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Nighttime ozone profiles in the stratosphere and mesosphere by the Global Ozone Monitoring by Occultation of Stars on Envisat

机译:通过Envisat上的星际掩星监测全球平流层和中层夜间臭氧分布。

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摘要

The Global Ozone Monitoring by Occultation of Stars (GOMOS) instrument on board the European Space Agency's Envisat satellite measures ozone and a few other trace gases using the stellar occultation method. Global coverage, good vertical resolution and the self-calibrating measurement method make GOMOS observations a promising data set for building various climatologies. In this paper we present the nighttime stratospheric ozone distribution measured by GOMOS in 2003. We show monthly latitudinal distributions of the ozone number density and mixing ratio profiles, as well as the seasonal variations of profiles at several latitudes. The stratospheric profiles are compared with the Fortuin-Kelder daytime ozone climatology. Large differences are found in polar areas and they can be shown to be correlated with large increases of NO2. In the upper stratosphere, ozone values from GOMOS are systematically larger than in the Fortuin-Kelder climatology, which can be explained by the diurnal variation. In the middle and lower stratosphere, GOMOS finds a few percent less ozone than Fortuin-Kelder. In the equatorial area, at heights of around 15–22 km, GOMOS finds much less ozone than Fortuin-Kelder. For the mesosphere and lower thermosphere, there has previously been no comprehensive nighttime ozone climatology. GOMOS is one of the first new instruments able to contribute to such a climatology. We concentrate on the characterization of the ozone distribution in this region. The monthly latitudinal and seasonal distributions of ozone profiles in this altitude region are shown. The altitude of the mesospheric ozone peak and the semiannual oscillation of the number density are determined. GOMOS is also able to determine the magnitude of the ozone minimum around 80 km. The lowest seasonal mean mixing ratio values are around 0.13 ppm. The faint tertiary ozone peak at 72 km in polar regions during wintertime is observed.
机译:欧洲航天局Envisat卫星上的全球星际掩星监测臭氧(GOMOS)仪器使用恒星掩星法测量臭氧和其他微量气体。全球覆盖,良好的垂直分辨率和自校准测量方法使GOMOS观测成为建立各种气候的有希望的数据集。在本文中,我们介绍了GOMOS在2003年测得的夜间平流层臭氧分布。我们显示了臭氧数密度和混合比分布的月度纬度分布,以及在多个纬度处的分布的季节性变化。将平流层剖面与Fortuin-Kelder白天的臭氧气候进行了比较。在极地地区发现很大的差异,可以证明它们与NO2的大量增加有关。在平流层上部,GOMOS的臭氧值系统地大于Fortuin-Kelder气候学中的臭氧值,这可以用日变化来解释。在平流层的中下部,GOMOS发现的臭氧量比Fortuin-Kelder少百分之几。在大约15-22 km的赤道区域,GOMOS发现的臭氧要比Fortuin-Kelder少得多。对于中层和较低的热层,以前没有全面的夜间臭氧气候学。 GOMOS是能够促成这种气候的首批新仪器之一。我们专注于该区域臭氧分布的特征。显示了该海拔地区臭氧剖面的月度纬度和季节分布。确定了中层臭氧峰的高度和数密度的半年振荡。 GOMOS还能够确定80公里左右的最小臭氧量。最低的季节性平均混合比值约为0.13 ppm。冬季在极地地区观察到在72 km处的第三臭氧微弱峰。

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