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Strontium and oxygen isotopic variations in Mesozoic and Tertiary plutons of central Idaho 总被引：2，自引：0，他引：2
Regional variations in initial 87Sr/86Sr ratios (r
i) of Mesozoic plutons in central Idaho locate the edge of Precambrian continental crust at the boundary between the late Paleozoic-Mesozoic
accreted terranes and Precambrian sialic crust in western Idaho. The r
i values increase abruptly but continuously from less than 0.704 in the accreted terranes to greater than 0.708 across a narrow,
5 to 15 km zone, characterized by elongate, lens-shaped, highly deformed plutons and schistose metasedimentary and metavolcanic
units. The chemical and petrologic character of the plutons changes concomitantly from ocean-arc-type, diorite-tonalite-trondhjemite
units to a weakly peraluminous, calcic to calcalkalic tonalite-granodiorite-granite suite (the Idaho batholith). Plutons in
both suites yield Late Cretaceous ages, but Permian through Early Cretaceous bodies are confined to the accreted terranes
and early Tertiary intrusions are restricted to areas underlain by Precambrian crust. The two major terranes were juxtaposed
between 75 and 130 m.y. ago, probably between 80 and 95 m.y.
Oxygen and strontium isotopic ratios and Rb and Sr concentrations of the plutonic rocks document a significant upper-crustal
contribution to the magmas that intrude Precambrian crust. Magmas intruding the arc terranes were derived from the upper mantle/subducted
oceanic lithosphere and may have been modified by anatexis of earlier island-arc volcanic and sedimentary units.
Plutons near the edge of Precambrian sialic crust represent simple mixtures of the Precambrian wall-rocks with melts derived
from the upper mantle or subducted oceanic lithosphere with r
i of 0.7035. Rb/Sr varies linearly with r
i, producing “pseudoisochrons” with apparent “ages” close to the age of the wall rocks. Measured δ
18O values of the wall rocks are less than those required for the assimilated end-member by Sr-O covariation in the plutons,
however, indicating that wall-rock δ
18O was reduced significantly by exchange with circulating fluids. Metasedimentary rocks of the Belt Supergroup are similarly
affected near the batholith, documenting a systematic depletion in 18O as much as 50 km from the margin of the batholith.
Plutons of the Bitterroot lobe of the Idaho batholith are remote from the accreted terranes and represent mixtures of Precambrian
wall-rocks with melts dominated by continental lower crust (r
i>0.708) rather than mantle. “Pseudoisochrons” resulting from these data are actually mixing lines that yield apparent “ages”
less than the true age of the wall rocks and meaningless “ri”. Assimilation/ fractional-crystallization models permit only insignificant amounts of crystal fractionation during anatexis
and mixing for the majority of plutons of the region. 相似文献
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Letícia Fleck Fadel Miguel Jorge Daniel Riera Ignacio Iturrioz 《国际地质力学数值与分析法杂志》2008,32(15):1857-1881
The numerical fracture analysis of non‐homogeneous rock or concrete dowels subjected to shear and compression is described in detail. The method of analysis allows the consideration of scale and rate effects due to material non‐homogeneity and fracture. The proposed approach is verified by comparing numerical predictions with experimental results reported in the literature for a series of small rock samples, since experimental evidence for large bodies is not yet available (2007). Results generated by Monte Carlo simulation using the so‐called discrete element method to model the dowels suggest that a simple three parameters law can be used to predict the relationship between tangential stress at the base and lateral distortion. It is observed that the larger the size of the cubes, the smaller both the peak tangential stress and the rupture distortion. Size effects are also evaluated in samples with vertical restraint. The influence of loading rate is likewise numerically assessed for two sample sizes. The effect is compatible with experimental evidence available for concrete using small samples. Copyright © 2008 John Wiley & Sons, Ltd. 相似文献
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Robert C. Fleck Jr. 《Astrophysics and Space Science》1991,182(1):81-84
It is shown that the development of vorticity in the wake of interstellar shocks provides a viable mechanism for the establishment of angular momentum in the interstellar medium (ISM). A plausible upper limit to the vorticity is estimated as a function of shock strength, geometry, and speed. Observations of rotating interstellar clouds and of stellar rotation in open clusters compare favourably with model predictions. 相似文献
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Robert C. Fleck Jr. 《Astrophysics and Space Science》1984,100(1-2):417-419
Two comments are prompted by the recent paper of Quiroga (1983). First, it is pointed out that Quiroga's identification of two distinct types of motion (hydrodynamic and turbulent) within the galactic disk supports the suggestion that turbulent motions in the Galaxy are generated by the shearig action of differential galactic rotation. Secondly, as a result of these turbulent motions dominating the systematic hydrodynamics of galactic rotation at scale sizes below 100–300 pc, it appears that some process(es) associated with interstellar turbulence rather than with galactic rotation should play a dominant role in the establishment of the angular momentum of interstellar material. 相似文献
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There are three major issues in modeling solar evanescent oscillations: the variation of the intensity [I]–velocity [V] phase difference of p-modes close to the base of photosphere; the existence of a plateau of negative I–V phase differences below and between the ridges of the low-frequency p-modes; the explanation of the I–V cross-spectra of the evanescent oscillations. We present new interpretations for the first two issues, based on modeling intensity fluctuations taking steep temperature gradients, opacity, and non-adiabatic cooling into account. We also discuss consequences of our model for the explanation of power spectra and cross-power spectra of p-modes. In particular, we present evidence that the acoustic sources that generate evanescent waves produce a coherent background that explains the plateau–interridge regime of negative I–V phase difference. 相似文献
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Determinations of δ18O values from 100 outcrops of Belt Supergroup (Wallace Fm.) metasedimentary rocks in the Idaho panhandle reveal a regular regional pattern that was produced by pervasive fluid infiltration and isotopic exchange. Low grade argillites at large distances (60 km) from the Idaho batholith have high δ18O values +15, compatible with their probable primary values. Pelitic rocks with anomalously low δ18O values of + 8.7 to + 12.7‰ occur in the following zones: (1) in a 5000 km2 zone of schist and gneiss peripheral to the Idaho batholith, generally coincident with high-grade (sillimanite-bearing) assemblages; (2) in high-grade metasedimentary roof pendants within the Idaho batholith; (3) peripheral to small Cretaceous stocks; and (4) within and near the scapolite-bearing zone south-west of St. Regis. On δ18O−δ18O plots, data from coexisting minerals define trends with unit slopes, indicating that the reductions in 18O occurred under high-grade metamorphic conditions. This metamorphism culminated in the emplacement of the Idaho batholith, probably as a consequence of profound crustal thickening associated with the Cretaceous accretion of the Wallowa-Seven Devils arc terranes with North America. The huge low-18O region is bounded by a “steep” δ18O gradient (0.1–0.5‰/km) that occurs in low-grade rocks along and near the Lewis and Clark Line, well below the biotite isograd. This boundary zone may be analogous to, but is not nearly as sharp as, those of meteoric-hydrothermal systems in many regions. The important ore deposits of the Coeur d'Alene district are located in this peripheral zone, suggesting that the metamorphic-hydrothermal system may have been intimately involved in their formation. In addition, the metamorphic-hydrotermal system in Idaho is larger, deeper and higher in temperature than typical meteoric-hydrothermal systems, and it involved fluids with much higher δ18O values that were probably dominantly derived from formation waters. Accordingly, this system produced rocks with δ18O values similar to those of the Idaho batholith, and mineral assemblages that approach isotopic equilibrium under high temperature conditions. 相似文献