Results of microwave monitoring of middle atmosphereozone in polar latitudes for two winter seasons 2017-2018 and 2018-2019.

Y. Kulikov, A. F. Andriyanov, V. Ryskin, V. M. Demkin, V. Demin, A. Kirillov, V. A. Shishaev
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Abstract

We present data continuous series of microwave observations of the middle atmosphere in winters 2017-2018, 2018-2019 and 2019-2020. In each of these winters sudden stratospheric warming were marked.Measurements were carried out with the help of mobile ozonemeter (observation frequency 110836.04 MHz), which was established at Polar Geophysical Institute in Apatity (67N, 33E). The parameters of the device allow to measure a spectrum of the ozone emission line for time about 15 min a precision of 2%. On the measured spectra were appreciated of ozone vertical profiles in the layer of 22 60 km which were compared to satellite data MLS/Aura and with the data of ozonesonde at station Sodankyla (67N, 27E). The microwave data on the behavior of mesospheric ozone (altitude 60 km) indicate the presence of bothphotochemical and dynamic components in its changes.
2017-2018年和2018-2019年冬季极纬地区大气中层臭氧微波监测结果
本文介绍了2017-2018年、2018-2019年和2019-2020年冬季中大气微波观测数据的连续序列。在每一个冬季,平流层的突然变暖都是明显的。利用在Apatity (67N, 33E)极地地球物理研究所建立的移动臭氧计(观测频率110836.04 MHz)进行测量。该装置的参数允许在大约15分钟的时间内测量臭氧发射线的光谱,精度为2%。利用MLS/Aura卫星资料和Sodankyla (67N, 27E)臭氧探空仪资料,对22 ~ 60 km层臭氧垂直剖面的实测光谱进行了比较。60 km高空的微波资料表明,大气中臭氧的变化既有光化学成分,也有动力成分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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