The 10-day planetary wave examined by Odin/OSIRIS ozone profiles during late March 2002: comparison with UKMO and MF radar data

被引:3
作者
Chen, Shengbo [1 ]
Meek, C. E. [2 ]
Manson, A. H. [2 ]
Chshyolkova, T. [2 ]
机构
[1] Jilin Univ, Coll Geoexplorat Sci & Technol, Changchun 130023, Peoples R China
[2] Univ Saskatchewan, Inst Space & Atmospher Studies, Saskatoon, SK S7N 0W0, Canada
基金
国家高技术研究发展计划(863计划);
关键词
MODE ROSSBY WAVES; NONUNIFORM BACKGROUND CONFIGURATIONS; UPPER-STRATOSPHERE; SPECTRAL-ANALYSIS; SYMMETRIC MODES; LEAST-SQUARES; TIME-SERIES; SPACED DATA; HOLE SPLIT; VARIABILITY;
D O I
10.1080/01431160903571817
中图分类号
TP7 [遥感技术];
学科分类号
081102 ; 0816 ; 081602 ; 083002 ; 1404 ;
摘要
Ozone profile data have been retrieved from the Optical Spectrograph and InfraRed Imager System (OSIRIS) instrument onboard the Odin Satellite, which was launched on 20 February 2001. Considering the irregular sampling of the OSIRIS, a least-squares fit method is employed to provide the wavenumber and frequency spectra of the waves affecting the OSIRIS ozone profile distributions. Meanwhile, criteria are developed and applied for reducing spectral biases. Then spectral analysis of the global OSIRIS ozone profiles data is perfomred at altitudes of 38.5 km and 40.5 km within two latitude bins 35 degrees-45 degrees N and 45 degrees-55 degrees N during days 75-105 of the year 2002. Specifically, a westward-propagating 10-day planetary wave is detected and validated by medium frequency (MF) Radar (MFR) at Platteville (40 degrees N, 105 degrees W) and Saskatoon (52 degrees N, 107 degrees W), and UKMO global stratospheric data (UK Meteorological Office assimilated model). The spatial and temporal distributions of the global OSIRIS ozone profile data are shown to allow identification of major planetary wave features in the middle atmosphere.
引用
收藏
页码:1531 / 1544
页数:14
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