The librations, tides, and interior structure of Io

The librations, tides, and interior structure of Io Tim Van Hoolst, Rose-Marie Baland, Antony Trinh, Marie Yseboodt, and Francis Nimmo For each of the 574 lines of the file Iomodels_results, corresponding to different interior structure models of Io, values of the following quantities are given: Thickness of the crust [km] Thickness of the magma ocean or asthenosphere [km] Radius of the core [km] Density of the mantle (equal to that of the crust and asthenosphere of magma ocean) [kg/m³] Density of the core [kg/m³] Polar flattening of the surface (defined as the relative difference between the mean equatorial and polar radii) Polar flattening of the outer surface of the magma ocean or asthenosphere Polar flattening of the outer surface of the mantle Polar flattening of the core Equatorial flattening of the surface (defined as the relative difference between the largest and smallest equatorial radii) Equatorial flattening of the outer surface of the magma ocean or asthenosphere Equatorial flattening of the outer surface of the mantle Equatorial flattening of the core Rigidity of the crust [GPa] Rigidity of the asthenosphere [GPa] Rigidity of the mantle [GPa] Rigidity of the core [GPa] Love number of the model with asthenosphere and liquid core Libration amplitude of the model with asthenosphere and liquid core, without deformation [m] Libration amplitude of the model with asthenosphere and liquid core, with deformation [m] Love number of the model with magma ocean Period of the out-of-phase eigenmode, without deformation [days] Period of the out-of-phase eigenmode, with deformation [days] Period of the in-phase eigenmode, without deformation [days] Period of the in-phase eigenmode, with deformation [days] Libration amplitude of the model with magma ocean, without deformation [m] Libration amplitude of the model with magma ocean, with deformation [m] Libration amplitude of the mantle below the magma ocean, without deformation [m] Libration amplitude of the mantle below the magma ocean, with deformation [m]本数据集关联研究《木卫一（Io）的天平动、潮汐与内部结构》（原标题：The librations, tides, and interior structure of Io），作者为Tim Van Hoolst、Rose-Marie Baland、Antony Trinh、Marie Yseboodt与Francis Nimmo。文件Iomodels_results中共包含574行数据，每一行对应一种不同的木卫一内部结构模型，各模型均给出以下物理量的取值： 1. 地壳厚度 [千米] 2. 岩浆洋或软流层厚度 [千米] 3. 核半径 [千米] 4. 幔密度（与地壳及岩浆洋软流层密度一致）[千克/立方米] 5. 核密度 [千克/立方米] 6. 表面极扁率（定义为平均赤道半径与极半径的相对差值） 7. 岩浆洋或软流层外表面极扁率 8. 幔外表面极扁率 9. 核极扁率 10. 表面赤道扁率（定义为最大与最小赤道半径的相对差值） 11. 岩浆洋或软流层外表面赤道扁率 12. 幔外表面赤道扁率 13. 核赤道扁率 14. 地壳刚度 [吉帕斯卡] 15. 软流层刚度 [吉帕斯卡] 16. 幔刚度 [吉帕斯卡] 17. 核刚度 [吉帕斯卡] 18. 含软流层与液态核的模型的勒夫数（Love number） 19. 含软流层与液态核的模型（无变形）的天平动振幅 [米] 20. 含软流层与液态核的模型（考虑变形）的天平动振幅 [米] 21. 含岩浆洋的模型的勒夫数（Love number） 22. 异相本征模（无变形）的周期 [日] 23. 异相本征模（考虑变形）的周期 [日] 24. 同相本征模（无变形）的周期 [日] 25. 同相本征模（考虑变形）的周期 [日] 26. 含岩浆洋的模型（无变形）的天平动振幅 [米] 27. 含岩浆洋的模型（考虑变形）的天平动振幅 [米] 28. 岩浆洋下方幔层（无变形）的天平动振幅 [米] 29. 岩浆洋下方幔层（考虑变形）的天平动振幅 [米]