian
AU - Chu, Xinzhao
AU - Fuller-Rowell, Tim J.
AU - Yu, Zhibin
AU - Roberts, Brendan R.
AU - Chen, Cao
AU - Gardner, Chester S.
AU - McDonald, Adrian J.
N1 - Funding Information:
We sincerely acknowledge Wentao Huang, John A. Smith, and Zhangjun Wang for their contributions to the McMurdo lidar campaign. We are indebted to Jeffery M. Forbes for his invaluable advice. We are grateful to Wenbin Wang and Elsayed Talaat for their inspirational suggestions. We also appreciate Fei Wu and Rashid A. Akmaev for running and preparing WAM data. We thank the staff of the United States Antarctic Program, McMurdo Station, Antarctica New Zealand, and Scott Base for their support. We offer special thanks to Vladimir Papitashvili for his encouragement and help in this research. The lidar project was supported by NSF grants ANT-0839091 and PLR-1246405. X.L. sincerely acknowledges the generous support of the CIRES Visiting Fellows Program (http://cires.colorado.edu/collaboration/ fellowships/). MERRA data used in this study were provided by the Global Modeling and Assimilation Office (GMAO) at NASA Goddard Space Flight Center through the NASA GES DISC online archive.
Publisher Copyright:
© 2014. American Geophysical Union. All Rights Reserved.
PY - 2014/3/27
Y1 - 2014/3/27
N2 - 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.
AB - 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.
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U2 - 10.1002/2013JD020784
DO - 10.1002/2013JD020784
M3 - Article
AN - SCOPUS:84898831164
SN - 0148-0227
VL - 119
SP - 2846
EP - 2863
JO - Journal of Geophysical Research
JF - Journal of Geophysical Research
IS - 6
ER -