Seasonal variations of the semi-diurnal and diurnal tides in the MLT:: multi-year MF radar observations from 2 to 70°N, and the GSWM tidal model

被引:90
作者
Manson, A
Meek, C
Hagan, M
Hall, C
Hocking, W
MacDougall, J
Franke, S
Riggin, D
Fritts, D
Vincent, R
Burrage, M
机构
[1] Univ Saskatchewan, Inst Space & Atmospher Studies, Saskatoon, SK S7N 5E2, Canada
[2] NCAR, Boulder, CO USA
[3] Univ Tromso, Auroral Observ, Tromso, Norway
[4] Univ Western Ontario, Dept Phys & Astron, London, ON, Canada
[5] Univ Illinois, Space Sci & Remote Sensing Lab, Urbana, IL USA
[6] Colorado Res Associates, Boulder, CO USA
[7] Univ Adelaide, Dept Phys & Math Phys, Adelaide, SA, Australia
[8] Univ Michigan, Space Phys Res Lab, Ann Arbor, MI 48109 USA
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词
D O I
10.1016/S1364-6826(99)00045-0
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Continuous observations of the wind field have been made by six Medium Frequency Radars (MFRs), located between the equator and high northern latitudes: Christmas Islands (2 degrees N), Hawaii (22 degrees N), Urbana (40 degrees N), London (43 degrees N), Saskatoon (52 degrees N) and Tromso (70 degrees N). Data have been sought for the time interval 1990-1997, and typically 5 years of data have become available from each station, to demonstrate the level of annual consistency and variability. Common harmonic analysis is applied so that the monthly amplitudes and phases of the semi-diurnal (SD) and diurnal (D) wind oscillations are available in the height range of (typically) 75-95 km in the upper Middle Atmosphere. Comparisons are made with tides from the Global Scale Wave Model (GSWM), which are available for 3-month seasons. The emphasis is upon the monthly climatologies at each location based upon comparisons of profiles, and also latitudinal plots of amplitudes and phases at particular heights. For the diurnal tide, the agreement between observations and model is now quite excellent with modelled values frequently lying within the range of yearly values. Both observations and model demonstrate strong seasonal changes. This result is a striking improvement over the comparisons of 1989 (JATP, Special issue). In particular, the phases and phase-gradients for the non-winter months at mid- to high-latitudes are now in excellent agreement. Some of the low latitude discrepancies are attributed to the existence of non-migrating tidal components associated with tropospheric latent heat release. For the semi-diurnal tide, the observed strong transitions between clear solstitial states are less well captured by the model. There is little evidence for improvement over the promising comparisons of 1989. In particular, the late-summer/autumnal tidal maximum of mid-latitudes is observed to be larger, and with strong monthly variability. Also the summer modelled tide has unobserved short (20 km) wavelengths at high latitudes, and much smaller amplitudes than observed at all extratropical locations. Possible improvements for the GSWM's simulations of the SD tide are discussed, which involve migrating tidal modes due to tropospheric latent heating. (C) 1999 Elsevier Science Ltd. All rights reserved.
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收藏
页码:809 / 828
页数:20
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