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On attenuation of torsional oscillations on Marsтезисы доклада
- Авторы: Gudkova T.V., Zharkov V.N., Batov A.V.
- Сборник: Moscow Solar system symposium 8M-S3
- Тезисы
- Год издания: 2017
- Место издания: IKI RAS Moscow, Russia
- Первая страница: 260
- Последняя страница: 262
- Аннотация: At present the scientists who study Mars are looking forward to the seis- mic study of Mars. As a result of preparing for the experiment, the papers in which seismic elds in the Martian interiors due to marsquakes are modeled [1-4]. In studies [5, 6] an attempt to model the distribution of the dissipative factor of Mars Qμ(l) has been made. The periods of free oscillations of a planet are its important physical characteristics. If during the seismic experiment of mission InSight [4] an event with low enough number of oscillation is recorded, the problem of interior structure of the planet and the distribution of the dissipative factor could be signi cantly moved forward.
- Добавил в систему: Батов Алексей Владимирович