2009
DOI: 10.1029/2008gc002350
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Origin of volcanism on the flanks of the Pacific‐Antarctic ridge between 41°30′S and 52°S

Abstract: [1] Non-hot spot, intraplate volcanism is a common feature near the East Pacific Rise or Pacific-Antarctic ridge. Volcanic ridges and seamount chains, tens to hundreds of kilometers long, are asymmetrically distributed about the ridge axis, with most volcanic features occurring on the Pacific plate. Their origins remain controversial. We have analyzed off-axis volcanic ridges near the Pacific-Antarctic ridge from bathymetry, backscatter, gravity, and geochemistry data of the Pacantarctic 2 cruise. K/Ar dating … Show more

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Cited by 13 publications
(14 citation statements)
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“…East of the AAD, a variety of observations suggests the presence of an area probably as anomalous as the AAD itself. The shallow residual basement depth [e.g., Marks et al ., ; Whittaker et al ., ], off‐axis volcanism, and the presence of westward propagators [ Phipps Morgan and Sandwell , ; Sempéré et al ., ; Briais et al ., ] suggest that the magma production under the South Tasmania SEIR section is not only larger than the cold AAD area, but also abnormally high compared to other sections of intermediate‐spreading MORs such as the Juan de Fuca Ridge [ Briais et al ., ].…”
Section: Introductionmentioning
confidence: 99%
“…East of the AAD, a variety of observations suggests the presence of an area probably as anomalous as the AAD itself. The shallow residual basement depth [e.g., Marks et al ., ; Whittaker et al ., ], off‐axis volcanism, and the presence of westward propagators [ Phipps Morgan and Sandwell , ; Sempéré et al ., ; Briais et al ., ] suggest that the magma production under the South Tasmania SEIR section is not only larger than the cold AAD area, but also abnormally high compared to other sections of intermediate‐spreading MORs such as the Juan de Fuca Ridge [ Briais et al ., ].…”
Section: Introductionmentioning
confidence: 99%
“…The number of seamounts > 1.5 km in height currently on the ocean floor is estimated to be more than 13 000 based on satellite altimetry (Wessel et al, 2010), and these numerous features often alter subduction zone by blocking the subducting interface or causing uplift in the accretionary prism . Seamounts can be formed by various processes: they can be the result of upper mantle mini-convection cells under mid-ocean ridges or transforms (Buck and Parmentier, 1986), deep mantle upwellings, short-lived hotspot volcanism, upper asthenospheric upwelling, and lithospheric cracking (Forsyth et al, 2006;Briais et al, 2009;Sandwell and Fialko, 2004). The geochemical signature of mafic accreted terranes is important in helping to determine if the accreted terrane was originally a plume-derived oceanic plateau, hot spot track submarine ridge, or the product of excess upper mantle magmatism.…”
Section: Oceanic Plateaus Submarine Ridges and Seamounts: General Smentioning
confidence: 99%
“…Major, trace element and Sr‐Nd‐Hf isotope data reveal tight and coherent geochemical variations along segments (Figure 2). Along axis geochemistry can be disturbed by local phenomena like the presence of nearby seamounts as seen in S2 and N2 (Figure 1) [ Briais et al , 2009]. These segments are the shortest and the less robust of the studied area.…”
Section: Analytical Techniques and Resultsmentioning
confidence: 99%