DR TERRANCE CHARLES RICHARDS     

John E. R. Wood 《Geophysical Prospecting》1980,28(2):314-315

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The Claygate Beds of Essex     

C.R. Bristow  R.A. Ellison  C.J. Wood 《Proceedings of the Geologists' Association. Geologists' Association》1980,91(4):261-277

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The interstellar dust as a precursor of Ca,Al-rich inclusions in carbonaceous chondrites     

John A. Wood 《Earth and Planetary Science Letters》1981

(1) The observed anomalies in meteoritic oxygen isotope compositions are not due to an incomplete mixing of several dust or gas-plus-dust components in the solar nebula. If they were, other elements would display similar anomalies. (The FUN inclusions in Allende appear to be exceptions to this premise.) (2) The anomalies must therefore stem from differing degrees of incomplete exchange of oxygen isotopes between the primordial gas and dust components of the nebula. The dust is more likely to have been the¹⁶O-enriched component. (3) Since the isotopic difference between dust and gas probably could not have been preserved if the dust was ever completely vaporized in the nebula, the Ca,Al-rich inclusions (CAI's) in carbonaceous chondrites are unlikely to be condensates, but instead are distillation residues. (4) If so, the observed depletion of super-refractory elements in the Group II CAI's cannot have been accomplished by fractional condensation in the solar nebula. (5) Then this depletion, and a number of other properties of the components of primitive meteoritic material, must be relics of pre-solar system fractionations among different populations of interstellar dust grains.  相似文献   

Relations between surface deformation,fault geometry,seismicity, and rupture characteristics during the El Asnam (Algeria) earthquake of 10 October 1980     

G. Yielding  J.A. Jackson  G.C.P. King  H. Sinvhal  C. Vita-Finzi  R.M. Wood 《Earth and Planetary Science Letters》1981

The El Asnam earthquake of October 10, 1980 (M_s=7.3) produced surface faulting on a northeast-trending thrust fault of 30 km length with displacements of up to 6.5 m, though average displacements were about 3 m. In addition, widespread tensional features were formed, some in clear association with folding above the thrust, and others, in an area beyond the exposure of the thrust at the surface, which may be related to buried reverse faults.The observed thrust fault is split into southern, central and northern segments. Local and teleseismic data are examined to show that the main shock nucleated at the southwest end of the fault, and propagated 12 km northeast where a second rupture of approximately equal moment occurred, continuing the faulting a further 12 km northeast along the central segment. Both ruptures nucleated at about 8–10 km depth. Displacements were largest on the central segment, where they were probably enlarged by aftershocks, including one of m_b=6.1 three hours after the main shock. The northern segment was much shorter than the other two, and showed smaller displacement.The junctions between fault segments are marked by distinct geomorphological characteristics and a change in strike of the faulting, as well as a sudden drop in the observed displacement. It appears that the rupture development is influenced by the changes in fault geometry between segments, and that such junctions or barriers have persisted through much of the late Quaternary.  相似文献   

Earthquake response of a steel frame building     

J. H. Wood 《地震工程与结构动力学》1976,4(4):349-377

A study has been made of the response, during the San Fernando earthquake 9 February 1971, of the nine-storey steel frame Building 180, located at the California Institute of Technology, Jet Propulsion Laboratory, Pasadena. The analysis throws light on the actual dynamical properties of the building during the earthquake, and also demonstrates that it is possible, when the ground motion is specified, to make accurate predictions of building motions during moderate earthquakes by using a linear viscously damped model. Methods of evaluating the lower mode periods and damping ratios from the earthquake records are described and the values obtained are compared with results from dynamic testing before and after the earthquake and with the periods computed from computer models of the building. Although no structural damage occurred and computed stresses in the steel frame were less than yield stresses, the periods measured by an ambient vibration test after the earthquake were of the order of 10 per cent higher than the pre-earthquake values. The maximum periods during the earthquake were found to be about 30 per cent higher than the post-earthquake periods.  相似文献   

The Otago schist megaculmination: Its possible origins and tectonic significance in the Rangitata orogen of New Zealand     

B.L. Wood 《Tectonophysics》1978,47(3-4)

In South Island, New Zealand, the Otago schist, 30,000 square km in extent, consists mainly of greenschist facies quartzo-feldspathic metagreywacke and meta-argillite with minor metavolcanics and metacherts. Before metamorphism the sediments were probably Carboniferous to Jurassic; the flanking, steeply dipping greywackes are Triassic in the northeast and southeast, and Permian in the west and southwest.Regional metamorphism culminating in the Late Jurassic was accompanied by pervasive deformation generating a variety of interrelated folds on all scales. The scarcity of distinctive reference units makes recognition of macroscopic structures difficult, and much progress has depended on observations of vergence of mesoscopic folds interpreted as defining macroscopic folds having axial plane separation of between 2 km and 6 km.At least two phases of synmetamorphic deformation are distinguishable locally, but regionally have an overlapping multiphase relationship. The regional schistosity structure is an irregular flat-crested antiform trending S and SE. The internal megascopic structure defined by the mesoscopic folds, appears to consist of a stack of nappe-folds facing east and northeast, which pass into reclining isoclinal folds in the west, southwest and north-east, and is interpreted to be a megaculmination. Mineral and textural metamorphic zones were developed during deformation, and a relatively simple regional pattern established at a late stage by continuing recrystallisation.The Otago schist originated in a complex sequence of Paleozoic—Mesozoic plate interactions near the southwest Pacific margin of Gondwanaland. It included part of a volcaniclastic frontal arc-basin assemblage (Murihiku and Caples Terranes) lying north or northeast of an older crystalline foreland, and a quartzo-feldspathic assemblage of plutonic-metamorphic provenance lying further to the northeast (Torlesse Terrane). Parts of these terranes underwent mainly greenschist facies metamorphism during Late Jurassic subduction-collision to form the Haast Schist Terrane of which the Otago schist is a major part.The earliest Torlesse sediments are thought to have prograded as a vast fan complex onto oceanic crust from the southwesterly crystalline foreland in the Carboniferous, then in the Permian were separated from their source by a spreading zone which thereafter isolated them from the sedimentary province of the newly developing arc system. Tectonic recycling of these sediments at a Permian to Jurassic oceanic subduction zone is considered to have developed the westward progradation features and the products of limited vulcanism found in the present Torlesse Terrane. The New Zealand Geosyncline appears to have consisted of a spreading zone between two inwardly facing convergent zones, one flanked by a foreland to the southwest, the other wholly oceanic.The metamorphic climax of the Rangitata Orogeny was the result of the medial spreading zone passing into the westerly subduction zone, so permitting the convergent zones to collide, with the Torlesse sediments caught between them.The mantle system driving the spreading zone appears to have continued to function, and soon after the collisional climax caused Late Jurassic—Cretaceous rifting of the sialic edge of Gondwanaland, igneous activity, differential shear of the New Zealand region, and initiation of the Alpine Fault. It subsequently commenced sea-floor spreading in the Tasman Sea, and later in the southwest Pacific Ocean.  相似文献   

Thermodynamic properties of almandine-grossular garnet solid solutions   总被引：1，自引：0，他引：1  

G. Cressey  R. Schmid  B. J. Wood 《Contributions to Mineralogy and Petrology》1978,67(4):397-404

The mixing properties of Fe₃Al₂Si₃O₁₂-Ca₃Al₂Si₃O₁₂ garnet solid solutions have been studied in the temperature range 850–1100° C. The experimental method involves measuring the composition of garnet in equilibrium with an assemblage in which the activity of the Ca₃Al₂Si₃O₁₂ component is fixed. Experiments on the assemblage garnet solid solution, anorthite, Al₂SiO₅ polymorph and quartz at known pressure and temperature fix the activity of the Ca₃Al₂Si₃O₁₂ component through the equilibrium: 1 $$\begin{gathered} {\text{3CaAl}}_{\text{2}} {\text{Si}}_{\text{2}} {\text{O}}_{\text{8}} \rightleftarrows {\text{Ca}}_{\text{3}} {\text{Al}}_{\text{2}} {\text{Si}}_{\text{3}} {\text{O}}_{{\text{12}}} \hfill \\ {\text{Anorthite garnet}} \hfill \\ {\text{ + 2Al}}_{\text{2}} {\text{SiO}}_{\text{5}} {\text{ + SiO}}_{\text{2}} \hfill \\ {\text{ sillimanite/kyanite quartz}}{\text{.}} \hfill \\ \end{gathered}$$ This equilibrium, with either sillimanite or kyanite as the aluminosilicate mineral, was used to control \({\text{a}}_{{\text{Ca}}_{\text{3}} {\text{Al}}_{\text{2}} {\text{Si}}_{\text{3}} {\text{O}}_{{\text{12}}} }^{{\text{gt}}} \) . The compositions of the garnet solutions produced were determined by measurement of their unit cell edges. At 1 bar Fe₃Al₂Si₃O₁₂-Ca₃Al₂Si₃O₁₂ garnets exhibit negative deviations from ideality at the Fe-rich end of the series and positive deviations at the calcium end. With increasing pressure the activity coefficients for the Ca₃Al₂Si₃O₁₂ component increase because the partial molar volume of this component is greater than the molar volume of pure grossular. Previous studies indicate that the activity coefficients for the Ca₃Al₂Si₃O₁₂ component also increase with increasing (Mg/Mg+Fe) ratio of the garnet. The region of negative deviation from ideality implies a tendency towards formation of a stable Fe-Ca garnet component. Evidence in support of this conclusion has been found in a natural Fe-rich garnet which was found to contain two different garnet phases of distinctly different compositions.  相似文献   

Capital investment and regional planning in Britain     

P.A. Wood 《Geoforum》1974,5(3):19-27

British regional problems increasingly emphasize the need to understand the exploitation and movement of all factors of production between different parts of the country. This paper reviews evidence, from work sponsored by the National Institute of Economic and Social Research, on the significance for the standard regions of capital investment, interregional capital flows and regional investment multipliers. A high level of economic interdependence allows the effects of investment to become widely spread throughout the British space economy. This limits the power of capital expenditure to lead growth in the region where it takes place. Studies of the spatial implications of capital investment should therefore form part of more general appraisals of factor supply and demand changes and their effects on the decisions of different investing agencies (including government). Two distinctive themes for the geographical study of capital investment are suggested: the examination of relationships between investment projects by different agencies at appropriate sub-regional scales; and the ways in which established patterns of physical capital stock may influence the expenditure of new, mobile funds.  相似文献   

New views of the Moon,edited by Bradley L. Jolliff,Mark A. Wieczorek,Charles K. Shearer,and Clive R. Neal     

Charles A. Wood 《Meteoritics & planetary science》2007,42(2):303-304

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GLAST large area telescope multiwavelength planning     

O. Reimer  P. F. Michelson  R. A. Cameron  S. W. Digel  D. J. Thompson  K. S. Wood 《Astrophysics and Space Science》2007,309(1-4):523-526

Gamma-ray astrophysics depends in many ways on multiwavelength studies. The Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT) Collaboration has started multiwavelength planning well before the scheduled 2007 launch of the observatory. Some of the high-priority multiwavelength needs include: (1) availability of contemporaneous radio and X-ray timing of pulsars; (2) expansion of blazar catalogs, including redshift measurements; (3) improved observations of molecular clouds, especially at high galactic latitudes; (4) simultaneous broad-band blazar monitoring; (5) characterization of gamma-ray transients, including gamma ray bursts; (6) radio, optical, X-ray and TeV counterpart searches for reliable and effective sources identification and characterization. Several of these activities are needed to be in place before launch.   相似文献