Lithospheric architecture beneath Hudson Bay

Hudson Bay overlies some of the thickest Precambrian lithosphere on Earth, whose internal structures contain important clues to the earliest workings of plate formation. The terminal collision, the Trans-Hudson Orogen, brought together the Western Churchill craton to the northwest and the Superior c...

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Published in:Geochemistry, Geophysics, Geosystems
Main Authors: Porritt, Robert W., Miller, Meghan, Darbyshire, Fiona A.
Format: Article in Journal/Newspaper
Language:unknown
Published: American Geophysical Union
Subjects:
Online Access:http://hdl.handle.net/1885/153131
https://doi.org/10.1002/2015GC005845
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spelling ftanucanberra:oai:openresearch-repository.anu.edu.au:1885/153131 2024-01-14T10:07:30+01:00 Lithospheric architecture beneath Hudson Bay Porritt, Robert W. Miller, Meghan Darbyshire, Fiona A. application/pdf http://hdl.handle.net/1885/153131 https://doi.org/10.1002/2015GC005845 unknown American Geophysical Union 1525-2027 http://hdl.handle.net/1885/153131 doi:10.1002/2015GC005845 Geochemistry, Geophysics, Geosystems Journal article ftanucanberra https://doi.org/10.1002/2015GC005845 2023-12-15T09:39:26Z Hudson Bay overlies some of the thickest Precambrian lithosphere on Earth, whose internal structures contain important clues to the earliest workings of plate formation. The terminal collision, the Trans-Hudson Orogen, brought together the Western Churchill craton to the northwest and the Superior craton to the southeast. These two Archean cratons along with the Paleo-Proterozoic Trans-Hudson internides, form the core of the North American craton. We use S to P converted wave imaging and absolute shear velocity information from a joint inversion of P to S receiver functions, new ambient noise derived phase velocities, and teleseismic phase velocities to investigate this region and determine both the thickness of the lithosphere and the presence of internal discontinuities. The lithosphere under central Hudson Bay approaches ∼350 km thick but is thinner (∼200-250 km) around the periphery of the Bay. Furthermore, the amplitude of the LAB conversion from the S receiver functions is unusually large for a craton, suggesting a large thermal contrast across the LAB, which we interpret as direct evidence of the thermal insulation effect of continents on the asthenosphere. Within the lithosphere, midlithospheric discontinuities, significantly shallower than the base of the lithosphere, are often imaged, suggesting the mechanisms that form these layers are common. Lacking time-history information, we infer that these discontinuities reflect reactivation of formation structures during deformation of the craton. Key Points: The thick lithosphere of Hudson Bay has significant structural variation We directly image the thermal blanketing on the asthenosphere The lithospheric thickness of Hudson Bay is 200-350 km Article in Journal/Newspaper Hudson Bay Australian National University: ANU Digital Collections Hudson Bay Hudson Geochemistry, Geophysics, Geosystems 16 7 2262 2275
institution Open Polar
collection Australian National University: ANU Digital Collections
op_collection_id ftanucanberra
language unknown
description Hudson Bay overlies some of the thickest Precambrian lithosphere on Earth, whose internal structures contain important clues to the earliest workings of plate formation. The terminal collision, the Trans-Hudson Orogen, brought together the Western Churchill craton to the northwest and the Superior craton to the southeast. These two Archean cratons along with the Paleo-Proterozoic Trans-Hudson internides, form the core of the North American craton. We use S to P converted wave imaging and absolute shear velocity information from a joint inversion of P to S receiver functions, new ambient noise derived phase velocities, and teleseismic phase velocities to investigate this region and determine both the thickness of the lithosphere and the presence of internal discontinuities. The lithosphere under central Hudson Bay approaches ∼350 km thick but is thinner (∼200-250 km) around the periphery of the Bay. Furthermore, the amplitude of the LAB conversion from the S receiver functions is unusually large for a craton, suggesting a large thermal contrast across the LAB, which we interpret as direct evidence of the thermal insulation effect of continents on the asthenosphere. Within the lithosphere, midlithospheric discontinuities, significantly shallower than the base of the lithosphere, are often imaged, suggesting the mechanisms that form these layers are common. Lacking time-history information, we infer that these discontinuities reflect reactivation of formation structures during deformation of the craton. Key Points: The thick lithosphere of Hudson Bay has significant structural variation We directly image the thermal blanketing on the asthenosphere The lithospheric thickness of Hudson Bay is 200-350 km
format Article in Journal/Newspaper
author Porritt, Robert W.
Miller, Meghan
Darbyshire, Fiona A.
spellingShingle Porritt, Robert W.
Miller, Meghan
Darbyshire, Fiona A.
Lithospheric architecture beneath Hudson Bay
author_facet Porritt, Robert W.
Miller, Meghan
Darbyshire, Fiona A.
author_sort Porritt, Robert W.
title Lithospheric architecture beneath Hudson Bay
title_short Lithospheric architecture beneath Hudson Bay
title_full Lithospheric architecture beneath Hudson Bay
title_fullStr Lithospheric architecture beneath Hudson Bay
title_full_unstemmed Lithospheric architecture beneath Hudson Bay
title_sort lithospheric architecture beneath hudson bay
publisher American Geophysical Union
url http://hdl.handle.net/1885/153131
https://doi.org/10.1002/2015GC005845
geographic Hudson Bay
Hudson
geographic_facet Hudson Bay
Hudson
genre Hudson Bay
genre_facet Hudson Bay
op_source Geochemistry, Geophysics, Geosystems
op_relation 1525-2027
http://hdl.handle.net/1885/153131
doi:10.1002/2015GC005845
op_doi https://doi.org/10.1002/2015GC005845
container_title Geochemistry, Geophysics, Geosystems
container_volume 16
container_issue 7
container_start_page 2262
op_container_end_page 2275
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