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• W2030349523 abstract "The Kronotsky Peninsula, in the forearc region of the Kamchatka magmatic arc, lies on trend with the Emperor Seamount chain situated on the currently subducting Pacific tectonic plate. Detrital modes of volcaniclastic sandstone interbedded with mafic Eocene(?) basement rocks and within the overlying sedimentary sequence provide insight into the late Cenozoic geologic history of this area. Eocene(?) and basal Miocene sandstones are primarily composed of variably altered mafic volcanic debris. Their detrital modes are similar to those of Emperor Seamount sandstones and Hawaiian beach sands. Although aspects of the stratigraphy and volcaniclastic sand composition are consistent with a seamount setting, there is no physical evidence for an accretion event, and the suggested Eocene age for this unit makes an Emperor Seamount origin unlikely. A seamount origin cannot be ruled out for older Kronotsky basement complexes, however. A Miocene lull in Kronotsky volcanism was followed by rapid basin subsidence and influx of arc-derived turbidites from the west. Detrital modes of these sandstones are typical of a moderately evolved continental or micro-continental arc. An anomalously high proportion of sedimentary lithic fragments is the only possible compositional fingerprint attributable to seamount or ridge subduction." @default.
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• W2030349523 date "1999-01-01" @default.
• W2030349523 modified "2023-09-26" @default.
• W2030349523 title "Evaluating the influence of aseismic ridge subduction and accretion(?) on detrital modes of forearc sandstone: an example from the Kronotsky Peninsula in the Kamchatka Forearc" @default.
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• W2030349523 doi "https://doi.org/10.1016/s0024-4937(98)00054-1" @default.
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