Nonmigrating diurnal tides in the thermosphere

被引:133
作者
Forbes, JM
Zhang, XL
Talaat, ER
Ward, W
机构
[1] Univ Colorado, Dept Aerosp Engn Sci, Boulder, CO 80309 USA
[2] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[3] Univ New Brunswick, Dept Phys, Fredericton, NB E3B 5A3, Canada
关键词
tides; nonmigrating; thermosphere; winds; UARS;
D O I
10.1029/2002JA009262
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] Horizontal wind measurements from the HRDI and WINDII instruments on the Upper Atmosphere Research Satellite are analyzed to reveal the most prominent nonmigrating diurnal tidal components at 95 km: the eastward propagating diurnal tide with zonal wave number s = 3 (DE3), the standing ( s = 0) diurnal oscillation (D0), and the westward propagating diurnal tide with s = 2 (DW2). The strongest DE3 occurs primarily during Northern Hemisphere summer/fall with maximum eastward winds near the equator of order 15 ms(-1) and is a vertical extension of the s = 3 Kelvin wave. The first antisymmetric mode of DE3 dominates during October-April, with maximum meridional winds near the equator of order 8 ms(-1). D0 exists during nearly all months and is nonsymmetric about the equator with maximum northward wind amplitudes in the Southern Hemisphere of order 7-10 ms(-1). DW2 closely resembles the first symmetric propagating mode from classical tidal theory, with maximum northward wind amplitudes of order 10-12 ms(-1) during September through February. The combination of DE3, D0, and DW2 with DW1 gives rise to significant longitude variations in the diurnal tide between +/-40degrees latitude. Forcing in the Global Scale Wave Model (GSWM) is calibrated according to the above observations, thus enabling global estimates of nonmigrating tidal temperatures and other fields. For instance, it is estimated that the temperature and eastward wind perturbations associated with DE3 may be as large as 20K and 35 ms(-1) at 145 km and 115 km, respectively, over the equatorial region during July.
引用
收藏
页数:10
相关论文
共 34 条
[1]   Validation of mesosphere and lower thermosphere winds from the high resolution Doppler imager on UARS [J].
Burrage, MD ;
Skinner, WR ;
Gell, DA ;
Hays, PB ;
Marshall, AR ;
Ortland, DA ;
Manson, AH ;
Franke, SJ ;
Fritts, DC ;
Hoffman, P ;
McLandress, C ;
Niciejewski, R ;
Schmidlin, FJ ;
Shepherd, GG ;
Singer, W ;
Tsuda, T ;
Vincent, RA .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1996, 101 (D6) :10365-10392
[2]  
COLL MAI, 2002, J GEOPHYS RES, V107, pA8, DOI DOI 10.1029/2001JA900179
[3]   Background wind effect on propagation of nonmigrating diurnal tides in the middle atmosphere [J].
Ekanayake, EMP ;
Aso, T ;
Miyahara, S .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 1997, 59 (04) :401-429
[4]   Climatological mean wind observations from the UARS high-resolution Doppler imager and wind imaging interferometer: Comparison with current reference models [J].
Fleming, EL ;
Chandra, S ;
Burrage, MD ;
Skinner, WR ;
Hays, PB ;
Solheim, BH ;
Shepherd, GG .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1996, 101 (D6) :10455-10473
[5]   Zonal mean and tidal dynamics from space: an empirical examination of aliasing and sampling issues [J].
Forbes, JH ;
Kilpatrick, M ;
Fritts, D ;
Manson, AH ;
Vincent, RA .
ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, 1997, 15 (09) :1158-1164
[6]   Nonmigrating tides in the thermosphere of Mars [J].
Forbes, JM ;
Bridger, AFC ;
Bougher, SW ;
Hagan, ME ;
Hollingsworth, JL ;
Keating, GM ;
Murphy, J .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2002, 107 (E11)
[7]  
Forbes JM, 2002, J GEOPHYS RES-ATMOS, V107, DOI 10.1029/2001JD001232
[8]   Diurnal Kelvin wave in the atmosphere of mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer [J].
Forbes, JM ;
Hagan, ME .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (21) :3563-3566
[9]   Dynamics of the tower thermosphere over South Pole from meteor radar wind measurements [J].
Forbes, JM ;
Portnyagin, YI ;
Makarov, NA ;
Palo, SE ;
Merzlyakov, EG ;
Zhang, X .
EARTH PLANETS AND SPACE, 1999, 51 (7-8) :611-620
[10]   FIRST RESULTS FROM THE METEOR RADAR AT SOUTH-POLE - A LARGE 12-HOUR OSCILLATION WITH ZONAL WAVE-NUMBER ONE [J].
FORBES, JM ;
MAKAROV, NA ;
PORTNYAGIN, YI .
GEOPHYSICAL RESEARCH LETTERS, 1995, 22 (23) :3247-3250