COMPARISON OF WAVE ACTIVITY IN THE MESOPAUSE REGION AT MAIMAGA STATION WITH EOS MLS (AURA) TEMPERATURE DATA AND ACTIVITY OF PLANETARY WAVES AT TIKSI STATION

• Published in: Вестник КРАУНЦ. Физико-математические науки
• Main Authors: V. I. Sivtseva, P.P. Ammosov, G. A. Gavrilyeva, I. I. Koltovskoi, A. M. Ammosova
• Format: Article in Journal/Newspaper
• Language: English; Russian
• Published: KamGU by Vitus Bering 2019
• Subjects: internal gravity waves; planetary waves; mesopause; stratopause; hydroxyl; Science; Q; Tiksi
• Online Access: https://doi.org/10.26117/2079-6641-2019-29-4-182-189; https://doaj.org/article/1c4b49990302448bb3aace77aedb159f

The temperature data of the mesopause region obtained for the period 2013-2018 at the station Maimaga (63.04° N, 129.51° E) and for the period 2015-2018 at the station Tiksi (71.58° N, 128.77° E) was investigated. During the winter period of the 2014–2015 observation season, the characteristic of the internal gravity waves (IGW) activity sgw has lower values than in other seasons, and the average night temperature of the mesopause region, on the contrary, exceeds corresponding values in other seasons. For comparison, satellite data of temperature profiles obtained by EOS MLS (Aura) are given. After isolating and subtracting the contribution of the gravitaty waves from the EOS MLS temperature profiles for the region above the st. Maimaga, the difference in the winter stratopause of the 2014-2015 season is noticeable. In this season in winter there is a lack of sharp warming in the stratopause region, in contrast to other seasons, taking into account the deduction of the contribution of temperature fluctuations due to IGW. Measurement of the parameters of planetary waves during the period 2015-2018 of joint observations at Maimaga and Tiksi stations showed that the phases of the waves observed at both stations coincide, and the amplitudes at Tiksi station are several (1-2 K) higher than the amplitudes at Maimaga station.