Modeling of Atmospheric Tides with Account of Diurnal Variations of Ionospheric Conductivity
- Авторы: Shevchuk N.O.1, Ortikov M.Y.2, Pogoreltsev A.I.1,3
-
Учреждения:
- Department of Atmospheric Physics
- Mozhaisky Military Space Academy
- Meteorological Forecasts Department
- Выпуск: Том 12, № 3 (2018)
- Страницы: 576-589
- Раздел: Chemical Physics of Atmospheric Phenomena
- URL: https://journals.rcsi.science/1990-7931/article/view/200719
- DOI: https://doi.org/10.1134/S199079311803017X
- ID: 200719
Цитировать
Аннотация
A semiempirical model of ionospheric conductivity for calculating the coefficients of ionic friction and magnetic twisting is described. The influence of diurnal variations of the ionic friction and magnetic twisting in the upper atmosphere on the formation of latitudinal and altitudinal structures of various components of atmospheric tides is considered. It is shown that taking into account diurnal variations of the ionic friction and magnetic twisting leads to an additional generation of non-migrating tides in the thermosphere due to the nonlinear interaction of migrating tides with these variations.
Ключевые слова
Об авторах
N. Shevchuk
Department of Atmospheric Physics
Автор, ответственный за переписку.
Email: n.o.shevchuk@mail.ru
Россия, Petrodvorets, St. Petersburg, 198904
M. Ortikov
Mozhaisky Military Space Academy
Email: n.o.shevchuk@mail.ru
Россия, St. Petersburg, 197082
A. Pogoreltsev
Department of Atmospheric Physics; Meteorological Forecasts Department
Email: n.o.shevchuk@mail.ru
Россия, Petrodvorets, St. Petersburg, 198904; St. Petersburg, 195196
Дополнительные файлы
