JpGU-AGU Joint Meeting 2020

講演情報

[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM12] 大気圏ー電離圏結合

コンビーナ:Huixin Liu(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-05] Studying atmospheric and ionospheric variabilities in the mesopause and ionospheric F2-region during winter sudden stratospheric warmings of various types

*Irina Medvedeva1,2Konstantin Ratovsky1Alla Suvorova3 (1.Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia 、2.Obukhov Institute of Atmospheric Physics RAS, Moscow, Russia 、3.GPSARC National Central University, Taoyuan, Taiwan)

キーワード:atmosphere, ionosphere, temperature, peak electron density , mesopause, sudden stratospheric warming

We present the results of studying the activity of atmospheric waves at the heights of the mesopause (80-100 km) and ionospheric F2-region during the periods of winter sudden stratospheric warmings (SSW) of various types. The analysis is based on the experimental data on the rotational temperature of the hydroxyl molecule (OH band (6-2) 834.0 nm) obtained from spectrometric measurements at the Geophysical Observatory of the ISTP SB RAS (51.8° N, 103.1° E, Tory), and on the peak electron density NmF2, from the Irkutsk ionosonde DPS-4 (52.3° N, 104.3° E) data. The rotational temperature of the hydroxyl molecule corresponds to the temperature of the atmosphere at the mesopause heights. In this study, we used the method for estimating the atmospheric and ionospheric variabilities described in (Medvedeva and Ratovsky, 2015), which allows one to analyze the manifestation of wave activity in a wide range of altitudes of the upper atmosphere. As a characteristic of atmospheric variability, we used standard deviations of the mesopause temperature in the annual and nightly variations, by which one can analyze the manifestation of the various timescale wave process activity in the upper atmosphere (Perminov et al., 2014, Medvedeva and Ratovsky, 2015). As a characteristic of ionospheric variability, we used the variability of the F2 peak electron density (NmF2). The values of atmospheric and ionospheric variability obtained using this technique during the SSWs, are compared with seasonally average values. We revealed significant differences in the manifestation of wave activity at the heights of the mesopause and ionospheric F2-region during the SSWs of various types. Thus, the major SSW in February 2018 led to an increase in the day-to-day atmospheric and ionospheric variability, which can be caused by the intensification of planetary wave activity in the upper atmosphere. The largest effects of the major January 2019 SSW in the upper atmosphere were observed in the behavior of diurnal atmospheric variability due to the effects of tides and internal gravity waves.



Acknowledgments

The reported study was funded by RFBR, Russian-Taiwanese joint research project number 18-55-52006 MHT_a. Experimental data recorded by the equipment of Center for Common Use «Angara» (http://ckp-rf.ru/ckp/3056/) obtained with budgetary funding of Basic Research program II.16 were used.



References

Medvedeva, I., and K. Ratovsky (2015), Studying atmospheric and ionospheric variabilities from long-term spectrometric and radio sounding measurements, J. Geophys. Res. Space Physics, 120, Issue 6, J. Geophys. Res. Space Physics, 120, 5151–5159, doi:10.1002/2015JA021289.

Perminov V.I., Semenov A.I., Medvedeva I.V., Zheleznov Yu.A., (2014), Variability of mesopause temperature from the hydroxyl airglow observations over midlatitudinal sites, Zvenigorod and Tory, Russia, Adv. Space Res., .54, 2511–2517.