Multimodel study of the influence of atmospheric waves from a tropospheric source on the ionosphere during a geomagnetic storm on may 27–29, 2017

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Abstract

The influence of atmospheric waves generated by a tropospheric convective source on the state of the upper atmosphere and ionosphere during the recovery phase of the geomagnetic storm on May 27–28, 2017 was studied. A new approach to accounting for atmospheric waves generated by tropospheric convective sources in large-scale atmospheric models without using wave parameterization is proposed and implemented. The developed approach makes it possible to comprehensively study the effects generated by atmospheric waves against the background of various geophysical events, including geomagnetic storms. The multimodel study has shown that the proposed approach allows us to reproduce perturbations of the critical frequency ionosphere F₂ layer caused by the propagation of atmospheric waves generated by a tropospheric meteorological source. It is shown that the inclusion of a heat inflow source simulating the propagation of atmospheric waves from the lower atmosphere in the global model enhances the effects of a geomagnetic storm, which manifests itself as an additional decrease in the critical frequency of the F₂ layer, which can reach 7 % of absolute values.

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About the authors

Y. A. Kurdyaeva

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

Email: olga.borchevkina@mail.ru
Russian Federation, Kaliningrad

F. S. Bessarab

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

Email: olga.borchevkina@mail.ru
Russian Federation, Kaliningrad

O. P. Borchevkina

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

Author for correspondence.
Email: olga.borchevkina@mail.ru
Russian Federation, Kaliningrad

M. V. Klimenko

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

Email: olga.borchevkina@mail.ru
Russian Federation, Kaliningrad

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2. Fig. 1. Variations in atmospheric pressure obtained by the network of microbarographs (IFA, MSU, Zvenigorod, Mosrentgen stations) of the A.M. Obukhov Institute of Atmospheric Physics of the Russian Academy of Sciences (IFA MSU, Zvenigorod, Mosrentgen stations) during the passage of a meteorological squall in the Moscow region on May 29, 2017.

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3. Fig. 2. Frequency characteristics of wave temperature oscillations at heights of 100, 200 and 300 km at different points (horizontal coordinate – x; vertical – z) relative to the location of the disturbance source. The center of the source is determined at the lower boundary in the region of the point x = 0 km.

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4. Fig. 3. The vertical structure of temperature disturbances obtained in numerical calculations in order to identify the characteristics of waves in the thermosphere. The source center is determined at the lower boundary in the region of the point x = 0 km.

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5. Fig. 4. Values ​​of heat influx (ew) created by the propagation of atmospheric waves into the upper atmosphere.

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6. Fig. 5. Variations in geomagnetic and solar activity indices from May 26 to May 30, 2017. F₁₀₇ – in s.f.u., 1 s.f.u. = 10⁻²² W/(m² Hz).

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7. Fig. 6. Dynamics of the F₂-layer critical frequency (time–latitude) on May 26–29, 2017.

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8. Fig. 7. a – Difference in the values ​​of the zonally averaged concentration of atomic oxygen between calculation options M² and M1 at an altitude of 200 km on May 29, 2017. b – Difference in the zonally averaged values ​​of f₀F₂ between calculation options M² and M1 on May 29, 2017.

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9. Fig. 8. Latitude-temporal changes in the critical frequency of the F₂ layer on May 29, 2017 at longitudes of 25° E (a), 35° E (b), 45° E (c).

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