Numerically modelling tidal dissipation with bottom drag in the oceans of Titan and Enceladus
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- 作者：Hamish C.F.C. Hay ; hhay@lpl.arizona.edu" class="auth_mail" title="E-mail the corresponding author ; Isamu Matsuyama
- 关键词：Satellites ; Ocean tides ; Bottom drag ; Titan ; Enceladus
- 刊名：Icarus
- 出版年：2017
- 出版时间：1 January 2017
- 年：2017
- 卷：281
- 期：Complete
- 页码：342-356
- 全文大小：3201 K
文摘
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A numerical model to simulate ocean tides on icy satellites is created.
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The model is used to explore ocean dissipation using bottom and Rayleigh drag.
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Obliquity tides can significantly dampen outward orbital migration on Titan.