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http://hdl.handle.net/2122/2573
DC Field | Value | Language |
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dc.contributor.authorall | Crespi, C.; DITS – Area di Geodesia e Geomatica, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.authorall | Cuffaro, M.; Dipartimento di Scienze della Terra, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.authorall | Doglioni, C.; Dipartimento di Scienze della Terra, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.authorall | Giannone, F.; DITS – Area di Geodesia e Geomatica, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.authorall | Riguzzi, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italia | en |
dc.date.accessioned | 2007-10-08T16:03:10Z | en |
dc.date.available | 2007-10-08T16:03:10Z | en |
dc.date.issued | 2006 | en |
dc.identifier.uri | http://hdl.handle.net/2122/2573 | en |
dc.description.abstract | Space geodesy data are used to verify whether plates move chaotically or rather follow a sort of tectonic mainstream. While independent lines of geological evidence support the existence of a global ordered flow of plate motions that is westerly polarized, the Terrestrial Reference Frame (TRF) presents limitations in describing absolute plate motions relative to the mantle. For these reasons we jointly estimated a new plate motions model and three different solutions of net lithospheric rotation. Considering the six major plate boundaries and variable source depths of the main Pacific hotspots, we adapted the TRF plate kinematics by global space geodesy to absolute plate motions models with respect to the mantle. All three reconstructions confirm (i) the tectonic mainstream and (ii) the net rotation of the lithosphere. We still do not know the precise trend of this tectonic flow and the velocity of the differential rotation. However, our results show that assuming faster Pacific motions, as the asthenospheric source of the hotspots would allow, the best lithospheric net rotation estimate is 13.4 ± 0.7 cm yr−1. This superfast solution seems in contradiction with present knowledge on the lithosphere decoupling, but it matches remarkably better with the geological constraints than those retrieved with slower Pacific motion and net rotation estimates. Assuming faster Pacific motion, it is shown that all plates move orderly ‘westward’ along the tectonic mainstream at different velocities and the equator of the lithospheric net rotation lies inside the corresponding tectonic mainstream latitude band (≈±7◦), defined by the 1σ confidence intervals. | en |
dc.language.iso | English | en |
dc.relation.ispartof | Geophys. J. Int. | en |
dc.subject | lithospheric | en |
dc.subject | geodesy | en |
dc.title | Space geodesy validation of the global lithospheric flow | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.subject.INGV | 04. Solid Earth::04.01. Earth Interior::04.01.99. General or miscellaneous | en |
dc.identifier.doi | 10.1111/j.1365-246X.2006.03226.x | en |
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dc.description.fulltext | reserved | en |
dc.contributor.author | Crespi, C. | en |
dc.contributor.author | Cuffaro, M. | en |
dc.contributor.author | Doglioni, C. | en |
dc.contributor.author | Giannone, F. | en |
dc.contributor.author | Riguzzi, F. | en |
dc.contributor.department | DITS – Area di Geodesia e Geomatica, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.department | Dipartimento di Scienze della Terra, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.department | Dipartimento di Scienze della Terra, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.department | DITS – Area di Geodesia e Geomatica, Universit`a di Roma ‘La Sapienza’, Roma. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | restricted | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | DITS – Area di Geodesia e Geomatica, Universit`a di Roma ‘La Sapienza’, Roma. | - |
crisitem.author.dept | Dipartimento di Scienze della Terra, Universit`a di Roma ‘La Sapienza’, Roma. | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione AC, Roma, Italia | - |
crisitem.author.dept | Niccolò Cusano University, Roma, Italy | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia | - |
crisitem.author.orcid | 0000-0002-8651-6387 | - |
crisitem.author.orcid | 0000-0003-3453-5110 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 04. Solid Earth | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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