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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Ozone quasi-biennial oscillations (QBO), semiannual oscillations (SAO), and correlations with temperature in the mesosphere, lower thermosphere, and stratosphere, based on measurements from SABER on TIMED and MLS on UARS
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Ozone quasi-biennial oscillations (QBO), semiannual oscillations (SAO), and correlations with temperature in the mesosphere, lower thermosphere, and stratosphere, based on measurements from SABER on TIMED and MLS on UARS

机译:基于TIMED的SABER和UARS的MLS的测量结果,臭氧准双年度振荡(QBO),半年振荡(SAO)及其与中层,较低热圈和平流层温度的相关性

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摘要

The ozone and temperature measurements from Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) on the Thermosphere-Ionosphere-Mesosphere-Energetics and Dynamics (TIMED) satellite form a unique set. They provide global information over the range of local solar times, from the lower stratosphere into the lower thermosphere, going back to 2002, by one instrument. On the basis of zonal means of these data, we present new results from 20 to 100 km in altitude and from 48°S to 48°N in latitude of ozone and temperature semiannual oscillations (SAO) and quasi-biennial oscillations (QBO). While some of the results are new for the stratosphere, such results for the mesosphere and lower thermosphere (MLT) have not been available before. The SAO and QBO components are mostly symmetric with respect to the Equator. The correlations of ozone and temperatures provide the opportunity to study the relative effects of dynamics and chemistry. Our results show that the ozone oscillations are largely and positively correlated to those of the temperature below about 30 km and above 80 km, and mostly anti-correlated with temperature between about 30 and 80 km. We compare with measurements made about 10 years earlier by the MLS instrument on UARS, and with results by others from the solar mesosphere explorer (SME) satellite, the solar backscatter ultraviolet (SBUV), space shuttle experiments (CRISTA), and ground-based measurements.
机译:在热层-电离层-中层层-能量和动力学(TIMED)卫星上使用宽带发射辐射法(SABER)从大气探测中测量臭氧和温度的方法构成了一个独特的集合。它们利用一种仪器提供了从低平流层到低热圈的局部太阳时间范围的全球信息,可以追溯到2002年。根据这些数据的区域平均值,我们给出了海拔20至100 km和臭氧纬度和温度半年度振荡(SAO)和准两年度振荡(QBO)从48°S至48°N的新结果。尽管对平流层来说有些结果是新的,但对于中层和低热层(MLT)来说,这种结果以前是不可用的。 SAO和QBO分量相对于赤道基本对称。臭氧与温度的相互关系为研究动力学和化学的相对影响提供了机会。我们的结果表明,臭氧振荡与低于30 km和高于80 km的温度在很大程度上呈正相关,并且与与在30至80 km之间的温度成反比。我们将其与UARS上的MLS仪器大约10年前进行的测量进行了比较,并将其与太阳中层探索器(SME)卫星,太阳反向散射紫外线(SBUV),航天飞机实验(CRISTA)和基于地面测量。

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