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Global circulation of the Earth’s atmosphere at altitudes from 0 to 135 Km simulated with the ARM model. Consideration of the solar activity contributionстатья
Информация о цитировании статьи получена из
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Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 10 апреля 2024 г.
- Авторы: Krivolutsky A.A., Cherepanova L.A., Dement’eva A.V., Repnev A.I., Klyuchnikova A.V.
- Журнал: Geomagnetism and Aeronomy
- Том: 55
- Номер: 6
- Год издания: 2015
- Издательство: Maik Nauka/Interperiodica Publishing
- Местоположение издательства: Russian Federation
- Первая страница: 780
- Последняя страница: 800
- DOI: 10.1134/s0016793215060067
- Аннотация: The results of simulations of the global circulation and temperature regime in the altitude range from the lower tropospheric layers to 135 km are presented. They were obtained with the Atmospheric Research Model (ARM), an advanced modification of a version of the Cologne Middle Atmosphere Model (COMMA). The ARM is characterized by higher spatial resolution and better parameterizations of the radiation sources and heat sinks. At the lower boundary of the model, wavy sources of perturbations, which are caused by internal gravity waves and planetary waves, are specified. The results of the modeling of the global temperature and wind fields for the mean solar activity level are presented, and their changes, which are caused by variations of the UV-radiation fluxes in the solar activity cycle and by solar proton flares, are also considered.
- Добавил в систему: Криволуцкий Алексей Александрович