The Role of Magmatism at Rifted Margins
Rifted margins form by the thinning and stretching of continental lithosphere until it ruptures, forming new oceanic crust and lithosphere, which can be accompanied by decompression melting and the addition of magmatic material. Despite numerous studies on magma-rich margins, we still do not fully u...
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ftunivliverpool:oai:livrepository.liverpool.ac.uk:3052622 2023-05-15T16:28:42+02:00 The Role of Magmatism at Rifted Margins Harkin, Caroline Kusznir, Nick 2019-03-29 text http://livrepository.liverpool.ac.uk/3052622/ http://livrepository.liverpool.ac.uk/3052622/1/200866281_Mar2019.pdf en eng http://livrepository.liverpool.ac.uk/3052622/1/200866281_Mar2019.pdf Harkin, Caroline (2019) The Role of Magmatism at Rifted Margins. PhD thesis, University of Liverpool. Thesis NonPeerReviewed 2019 ftunivliverpool 2023-01-19T23:44:54Z Rifted margins form by the thinning and stretching of continental lithosphere until it ruptures, forming new oceanic crust and lithosphere, which can be accompanied by decompression melting and the addition of magmatic material. Despite numerous studies on magma-rich margins, we still do not fully understand how and when magmatic features form at rifted margins. To address this I investigate the formation of various magmatic features on three rifted margins, the East Indian margin, the Pelotas margin and the Southeast (SE) Greenland margin, using a range of quantitative techniques. The East Indian margin is an often-cited example of a magma-poor margin; however, some interpretations suggest the transition from exhumed mantle to oceanic crust consists of 9 km thick magmatic crust. Gravity inversion, RDA analysis, subsidence analysis and joint inversion of seismic and gravity data alongside seismic observations, reveal the presence of magma-poor and magma-rich characteristics in the form of exhumed mantle and 9 km thick magmatic crust juxtaposed against each other, resulting from a two-stage breakup. Juxtaposition of end-member characteristics suggests that the use of end-member terminology based on volumes of magma alone is misleading. The Pelotas margin in the South Atlantic shows an extraordinarily thick sequence of seaward dipping reflectors (SDRs), of which the composition and formation is poorly understood. I investigate these SDRs using gravity inversion with a sensitivity to basalt/sediment composition, flexural backstripping and reverse thermal subsidence modelling, joint inversion of seismic and gravity data and seismic observations. I show there are two types of SDRs present on the Pelotas margin, an inner subaerial set of SDRs formed of basalt during pre-breakup intra-continental rifting and an outer set of SDRs formed of a mix of volcaniclastics and basalts during breakup in a subaqueous environment at an embryonic mid-ocean ridge. The SE Greenland margin in the North Atlantic has a broad region of ... Thesis Greenland North Atlantic The University of Liverpool Repository Greenland Indian |
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The University of Liverpool Repository |
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ftunivliverpool |
language |
English |
description |
Rifted margins form by the thinning and stretching of continental lithosphere until it ruptures, forming new oceanic crust and lithosphere, which can be accompanied by decompression melting and the addition of magmatic material. Despite numerous studies on magma-rich margins, we still do not fully understand how and when magmatic features form at rifted margins. To address this I investigate the formation of various magmatic features on three rifted margins, the East Indian margin, the Pelotas margin and the Southeast (SE) Greenland margin, using a range of quantitative techniques. The East Indian margin is an often-cited example of a magma-poor margin; however, some interpretations suggest the transition from exhumed mantle to oceanic crust consists of 9 km thick magmatic crust. Gravity inversion, RDA analysis, subsidence analysis and joint inversion of seismic and gravity data alongside seismic observations, reveal the presence of magma-poor and magma-rich characteristics in the form of exhumed mantle and 9 km thick magmatic crust juxtaposed against each other, resulting from a two-stage breakup. Juxtaposition of end-member characteristics suggests that the use of end-member terminology based on volumes of magma alone is misleading. The Pelotas margin in the South Atlantic shows an extraordinarily thick sequence of seaward dipping reflectors (SDRs), of which the composition and formation is poorly understood. I investigate these SDRs using gravity inversion with a sensitivity to basalt/sediment composition, flexural backstripping and reverse thermal subsidence modelling, joint inversion of seismic and gravity data and seismic observations. I show there are two types of SDRs present on the Pelotas margin, an inner subaerial set of SDRs formed of basalt during pre-breakup intra-continental rifting and an outer set of SDRs formed of a mix of volcaniclastics and basalts during breakup in a subaqueous environment at an embryonic mid-ocean ridge. The SE Greenland margin in the North Atlantic has a broad region of ... |
author2 |
Kusznir, Nick |
format |
Thesis |
author |
Harkin, Caroline |
spellingShingle |
Harkin, Caroline The Role of Magmatism at Rifted Margins |
author_facet |
Harkin, Caroline |
author_sort |
Harkin, Caroline |
title |
The Role of Magmatism at Rifted Margins |
title_short |
The Role of Magmatism at Rifted Margins |
title_full |
The Role of Magmatism at Rifted Margins |
title_fullStr |
The Role of Magmatism at Rifted Margins |
title_full_unstemmed |
The Role of Magmatism at Rifted Margins |
title_sort |
role of magmatism at rifted margins |
publishDate |
2019 |
url |
http://livrepository.liverpool.ac.uk/3052622/ http://livrepository.liverpool.ac.uk/3052622/1/200866281_Mar2019.pdf |
geographic |
Greenland Indian |
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Greenland Indian |
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Greenland North Atlantic |
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Greenland North Atlantic |
op_relation |
http://livrepository.liverpool.ac.uk/3052622/1/200866281_Mar2019.pdf Harkin, Caroline (2019) The Role of Magmatism at Rifted Margins. PhD thesis, University of Liverpool. |
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1766018382649360384 |