Impact of the meteorological storm in the Moscow region in May 2017 on variations in upper atmosphere parameters

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A numerical simulation of atmospheric wave propagation ahead of a strong pressure spike during a squall in Moscow on May 29, 2017, was performed using a three-dimensional version of the high-resolution nonlinear numerical model AtmoSym. The meteorological source was specified based on experimental observations of a network of 4 microbarographs located in the Moscow region. Wave perturbations in the upper atmosphere caused by the generation of internal gravity waves by the meteorological source were estimated.

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作者简介

Yu. Kurdyaeva

Kaliningrad Branch of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences

编辑信件的主要联系方式.
Email: yakurdyaeva@gmail.com
俄罗斯联邦, Kaliningrad

O. Borchevkina

Kaliningrad Branch of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences

Email: yakurdyaeva@gmail.com
俄罗斯联邦, Kaliningrad

E. Golikova

Obukhov Institute of Atmospheric Physics of the Russian Academy of Sciences

Email: yakurdyaeva@gmail.com
俄罗斯联邦, Moscow

I. Karpov

Kaliningrad Branch of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences

Email: yakurdyaeva@gmail.com
俄罗斯联邦, Kaliningrad

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2. Fig. 1. Atmospheric pressure variations obtained at the microbarograph network of the Obukhov Institute of Atmospheric Physics of the Russian Academy of Sciences during the passage of the meteorological front over the Moscow region on 29 May 2017

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3. Fig. 2. Wave additive distribution (cross-section by OY plane) to temperature, K, for time t = 1 h (a) and 2 h (b)

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4. Fig. 3. Frequency characteristics of wave temperature fluctuations at different heights at different points (horizontal coordinate - x; vertical coordinate - z). The source centre is defined at the lower boundary near the point x = 0 km

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5. Fig. 4. Wavelet analysis of the vertical structure of temperature perturbations obtained in numerical calculations to extract the characteristics of waves in the thermosphere. The source centre is defined at the lower boundary near the point x = 0 km

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6. Fig. 5. Heat flux created by atmospheric wave propagation into the upper atmosphere

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