Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame
The HS2-NUVEL1 model being used for current plate velocities relative to hotspots is shown to be generally inconsistent with the observed hotspot data sampled from non-Pacific regions. Instead, we determine the T22A model, which provides a good and consistent fit to the trends of globally distribute...
Published in: | Earth and Planetary Science Letters |
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Online Access: | https://hdl.handle.net/20.500.11897/155462 https://doi.org/10.1016/S0012-821X(01)00351-X |
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ftpekinguniv:oai:localhost:20.500.11897/155462 2023-05-15T13:43:50+02:00 Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame Wang, SM Wang, R Wang, SM (reprint author), Peking Univ, Dept Geophys, Beijing 100871, Peoples R China. Peking Univ, Dept Geophys, Beijing 100871, Peoples R China. 2001 https://hdl.handle.net/20.500.11897/155462 https://doi.org/10.1016/S0012-821X(01)00351-X en eng earth and planetary science letters EARTH AND PLANETARY SCIENCE LETTERS.2001,189,(3-4),133-140. 776027 0012-821X http://hdl.handle.net/20.500.11897/155462 doi:10.1016/S0012-821X(01)00351-X WOS:000169902700003 SCI hot spots plate tectonics mantle convection viscosity models SEISMIC EVIDENCE ATLANTIC HOTSPOTS CONVECTION PLUMES HAWAIIAN HOTSPOT POLAR WANDER PACIFIC SCALE ANTARCTICA KINEMATICS TECTONICS Journal 2001 ftpekinguniv https://doi.org/20.500.11897/155462 https://doi.org/10.1016/S0012-821X(01)00351-X 2021-08-01T08:02:38Z The HS2-NUVEL1 model being used for current plate velocities relative to hotspots is shown to be generally inconsistent with the observed hotspot data sampled from non-Pacific regions. Instead, we determine the T22A model, which provides a good and consistent fit to the trends of globally distributed hotspot traces, but predicts plate velocities at hotspots systematically lower than the observed rates of hotspot volcanic migrations. As a result, it implies that the return flow in the lower mantle has a velocity about 1/4 of the plate velocity, and that the lower mantle is about 20 times more viscous than the upper mantle. Although hotspots are not relatively fixed, they do define a global reference frame for plate motion and mantle convection. (C) 2001 Elsevier Science B.V. All rights reserved. Geochemistry & Geophysics SCI(E) 22 ARTICLE 3-4 133-140 189 Journal/Newspaper Antarc* Antarctica Peking University Institutional Repository (PKU IR) Pacific Earth and Planetary Science Letters 189 3-4 133 140 |
institution |
Open Polar |
collection |
Peking University Institutional Repository (PKU IR) |
op_collection_id |
ftpekinguniv |
language |
English |
topic |
hot spots plate tectonics mantle convection viscosity models SEISMIC EVIDENCE ATLANTIC HOTSPOTS CONVECTION PLUMES HAWAIIAN HOTSPOT POLAR WANDER PACIFIC SCALE ANTARCTICA KINEMATICS TECTONICS |
spellingShingle |
hot spots plate tectonics mantle convection viscosity models SEISMIC EVIDENCE ATLANTIC HOTSPOTS CONVECTION PLUMES HAWAIIAN HOTSPOT POLAR WANDER PACIFIC SCALE ANTARCTICA KINEMATICS TECTONICS Wang, SM Wang, R Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
topic_facet |
hot spots plate tectonics mantle convection viscosity models SEISMIC EVIDENCE ATLANTIC HOTSPOTS CONVECTION PLUMES HAWAIIAN HOTSPOT POLAR WANDER PACIFIC SCALE ANTARCTICA KINEMATICS TECTONICS |
description |
The HS2-NUVEL1 model being used for current plate velocities relative to hotspots is shown to be generally inconsistent with the observed hotspot data sampled from non-Pacific regions. Instead, we determine the T22A model, which provides a good and consistent fit to the trends of globally distributed hotspot traces, but predicts plate velocities at hotspots systematically lower than the observed rates of hotspot volcanic migrations. As a result, it implies that the return flow in the lower mantle has a velocity about 1/4 of the plate velocity, and that the lower mantle is about 20 times more viscous than the upper mantle. Although hotspots are not relatively fixed, they do define a global reference frame for plate motion and mantle convection. (C) 2001 Elsevier Science B.V. All rights reserved. Geochemistry & Geophysics SCI(E) 22 ARTICLE 3-4 133-140 189 |
author2 |
Wang, SM (reprint author), Peking Univ, Dept Geophys, Beijing 100871, Peoples R China. Peking Univ, Dept Geophys, Beijing 100871, Peoples R China. |
format |
Journal/Newspaper |
author |
Wang, SM Wang, R |
author_facet |
Wang, SM Wang, R |
author_sort |
Wang, SM |
title |
Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
title_short |
Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
title_full |
Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
title_fullStr |
Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
title_full_unstemmed |
Current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
title_sort |
current plate velocities relative to hotspots: implications for hotspot motion, mantle viscosity and global reference frame |
publisher |
earth and planetary science letters |
publishDate |
2001 |
url |
https://hdl.handle.net/20.500.11897/155462 https://doi.org/10.1016/S0012-821X(01)00351-X |
geographic |
Pacific |
geographic_facet |
Pacific |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
SCI |
op_relation |
EARTH AND PLANETARY SCIENCE LETTERS.2001,189,(3-4),133-140. 776027 0012-821X http://hdl.handle.net/20.500.11897/155462 doi:10.1016/S0012-821X(01)00351-X WOS:000169902700003 |
op_doi |
https://doi.org/20.500.11897/155462 https://doi.org/10.1016/S0012-821X(01)00351-X |
container_title |
Earth and Planetary Science Letters |
container_volume |
189 |
container_issue |
3-4 |
container_start_page |
133 |
op_container_end_page |
140 |
_version_ |
1766193870096302080 |