The effect of aquaculture practices on the benthic macroinvertebrate community of a lagoon system in the Bay of Cádiz (southwestern Spain)

Monthly quantitative Ekman-Birge grab sampling was used to characterize and compare the composition and structure of the benthic macroinvertebrate community inhabiting semi-enclosed polyculture lagoons (SPL) (three sampling sites) and enclosed monoculture ponds (EMP) (two sampling sites) of a lagoonal system of the Bay of Cádiz. The two areas differed considerably in habitat characteristics and aquaculture management. The SPL area was characterized by low rates of water exchange, low fish densities, and the presence of a macroalgal cover. In the EMP area, there was a complete exchange of water daily (by pumping) and a supply of food pellets, density of fish was high, and no vegetative cover was present. There were considerable differences in species composition between habitats with different culture methods: 11 of the 21 most abundant species were exclusive to one or the other. Several epibenthic species were abundant in the polyculture lagoon but were low in density or were absent in monoculture ponds. Some infaunal species, on the other hand, were more abundant in the monoculture ponds. Univeriate measures of community structure (abundance and biomass, Margalef’s species richness, Shannon-Wiener diversity, and Pielou’s evenness indices) did not indicate significant differences between the SPL and EMP areas. Conversely, the abundance-biomass comparison (ABC) method indicated that, on average, the macrobenthic community was moderately disturbed in the SPL and undisturbed in the EMP areas. Multidimensional scaling (MDS) ordination and hierarchical cluster analysis (Bray-Curtis similarity measure) revealed the occurrence of two main benthic assemblages that corresponded to the aquaculture methods. The different rates of water exchange for the two aquaculture practices seem to have contributed to differences in the composition and structure of the benthic communities.     

Depositional fabrics in basal till reflect alignments during transportation

The fabrics of tills deposited by continental glaciers are usually assumed to reflect clast orientation during transportation and yet might only be imprinted during depositional processes. However, the striated surfaces of clasts must be acquired during transportation and by relating striation patterns to clast shape one can deduce the positions most frequently maintained by each group of clasts. Comparison of these orientations with the actual depositional fabrics of the same shape groups, demonstrates that dast orientations are maintained from transportation through deposition. Therefore subglacial transportation processes grade smoothly into those of deposition. The favoured interpretation is that bottom melting is the dominant mechanism leading to final deposition and that lodgement and smearing are likely restricted more to preliminary cycles of redeposition and re-erosion.     

Composition and evolution of the eucrite parent body: evidence from rare earth elements

Eucrites are extraterrestrial plagioclase-pigeonite basalts. Experimental studies suggest that they were produced by partial melting of an olivine (Fo₆₅)-pigeonite (Wo₅En₆₅)-plagioclase (An₉₄)-spinel-metal source region. Quantitative modeling of the evolution of REE abundances in the eucrites indicates that the main group of eucrites (e.g. Juvinas) may be produced by approximately 10% equilibrium partial melting of a source region with initial REE abundances which were chondritic relative and absolute. Other eucrites appear to represent greater (e.g. Sioux County—15%) or smaller (e.g. Stannern—4%) degrees of melting. Moore County and Serra de Magé appear to be cumulates of pyroxene and plagioclase produced by fractional crystallization of a Juvinas-like melt. Nuevo Laredo may represent a residual liquid after such fractional crystallization. Our calculations are consistent with the conclusion that the eucrites were derived from a single type of source region. The close correspondence of the age of the eucrites (? 4.6 AE) to the age of the solar system appears to preclude the possibility of extensive chemical differentiation of the eucrite parent body prior to the event which produced the eucritic melts. Thus our calculations have yielded not only the mode of the source region but, assuming homogeneous accretion, the mode and hence the bulk composition of the eucrite parent body as well. We are unable to estimate quantitatively the ratio of metal to olivine in the parent body. If no metal is present, the bulk composition (in oxide wt%) is Na₂O—0.04, MgO—29.7, Al₂O₃—1.8, SiO₂—39.0, CaO—1.2, FeO—28.3. If, in contrast, the parent body contained 30% metal, the bulk composition of the silicate portion of the eucrite parent body is Na₂O—0.06, MgO—28.0, Al₂O₃—2.6, SiO₂—41.3, CaO—1.9, FeO—26.3. Relative abundances of the meteorites suggest that the eucrite parent body is still intact. The solar system object most closely resembling the eucrites is asteroid 4 Vesta. Because Vesta is unique among the asteroids, we have license to conclude that it is the source of the eucrites and its bulk composition is close to the analyses given above.     

Quantitative microautoradiography by X-ray emission micro-analysis

Silver concentration in developed photographic emulsions exposed by β-emission may be measured on spots with a minimum diameter of about 10μm using an electron microprobe or a scanning electron microscope. Silver concentration is directly proportional to the integrated flux of β-particles bombarding the emulsion. Thus analysis for silver provides a method for quantitative microautoradiography which is comparable in accuracy and precision to other available methods and which can be performed on readily available equipment.     

The metal content of the eucrite parent body: constraints from the partitioning behavior of tungsten

The solid metal/silicate melt partition coefficient for W has been determined experimentally to have a value of 25 ± 5 at 1190°C and an oxygen fugacity of 10^?13.4, the temperature and oxygen fugacity conditions at which eucritic basalts formed. Given this partition coefficient, scenarios for the metal content and evolution of the eucrite parent body (EPB) are constructed to explain the reduction by a factor of 30, relative to the chondrites, of the $\text{W}\text{La}$ ratio in the eucrites.A possible model for the early geologic history of the EPB begins with accretion of a parent body, chondritic in composition with respect to nonvolatile siderophile and lithophile elements. The solid metal content was between 2% and 10%, which is within the range observed in the ordinary chondrites. Subsequent heating of the EPB caused the metal phase to separate and become isolated from the silicate phases before the degree of partial melting of the silicates reached 4% to 5%. Equilibrium partitioning of most of the W into the solid metal phase at low degrees of partial melting reduced the $\text{W}\text{La}$ ratio in the remaining silicates. Continued partial melting of the silicates generated primary eucritic magmas which recorded the reduced $\text{W}\text{La}$ ratio.     

Equivalence of equations describing trace element distribution during equilibrium partial melting

The mathematical equivalence of several equations used to calculate the evolution of trace element abundances during equilibrium partial melting is demonstrated.     

Airflow pattern and droplet trajectories about an electrostatic cloud droplet probe

Summary This study considers the numerical results for the airflow pattern to obtain droplet trajectories around and into a leading edge hole of a cloud droplet sampling probe. The probe was initially conceived at MIT and developed into a practical airborne system in the Cloud Physics Program at the National Center for Atmospheric Research. The probe is designed to be an ellipsoid of revolution with a circular sampling hole at the forward stagnation point. The external flow field is assumed to be steady, axisymmetric, irrotational and incompressible and depends on four parameters: the hole radius, axial speed in the hole, free stream velocity and the fineness ratio of the ellipsoid. The trajectory calculations are based on a three-dimensional gravity field with a fluid resistance computed from experimental drag coefficients on spheres. Both numerical and theoretical solutions for the flow field have been obtained for various combinations of the above parameters. For these flow fields, trajectories for droplets have been obtained. From the trajectory calculations we have obtained collection efficiencies for the probe and have compared these trajectories with experimental trajectories obtained at NCAR.The National Center for Atmospheric Research is sponsored by the National Science Foundation.     

Effect of elevated CO2 on carbon pools and fluxes in a brackish marsh

The effects of long-term exposure to elevated atmospheric CO₂ (ambient + 340 ppmv) on carbon cycling were investigated for two plant communities in a Chesapeake Bay brackish marsh, one dominated by the C₃ sedgeSchoenplectus americanus and the other by the C₄ grassSpartina patens. Elevated CO₂ resulted in a significant increase in porewater concentrations of DIC at 30 cm depth (p < 0.1). The CO₂ treatment also yielded increases in DOC (15 to 27%) and dissolved CH₄ (12–18%) in the C₃ marsh (means for several depths over the period of June 1998 and June 1999), but not at a significant level. Elevated CO₂ increased mean ecosystem emissions of CO₂ (34–393 g C m⁻² yr⁻¹) and CH₄ (0.21–0.40 g C m⁻² yr⁻¹) in the C₃ community, but the effects were only significant on certain dates. For example, CO₂ enrichment increased C export to the atmosphere in the C₃ community during one of two winter seasons measured (p = 0.09). In the C₄ community, gross photosynthesis responded relatively weakly to elevated CO₂ (18% increase, p > 0.1), and the concomitant effects on dissolved carbon concentrations, respiration, and CH₄ emissions were small or absent. We concluded that elevated CO₂ has the potential to increase dissolved inorganic carbon export to estuaries.     

Community succession along a chronosequence of vegetation restoration on sand dunes in Horqin Sandy Land

Species diversity influences plant community structure and function. This paper examines the patterns and dynamics of species diversity along a chronosequence of vegetation recovery on sand dunes in a semi-arid region to assess the probability of vegetation recovery via succession, and provides some implications for revegetation practices in this region. Species richness and diversity indices gradually increased with succession, except for a decline in the community of 18 years, which is attributed to the strong dominance of Artemisia halodendron. In each stage of the restoration process, there was a dominant species with particular life history traits which contribute to the dominance of this species. Species replacement and habitat changes were the main drivers of succession, while plant species and community succession drove the process of vegetation recovery. Results showed that restoration via succession holds promise for vegetation recovery and desertification control within protected, fenced enclosures.     

Salt ramps: Wind-induced depositional features on Tunisian playas

Semicircular and crescent-shaped accumulations of salt crystals developed on salt crusts were measured on three Tunisian playas in September 1990. These features have been termed salt ramps. Their morphology and chemistry suggest that they are formed in the late stages of shallow ephemeral lake desiccation in playa basins. They form by salt precipitation from shallow brine lakes that are blown across salt-encrusted playa surfaces by the wind. Moreover, they appear to be short-lived features and their degradation is related to the flooding of playas with less saline water, and possibly rainfall and deflation.