Galveston Bay: Temporal changes in the concentrations of trace organic contaminants in national status and trends oysters (1986–1994)

The temporal distributions for six classes of trace organic contaminants (chlordanes, DDTs, dieldrin, PAHs, PCBs, and butyltins) in oysters from six Galveston Bay sites from National Oceanic and Atmospheric Administration’s National Status and Trends (NS&T) Mussel Watch Program are compared with other NS&T sites from the Gulf of Mexico as well as all NS&T sites of the United States (East Coast, West Coast, and Gulf of Mexico). Decreases in the median for the Gulf-wide concentration of chlordanes, dieldrin, and butyltins occurred during 1986–1994. The Gulfwide median concentrations of DDTs, PAHs, and PCBs exhibited a strong cyclic distribution with time. For Galveston Bay oysters, “high” concentration is defined as the concentration greater than the median plus one standard deviation for all Gulf of Mexico sites. The percentage of sites having high concentrations during 1986–1994 for Galveston Bay oysters are 49% for dieldrin, 45% for butyltins, 40% for chlordanes, 38% for PCBs, 30% for PAHs, and 21% for DDTs. For PCBs, 43% of Galveston Bay oyster samples analyzed over the first 9 yr have concentrations high enough for potential biological effects to be observed in oysters. The percentages in other agents were chlordanes (22%), butyltins (22%), dieldrin (5%), and PAHs (4%). National Academy of Science-proposed regulatory limits for oysters were exceeded in only 2% of Galveston Bay samples for DDTs and 1% for PCBs. All other contaminants were below proposed NAS limits.     

An ultraviolet-selected galaxy redshift survey: new estimates of the local star formation rate

We present the first results of an ongoing spectroscopic survey of galaxies selected in the rest frame ultraviolet (UV). The source catalogue has been constructed from a flux-limited sample of stars, galaxies and QSOs imaged at 2000 Å in Selected Area 57 with the FOCA balloon-borne imaging camera. Accurate positions for the UV sources have been obtained by matching with optical counterparts using APM scans of the Palomar Sky Survey limited at B   20.5. Here we present results derived from optical spectroscopy conducted with the WIYN telescope and the WHT for 142 faint sources. The redshift distribution for this UV-selected sample extends over 0 <  z  < 0.5, and a high fraction of the sources show intense nebular emission lines and UV–optical colours bluer than normal Hubble sequence galaxies. Such UV-selected surveys are thus a very efficient way to locate and study intermediate-redshift galaxies undergoing intense star formation. Although our sample is currently small, we derive a rest frame UV luminosity function with a steep faint-end slope consistent with that found for late-type galaxies in optical samples. However, the integrated luminosity density derived implies a volume-averaged star formation rate higher than other recent estimates, assuming a normal initial mass function. If representative of other UV fields, as suggested by UV number count studies, our data imply that the local abundance of star-forming galaxies may have been underestimated, and consequently claims for strong evolution in the global star formation rate in the range 0 <  z  < 1 overstated. An intensive study of a large UV-selected sample is likely to reveal important information on the declining population of star-forming galaxies of all types.     

Tourmaline-rich Rocks Associated with the Submarine Hydrothermal Rosebery Zn-Pb-Cu-Ag-Au Deposit and Granites in Western Tasmania,Australia

Summary The stratiform massive Zn-Pb sulphide Rosebery deposit of western Tasmania is hosted by metamorphosed deformed acid volcanics and sediments of the Cambrian Mt. Read Volcanics. Tourmalinite, a boron-rich siliceous sulphide facies iron formation, overlies and occurs as an exhalite facies equivalent of the massive sulphides. The orebody is partially replaced by post deformation tourmaline-bearing pyrrhotite-pyrite rocks associated with an alteration facies comprising magnetite-pyrite-tourmaline-phlogopite and the host metavolcanics are transgressed by quartz-tourmaline veins and tourmaline-filled joints. Tourmalinite and tourmaline in alteration zones are associated with other base metal deposits in the area. Tourmaline also occurs as fault-fill and in granitic rocks and associated Sn-W mineralization nearby. Tourmaline associated with the Cambrian massive sulphides is schorl > dravite in contrast to schorl in the Devonian granites.It is suggested that boron was an integral part of the ore fluids at Rosebery which precipitated tourmaline in exhalites immediately after and distal to the mineralization event. Tourmaline from the tourmalinite exhalites appears to have derived from submarine hydrothermal precipitation. Joint- and fracture-fill tourmaline could have derived from remobilization from tourmalinites during Devonian tectonism, however, it is more probable that these discordant tourmaline-bearing veins, tourmaline in the post-cleavage Rosebery Fault and tourmaline-bearing pyrrhotite-pyrite replacement of the Rosebery orebody derived from Devonian granite at a shallow depth which has been intersected in drilling. Tourmaline replacement associated with discordant structures is no different in composition from that from tourmalinites associated with the orebody and hence has undergone re-equilibration with the host rocks during multiple events of deformation and metamorphism associated with Devonian tectonism. In contrast, the composition of tourmaline from the Devonian granites is markedly different from that of the Rosebery area.

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Zusammenfassung Die stratiforme, massive Zn-Pb-Sulfidlagerstätte Rosebery in West-Tasmanien sitzt in metamorphen und deformierten sauren Vulkaniten und Sedimenten der Kambrischen Mt. Read Vulkanit-Serie auf. Turmalingesteine treten im Hangenden dieser Serie auf. Sie stellen eine Bor-reiche Eisenformation in silizuiumreicher Sulfidfazies dar und sind als das exhalative Äquivalent der massiven Sulfide anzusehen. Der Erzkörper wird teilweise von postdeformativen Turmalin-fährenden Pyrrhotin-Pyrit-Gesteinen verdrängt, die mit einer Alterationsfazies, bestehend aus Magnetit-Pyrit-Turmalin-Phlogopit, assoziiert sind. Die erzfährenden Metavulkanite werden von Quarz-Turmalin-Gängen und Turmalinadern durchschlagen. Turmalingesteine wie auch Turmalin in Alterationszonen kommen auch mit anderen Buntmetall-Vererzungen des Arbeitsgebietes vor. Turmalin tritt weiters in Störungszonen, in Graniten und in an diese gebundenen Sn-W Mineralisationen auf.Der mit den kambrischen, massiven Vulkaniten assozierte Turmalin ist ein Schörl > Dravit, während in den devonischen Graniten Schörl dominiert. Es ist anzunehmen, daß Bor einen integralen Anteil der Erzlösungen in der Rosebery-Lagerstätte darstellt. Aus diesen ist Turmalin exhalativ, kurz nach der Sulfidmineralisation distal gebildet worden. Es zeigt sich, daß der Turmalin aus submarin hydrothermalen Absätzen herzuleiten ist. Gangturmaline könnten durch Remobilisation der Turmalingesteine während devonischer Deformation entstanden sein. Es scheint jedoch wahrscheinlicher, daß diese diskordanten Gänge, wie auch der Turmalin in der Rosebery-Störung und die Turmalin-führenden Pyrrhotin-Pyrit-Verdrängungen aus dem devonischen Granit stammen. Verdrängter Turmalin, assoziiert mit diskordanten Strukturen, zeigt in seiner Zusammensetzung keinerlei Unterschiede zum Turmalin in Turmalingesteinen aus dem Erzkörper. Im Zuge mehrphasiger, devonischer Deformation und Metamorphose ist es somit zu Reäquilibrierung des Turmalins mit dem Trägergestein gekommen. Die Zusammensetzung des Turmalins in den devonischen Graniten unterscheidet sich deutlich von der des Rosebery-Gebietes.

     

Accuracy of cosmogenic ages for moraines

Analyses of all published cosmogenic exposure ages for moraine boulders show an average age range of 38% between the oldest and youngest boulders from each moraine. This range conflicts with the common assumption that ages of surface boulders are the same as the age of the landform. The wide spread in boulder ages is caused by erosion of the moraine surface and consequent exhumation of fresh boulders. A diffusion model of surface degradation explains the age range and shows that a randomly sampled small set of boulders (n = 3-7) will always yield a lower age limit for the moraine. The model indicates that for identical dating accuracy, six to seven boulders are needed from old and tall moraines (40,000-100,000 yr, 50-100 m initial height) but only one to four boulders from small moraines (20,000-100,000 yr, 10-20 m). By following these guidelines the oldest obtained boulder age will be ≥90% of the moraine age (95% probability). This result is only weakly sensitive to a broad range of soil erosion rates. Our analysis of published boulder ages indicates that <3% of all moraine boulders have prior exposure, and 85% of these boulders predate the dated moraine.     

Biostratigraphy,sedimentology and palaeobathymetry of Waulsortian buildups and peri-Waulsortian rocks during the late Tournaisian regression,Dinant area,Belgium

Recent revision of the biostratigraphy allows the recognition of a stratigraphic entity (here termed Freyrian) between the base of the Moliniacian stage and the base of the Viséan and simplifies sedimentological interpretation of late Tournaisian events around Dinant, in Belgium. Petrographic analysis of Freyrian rocks in Waulsortian buildups and peri-Waulsortian facies reveals a pattern of carbonate sedimentation related to the submarine topography developed by the buildups, and to sea-level changes. Graded beds and thin layers of grainstone in the predominantly fine-grained peri-Waulsortian sediments represent influxes derived mainly from nearby buildups during a period of shallowing. Using the sequence of foraminiferan assemblages which colonized the buildups as a stratigraphic scale, the earlier influxes are shown to have occurred only close to the presumed source, whereas later influxes extended further and marked the culmination of the shallowing phase. Deposition during the latter part of the Freyrian appears to have occurred in rather deeper, less disturbed water. The Moliniacian and Viséan boundary stratotypes, both in peri-Waulsortian facies, are critically assessed because almost all the stratigraphically useful foraminiferans occur in the rare grainstones resulting from sediment influxes. Tetrataxis was one of the few foraminiferans to colonize proximal peri-Waulsortian areas and appears to have ranged to a water depth of about 200 m. Downslope diachronism of colonization is interpreted as evidence of a sea-level fall of about 140 m and is used to draw a sea-level curve for this late Tournaisian regression. Using the same depth scale, microbial coating extended to about 300 m and its development appears to have been related to low sedimentation rates rather than photic conditions. © 1997 John Wiley & Sons, Ltd.     

Scenario Evaluator for Electrical Resistivity Survey Pre‐modeling Tool

Geophysical tools have much to offer users in environmental, water resource, and geotechnical fields; however, techniques such as electrical resistivity imaging (ERI) are often oversold and/or overinterpreted due to a lack of understanding of the limitations of the techniques, such as the appropriate depth intervals or resolution of the methods. The relationship between ERI data and resistivity is nonlinear; therefore, these limitations depend on site conditions and survey design and are best assessed through forward and inverse modeling exercises prior to field investigations. In this approach, proposed field surveys are first numerically simulated given the expected electrical properties of the site, and the resulting hypothetical data are then analyzed using inverse models. Performing ERI forward/inverse modeling, however, requires substantial expertise and can take many hours to implement. We present a new spreadsheet‐based tool, the Scenario Evaluator for Electrical Resistivity (SEER), which features a graphical user interface that allows users to manipulate a resistivity model and instantly view how that model would likely be interpreted by an ERI survey. The SEER tool is intended for use by those who wish to determine the value of including ERI to achieve project goals, and is designed to have broad utility in industry, teaching, and research.     

Laboratory and theoretical evaluation of impact of packing density,particle shape,and uniformity coefficient on erodibility of coarse-grained soil particles

Sedimentation – including erosion, transport, and deposition of coarse-grained particles – is a primary and growing environmental, engineering, and agricultural issue around the world. Soil erosion occurs when the hydrodynamic force induced by flowing water exceeds the geotechnical resistance of soils, as measured by critical shear stress for initiation of soil-particle motion. Even though various quantitative methods have been suggested with respect to different types of soil, the most widely accepted formula to estimate critical shear stress for coarse-grained soil is a direct function of the median grain size of the soil particles; however, the erosion resistance of soils also varies with other geotechnical properties, such as packing density, particle shape, and uniformity coefficient. Thus, in this study, a combined rolling–lift model for particle detachment was derived based on theoretical analysis. A series of experimental flume tests were conducted with specimens prepared with standard soil types, as well as laboratory-prepared mixtures of coarse-grained soil to validate the theoretical model and determine the effect of other geotechnical properties on the erosion characteristics of coarse grains, coupled with the effect of median particle size. The results indicated that the median grain size is the primary variable determining the resistance of coarse grains, but the critical shear stress also varies with the packing density of the soil matrix. In addition, angular particles show more erosion resistance than rounded particles, and the erosion potential of a soil decreased when the grain is well graded (higher value of uniformity coefficient). Additionally, regression analysis was performed to quantify the effect of each parameter on the critical shear stress of coarse grains. © 2020 John Wiley & Sons, Ltd.