2015年3月20日和2022年10月25日日食期间莫斯科地区中间层臭氧变化的地基微波测量

Remote. Sens. Pub Date : 2023-07-07 DOI:10.3390/rs15133440
S. Rozanov, A. Ignatyev, A. Zavgorodniy
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引用次数: 0

摘要

在2015年3月20日和2022年10月25日的日食期间,利用地面微波辐射计在臭氧谱线142.175 GHz频率上观测到莫斯科地区中间层臭氧含量的增加。估算了海拔90 km和65 km处臭氧混合比(OMR)的变化,并与最接近事件的日期测量的臭氧日变化进行了比较。研究发现,2015年3月20日日食期间观测到的90公里处的OMR增加几乎是2022年10月25日日食期间的两倍,尽管这两次日食的最大太阳掩度彼此接近(0.625和0.646)。最有可能的是,这种差异可以用原子氢浓度的差异来解释,这在90公里及以上高度的臭氧破坏中起着重要作用。
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Ground-Based Microwave Measurements of Mesospheric Ozone Variations over Moscow Region during the Solar Eclipses of 20 March 2015 and 25 October 2022
An increase in the ozone content in the mesosphere over the Moscow region during the solar eclipses of 20 March 2015 and 25 October 2022 was observed by means of a ground-based microwave radiometer operated at frequencies of the ozone spectral line of 142.175 GHz. Changes in ozone mixing ratio (OMR) at altitudes of 90 km and 65 km were estimated and compared with diurnal ozone variations measured on the dates closest to the events. It was found that the observed increase in the OMR at 90 km during the 20 March 2015 eclipse was almost two times greater than during the 25 October 2022 eclipse, although the maximum Sun’s obscurations of these eclipses were close to each other (0.625 and 0.646). Most likely, this difference can be explained by the difference in concentration of atomic hydrogen, which plays an important role in ozone destruction at altitudes of around 90 km and above.
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