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921.
The major bedforms of gravel bed rivers, whether braided, meandering or straight, may be usefully resolved into pool-riffle units, each comprising a single scour pool together with an associated depositional shoal downstream. At low flow, the latter may be characterized by a single emergent bar-head and submerged riffle, or by a variety of remnant braid bars, depending upon the type of channel. Identification of pool-riffle units and observation of associated flow structures on a small meandering stream in northwest England has demonstrated important links between bedforms, flow patterns and channel change. Each unit appears to be associated with a systematic pattern of secondary flows, which are able to modify the bedforms and initiate meander development. Feedback links between plan morphology, flow patterns and erosive and depositional forces within these units ensure that each stage of meander growth has a characteristic style of channel change. Consequently, meanders tend to evolve by regular cycles of increasing curvature and complexity.  相似文献   
922.
Nineteen surveys were carried out over a two-year period to determine the surface height of a salt marsh creek located on the north side of the River Esk, Cumbria, England. An AGA 112 electromagnetic distance measurer mounted on a Wild TI theodolite was used in conjunction with acrylic reflectors to follow the form of the ground. The results showed that there were no significant net trends in surface level, although seasonal variations of the order of 2 cm occurred. Vegetated areas responded in similar fashion to bare surfaces. It is thought that the elevational changes were attributable to the swelling of clay particles during the winter months rather than the effects of erosion and accretion.  相似文献   
923.
The physicochemistry of the Black River and adjacent marine beach, in terms of tidal, daily and seasonal fluctuations of temperature and salinity, presents a highly stressed environment exacerbated by canalization of the river mouth. Riverine pollution further stresses this environment, producing low densities and diversities of marine infauna adjacent to the river. No fauna were found in the river mouth where typical estuarine conditions exist only during high tide. Tolerance of the dominant marine species, Cerebratulus fuscus, to temperature, salinity and river water combinations showed that mortality was more rapid after exposure to river water dilutions than after exposure to distilled water dilutions. Computer-generated models suggested that this species should survive conditions closer to the river than were observed. This confirmed additional stress due to pollution carried in the river from urban and industrial drainage. Lower river water temperatures during winter appear to ameliorate pollution stress, enhancing survivability of the infauna.  相似文献   
924.
Victorian brown coal occurs in five major lithotypes distinguishable by colour index, petrography and bulk chemical analyses. The distributions of solvent extractable (free) and base hydrolysable (bound) n-alkanes, n-monocar?ylic acids, n-?,ω-dicar?ylic acids, n-ω-hydroxycar?ylic acids and n-alcohols were determined for samples of each of the five lithotypes (lithotype profile) and for seven samples of identical lithotype classification spanning a 100 m interval (depth profile) taken from a continuous bore core. The distributions of free molecular components in all classes are indicative of the predominant higher plant origin of this immature coal and provide strong support for the view that different lithotypes have derived from different, yet fairly specific paleobotanical communities. Despite an overall similarity in the distributions of aliphatic components from samples of identical lithotype classification, changes in the absolute concentrations and carbon preference indices (CPIs) of specific functional classes are observed in response to catagenetic influences even across the very small rank interval of the depth profile samples. Molecular distributions of bound components are similar to those of their free counterparts except that CPIs are generally lower and the relative contributions of lower molecular weight homologues (i.e. <C22) are higher. Thedistributions of bound dicar?ylic acids and hydroxycar?ylic acids appear to reflect variations in the oxic/anoxic nature of the depositional paleoenvironments.  相似文献   
925.
Blithfield (EL6) is one of five known enstatite chondrite breccias. It consists of troilite-rich clasts (35 ± 5vol.%) embedded in an extremely metallic Fe,Ni-rich matrix (65 ± 5 vol.%) that contains metal nodules up to 17 mm in size. Clasts and matrix agglomerated independently in the solar nebula under conditions of high and lowpS2/pO2 ratios, respectively. The matrix accreted to an EL chondrite planetesimal and was metamorphosed to~ 1000°C, above the FeNiS eutectic; chondrule textures were obliterated. The S-rich eutectic melt was lost from the matrix. The matrix material was buried to a depth of at least 3 km; accreting troilite-rich material was incorporated into the matrix as clasts. The breccia cooled through~ 500°C at 1000–10,000°C/Myr. After cooling below~ 500°C, Blithfield was quenched, possibly by impact excavation from depth and deposition onto the surface.Clasts or inclusions that are enriched in sulfide and depleted in metallic Fe,Ni are common in brecciated enstatite chondrites. Variations in thepS2/pO2 ratio in the nebular regions where these materials formed may explain many of their petrologic properties. The silica-rich clasts in Adhi Kot (EH4) formed at very highpS2/pO2ratios(> 1027); niningerite, free silica and troilite were produced from the sulfurization of enstatite and metallic Fe. The troilite-rich clasts in Blithfield and Atlanta (EL6) as well as the troilite-rich regions of the Hvittis (EL6) matrix formed at somewhat lowerpS2/pO2 ratios where sulfurization of metalic Fe produced troilite. The Ni content of the residual metal increased, forming some metal of martensitic composition. The dark inclusions in Abee (EH 4), which contain up to 9 wt.% oldhamite, formed at highpS2/pO2 ratios in the presence of an additional Ca-rich component.  相似文献   
926.
Fifty-eight chondrules were separated from the Dhajala H3.8 chondrite and their thermoluminescence properties were measured. Chips from 30 of the chondrules were examined petrographically and with electron-microprobe techniques; the bulk compositions of 30 chondrules were determined by the fused bead technique. Porphyritic chondrules, especially 5 which have particularly high contents of mesostasis, tend to have higher TL (mass-normalized) than non-porphyritic chondrules. Significant correlations between log(TL) and the bulk CaO, Al2O3 and MnO content of the chondrules, and between log(TL) and the CaO, Al2O3, SiO2 and normative anorthite content of the chondrule glass, indicate an association between TL and the abundance and composition of mesostasis. Unequilibrated chondrules ( i.e. those whose olivine is compositionally heterogeneous and high in Ca) have low TL, whereas equilibrated chondrules have a wide range of TL, depending on their chemical and petrographic properties.We suggest that the TL level in a given chondrule is governed by its bulk composition (which largely determined the abundance and composition of constituent glass) and by metamorphism (which devitrfied the glass in those chondrules with high Ca glass to produce the TL phosphor). We also suggest that one reason why certain chondrules in type 3 ordinary chondrites are unequilibrated, while others are equilibrated, is that the mesostasis of the unequilibrated chondrules resisted the devitrification. This devitrification is necessary for the diffusive communication between chondrule grains and matrix that enables equilibration.  相似文献   
927.
A wind tunnel study of turbulent flow over model hills   总被引:1,自引:1,他引:1  
Detailed wind tunnel measurements have been made of mean flow and turbulence over a two-dimensional ridge and a circular hill, both having cosine-squared cross-section and maximum slope about 15 °. The measurements were made in an artificially thickened neutrally stratified boundary layer, and have been compared with results from linear models and rapid distortion theory as appropriate.Our study shows that linear theory gives generally good predictions of the mean flow on the upwind side of the hills, and especially of the flow speedup at the hill top, but that the turbulence is less well predicted. In particular, the measurements show a major increase in the vertical component of turbulence and in the shear stress on the upwind slope of both the two- and three-dimensional hills which is not predicted by either equilibrium or isotropic rapid-distortion theories, although this may be partly due to the effect of streamline curvature. Rapid-distortion theory is successful only in describing the streamwise component of turbulence in the outer region of the flow, while in the upper part of the inner region of the flow, the turbulence measurements show disagreement with both the equilibrium and the rapid-distortion theories. Our experiments also confirm that the equilibrium region is a very thin layer close to the surface, while above this region and below the outer region, there is a transitional region where all terms in the stress equation are important.The measurements over the three-dimensional hill suggest that the mean flow and turbulence are broadly similar to those over the two-dimensional ridge, but with reduced perturbation amplitudes. The major differences between the two cases are found on the upwind slope and in the wake where, respectively, horizontal divergence and convergence of the three-dimensional flow are most pronounced.  相似文献   
928.
929.
New K-Ar determinations for granitoid rocks and ores from the northern Bolivian segment (ca. 15°-18° S.) of the Central Andean Cordillera Oriental (Eastern Cordillera) confirm that this region displays a remarkable repetition of magmatic activity and associated lithophile metal mineralization. Intrusion of monzogranites, in part peraluminous, and granodiorites took place in the Mid—to—Late Triassic (apparent age range: 225-202 Ma) and Late Oligocene-Early Miocene (28.4-ca. 19.2 Ma); the two plutonic domains are juxtaposed, with little or no areal overlap, along an essentially linear belt defining the inner boundary of the Central Andean magmatic arc. There is no conclusive evidence of granitoid intrusion during the intervening period, although at least two centres of Upper Cretaceous basic-intermediate hypabyssal-volcanic rocks are known. Whereas the Triassic episode simultaneously affected ca. 200 km of the belt, the Oligocene-Miocene domain experienced a longitudinal (southeastward) migration of activity which, in its later stages (22-19 Ma), coincided with the initiation of widespread volcanism and intrusion on the altiplano, to the west of the granitoid belt.Both intrusive domains may be regarded as the innermost expressions of relatively brief episodes of radical broadening of the Central Andean magmatic arc, possibly generated through abrupt, but minor, decrease in the inclination of eastward subduction at the western plate margin, and attended by a degree of crustal anatexis unattained in the outer parts of the arc. Our radiometric data permit the delimitation of two metallogenetic (W-Sn) sub-provinces in the northern part of the Bolivian tin belt. The tungsten-tin vein deposits associated with the Triassic and Tertiary plutons are very similar, although tungsten appears to be enriched relative to tin in the older domain. There is no radio-metric or petrographic evidence of significant reactivation of older hydrothermal systems in the Tertiary. The late-Early Miocene age (16.3 Ma) determined for the important Oruro Sn-Ag epithermal centre (17° 56' S.) represents an anomaly in the broad southward migration of volcanic and hydrothermal activity defined byGrant et al. (1979) in the central and southern, sub-volcanic, segments of the Bolivian tin-polymetallic belt. Minor Pb-Zn-Ag vein mineralization was probably associated with the Upper Cretaceous basic-intermediate magmatism.
Zusammenfassung Neue K-Ar Bestimmungen für die granitoiden Gesteine und Erze aus dem nord-bolivischen Segment (ca. 15°-18° S) der mittleren andeanischen Cordillera Oriental (östlichen Cordillera) bestätigen, daß dieses Gebiet eine beachtenswerte Wiederholung der magmatischen Aktivität und der damit verbundenen Erzmineralisierung aufweist. Granodiorite und teilweise Monzogranite mit Aluminium-Überschuß sind in der Mittel- und Spät-Trias (225-202 Ma) und im Spät-Oligozän bis Früh-Miozän (28.4-ca. 19.2 Ma) eingedrungen; die beiden plutonischen Bereiche liegen mit nur geringer oder fehlender Überlappung benachbart längs einem im wesentlichen linearen Gürtel, der den inneren Rand des mittelandinischen magmatischen Bogen abgrenzt. Es gibt keine entscheidende Anzeichen für granitische Intrusionen in der dazwischen liegenden Zeit, obwohl wenigstens zwei Zentren der oberkretazischen basischen bis intermediären, hypabyssalen bis vulkanischen Gesteinen bekannt sind. Während die triassische Episode gleichzeitig ungefähr 200 km des Gebiets beeinflußte, erfuhr der oligozän-miozäne Bereich jedoch eine longitudinale (südöstliche) Wanderung der Aktivität, die, in den jüngeren Stufen, mit der Einleitung des ausgedehnten Vulkanismus und der Intrusion auf dem Altiplano, westlich des granitoiden Gebietes zusammenfiel.Die beiden intrusiven Gebiete könnte man als die innersten Vorgänge verhältnismägig kurzer Episoden einer drastischen Verbreitung des mittleren andinischen magmatischen Bogens betrachten. Diese könnten vielleicht durch die plötzliche Verringerung des Winkels der östlichen Subduktion an der westlichen Plattengrenze entstanden sein, mit einem Grad der Anatexis, der in den äußeren Teilen des Bogens nicht erreicht wurde. Unsere radiometrischen Daten ermöglichen die Abgrenzung zweier metallogenetischen (W-Sn) Unterprovinzen im nördlichen Teil des bolivischen Zinn-Gebiets. Obwohl die mit den triassischen und tertiären Plutonen verbundenen Wolfram-Zinn-Erzgänge einander sehr ähneln, scheint das Wolfram im älteren Bereich dem Zinn gegenüber etwas angereichert zu sein. Es liegen keine radiometrischen oder petrographischen Zeugnisse für eine erhebliche Reaktivierung von älteren hydrothermalen Systemen im Tertiär vor. Ein spätes früh-miozänes Alter (16.3 Ma) wurde für das wichtige Sn-Ag epithermale Zentrum von Oruro bestimmt. Dieses weicht von der allgemeinen nach S gerichteten Wanderung der vulkanischen und hydrothermalen Aktivität in den zentralen und südlichen subvulkanischen Segmenten der bolivischen Zinn-polymetallischen Gürtel ab, die vonGrant et al. (1979) beschrieben wurde. Geringere Pb-Zn-Ag-Erzgangbildung stand wahrscheinlich mit dem oberkretazischen basisch-intermediären Magmatismus in Verbindung.

Résumé De nouvelles determinations K-Ar sur des roches granitiques et sur du minerais provenant du segment bolivien septentrional (ca. 15°-18° S) de la Cordillère orientale des Andes centrales (Cordillère est) confirme que cette région fut affectée par une activité magmatique répétée auquelle s'associa une activité metalifère riche en métaux lithophiles. Des intrusions de monzogranites, en partie peralumineux et de granodiorites se mirent en place durant le Triassique moyen et supérieur (intervalle d'âge apparent: 225-202 Ma) et durant l'Oligocène moyen et le début du Miocène (24.4-ca. 19.2 Ma). Ces deux domaines plutoniques se juxtaposent avec un recouvrement spatial faible ou nul, le long d'une ceinture essentiellement linéaire définissant la bordure interne de l'arc magmatique des Andes centrales. Bien qu'aucune indication concluante nesitue la mise en place d'intrusions granitiques durant la période intermédiaire, au moins deux centres volcaniques hypabyssaux de composition basique à intermédiaire se sont formés au Crétacé supérieur. L'épisode magmatique du Triassique a affecté simultanément ca. 200 km de la ceinture. Le domaine Oligocène-Miocène, pour sa part, a subi une migration longitudinale (sudest) de l'activité magmatique dont les étapes tardives (22-19 Ma) coîcident avec le déput d'une longue période de volcanisme et d'intrusions sur l'altiplano, à l'ouest de la ceinture granitique.celle des aggregats de grande taille, par des mécanismes de dislocation. La transition est Les deux domaines intrusifs peuvent être causés par un fort élargissement répété et bref de l'arc magmatique des Andes centrales. neut-être dû à une diminution abrupte de l'inclinaison de la zone de subduction orientale à la bordure ouest de la plaque, accompagnée par un degré d'anatexie crustale qui n'atteignit pas la partie externe de l'arc. Les résultats radiométriques obtenus permettent de délimiter deux sous-provinces métallogéniques (W-Sn) dans la partie septentrionale de la ceinture bolivienne stannifère. Les gisements filoniens d'étain et de tungsténe associés aux plutons triassiques et tertiaires sont très semblables; cependant le tungstène semble être plus abondant rapport à l'étain dans le plus vieux domaine. Il n'y a aucune évidence radiométrique ou pétrographique d'une réactivation signicative du système hydrothermal tertiaire. L'age Miocène (16.3 Ma) obtenu pour l'important centre épithermal Sn-Ag d'Oruro (17° 56' S.) représente une anomalie dans la vaste migration sud-est de l'activité volcanique et hydrothermale définie parGrant et al. (1979) dans les segments «sub-volcaniques» central et sud-est de la ceinture polymétallique et stannifére bolivienne. Une faible minéralisation filonienne Pb-Zn-Ag était probalement associée avec le magmatisme intermédiaire à basique du Crétacé supérieur.

- ( 15–18° ) . , , . (225-202 ) (28,4-. 19,2 ) . , , . , , no- , : ( ) . , 200 , - , , . , . , , . . - , , , , . , , . - (16,3 ). - , Grant . (1979). , , , .
  相似文献   
930.
The Adhi Kot EH4 enstatite chondrite breccia consists of silica-rich clasts (12+mn; 5 vol.%), chondrule-rich clasts (55+mn; 10 vol.%) and matrix (35+mn; 10 vol.%). The silica-rich clasts are a new kind of enstatite chondritic material, which contains more cristobalite (18–28 wt.%) than enstatite (12–14 wt.%), as well as abundant niningerite and troilite. The bulk atomic Mg/Si ratios of the clasts (0.22–0.40) are much lower than the average for enstatite chondrites (0.79). Kamacite and martensite (with 8–11 wt.% Ni and a martensitic structure) occur in all three breccia components. The clasts have kamacite-rich rims, and kamacite-rich aggregates occur in the matrix.A unidirectional change in the ambient pS2/pO2 ratio in the region of the solar nebula where Adhi Kot agglomerated can explain many of the breccia's petrologic features. If this region initially had a very high pS2/pO2 ratio in a gas of non-cosmic composition, sulfurization of enstatite and metallic Fe (e.g., MgSiO3 + 2Fe + C + 3H2S = MgS + SiO2 + 2FeS + H2O + CH4) may have occurred, producing abundant niningerite, free silica and troilite at the expense of enstatite and metallic Fe. The Ni content of the residual metal would have increased, perhaps to ~ 8–10 wt.%. The silica-rich clasts agglomerated under these conditions; a significant fraction of the originally produced niningerite was lost (perhaps by aerodynamic size-sorting processes), lowering the clasts' bulk Mg/Si ratios.The pS2/pO2 ratio then decreased (perhaps because of infusion of additional H2O) and sulfurization of metallic Fe and enstatite ceased. The chondrule-rich clasts agglomerated under these conditions, acquiring little free silica and niningerite. An episode of chondrule formation occurred at this time (by melting millimeter-sized agglomerates of this relatively silica-poor enstatite chondrite material and concomitant fractionation of an immiscible liquid of metallic Fe,Ni and sulfide). The chondrule-rich clasts agglomerated many such chondrules. Subsequently, the matrix agglomerated, acquiring the few remaining chondrules. Kamacite-rich aggregates formed, after the cessation of metal sulfurization, and agglomerated with the matrix. The kamacite-rich clast rims were acquired at this time.The components of Adhi Kot accreted to the EH chondrite parent body, where the breccia was assembled, buried beneath additional accreting material, and metamorphosed at temperatures of ? 700°C. Impact-excavation of the breccia and deposition onto the surface caused the formation of martensite from taenite inside the clasts and the matrix. At the surface, impact-melting produced an albite glass spherule, which was incorporated into the matrix. However, the absence of solar-wind-implanted rare gases in bulk Adhi Kot indicates that the breccia spent little time in a regolith.  相似文献   
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