Geophysical Modelling of the Polar Motion / / Christian Bizouard.
Polar motion is an important geophysical process, and difficult to understand given the various parameters involved. But it is of key importance to our climate and climate change. Understanding and modeling also has implications on key technologies such as space geodesy and satellite navigation. Add...
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| Superior document: | Title is part of eBook package: De Gruyter DG Ebook Package English 2020 |
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| Place / Publishing House: | Berlin ;, Boston : : De Gruyter, , [2020] ©2020 |
| Year of Publication: | 2020 |
| Language: | English |
| Series: | De Gruyter Studies in Mathematical Physics ,
31 |
| Online Access: | |
| Physical Description: | 1 online resource (XXVI, 372 p.) |
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| 100 | 1 | |a Bizouard, Christian, |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Geophysical Modelling of the Polar Motion / |c Christian Bizouard. |
| 264 | 1 | |a Berlin ; |a Boston : |b De Gruyter, |c [2020] | |
| 264 | 4 | |c ©2020 | |
| 300 | |a 1 online resource (XXVI, 372 p.) | ||
| 336 | |a text |b txt |2 rdacontent | ||
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| 490 | 0 | |a De Gruyter Studies in Mathematical Physics , |x 2194-3532 ; |v 31 | |
| 505 | 0 | 0 | |t Frontmatter -- |t Contents -- |t Acronyms, abbreviations and common notation -- |t Forewords -- |t Introduction -- |t Part I: Astrometric estimation -- |t 1. Earth rotation and space-time reference systems -- |t 2. Geophysical irregularities of Earth’s rotation: an overview -- |t 3. Astro-geodetic observations -- |t Part II: Polar motion theory -- |t 4. Liouville equations -- |t 5. Dissipative rotational excitation function -- |t 6. Ocean pole tide -- |t 7. Influence of the fluid core -- |t Part III: Geophysical forcing -- |t 8. Hydro-atmospheric excitation -- |t 9. Equatorial angular momentum balance from two days to decadal time scale -- |t 10. Rapid, seasonal, inter-annual, and decadal excitations -- |t 11. Chandler’s wobble -- |t 12. Diurnal and sub-diurnal hydro-atmospheric effect -- |t 13. Fluid layer effect on nutation -- |t 14. Seismic effect -- |t 15. Epilogue: Geological polar motion -- |t Synthesis -- |t Appendix -- |t A. Generalized Liouville equations -- |t B. Spherical harmonic coefficients of the geopotential and moments of inertia -- |t C. Earth figure -- |t D. Tidal perturbation and Love number resonance in the diurnal band -- |t E. Matter term, pressure torque and loading effect -- |t F. Modeling the fluid core motion -- |t G. Statistics -- |t H. Usual constants -- |t Bibliography -- |t Index |
| 506 | 0 | |a restricted access |u http://purl.org/coar/access_right/c_16ec |f online access with authorization |2 star | |
| 520 | |a Polar motion is an important geophysical process, and difficult to understand given the various parameters involved. But it is of key importance to our climate and climate change. Understanding and modeling also has implications on key technologies such as space geodesy and satellite navigation. Additionally, long term polar motion has close links to decadal climate change and ice cap development. It also reflects the global circulation in the hydro-atmospheric layers and the internal properties of the Earth. Therefore the topic is of primary interest for geophysics as well as climatology. | ||
| 530 | |a Issued also in print. | ||
| 538 | |a Mode of access: Internet via World Wide Web. | ||
| 546 | |a In English. | ||
| 588 | 0 | |a Description based on online resource; title from PDF title page (publisher's Web site, viewed 28. Feb 2023) | |
| 650 | 0 | |a Climatic changes. | |
| 650 | 0 | |a Geophysics. | |
| 650 | 0 | |a Polar wandering |x Mathematical models. | |
| 650 | 4 | |a climatology. | |
| 650 | 4 | |a geophysics. | |
| 650 | 4 | |a modelling. | |
| 650 | 4 | |a polar motion. | |
| 650 | 7 | |a SCIENCE / Earth Sciences / General. |2 bisacsh | |
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