Preliminary Examination of How Human-driven Freshwater Flow Alteration Affects Trophic Ecology of Juvenile Snook (<Emphasis Type="Italic">Centropomus undecimalis</Emphasis>) in Estuarine Creeks     

Aaron J. Adams  R. Kirby Wolfe  Craig A. Layman 《Estuaries and Coasts》2009,32(4):819-828

Maintaining proper freshwater and marine inputs is essential for estuarine function. Alteration of freshwater flows into small tributaries that traverse the upland-estuarine margin may be especially problematic, e.g., by impacting the nursery areas for juvenile finfish and shellfish. We used stomach contents and stable isotope analysis (δ¹³C, δ¹⁵N) to examine effects of freshwater flow alterations on the trophic ecology of juvenile common snook (Centropomus undecimalis) in four mangrove creeks with different freshwater flow regimes. Diet diversity in less degraded creeks was greater than in more degraded creeks, and the importance (by % mass) of the top three preys was disproportionately higher in the more degraded creeks. Stable isotope measures of trophic diversity corroborate these trends, suggesting higher intraspecific trophic diversity in less degraded creeks. The difference in diet diversity of juvenile snook may be an indicator of an overall change in ecosystem function and these shifts in food web structure may affect the rate that juveniles of this and other species with similar habitat requirements successfully join the adult population.  相似文献   

A Landscape-Scale Assessment of Above- and Belowground Primary Production in Coastal Wetlands: Implications for Climate Change-Induced Community Shifts     

Camille L. Stagg  Donald R. SchoolmasterJr.  Sarai C. Piazza  Gregg Snedden  Gregory D. Steyer  Craig J. Fischenich  Robert W. McComas 《Estuaries and Coasts》2017,40(3):856-879

Above- and belowground production in coastal wetlands are important contributors to carbon accumulation and ecosystem sustainability. As sea level rises, we can expect shifts to more salt-tolerant communities, which may alter these ecosystem functions and services. Although the direct influence of salinity on species-level primary production has been documented, we lack an understanding of the landscape-level response of coastal wetlands to increasing salinity. What are the indirect effects of sea-level rise, i.e., how does primary production vary across a landscape gradient of increasing salinity that incorporates changes in wetland type? This is the first study to measure both above- and belowground production in four wetland types that span an entire coastal gradient from fresh to saline wetlands. We hypothesized that increasing salinity would limit rates of primary production, and saline marshes would have lower rates of above- and belowground production than fresher marshes. However, along the Northern Gulf of Mexico Coast in Louisiana, USA, we found that aboveground production was highest in brackish marshes, compared with fresh, intermediate, and saline marshes, and belowground production was similar among all wetland types along the salinity gradient. Multiple regression analysis indicated that salinity was the only significant predictor of production, and its influence was dependent upon wetland type. We concluded that (1) salinity had a negative effect on production within wetland type, and this relationship was strongest in the fresh marsh (0–2 PSU) and (2) along the overall landscape gradient, production was maintained by mechanisms at the scale of wetland type, which were likely related to plant energetics. Regardless of wetland type, we found that belowground production was significantly greater than aboveground production. Additionally, inter-annual variation, associated with severe drought conditions, was observed exclusively for belowground production, which may be a more sensitive indicator of ecosystem health than aboveground production.  相似文献   

Earth analog for high-latitude landforms and recent flows on Mars: Icy debris fans in the Wrangell Volcanic Field, Alaska     

R. Craig Kochel  Jeffrey M. Trop 《Icarus》2008,196(1):63-77

New Mars Reconnaissance Orbiter HiRise and CRISM imagery of polar layered terrain of Mars reveals striking similarities to icy debris fans along the base of steep escarpments in Alaska formed in high-latitude periglacial environments. Process and morphologic observations of a deglaciating site in the Wrangell Mountains reveal a complex suite of supraglacial processes involved in the construction of icy debris fans. Snow, ice, and sediment are delivered to the fans from degradation of an upper-level icecap. Alaskan icy debris fans were studied during an 8-day reconnaissance mission in July 2006. We directly observed 289 major depositional events dominated by dry snow/ice avalanches, but also including icy debris flows, rockfalls, small jokulhlaups, and glacial calving. Small fans with larger catchments receive episodic icy debris flows triggered by outburst flows that mobilize rockfall sediment temporarily stored in catchments above the fan apex. Large fans with smaller catchments have better linkage to the upper icecap, providing a direct pathway for frequent large avalanches. The large, avalanche-dominated fans thicken rapidly from an overabundance of snow/ice supply to the point where they become hybrid fan-glaciers. Surficial geology evolves rapidly in this high-latitude environment through both depositional events and solar-driven albedo changes that occur daily. Ground penetrating radar surveys show that subsurface sedimentary architecture and fan evolution is similar to the active surface processes and deposits observed on the fans. Direct field observations of active geomorphic processes provide unique insights on the pace and nature of high-latitude landscape evolution during climate changes on both planets.  相似文献   

Runoff generation in zero-order precambrian shield catchments: The stormflow response of a heterogeneous landscape     

Craig J. Allan  Nigel T. Roulet 《水文研究》1994,8(4):369-388

Hydrometric and isotopic (oxygen-18) observations were used to delineate the runoff processes operating in several headwater catchments on the Precambrian Shield of Canada. The catchments comprise patches of conifer forest situated on thin soils among areas of lichen-covered granitic bedrock. Horton overland flow occurred from the lichen-bedrock areas in all precipitation events that exceeded 4–6 mm. Runoff from the forest stands occurred mainly as subsurface stormflow, but in some instances saturation overland flow was observed. The occurrence of saturation overland flow was controlled by the topography of the bedrock beneath the forest soils. The area contributing runoff and the pathway by which water was conveyed to the catchment outflow switched from the open lichen-bedrock areas producing overland flow on the rising limb of the storm hydrograph to the forest stands contributing subsurface stormflow on the recession limb of the hydrograph. The areal extent and position of the landscape units in the basin were important to the rate and magnitude of stormflow production. Runoff was generated from the catchments only during and immediately after snowmelt and/or rainfall events. The catchments were dry and/or frozen for about 70% of the year.  相似文献   

High-resolution imaging of the radio continuum and neutral gas in the inner kiloparsec of the radio galaxy 3C 293     

R. J. Beswick  A. B. Peck  G. B. Taylor  G. Giovannini 《Monthly notices of the Royal Astronomical Society》2004,352(1):49-60

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Localization of the source of flare X-ray emission during the eclipse of 7 March, 1970     

R. W. Kreplin  R. G. Taylor 《Solar physics》1971,21(2):452-459

An occultation of X-ray emission from a solar flare occurred during the eclipse of 7 March, 1970 and was observed by an NRL instrument aboard the OSO-5 satellite. Ionization chamber photometers covering the wavelength ranges 0.5–3 Å, 1–8 Å, and 8–16 Å provided flux measurements once every 15 s providing a spatial resolution of 20 arc sec at the solar surface. Within this limitation the X-ray flare was observed to be confined within a region 136 000 km in one dimension.However, the measurements indicate the existence of a denser core 54 000 km wide in the direction of advance of the Moon's limb. Comparison of these results with X-ray photographs of flare regions are made and a model for the development of the soft X-ray flare is proposed.  相似文献   

Worldwide photometry and lightcurve observations of 1 Ceres during the 1975–1976 apparition     

E.F. Tedesco  R.C. Taylor  J. Drummond  D. Harwood  I. Nickoloff  F. Scaltriti  H.J. Schober  V. Zappala 《Icarus》1983,54(1):23-29

We present 19 lightcurves of asteroid 1 Ceres obtained during a global campaign in 1975–1976. The synodic period is 0.37812 ± 0.00004 day. The mean absolute V magnitude is 3.61 ± 0.03 and the phase coefficient is 0.40 ± 0.001 mag/deg. The U-B and B-V phase coefficients are +0.0015 ± 0.0007 and +0.0006 ± 0.0003 mag/deg, respectively. The colors at zero phase are B-V = +0.70 ± 0.01 and U-B = +0.41 ± 0.01.  相似文献   

Origin of granite batholiths: Geochemical evidence | M.P. Atherton and J. Tarney (Editors), 1979. Shiva Publishing,Kent, 148 pp., £4.50.     

S.R. Taylor 《Earth》1981,17(3):300-301

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Multiscale sources of spatial variation in soil. III. Improved methods for fitting the nested model to one-dimensional semivariograms     

C. C. Taylor  P. A. Burrough 《Mathematical Geology》1986,18(8):811-821

The previous paper in this series presented a one-dimensional stochastic nested model to account for superimposed sources of soil variation at various scales. This paper shows how the nested model can be fitted to experimental data using weighted or generalized least-squares methods that account for correlations between consecutive terms that had previously been neglected. This paper also presents a method of estimating effective degrees of freedom for each sampling interval and thus for estimating 90% confidence limits for the semivariogram of the nested model.  相似文献   

THE COMPOSITION OF THE CHASSIGNY METEORITE     

Brian Mason  J.A. Nelon  P. Muir  S.R Taylor 《Meteoritics & planetary science》1976,11(1):21-27

Spark source mass spectrometric analysis of the Chassigny meteorite has given the following data (in ppm): Rb 0.4, Sr 7.2, Y 0.64, Zr 1.5, Nb 0.32, Ba 7.1, La 0.39, Ce 1.12, Pr 0.13, Nd 0.54, Sm 0.11, Eu 0.038, Gd 0.11, Tb 0.02, Dy 0.12, Ho 0.03, Er 0.09, Yb 0.10, Pb 1.0, Th 0.057, U 0.021. These data, in conjunction with major element composition and mineralogical and textural features, indicate that this meteorite is an olivinerich cumulate, possibly genetically related to the nakhlites.  相似文献