Structural analysis of the superficial deformation of the 1969 Pariahuanca earthquakes (Central Peru)     

H. Philip  F. Megard 《Tectonophysics》1977,38(3-4)

An analysis of the superficial structures related to the Huaytapallana fault is presented. This fault was formed during the Pariahuanca earthquakes of July 24 and October 1, 1969. The fault trends N120E and is 3.5 km long, the displacement is 0.70 m left-lateral slip and 1.6 vertical upthrust. At most places the fault appears as a steep flexure associated with open fractures and mostly gravity folds, all of them almost parallel to it. Oblique, “en échelon” shears, often associated with small folds, are developed in the turf which is partly detached from its substratum. The analysis of these fractures is consistent with a mean N65E shortening direction. The compressional and dilatational quadrants obtained by means of this analysis fit rather well with the focal-mechanism data. On the other hand, some of the en échelon fold and fault systems provide a model of similar features with a magnitude of several kilometers.  相似文献   

Trace element model studies of Nyanzian greenstone belts,western Kenya     

Philip A. Davis  Kent C. Condie 《Geochimica et cosmochimica acta》1977,41(2):271-277

The Archean greenstone belts of the Nyanzian System in western Kenya are composed principally of andesite with minor tholeiitic basalt and siliceous volcanics. The Nyanzian tholeiite is an intermediate-K tholeiite with a flat REE pattern. There are two chemically-distinct andesites: a low-K andesite (Andesite I) and a high-K andesite (Andesite II). The REE pattern of the Andesite II is enriched in light REE and depleted in heavy REE relative to Andesite I.Major and trace element calculations indicate an origin for the Nyanzian tholeiite by 35–40% equilibrium melting of a lherzolite source followed by 10% shallow fractional crystallization. Similar calculations best explain Andesite I and Andesite II by 20 and 5% melting, respectively, of an ecologite or garnet amphibolite source of Nyanzian tholeiite composition. The rhyolite may have formed either by 20–30% partial melting of a siliceous granulite or by 20–30% fractional crystallization of a granodiorite parent magma.With respect to total exposure areas, the Nyanzian volcanics have significantly less tholeiite and more Andesite and siliceous volcanics than other Archean greenstone belts. If these abundances are representative, two models are proposed to explain the anomalous abundances of Andesite and siliceous volcanics. The first model involves an Archaen upper mantle with a relatively low geothermal gradient beneath Kenya, while the second model involves a relatively cool mantle plume. Both models inhibit ascent of a significant amount of primary tholeiite to the surface and prevent formation of secondary tholeiite. Other Archean greenstone terranes with higher mantle geotherms or hotter mantle plumes would receive higher proportions of mafic and ultramafic magmas.  相似文献   

International viewpoint and news     

Andrea Martin  Philip E. LaMoreaux 《Environmental Geology》2007,52(6):1223-1224

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PROFESSOR MICHAEL J BARNSLEY     

Adrian  Luckman 《The Geographical journal》2008,174(2):182-182

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Mass‐dependent fractionation of nickel isotopes in meteoritic metal     

David L. COOK  Meenakshi WADHWA  Robert N. CLAYTON  Nicolas DAUPHAS  Philip E. JANNEY  Andrew M. DAVIS 《Meteoritics & planetary science》2007,42(12):2067-2077

Abstract— We measured nickel isotopes via multicollector inductively coupled plasma mass spectrometry (MC‐ICPMS) in the bulk metal from 36 meteorites, including chondrites, pallasites, and irons (magmatic and non‐magmatic). The Ni isotopes in these meteorites are mass fractionated; the fractionation spans an overall range of ～0.4‰ amu^?1. The ranges of Ni isotopic compositions (relative to the SRM 986 Ni isotopic standard) in metal from iron meteorites (～0.0 to ～0.3‰ amu^?1) and chondrites (～0.0 to ～0.2‰ amu^?1) are similar, whereas the range in pallasite metal (～–0.1 to 0.0‰ amu^?1) appears distinct. The fractionation of Ni isotopes within a suite of fourteen IIIAB irons (～0.0 to ～0.3‰ amu^?1) spans the entire range measured in all magmatic irons. However, the degree of Ni isotopic fractionation in these samples does not correlate with their Ni content, suggesting that core crystallization did not fractionate Ni isotopes in a systematic way. We also measured the Ni and Fe isotopes in adjacent kamacite and taenite from the Toluca IAB iron meteorite. Nickel isotopes show clearly resolvable fractionation between these two phases; kamacite is heavier relative to taenite by ～0.4‰ amu^?1. In contrast, the Fe isotopes do not show a resolvable fractionation between kamacite and taenite. The observed isotopic compositions of kamacite and taenite can be understood in terms of kinetic fractionation due to diffusion of Ni during cooling of the Fe‐Ni alloy and the development of the Widmanstätten pattern.  相似文献   

A method for assessing local variation among scattered measurements     

G. M. Philip  D. F. Watson 《Mathematical Geology》1986,18(8):759-764

Automatic triangulation of scattered locations permits analysis of local variation in a dependent variable through calculation of a roughness index. This is approached by treating triangles of the triangulation (including the dependent variable) as vectorial structures, and accumulating at each data point the vector sum of the cluster of triangles surrounding it. The roughness index is defined as the complement of the ratio of the area of a triangle cluster to the area of component triangles as projected onto a gradient plane defined by their vector sum. The roughness index provides a measure of consistency of data values relative to surrounding observations and can be interpreted as a local index of reliability of interpolation.  相似文献   

The spin and shape of dark matter haloes in the Millennium simulation of a Λ cold dark matter universe     

Philip Bett  Vincent Eke  Carlos S. Frenk  Adrian Jenkins  John Helly  Julio Navarro 《Monthly notices of the Royal Astronomical Society》2007,376(1):215-232

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Geostatistics and spatial data analysis     

G. M. Philip  D. F. Watson 《Mathematical Geology》1986,18(5):505-509

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Cassini imaging of Saturn's rings: II. A wavelet technique for analysis of density waves and other radial structure in the rings     

Matthew S. Tiscareno  Joseph A. Burns  Philip D. Nicholson  Carolyn C. Porco 《Icarus》2007,189(1):14-34

We describe a powerful signal processing method, the continuous wavelet transform, and use it to analyze radial structure in Cassini ISS images of Saturn's rings. Wavelet analysis locally separates signal components in frequency space, causing many structures to become evident that are difficult to observe with the naked eye. Density waves, generated at resonances with saturnian satellites orbiting outside (or within) the rings, are particularly amenable to such analysis. We identify a number of previously unobserved weak waves, and demonstrate the wavelet transform's ability to isolate multiple waves superimposed on top of one another. We also present two wave-like structures that we are unable to conclusively identify. In a multi-step semi-automated process, we recover four parameters from clearly observed weak spiral density waves: the local ring surface density, the local ring viscosity, the precise resonance location (useful for pointing images, and potentially for refining saturnian astrometry), and the wave amplitude (potentially providing new constraints upon the masses of the perturbing moons). Our derived surface densities have less scatter than previous measurements that were derived from stronger non-linear waves, and suggest a gentle linear increase in surface density from the inner to the mid-A Ring. We show that ring viscosity consistently increases from the Cassini Division outward to the Encke Gap. Meaningful upper limits on ring thickness can be placed on the Cassini Division (3.0 m at r∼118,800 km, 4.5 m at r∼120,700 km) and the inner A Ring (10-15 m for r<127,000 km).  相似文献   

Climate change,climate justice and the application of probabilistic event attribution to summer heat extremes in the California Central Valley     

Roberto Mera  Neil Massey  David E. Rupp  Philip Mote  Myles Allen  Peter C. Frumhoff 《Climatic change》2015,133(3):427-438

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