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首页> 外文期刊>Annales Geophysicae >Planetary waves in ozone and temperature in the Northern Hemisphere winters of 2002/2003 and early 2005
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Planetary waves in ozone and temperature in the Northern Hemisphere winters of 2002/2003 and early 2005

机译:2002/2003年和2005年初北半球冬季臭氧和温度的行星波

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摘要

Temperature and ozone data from the sub-millimetre radiometer (SMR)installed aboard the Odin satellite have been examined to study therelationship between temperature and ozone concentration in the lower andupper stratosphere in winter time. The retrieved ozone and temperatureprofiles have been considered between the range of 24–46 km during theNorthern Hemisphere (NH) winter of December 2002 to March 2003 and Januaryto March 2005. A comparison between the ozone mixing ratio and temperaturefields has been made for the zonal means, wavenumber one variations and5-day planetary waves. The amplitude values in temperature variations are~5 K in the wavenumber one and 0.5–1 K in the 5-day wave. In ozonemixing ratio, the amplitudes reach ~0.5 ppmv in the wavenumber oneand 0.05–0.1 ppmv in the 5-day wave.Several stratospheric warming events were observed during the NH winters of2002/2003 and early 2005. Along with these warming events, amplification ofthe amplitude has been detected in wavenumber one (up to 30 K in temperatureand 1.25 ppmv in ozone) and partly in the 5-day perturbation (up to 2 K intemperature and 0.2 ppmv in ozone).In general, the results show the expected in-phase behavior between thetemperature and ozone fields in the lower stratosphere due to dynamiceffects, and an out-of-phase pattern in the upper stratosphere, which isexpected as a result of photochemical effects. However, these relationshipsare not valid for zonal means and wavenumber one components when the waveamplitudes are changing dramatically during the strongest stratosphericwarming event (at the end of December 2002/beginning of January 2003). Also,for several shorter intervals, the 5-day perturbations in ozone andtemperature are not well-correlated at lower heights, particularly whenconditions change rapidly.Odin's basic observation schedule provides stratosphere mode data everythird day and to validate the reliability of the 5-day waves extracted fromthe Odin measurements, additional independent data have been analysed inthis study: temperature assimilation data by the European Centre forMedium-range Weather Forecasts (ECMWF) for the NH winter of 2002/2003, andsatellite measurements of temperature and ozone by the Microwave LimbSounder (MLS) on board the Aura satellite for the NH winter in early 2005.Good agreement between the temperature fields from Odin and ECMWF data isfound at middle latitude where, in general, the 5-day perturbations from thetwo data sets coincide in both phase and amplitude throughout the examinedinterval. Analysis of the wavenumber one and the 5-day wave perturbations intemperature and ozone fields from Odin and from Aura demonstrates that, forthe largest part of the examined period, quite similar characteristics arefound in the spatial and temporal domain, with slightly larger amplitudevalues seen by Aura. Hence, the comparison between the Odin data, sampledeach third day, and daily data from Aura and the ECMWF shows that the Odindata are sufficiently reliable to estimate the properties of the 5-dayoscillations, at least for the locations and time intervals with strong waveactivity.
机译:已经检查了安装在奥丁卫星上的亚毫米辐射计(SMR)的温度和臭氧数据,以研究冬季平流层上下两层的温度与臭氧浓度之间的关系。在2002年12月至2003年3月的北半球冬季(NH)和2005年1月至2005年3月的24-46 km范围内,已考虑了所获得的臭氧和温度分布图。比较了臭氧混合比和温度场的区域平均值。 ,一号变星和5天的行星波。在第一波中,温度变化的幅度值为〜5 K,在5天波中,其幅度值为0.5-1K。在臭氧混合比中,一号波的振幅达到〜0.5 ppmv,五日波的振幅达到0.05-0.1 ppmv。 在2002/2003年和2005年初的NH冬季观测到几次平流层变暖事件。在这些变暖事件中,在第一波中(温度高达30 K,在臭氧中为1.25 ppmv)检测到振幅的放大,在第五天扰动中(温度高达2 K,在臭氧中为0.2 ppmv)检测到了振幅的放大。 <通常,结果表明,由于动态效应,平流层下部的温度和臭氧场之间具有预期的同相行为,而平流层上部的相变模式则是由于光化学效应而预期的。但是,当在最强的平流层变暖事件中(2002年12月底/ 2003年1月初)波幅发生剧烈变化时,这些关系对于区域平均值和波数为1的分量无效。另外,在几个较短的时间间隔内,在较低高度下,臭氧和温度的5天扰动并没有很好的相关性,尤其是在条件迅速变化的情况下。 Odin的基本观测计划每三天提供一次平流层模式数据并验证其可靠性从Odin测量中提取的5天波中,本研究还分析了其他独立数据:2002/2003 NH冬季欧洲中距离天气预报中心(ECMWF)的温度同化数据,以及温度和臭氧的卫星测量由Microwave LimbSounder(MLS)于2005年初安装在Aura卫星上,用于NH冬季。 在中纬度地区(通常为5天),Odin和ECMWF数据的温度场之间存在良好的一致性。在整个检查间隔中,来自两个数据集的扰动在相位和幅度上都一致。对来自Odin和Aura的温度和臭氧场的第一波和5天波扰动的分析表明,在所考察的大部分时间段中,在时空范围内都发现了非常相似的特征,Aura看到的振幅值略大。因此,第三天采样的奥丁数据与来自Aura和ECMWF的每日数据之间的比较表明,奥丁数据至少在具有强波活动性的位置和时间间隔上足够可靠,可以估计5天振荡的性质。

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