Geochemistry,geochronology, and petrogenesis of a Late Precambrian (∼ 590 Ma) composite dike from the North Eastern Desert of Egypt

Late Precambrian (575–600 Ma) igneous activity in the North Eastern Desert of Egypt produced large volumes of compositionally bimodal magmas. A single composite dike was studied to further examine petrogenetic relationships between andesitic and rhyolitic melts. The dike consists of 1.5–2 m of andesite on either side of a 5–6 m wide rhyolite core. Contact relations indicate that the andesite and rhyolite simultaneously existed as porphyritic liquids. Wholerock Rb-Sr dating indicates an age of 591 Ma, but with considerable scatter. Andesite and rhyolite had similar initial⁸⁷Sr/⁸⁶Sr of 0.7032±2, indicating derivation from a low Rb/Sr source, either the upper mantle, very young upper crust, or depleted lower crust. The composition of the andesites on either margin cannot be distinguished; these are very similar to andesites of the Dokhan Volcanics of similar age. Correspondingly, the rhyolite is compositionally similar to the epizonal Pink Granites. This dike and others like it represent hypabyssal feeders for the extrusive and shallow intrusive members of the North Eastern Desert bimodal suite.Major and trace element studies of the dike rocks show no evidence of mixing. With the exception of the alkaline earths, there is no evidence of diffusional transport across the rhyolite-andesite contacts. REE patterns indicate that petrogenesis of the andesite must have left a garnetiferous residue: either 10% melting of LREE-enriched garnet lherzolite or 25% melting of eclogite, followed by a small amount of shallow fractionation. Petrogenesis of the rhyolites remains enigmatic. Partitioning of trace elements and different plagioclase compositions in andesite and rhyolite argue against an origin by liquid immiscibility. Major and trace element models indicate that the rhyolite formed by fractional crystallization of the andesite or by anatexis of young amphibolite-facies crust.

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Zusammenfassung SpÄtprÄkambrische (575–600 Ma) magmatische AktivitÄt in der »North Eastern Desert« Ägyptens förderte gro\e Mengen bimodaler Magmen. Um die petrogenetischen Beziehungen zwischen andesitischen und rhyolitischen Schmelzen zu studieren, wurde ein einzelner, »bimodaler« Gang (composite dyke) untersucht.Der Gang besteht aus einem Rand von 1,5–2 m mÄchtigem Andesit auf beiden Seiten eines 5–6 m mÄchtigen Kernbereiches von Rhyolit. Die Kontaktbeziehungen zeigen, da\ Andesite und Rhyolite gleichzeitig als porphyritische Schmelzen existierten. »Whole-Rock« Rb-Sr Datierung ergab ein Alter von 591 Ma, jedoch mit einem erheblichen Fehler. Andesit und Rhyolith hatten Ähnliche initiale⁸⁷Sr/⁸⁶Sr VerhÄltnisse von 0.7032±2, die eine Herkunft aus Bereichen mit niedrigen Rb/Sr VerhÄltnissen erkennen lassen: Oberer Mantel, sehr junge obere Kruste, oder verarmte untere Kruste. Die Zusammensetzung der Andesite von den verschiedenen Seiten des Ganges ist nicht zu unterscheiden. Sie sind den Andesiten der Dokhan Vulkanite Ähnlich und etwa gleich alt. Entsprechend sind die Rhyolite den epizonalen rosa Graniten (»pink granite«) in der Zusammensetzung Ähnlich. Dieser Gang und andere gleich ihm stellen die Zufuhrspalten für die extrusiven und seichtintrusiven Magmatite der »North Eastern Desert« bimodalen Folge dar.Haupt- und Spurenelemente der Ganggesteine zeigen keine Anzeichen einer Mischung. Mit Ausnahme der Erdalkalien gibt es keinen Hinweis auf eine Diffusion der Elemente über den Rhyolit-Andesit Kontakt. Die Verteilung der Seltenen Erden deutet auf ein granatführendes Residuum bei der Petrogenese der Andesite: entweder10% Aufschmelzen von Granat-Lherzolit, angereichert an leichten Seltenen Erden, oder 25% Aufschmelzen von Eklogit, gefolgt von geringer Fraktionierung unter niedrigem Druck.Die Petrogenese der Rhyolite bleibt unklar. Die Verteilung der Spurenelemente und die unterschiedliche Plagioklas-Zusammensetzung in Andesit und Rhyolith sprechen gegen eine Entstehung aus unvermischbaren Schmelzen. Modelle basierend auf Haupt- und Spurenelementen deuten darauf hin, da\ der Rhyolit entweder durch fraktionierte Kristallisation des Andesits entstand oder durch Anatexis junger Kruste im Bereich der Amphibolit-Fazies.

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Résumé L'activité magmatique au Précambrien supérieur (575–600 Ma) dans le »North Eastern Desert« d'Egypte a engendré de grandes quantités de magmas bimodaux. De manière à préciser les relations entre fusions andésitiques et rhyolitiques, un dyke composite a été étudié.Ce dyke est constitué d'un coeur rhyolitique de 5 à 6 m, encadré de deux bordures andésitiques de 1,5 à 2 m. Les contacts indiquent que ces deux roches ont coexisté sous la forme de liquides porphyriques. Une datation Rb-Sr sur roche totale donne un âge de 591 Ma, mais avec une approximation importante. L'andésite et la rhyolite ont un mÊme rapport initial de 0,7032±2, indiquant une source à faible rapport Rb/Sr: manteau supérieur, croûte supérieure jeune ou croûte inférieure appauvrie. Les compositions des deux bordures andésitiques sont identiques et très semblables à celle des andésites de mÊme âge du complexe volcanique du Dokhan. De mÊme, la rhyolite a une composition semblable à celle des granites roses épizonaux. Ce dyke et d'autres du mÊme type représentent les voies d'alimentation des termes extrusifs et intrusifs superficiels de la série bimodale du »North Eastern Desert«.L'étude des éléments majeurs et en traces ne montre aucun mélange entre les roches du dyke. A l'exception des alcalino-terreux, il n'existe aucune indication de diffusion des éléments à travers le contact rhyolite — andésite. La distribution des terres rares montre que la genèse de l'andésite doit avoir laissé un résidu grenatifère: soit une lherzolite à grenat enrichie en terres rares légères et représentant moins de 10% de taux de fusion, soit une éclogite (jusqu'à 25% de taux de fusion) suivie d'un léger fractionnement à basse pression.La pétrogenèse de la rhyolite reste obscure. La répartition des éléments en traces et la différence de composition du plagioclase entre l'andésite et la rhyolite plaident contre une origine par immiscibilité. Les modèles tirés des éléments majeurs et en traces indiquent comme origine pour la rhyolite soit la cristallisation fractionnée de l'andésite, soit l'anatexie de matériaux crustaux jeunes dans les conditions du facies des amphibolites.

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Possible effects of pre-existing basement topography on thrust fault ramping

Finite-element models show that one way in which thrust ramps may arise is through the mechanical interaction between basement and overlying sediments. In the simplest case, shear coupling between a planar basement—sediment contact causes the differential stresses in the sediments to die out with depth and distance from the applied load. For such cases, curved thrust faults may result if the strength of the rock is exceeded. Basement topography may also affect the location and shape of ramps by acting as a stress concentrator, by producing a stress shadow and by changing principal stress orientations. Modeling suggests that whether or not these basement topographic features cause ramping will depend on the height and angularity of the feature as well as the rock types that overlie it.Under the assumption of linear elasticity and for given boundary conditions, the Poisson's ratio plays an important role in determining the orientation and magnitude of the principal stresses. Calculations using experimentally measured Poisson's ratios predict that the earliest maximum compressive stress directions should be nearly vertical in the more cratonward portions of thrust belts. However, the stress directions which are inferred to have occurred earliest in this part of thrust belts are nearly horizontal. This suggests that non-elastic or ductile processes have an effect on the propagation of thrust faults.     

Petrographic constraints on models of intergranular pressure solution in quartzose sandstones

Petrographic and SEM observations on 478 samples of six quartzose sandstones provide a data base that can be used to evaluate the role of intergranular pressure solution (IPS) in sandstone diagenesis and to constrain predictive models of the pressure solution process. SEM examination of grain contacts that have experienced pressure solution suggests that IPS occurs at the interior portions of contacts where the greatest stress is concentrated and that granulation of quartz grains at points of contact may contribute to the process. The chemical compaction fabrics that result from IPS suggest that the process is most commonly induced by effective lithostatic stress and that the resulting strain is uniaxial.Numerous geological variables influence IPS. Grain size exerts a fundamental influence, with finer grained samples experiencing more IPS than coarser grained samples. On both local and regional scales, IPS is inhibited by poor sorting, an abundance of ductile grains, the presence of “shallow” cement, slow rates of shallow burial, and overpressured conditions. In contrast, IPS is enhanced by the presence of illite grain coatings, increased maximum burial depth, rapid rates of shallow burial, longer times spent at great depths, higher temperatures, and high volumes and rates of fluid flow.Silica budgets indicate that some of the analyzed sandstones approximate mass balance whereas others have exported silica. Calculations of fluid flow requirements indicate that advanced stages of IPS are favored by high volume, high velocity fluid flow. Such flow can occur as a result of uplift of basin margins, which is typical of foreland and intractonic basins.     

Similarity forms for ground-source surface-layer diffusion

Past work on analyzing ground-source diffusion data in terms of surface-layer similarity theory is reviewed; these analyses assume that _z /L orh/L is a function of u ^* x/L (where h = Q/ dy). It is argued that an alternative scaling, h ^*/L versus x/L, is nearly as universal in that it is very weakly influenced by surface roughness, except for a modest influence in the free convective case (h ^* = Q/u ^* dy); the advantage of this scaling is that it eliminates the need to reassess as vertical diffusion progresses. The Prairie Grass data set is adjusted for the difference in source and sampling heights, and is plotted with this scaling. Simple analytic equations are suggested that fit the resultant data plots for stable and unstable conditions, and suggestions are made towards practical application of these results.On assignment from the National Oceanic and Atmospheric Administration, U.S. Department of Commerce.     

An inverse method for determining wind stress from water-level fluctuations

The hydrodynamic equations governing the water-level response of a lake to wind stress are inverted to determine wind stress from water-level fluctuations. In order to obtain a unique solution, the wind-stress field is represented in terms of a finite number of spatially dependent basis functions with time-dependent coefficients. The discretized version of the inverse equation is solved by a least-squares procedure to obtain the coefficients, and thereby the stress. The method is tested for several ideal cases with Lake Erie topography. Real water-level data is then used to determine hourly values of vector wind stress over Lake Erie for the period 5 May–31 October, 1979. Results are compared with measurements of wind speed and direction from buoys deployed in the lake. Calculated stress direction agrees with observed wind direction for wind speeds > 7.5 m s⁻¹. Under neutral conditions, calculated drag coefficients increase with the wind speed from 1.53 × 10⁻³ for 7.5−10 m s⁻¹ winds to 2.04 × 10⁻³ for 15−17.5 m s⁻¹ winds. Drag coefficients are lower for stable conditions and higher for unstable conditions.     

Patterns in seasonal abundance,growth and biomass of the atlantic silverside,Menidia menidia,in a New England estuary

Patterns in seasonal abundance (no. per m² surface area), growth and biomass (g per m² surface area) of an annual fish, the Atlantic silverside, Menidia menidia (L.) were investigated in a marsh and more seaward bay region of Essex Bay, Massachusetts from August 1976 to May 1978 using a quantitative beach seining technique. Silverside abundance varied greatly by season and year class during the study period. Abundance was high in 1976 but winter mortality (99%) left an adult density of only .01 per m² surface area in the marsh during spring 1977. Resultant 1977 year class density in the marsh was 1.88 per m² by late fall 1977 but winter mortality again produced an adult density of .01 per m² in spring 1978. Abundance was generally higher in the marsh than in the bay region especially during spring and late fall when catches in the bay were negligible. Based on catch rate comparisons, the summer and fall juvenile abundance of the 1976 year class was much higher than the juvenile abundance of the 1977 year class. Coincidentally, mean lengths and condition of the abundant 1976 year class in the late fall were significantly lower than those of the 1977 year class, suggesting density dependent population regulation. In both years, juveniles grew rapidly and reached full adult size by November when an offshore movement to deeper waters outside Essex Bay occurred. Biomass peaked in the marsh region in late fall 1977 at 7.8 g per m² wet weight. Winter mortality was size selective, favoring larger individuals. The annual life history design of M. menidia including an offshore winter movement and high winter mortality suggests that silversides represent an important pathway of energy flow from marsh to offshore trophic systems.     

The American oyster as a coastal zone pollution monitor: A pilot study

The Condition Index [(dry meat weight)(100)/(internal cavity volume)] has been analyzed and compared in the American oyster,Crassostrea virginica, from two South Carolina estuaries, one of which was considered polluted by coliform bacteria standards. During the warmer months, oysters from the unpolluted habitat showed a consistently and significantly higher Condition Index. Best fit and power function regressions of Condition Index on total coliform bacteria levels conform with previously cited effects of pollutants on oysters. Condition Index droped markedly as the incidence of total coliforms increased toward levels of 100 per 100 ml of water. Our results and the known sensitivity of oysters to a spectrum of pollutants suggest that their condition could be used to monitor waterborne pollution in coastal zone areas.     

Strontium-calcium ratios in Cenozoic planktonic foraminifera

The $\text{Sr}\text{Ca}$ ratio and other parameters have been measured in fossil planktonic foraminifera from the Atlantic and Pacific Ocean basins in order to evaluate the $\text{Sr}\text{Ca}$ ratio of seawater during the last 75 million years. Results on well-preserved samples indicate that the ratio has increased to its present value by 10–15% during the Cenozoic, and that minima occurred between 55-45 Ma and 10-5 Ma, when the ratio was 15–25% less than at present. The long-term increase may reflect either decreasing deposition of aragonite with a high $\text{Sr}\text{Ca}$ ratio in shallow seas, or decreasing seafloor spreading rates and consequently decreasing hydrothermal supply of Ca during the Cenozoic. Other geologic evidence suggests that the Eocene minimum (near 50 Ma) may have resulted from increased aragonite sedimentation, while the Late Miocene minimum (between 10-5 Ma) may have been caused by an increased rate of seawater-basalt exchange when seafloor spreading rates increased on the East Pacific Rise near 10 Ma.