“Equator Crossing” of Shatsky Rise?: New insights on Shatsky Rise tectonic motion from the downhole magnetic architecture of the uppermost lava sequences at Tamu Massif

dc.contributor.author Tominaga, Masako
dc.contributor.author Evans, Helen F.
dc.contributor.author Iturrino, Gerardo
dc.date.accessioned 2012-12-06T18:36:03Z
dc.date.available 2014-10-22T08:57:23Z
dc.date.issued 2012-11-03
dc.description Author Posting. © American Geophysical Union, 2012. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geophysical Research Letters 39 (2012): L21301, doi:10.1029/2012GL052967. en_US
dc.description.abstract Shatsky Rise is a Large Igneous Province (LIP) currently located in the northwestern Pacific. New downhole magnetic logging data from Integrated Ocean Drilling Program (IODP) Hole U1347A at Tamu Massif of Shatsky Rise captured the magnetic architecture in the uppermost lava sequence, providing a rare opportunity to investigate a time series of the intra-plate volcanism in conjunction with the Pacific plate construction history centered at the triple junction. Logging data results indicate that Tamu Massif was formed during normal polarity periods south of the paleoequator and crossed the equator at some point in the M19–M17 period. Combining these new observations with previous interpretations of the massif's tectonic history, a time series of the latitudinal tectonic motion of a LIP and the underlying Pacific plate during the plateau formation is postulated. en_US
dc.description.embargo 2013-05-03 en_US
dc.description.sponsorship This project was supported by the IODP-US Science Support Program (Consortium for Ocean Leadership) Expedition 324 Post Expedition Award. en_US
dc.format.mimetype image/jpeg
dc.format.mimetype application/pdf
dc.format.mimetype text/plain
dc.identifier.citation Geophysical Research Letters 39 (2012): L21301 en_US
dc.identifier.doi 10.1029/2012GL052967
dc.identifier.uri https://hdl.handle.net/1912/5595
dc.language.iso en_US en_US
dc.publisher American Geophysical Union en_US
dc.relation.uri https://doi.org/10.1029/2012GL052967
dc.subject Integrated Ocean Drilling Program en_US
dc.subject Downhole logging en_US
dc.subject Large igneous province en_US
dc.subject Magnetic architecture en_US
dc.title “Equator Crossing” of Shatsky Rise?: New insights on Shatsky Rise tectonic motion from the downhole magnetic architecture of the uppermost lava sequences at Tamu Massif en_US
dc.type Article en_US
dspace.entity.type Publication
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relation.isAuthorOfPublication 1aa224fa-4699-43c2-b604-095bc2d53671
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relation.isAuthorOfPublication.latestForDiscovery bdca27d3-bce4-4d77-9fa9-54a5b8b9c6fd
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Figure S1: Diagrams showing how we can uniquely determine the polarity and hemisphere origins of magnetized layer from GPIT signals in a borehole.
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Figure S2: Caliper data that exhibit the borehole condition and IGRF-corrected GPIT data.
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Table S1: FMS downhole structural orientations.
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