“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
“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 | |
relation.isAuthorOfPublication | bdca27d3-bce4-4d77-9fa9-54a5b8b9c6fd | |
relation.isAuthorOfPublication | 1aa224fa-4699-43c2-b604-095bc2d53671 | |
relation.isAuthorOfPublication | 71e9d856-667a-4da3-867b-0048dc2c719d | |
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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