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231.
R.S. Rajan J.C. Huneke S.P. Smith G.J. Wasserburg 《Earth and Planetary Science Letters》1975,27(2):181-190
High resolution40Ar-39Ar age spectra have been measured on plagioclase and glass from two howardites. Both the plagioclase and glass from the gas-rich Bununu howardite show well-defined age plateaux, yielding distinct ages of 4.42 ± 0.04 and 4.24 ± 0.05 AE, respectively. These age patterns are rather well behaved and are interpreted as representing the distinct times of formation of plagioclase from igneous processes and of glass fragments produced by impact on the meteorite body. The release pattern for the glass from the heavily shocked Malvern howardite is undulating at low and intermediate temperatures but does have a high-temperature plateau. Its age spectrum indicates little apparent diffusion loss, but rather an extensive redistribution of either40Ar during the shock event or of39Ar during the neutron irradiation or both. The total K-Ar age of Malvern glass is 3.64 ± 0.04 AE and the high-temperature plateau is 3.73 ± 0.05 AE. The age spectrum of the Malvern plagioclase has an intermediate temperature “plateau” at 3.80 AE that represents 20% of the total40Ar content and increases towards a high-temperature plateau at 4.29 ± 0.04 AE containing 26% of the total gas release. It seems likely that the event which formed the Malvern glass also reset part of the plagioclase. The distinct histories observed for the different phases of these howardites are consistent with their formation from a regolith. The present results along with similar young ages for igneous clasts from Kapoeta clearly show that the regoliths were extant on the parent bodies of howardites and that they were subjected to violent impact events at least as recently as 3.7 AE ago. 相似文献
232.
In an earlier paper by one of the authors (Smith, 1968), a momentum integral method was developed to parameterize the gross
constraint imposed by the surface boundary layer of a steady, axisymmetric, tropical cyclone on the meridional circulation
within the vortex itself. Specifically, the method provides an effective means of estimating the radial variation of mean
upflow/downflow induced by the boundary layer, compatible with a prescribed radial variation of azimuthal velocity just above
the boundary layer,V
gr. However, it relies on a judicious choice of vertical profiles of radial and azimuthal velocity components within the boundary
layer. An especially suitable set of profiles is discussed herein; these are Ekman-like profiles in which turbulent mixing
is characterized by a vertically constant eddy diffusivityK
M
, matched to a constant stress sublayer just above the sea surface. An attractive feature of the formulation is that a suitable
value forK
M
as a function of radius, which is extremely difficult to extract from observational data, can be calculated when the state
of the sea surface, described by a roughness lengthZ
0, is prescribed. Although observations ofZ
0 at high wind speeds are not yet available, the effect of radial variations in sea surface roughness can be assessed and it
is shown that these affect the upflow to a significant degree. 相似文献
233.
234.
Seven petrographic thin sections of lunar rock sample 14321, ‘Big Bertha’, have been examined. It is a complex rock incorporating diverse lithic and single crystal fragments and represents a sampling of the heterogeneous Fra Mauro formation, considered by the writers to be lithified debris from the Imbrium impact event. Electron probe microanalysis and microscopic study of textures reveal the assembly history of this breccia which in turn allows some interpretation of the nature of the pre-Imbrium crust and the effect of the Imbrium impact and the subsequent transportation to the Apollo 14 site. The present-day polymict breccia 14321 is composed of basaltic clasts originating from the fragmentation of a single or closely related set of lava cooling units, a set of fragmental clasts designated as microbreccia 3 (themselves polymict microbreccias), and a light colored matrix which formed rock 14321 by cementing the two major groups of clasts. The light colored matrix material is derived from the fragmentation and mutual abrasion of the basalt and microbreccia 3. On the basis of consistent textural relations two older sets of microbreccias have been identified within microbreccia 3. Microbreccia 1 clasts are well-rounded, relatively light colored, and noritic. They are always completely enclosed within microbreccia 3, most often forming the central cores of rounded accretionary lapilli structures which we have designated as microbreccia 2. Microbreccias 1, 2, 3, and macrobreccia 14321 represent a chronological series of fragmentation and lithification events. Each of these events involved some thermal and/or shock metamorphism as evidenced by mineralogical and textural criteria, and the chronological order of formation of the breccias also corresponds to a decreasing intensity of associated thermal effects. The petrology and mineralogy of 14321 are described in detail in this paper. A more general interpretation of the combined petrographic and chemical data is given in Duncanet al. (1975a). 相似文献
235.
236.
David M. Smith 《Geoforum》1979,10(3):297-310
The problems of the inner city are a subject of growing concern in the advanced capitalist world. The level of social deprivation may be identified on a territorial basis, by mapping numerical indicators relating to various relevant conditions. However, the application of conventional geographical methodology with its emphasis on pattern identification and ecological analysis provides an inadequate foundation for the explanation of localized deprivation and for the design of remedial policy. Inner-city deprivation arises from the operation of the contemporary capitalist system, the understanding of which requires a holistic social-science perspective. 相似文献
237.
The Spaceborne Laser Ranging System is a proposed short pulse laser on board an orbiting spacecraft.1,2,3,4 It measures the distance between the spacecraft and many laser retroreflectors (targets) deployed on the Earth’s surface.
The precision of these range measurements is assumed to be about ±2 cm (M. W. Fitzmaurice, private communication). These measurements are then used together with the orbital dynamics of the spacecraft, to derive
the relative position of the laser ground targets. Assuming a six day observing period with 50% cloud cover, uncertainties
in the baseline for target separations of 50 km to 1200 km were estimated to be on the order of 1 to 3 cm and the corresponding
values in the vertical direction, ranged from 1 cm to 12 cm. By redetermining the measurements of the relative target positions,
the estimated precision in the baseline for a target separation of 50 km is less than 0.3 cm and for a separation of 1200
km is less than 1 cm. In the vertical direction, the estimated precision ranged from 0.4 cm to 4.0 cm respectively. As a result
of the repeated estimation of the relative laser target positions, most of the non-temporal effects of error sources as exemplified
by the errors in geopotential are reduced.
The Spaceborne Laser Ranging System’s capability of determining baselines to a high degree of precision provides a measure
of strain and strain rate as shown byCohen, 1979. These quantities are essential for crustal dynamic studies which include determination and monitoring of strain near
seismic zones, land subsidence, and edifice building preceding volcanic eruptions. It is evident that such a system can also
be used for geodetic surveys where such precisions are more than adquate. 相似文献
238.
R.L. Hervig J.V. Smith I.M. Steele J.B. Dawson 《Earth and Planetary Science Letters》1980,50(1):41-58
Ion and electron microprobe analyses of twenty-one CrAl-spinel harzburgite xenoliths from southern African kimberlites show two chemical groups. Orthopyroxenes from “fertile” harzburgites have higher CaO (mean of 11, 0.95 wt.%), Al2O3 (3.05 wt.%), Cr2O3 (0.85 wt.%) and Li (0.8 ppmw) than those from “barren” harzburgites (mean of 10, CaO 0.24 wt.%, Al2O3 1.10 wt.%, Cr2O3 0.35 wt.%, Li 0.3 ppmw). Olivines from all harzburgites have similar chemistry except that mean values of Li and Na are higher for barren than fertile harzburgites (Li 0.9 vs. 0.4 ppmw; Na2O 16 vs. 7 ppmw). Orthopyroxenes from fertile harzburgites are chemically distinct from those in garne lherzolites from southern Africa and spinel lherzolites from southwest U.S.A., but orthopyroxenes from barren harzburgites are indistinguishable from those in many coarse garnet lherzolites.Chromium, Ca, Ni, Na and Li in coexisting olivines and orthopyroxenes from the above rock types show complex patterns, which for Ca, Cr and Ni can be related to pressure and temperature. Temperatures from an empirically calibrated thermometer based on Ni-Mg exchange between olivine and orthopyroxene, measured modes of harzburgites (fertile, mean of 10: ol 68, opx 31, spinel-silicate intergrowth <0.5; barren, mean of 8: ol 76, opx 23, spinel and spinel-silicate intergrowth 1), and high-pressure experimental studies suggest (a) that harzburgites are residues of partial melting, (b) that barren harzburgites were melted to a greater extent at a higher temperature (though probably at a similar depth) than fertile harzburgites, and (c) that incomplete reequilibration during retrograde metamorphism has led to development of complex inter- and intragranular textures, probably in the range ~700–900°C. 相似文献
239.
240.
J.S. Delaney J.V. Smith D.A. Carswell J.B. Dawson 《Geochimica et cosmochimica acta》1980,44(6):857-872
Micas from coarse granular Iherzolites in S. African kimberlites may be separated into two groups; those showing primary textural relationships with coexisting silicates and those with secondary, alteration relationships with other silicates. Primary-textured micas form a tight cluster with a mean composition from 10 coarse garnet lherzolites of: SiO2 41.0, TiO2 0.18, Al2O3 13.5, Cr2O3 0.82, total Fe as FeO 2.60, MnO 0.02, MgO 26.0, NiO 0.22, CaO 0.01, BaO 0.29, Na2O 0.31, K2O 10.0, Rb2O 0.028, Cl 0.08, F 0.43 wt%. Primary-textured micas in aggregates with clinopyroxene have higher TiO2 and four specimens which look similar to the primary group but have textural ambiguities have still higher TiO2Micas with secondary textures have wide ranges of composition which may be correlated with details of the textural parageneses. Micas from kelyphitic rims around garnets tend to be Cr-rich while those from veinlets are Cr-poor. Both groups tend to have higher FeO and TiO2 than the primary group. Micas produced by alteration of, or filling veinlets through, orthopyroxene have a wide compositional range which overlaps that of the primary-textured micas, especially for harzburgite specimens.The primary-textured micas show a positive correlation with coexisting pyroxenes for MgO/(MgO + FeO) and TiO2, but not for Cr2O3. Secondary-textured micas do not show correlations with coexisting pyroxenes for any elements.The ‘primary-metasomatic’ micas described by Harte and Gurney (1975) and metasomatic and other micas described by Boettcher et al. (1979) and Boettcher and O'neil (1979) are richer in FeO and TiO2 than the present primary-textured micas, and are attributed to crystallization from fractionated fluids. 相似文献