Petrogenesis of the gabbros from Mt. St. Hilaire,Quebec, Canada     

R. C. Greenwood  A. D. Edgar 《Geological Journal》1984,19(4):353-376

Mt. St. Hilaire occurs as a small funnel-shaped intrusion in the Monteregian petrographic province of Quebec and consists of alkali gabbros and later nepheline syenites. Based on field relations, petrography, and geochemistry, five types of gabbro are recognized. In order of intrusion these are: leucogabbro, foliated gabbro, kaersutite-biotite gabbro, kaersutite gabbro, and a gabbro-melagabbro series. Based on analyses of the early-forming ilmenite-titanomagnetite, the gabbros crystallized under high fO₂ conditions which lead to subsequent crystallization of olivines with high MnO contents. Fractionation of ilmenite and titanomagnetite was a major control on the Ti and A[TV]concentrations in the clinopyroxenes. Plagioclase compositions in the gabbros became richer in Ab contents in the sequence gabbro-melagabbro to leucogabbro. Whole-rock analyses suggest that the parental magma of alkali basaltic composition was fairly evolved prior to emplacement. Lack of olivine in the cumulate gabbro-melagabbros and low Ni and Cr in all gabbros may reflect either extreme olivine fractionation and/or a very low olivine content in the source material for these basalts. Differentiation of the gabbros occurred both pre- and post-emplacement, probably by a process of crystal-liquid fractionation at depths between 3-5 and 8 km. This is in accordance with geophysical measurements for other Monteregian intrusions. A model is presented for the mechanism of emplacement.  相似文献   

Identifying Nonstationarity in Turbulence Series   总被引：1，自引：1，他引：0  

Edgar L Andreas  Cathleen A. Geiger  George Treviño  Kerry J. Claffey 《Boundary-Layer Meteorology》2008,127(1):37-56

Because of rapid forcing by varying cloud and sky conditions, turbulence time series collected in the atmospheric surface layer over land may often be nonstationary. The meteorological community, however, has no consensus definition of what nonstationarity is and, thus, no consensus method for how to identify it. This study, therefore, adopts definitions for first-order and second-order stationarity taken from the time series analysis literature and implements new analysis techniques and probabilistic tests to quantify first-order and second-order nonstationarity. First-order nonstationarity manifests as a change in the series mean; second-order nonstationarity, as a change in the variance. The analysis identifies nonstationarity in surface-level turbulent temperature and water vapour series collected during two sample days with solar forcing influenced by cirrus and cirrostratus clouds, but that nonstationarity is not as severe as expected despite the rapid thermal forcing by these clouds. On the other hand, even with negligible cloud forcing, both sample days exhibited severe nonstationarity at night.  相似文献   

Affluence drives the global displacement of land use   总被引：2，自引：0，他引：2  

Jan Weinzettel  Edgar G. Hertwich  Glen P. Peters  Kjartan Steen-Olsen  Alessandro Galli 《Global Environmental Change》2013,23(2):433-438

Increasing affluence is often postulated as a main driver for the human footprint on biologically productive areas, identified among the main causes of biodiversity loss, but causal relationships are obscured by international trade. Here, we trace the use of land and ocean area through international supply chains to final consumption, modeling agricultural, food, and forestry products on a high level of resolution while also including the land requirements of manufactured goods and services. In 2004, high-income countries required more biologically productive land per capita than low-income countries, but this connection could only be identified when land used to produce internationally traded products was taken into account, because higher-income countries tend to displace a larger fraction of land use. The equivalent land and ocean area footprint of nations increased by a third for each doubling of income, with all variables analyzed on a per capita basis. This increase came largely from imports, which increased proportionally to income. Export depended mostly on the capacity of countries to produce useful biomass, the biocapacity. Our analysis clearly shows that countries with a high biocapacity per capita tend to spare more land for nature. Biocapacity per capita can be increased through more intensive production or by reducing population density. The net displacement of land use from high-income to low-income countries amounted to 6% of the global land demand, even though high-income countries had more land available per capita than low-income countries. In particular, Europe and Japan placed high pressure on ecosystems in lower-income countries.  相似文献   

Laboratory investigation of pressure gradients induced by plunging breakers     

Adrián Pedrozo-Acuña  Amaia Ruiz de Alegría-Arzaburu  Alec Torres-Freyermuth  Edgar Mendoza  Rodolfo Silva 《Coastal Engineering》2011

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Comments on ‘on the contribution of spray droplets to evaporation’ by Lutz Hasse     

Edgar L Andreas 《Boundary-Layer Meteorology》1994,68(1-2):207-214

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A new algorithm for radiative feedback and its application to the formation of massive stars     

Richard Edgar  Cathie Clarke 《Monthly notices of the Royal Astronomical Society》2003,338(4):962-972

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The minimum gap-opening planet mass in an irradiated circumstellar accretion disc     

Richard G. Edgar  Alice C. Quillen  Jaehong Park 《Monthly notices of the Royal Astronomical Society》2007,381(3):1280-1286

We consider the minimum mass planet, as a function of radius, that is capable of opening a gap in an α-accretion disc. We estimate that a half-Jupiter mass planet can open a gap in a disc with accretion rate     for viscosity parameter  α= 0.01  , and solar mass and luminosity. The minimum mass is approximately proportional to     . This estimate can be used to rule out the presence of massive planets in gapless accretion discs. We identify two radii at which an inwardly migrating planet may become able to open a gap and so slow its migration; the radius at which the heating from viscous dissipation is similar to that from stellar radiation in a flared disc, and the radius at which the disc becomes optically thin in a self-shadowed disc. In the inner portions of the disc, we find that the minimum planet mass required to open a gap is only weakly dependent on radius. If a migrating planet is unable to open a gap by the time it reaches either of the transition radii, then it is likely to be lost on to the star. If a gap-opening planet cuts off disc accretion allowing the formation of a central hole or clearing in the disc then we would estimate that the clearing radius would approximately be proportional to the stellar mass.  相似文献   

Travelling wave convection in a rotating layer     

Edgar Knobloch  Mary Silber 《地球物理与天体物理流体动力学》2013,107(1-4):195-209

Abstract

Small amplitude two-dimensional Boussinesq convection in a plane layer with stress-free boundaries rotating uniformly about the vertical is studied. A horizontally unbounded layer is modelled by periodic boundary conditions. When the centrifugal force is balanced by an appropriate pressure gradient the resulting equations are translation invariant, and overstable convection can take the form of travelling waves. In the Prandtl number regime 0.53 < [sgrave] < 0.68 such solutions are preferred over the more usual standing waves. For [sgrave] < 0.53, travelling waves are stable provided the Taylor number is sufficiently large.  相似文献   

The outbursts of dwarf novae     

M. R. Truss  J. R. Murray  G. A. Wynn  R. G. Edgar 《Monthly notices of the Royal Astronomical Society》2000,319(2):467-476

We present a numerical scheme for the evolution of an accretion disc through a dwarf nova outburst. We introduce a time-varying artificial viscosity into an existing smoothed particle hydrodynamics code optimized for two- and three-dimensional simulations of accretion discs. The technique gives rise to coherent outbursts and can easily be adapted to include a complete treatment of thermodynamics. We apply a two-dimensional isothermal scheme to the system SS Cygni, and present a wide range of observationally testable results.  相似文献   

Phase relations of talc and tremolite in metamorphic calcite-dolomite sediments in the southern portion of the Damara Belt (South West Africa)     

D. Puhan  E. Hoffer 《Contributions to Mineralogy and Petrology》1973,40(3):207-214

The occurrence of talc and tremolite in a temperature gradient was investigated in siliceous calcite-dolomite sediments exposed along a strip in the southeastern part of the Damara Orogen. Five bivariant reactions may lead to the formation of talc and tremolite:

1. 3 dolomite+4 quartz+1 H₂O ? 1 talc+3 calcite+3 CO₂
2. 5 talc+6 calcite+4 quartz ? 1 tremolite+6 CO₂+2 H₂O
3. 2 talc+3 calcite ? 1 tremolite+1 dolomite+1 CO₂+1 H₂O
4. 5 dolomite+8 quartz+1 H₂O ? 1 tremolite+3 calcite+7 CO₂
5. 2 dolomite+1 talc+4 quartz ? 1 tremolite+4 CO₂.

The common paragenesis of four mineral assemblages tc+cc+dol+qtz¹ and tre+tc+ cc+qtz with increasing temperature over an extended area show that the reactions must have taken place along the equilibrium curve or when fluid pressure is not constant along the equilibrium plane of reactions (1) or (2). The described occurrence of the five mineral assemblage tre+tc+cc+dol+qtz can be stable only on the isobaric intersection point, or when P _f is variable on the univariant intersection curve of the equilibrium planes of all five reactions. The genetic relations of the described parageneses are illustrated with the help of a phase diagram. Minimum P-T conditions which prevailed during metamorphism in this part of the Damara Orogen have been estimated to be about 590° C and 5 kb.  相似文献