A Numerical–Analytical Approach to Modeling the Axial Rotation of the Earth
- Авторы: Markov Y.G.1, Perepelkin V.V.1, Rykhlova L.V.2, Filippova A.S.1
-
Учреждения:
- Moscow Institute of Aviation
- Institute of Astronomy
- Выпуск: Том 62, № 4 (2018)
- Страницы: 299-308
- Раздел: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/191582
- DOI: https://doi.org/10.1134/S1063772918040042
- ID: 191582
Цитировать
Аннотация
A model for the non-uniform axial rotation of the Earth is studied using a celestial-mechanical approach and numerical simulations. The application of an approximate model containing a small number of parameters to predict variations of the axial rotation velocity of the Earth over short time intervals is justified. This approximate model is obtained by averaging variable parameters that are subject to small variations due to non-stationarity of the perturbing factors. The model is verified and compared with predictions over a long time interval published by the International Earth Rotation and Reference Systems Service (IERS).
Об авторах
Yu. Markov
Moscow Institute of Aviation
Email: vadimkin1@yandex.ru
Россия, Volokolamskoe sh. 4, Moscow, 125080
V. Perepelkin
Moscow Institute of Aviation
Автор, ответственный за переписку.
Email: vadimkin1@yandex.ru
Россия, Volokolamskoe sh. 4, Moscow, 125080
L. Rykhlova
Institute of Astronomy
Email: vadimkin1@yandex.ru
Россия, ul. Pyatnitskaya 48, Moscow, 109017
A. Filippova
Moscow Institute of Aviation
Email: vadimkin1@yandex.ru
Россия, Volokolamskoe sh. 4, Moscow, 125080
Дополнительные файлы
