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  • 2010-2014  (56)
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  • 1
    Publication Date: 2022-05-25
    Description: Author Posting. © The Authors, 2010. This article is posted here by permission of John Wiley & Sons for personal use, not for redistribution. The definitive version was published in Geophysical Journal International 182 (2010): 203-232, doi:10.1111/j.1365-246X.2010.04619.x.
    Description: The current M-anomaly geomagnetic polarity timescale (GPTS) is mainly based on the Hawaiian magnetic lineations in the Pacific Ocean. M-anomaly GPTS studies to date have relied on a small number of magnetic profiles, a situation that is not ideal because any one profile contains an uncertain amount of geologic 'noise' that perturbs the magnetic field signal. Compiling a polarity sequence from a larger array of magnetic profiles is desirable to provide greater consistency and repeatability. We present a new compilation of the M-anomaly GPTS constructed from polarity models derived from magnetic profiles crossing the three lineation sets (Hawaiian, Japanese and Phoenix) in the western Pacific. Polarity reversal boundary locations were estimated with a combination of inverse and forward modelling of the magnetic profiles. Separate GPTS were established for each of the three Pacific lineation sets, to allow examination of variability among the different lineation sets, and these were also combined to give a composite timescale. Owing to a paucity of reliable direct dates of the M-anomalies on ocean crust, the composite model was time calibrated with only two ages; one at each end of the sequence. These two dates are 125.0 Ma for the base of M0r and 155.7 Ma for the base of M26r. Relative polarity block widths from the three lineation sets are similar, indicating a consistent Pacific-wide spreading regime. The new GPTS model shows slightly different spacings of polarity blocks, as compared with previous GPTS, with less variation in block width. It appears that the greater polarity chron irregularity in older models is mostly an artifact of modelling a small number of magnetic profiles. The greater averaging of polarity chron boundaries in our model gives a GPTS that is statistically more robust than prior GPTS models and a superior foundation for Late Jurassic–Early Cretaceous geomagnetic and chronologic studies.
    Description: This work was supported by the Jane & R. Ken Williams'45 Chair of Ocean Drilling Science and Technology.
    Keywords: Magnetic anomalies: modelling and interpretation ; Reversals: process, time scale, magnetostratigraphy ; Marine magnetics and palaeomagnetics
    Repository Name: Woods Hole Open Access Server
    Type: Article
    Format: application/pdf
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  • 2
    Publication Date: 2022-05-25
    Description: Author Posting. © American Geophysical Union, 2008. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 113 (2008): B07110, doi:10.1029/2007JB005527.
    Description: The Jurassic Quiet Zone (JQZ) is a region of low-amplitude magnetic anomalies whose distinctive character may be related to geomagnetic field behavior. We collected deep-tow magnetic profiles in Pigafetta Basin (western Pacific) where previous deep-tow data partially covered the JQZ sequence. Our goals were to extend the survey through the JQZ, examine anomaly correlations, and refine a preliminary geomagnetic polarity timescale (GPTS) model. We collected a series of closely spaced profiles over anomaly M34 and Ocean Drilling Program Hole 801C to examine anomaly correlation in detail, one profile in between previous profiles, and two long profiles extending the survey deeper into the JQZ. Anomaly features can be readily correlated except in a region of low-amplitude, short-wavelength anomalies in the middle of the survey area (“low-amplitude zone” or LAZ). The small multiprofile surveys demonstrate anomaly linearity, implying that surrounding anomalies are also linear and likely result from crustal recording of geomagnetic field changes. We constructed a GPTS model assuming that most anomalies result from polarity reversals. The polarity timescale is similar to the polarity sequences from previous studies, but its global significance is uncertain because of problems correlating anomalies in the LAZ and the ambiguous nature of the small JQZ anomalies. Overall anomaly amplitude decreases with age into the LAZ and then increases again, implying low geomagnetic field strength, perhaps related to a rapidly reversing field. Other factors that may contribute to the LAZ are interference of anomalies over narrow, crustal polarity zones and poorly understood local tectonic complexities.
    Description: This research was supported by the National Science Foundation grants OCE-0099161 and OCE-0099237. Tominaga was partly supported by funds from the Jane and R. Ken Williams ’45 Chair in Ocean Drilling Science, Education, and Technology.
    Keywords: Magnetic anomalies ; Pacific Jurassic Quiet Zone ; Geomagnetic polarity ; Timescales
    Repository Name: Woods Hole Open Access Server
    Type: Article
    Format: application/postscript
    Format: application/pdf
    Format: text/plain
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  • 3
    Publication Date: 2022-05-26
    Description: Author Posting. © American Geophysical Union, 2010. 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 37 (2010): L01304, doi:10.1029/2009GL040984.
    Description: Late Jurassic-Early Cretaceous marine magnetic anomalies observed in the North Atlantic exhibit an abrupt change in character in M5-M15 crust. The anomalies are smoother with low amplitudes, and are difficult to correlate among nearby profiles. The accepted explanation for the origin of this smooth zone is diminished resolution and anomaly interference due to slow spreading rates, which narrows the widths of polarity reversals in the crust and causes interference among sea-surface anomalies. Magnetic modeling of these anomalies indicates that neither slow spreading rates alone nor slow spreading rates in combination with a decrease in geomagnetic field intensity can explain the basic character of the smooth zone. Combined with other geophysical evidence, our study suggests that one consequence of slow spreading rates that is responsible for the magnetic “smooth zone” is a thinned crustal basalt layer or a non-basaltic magnetic source layer resulting from low melt supply during a period of ultra-slow spreading.
    Description: This work was supported by the Jane & R. Ken Williams '45 Chair of Ocean Drilling Science and Technology.
    Keywords: Mid-oceanic ridge processes ; Marine magnetics and paleomagnetics ; Ocean core complex
    Repository Name: Woods Hole Open Access Server
    Type: Article
    Format: application/pdf
    Format: image/jpeg
    Format: text/plain
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  • 4
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    AGU (American Geophysical Union)
    In:  Eos, Transactions American Geophysical Union, 92 (5). pp. 37-38.
    Publication Date: 2017-02-10
    Description: Oceanic plateaus are huge basaltic constructions whose eruptions may briefly outstrip even global mid-ocean ridge magma production. Although they form great undersea mountains, their origins are poorly understood. A widely accepted explanation is that oceanic plateaus are built by massive eruptions from the head of nascent thermal mantle plumes that rise from deep in the mantle to the surface [e.g., Duncan and Richards, 1991]. An alternative is that plateaus erupt by decompression melting of fusible patches in the upper mantle at plate edges or zones of extension [Foulger, 2007].
    Type: Article , NonPeerReviewed
    Format: text
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  • 5
    Publication Date: 2013-04-08
    Description: Integrated Ocean Drilling Program (IODP) Expedition 324 cored Shatsky Rise at five sites (U1346–U1350) to study processes of oceanic plateau formation and evolution. Site penetrations ranged from 191.8 m to 324.1 m with coring of 52.6 m to 172.7 m into igneous basement at four of the sites. Average recovery in basement was 38.7%–67.4%. Cored igneous sections consist mainly of variably evolved tholeiitic basalts emplaced as pillows or massive flows. Massive flows are thickest and make up the largest percentage of section on the largest and oldest volcano, late Jurassic age Tamu Massif; thus, it may have formed at high effusion rates. Such massive flows are characteristic of flood basalts, and similar flows were cored at Ontong Java Plateau. Indeed, the similarity of igneous sections at Site U1347 with that cored on Ontong Java Plateau implies similar volcanic styles for these two plateaus. On younger, smaller Shatsky Rise volcanoes, pillow flows are common and massive flows thinner and fewer, which might mean volcanism waned with time. Cored sediments from summit sites contain fossils and structures implying shallow water depths or emergence at the time of eruption and normal subsidence since. Summit sites also show pervasive alteration that could be due to high fluid fluxes. A thick section of volcaniclastics cored on Tamu Massif suggests that shallow, explosive submarine volcanism played a significant role in the geologic development of the plateau summit. Expedition 324 results imply that Shatsky Rise began with massive eruptions forming a huge volcano and that subsequent eruptions waned in intensity, forming volcanoes that are large, but which did not erupt with unusually high effusion rates. Similarities of cored sections on Tamu Massif with those of Ontong Java Plateau indicate that these oceanic plateaus formed in similar fashion.
    Type: Article , NonPeerReviewed
    Format: text
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  • 6
    Publication Date: 2023-06-27
    Keywords: 324-U1346A; Curated Length; Date/time end; Depth, bottom/max; DRILL; Drilled; Drilling/drill rig; DSDP/ODP/IODP sample designation; Exp324; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution; Number; Record length; Recovery; Sample code/label; Section Top in meters below surface; Shatsky Rise
    Type: Dataset
    Format: text/tab-separated-values, 176 data points
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  • 7
    Publication Date: 2023-06-27
    Keywords: 324-U1346A; Calcium; Calcium carbonate; Calculated; Carbon, inorganic, total; Carbon, organic, total; Carbon, total; Coulometry; Depth, bottom/max; DEPTH, sediment/rock; Depth, top/min; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Element analyser CHNS; Exp324; Hydrogen; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution; Sample code/label; Shatsky Rise; Sulfur, total
    Type: Dataset
    Format: text/tab-separated-values, 69 data points
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  • 8
    Publication Date: 2023-06-27
    Keywords: 324-U1346A; Density; DEPTH, sediment/rock; Depth, top/min; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Exp324; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution; Multi-Sensor Core Logger; Sample code/label; Shatsky Rise; Time Stamp
    Type: Dataset
    Format: text/tab-separated-values, 3508 data points
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  • 9
    Publication Date: 2023-06-27
    Keywords: 324-U1346A; DEPTH, sediment/rock; Depth, top/min; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Exp324; Instrument; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution; Sample code/label; Shatsky Rise; Susceptibility; Time Stamp
    Type: Dataset
    Format: text/tab-separated-values, 17040 data points
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  • 10
    Publication Date: 2023-06-27
    Keywords: 324-U1346A; DEPTH, sediment/rock; Depth, top/min; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Error, absolute; Error, relative; Exp324; Integrated Ocean Drilling Program / International Ocean Discovery Program; IODP; Joides Resolution; Natural gamma ray; Sample code/label; Shatsky Rise; Time Stamp
    Type: Dataset
    Format: text/tab-separated-values, 2100 data points
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