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971.
Many Gulf of Mexico estuaries have low ratios of water volume to bottom surface area, and benthic processes in these systems
likely have a major influence on system structure and function. The purpose of this study was to determine the spatiotemporal
distribution of biomass and community composition of subtidal benthic microalgal (BMA) communities in Galveston Bay, TX, USA,
compare BMA community composition and biomass to phytoplankton in overlying waters, and estimate the potential contribution
of BMA to the trophodynamics in this shallow, turbid, subtropical estuary. The estimates of BMA biomass (mean = 4.21 mg Chl
a m−2) for Galveston Bay were within the range of the reported values for similar Gulf of Mexico estuaries. BMA biomass in the
central part of the bay was essentially homogeneous, whereas biomass at the seaward and upper bay ends of the transect were
significantly lower. Peridinin, fucoxanthin, and alloxanthin were the three carotenoids with the highest concentrations, with
fucoxanthin having the highest mean concentration (1.82 mg m−2). The seaward and landward ends of the transect differed from the central region of the bay with respect to the relative
abundances of chlorophytes, cyanobacteria, and photosynthetic bacteria. Benthic microalgal community composition also showed
a gradual shift over time due to changes in the relative abundances of photosynthetic bacteria, cryptophytes, dinoflagellates,
and cyanobacteria. Major changes in community composition occurred in the spring months (March to April). On an areal basis,
BMA biomass in Galveston Bay occurred at minor concentrations (16.5%) relative to phytoplankton. Furthermore, the concentrations
of carotenoid pigments for phytoplankton and BMA (fucoxanthin, alloxanthin, and zeaxanthin) were correlated (r = 0.48 to 0.61), suggesting a close linkage between microalgae in the water column and sediments. The contribution of BMA
to the primary productivity of the deeper waters (>2 m) of Galveston Bay is probably very small in comparison to shallower
waters along the bay margins. The significant similarities in the community composition of phytoplankton and BMA illustrate
the potential importance of deposition and resuspension processes in this turbid, shallow estuary. 相似文献
972.
Although the supply and fate of suspended sediment is of fundamental importance to the functioning and morphological evolution
of muddy estuaries, reliable sediment budgets have been established in only a few cases. Especially for smaller estuaries,
inadequate bathymetric surveys and a lack of intertidal sedimentation data often preclude estimation of the sediment budget
from morphological change, while instrument-derived residual fluxes typically lie well within the errors associated with measurement
of much larger gross tidal transports. Given suitably long-term records of continuously monitored suspended sediment concentration
(SSC), however, analysis of the major scales of variation in sediment transport and their relation to hydrodynamic and meteorological
forcing permits qualitative testing of hypotheses suggested by directly measured residual fluxes. This paper analyzes data
from a 1-year acoustic Doppler profiler deployment in the Blyth estuary, a muddy mesotidal barrier-enclosed system on the
UK east coast. Flux calculations indicate a small sediment import equivalent to just 1.5% of the gross flood tide transport.
Little confidence can be assigned to either the magnitude or direction of such a small residual when considered in isolation.
However, the inference that the sediment regime is finely balanced is qualitatively supported by the close similarity between
flood-tide and ebb-tide SSC values. Singular spectrum analysis of the SSC time series shows the expectedly large contributions
to the variance in SSC at intratidal and subtidal (semimonthly and monthly) scales but also picks out intermittent variability
that is initially attributed to a combination of non-tidal surge and wind stress forcing. Closer examination of the data through
cross-correlograms and event-scale analysis indicates that local meteorological forcing is the major factor. Acting through
the resuspension of intertidal mudflat sediments at times of strong westerlies, meteorological forcing is directly implicated
in episodic sediment export from the estuary. Thresholding of tide-averaged fluxes using a range of critical wind stress values
further indicates that ‘tide-dominated’ (i.e., low wind stress) and ‘wave-dominated’ (high wind stress) conditions are associated
with sediment import and export. Sediment balance is potentially sensitive to the frequency of high wind stress events, since
the associated sediment exports are several times larger than the average import under calm conditions. Intermittent meteorological
forcing may thus exert an important control on the sedimentary balance of otherwise tidally dominated muddy estuarine systems,
and the role of wind climate should not be overlooked in studies of estuary response to environmental change. 相似文献
973.
974.
Identifying Source Soils in Contemporary Estuarine Sediments: A New Compound-Specific Isotope Method 总被引:2,自引:0,他引:2
M. M. Gibbs 《Estuaries and Coasts》2008,31(2):344-359
A new method is proposed for the identification and apportionment of contemporary source soils contributing to estuarine sediments.
The method uses compound-specific isotopic analysis of naturally occurring biomarkers (fatty acids) derived from plants to
link source soils to land use within a single catchment. For identification and apportionment of source soils in the estuarine
samples, the method uses the isotopic mixing model, IsoSource. The feasible proportions obtained from IsoSource are then scaled
to allow for the percent organic carbon in the source soils. With this approach, the estimation of each source soil contribution
to a location in the estuary is independent of any degradation of the biomarkers through microbial or biogeochemical processes.
Identification relies on the evaluation of the sediment sample relative to a “library” of reference source soils from different
land use within the catchment. Selection of potential sources is geographically constrained by the requirement for a natural
linkage between each source soil and the sediment site sampled. A case study, using this method, mapped the distribution of
three main land use source soils (pasture, native forest, and pine forest) across the river delta in a small estuary fringed
with mangroves. Rather than being uniformly distributed, the results indicated that the source soil contributions varied markedly
across the delta, raising concerns about the validity of taking single cores to characterize the sediments of an estuary.
Coupling the source apportionment results with land use data indicated that the mean percent contribution of pine forest soil
in the river delta sediments was almost three times greater than the percent land use area of pine forest in the catchment.
Furthermore, isotopic signatures indicated that most of the pine forest soil came from the much smaller areas exposed to erosion
by clear cut harvesting and that the soil contribution from recently harvested areas of pine forest could be as much as 20
times greater than that land use area in this catchment. This is the first method that can identify and apportion, by land
use on a catchment scale, the sources of soil contributing to the sediment at a location of an estuary. The results are given
as a “best estimate”, within definable limits, of the proportional contribution of each potential source soil. Information
obtained using this method will allow development of management strategies to alter land use practices to reduce the sediment
load to rivers, and thus, the impact on the aquatic ecosystem downstream in estuaries. 相似文献
975.
We developed light requirements for eelgrass in the Pacific Northwest, USA, to evaluate the effects of short- and long-term
reductions in irradiance reaching eelgrass, especially related to turbidity and overwater structures. Photosynthesis-irradiance
experiments and depth distribution field studies indicated that eelgrass productivity was maximum at a photosynthetic photon
flux density (PPFD) of about 350–550 μmol quanta m−2 s−1. Winter plants had approximately threefold greater net apparent primary productivity rate at the same irradiance as summer
plants. Growth studies using artificial shading as well as field monitoring of light and eelgrass growth indicated that long-term
survival required at least 3 mol quanta m−2 day−1 on average during spring and summer (i.e., May-September), and that growth was saturated above about 7 mol quanta m−2 day−1. We conclude that non-light-limited growth of eelgrass in the Pacific Northwest requires an average of at least 7 mol quanta
m−2 day−1 during spring and summer and that long-term survival requires a minimum average of 3 mol quanta m−2 day−1. 相似文献
976.
Cambrian explosion: Birth of tree of animals 总被引:5,自引:5,他引:0
Excluding the sponges the Kingdom Animalia is usually divided into three subkingdoms: Diploblasta, Protostomia and Deuterostomia. The Cambrian Explosion consists of three major episodes, two of which were in the early Early Cambrian (one represented by the small skeletal fossils “SSFs” at the base of the Cambrian and the other represented by the succeeding Chengjiang faunas “CFs”), and the other episode as their prelude took place in the “Eocambrian” (i.e. the latest Precambrian), represented by the Ediacaran faunas. This unique Big Bang of life has been recognized as giving birth to the entire morphological Tree Of Animals (or metazoans), in short the TOA. Its “seed” in the deep Precambrian, represented by some sort of protist from which the complete TOA must have grown, remains unknown paleontologically. However, the fossil evidence suggests that the three major episodes of the Cambrian Explosion are responsible for the earliest radiations of the three subkingdoms of animals respectively. While the observed Ediacaran fauna might constitute only a small part of the whole Ediacaran biota, our evidence supports that it was dominated by diploblasts (the “trunk” of the TOA) with only a few possible stem-group triploblasts. The Early Cambrian in turn in two phases explosively yielded almost all the major triploblastic crown-branches (Bilateria: the huge “crown” of the TOA), which include the other two subkingdoms: first the extremely diverse protostomes in the Meishucunian Age and then followed by a nearly entire lineage of early deuterostomes from the Chengjiang, including even its most derived member – the earliest true vertebrates. Among the four most significant milestones of morphological origins and radiations in animal history, the first one (i.e. appearance of metazoans) took place in the Ediacaran Period or earlier times, and the other three can be seen in the windows available from the Chengjiang and the Meishucunian fossil assemblages. The newly discovered extinct Phylum Vetulicolia, which has primitively segmented body with simple gill slits in its anterior division, most probably represents one of the roots of the deuterostome subkingdom. Showing a mosaic of basic features possessed in both the bilateral vetulicolians and some primitive echinoderms, the soft-bodied vetulocystids are best regarded as one of the roots of the extant pentamerous echinoderms. Standing on the “top” of the deuterostome super-branch in the early Cambrian TOA are the “the first fish” Myllokunmingia and Haikouichthys, which bear paired eyes and salient proto-vertebrae. These animals represent the real root of the remainder of the vertebrates or craniates. On the contrary, yunnanozoans, including Yunnanozoon and Haikouella, possess neither eyes nor unequivocal vertebrae, and may have nothing to do with the craniates, let alone the vertebrates. Those enigmatic creatures share a similar body-plan with vetulicolians and should be treated as a side-branch within the lower deuterostomes. 相似文献
977.
N. G. Patyk-Kara E. N. Levchenko A. I. Stekhin V. V. Barsegyan A. A. Bochneva I. A. Chizhova E. A. Andrianova V. T. Dubinchuk 《Geology of Ore Deposits》2008,50(3):218-239
The study of mineral assemblages at the Central deposit allowed us to substantially refine the evolutionary model of the deposit and reveal the two main factors that control the variability of its mineralic space: (1) heterogeneity of the ore layer, consisting of a sublittoral bottom placer (the lower part) and a subaerial dune complex partly reworked in the course of a new transgression (the upper part), and (2) postore epigenetic alteration of the ore constituent of sands, which affected the quality of ore concentrates. The results obtained will be used in geological and technological mapping and development of the production program. 相似文献
978.
O. G. Den 《Astronomy Reports》2008,52(11):931-936
We analyze the flare events of October 28 and May 27, 2003 to examine the possible connection of solar flares with singularities in the differential characteristics of solar magnetic fields. The relation between flares and the behavior of F indicators (which describe structural singularities of the magnetic fields) introduced earlier is analyzed. It is shown that the generation of flares can be associated with self-intersections (or reconnection) of the F = 0 curves, where magnetic reconnection can occur. Consequently, the current sheets generated in such regions can be sources of energy release. 相似文献
979.
It is shown that the centroid of the heliospheric equator undergoes quasi-periodic oscillations. During the minimum of the 11-year cycle, the centroid shifts southwards (the so-called bashful-ballerina effect). The direction of the shift reverses during the solar maximum. The solar quadrupole is responsible for this effect. The shift is compared with the tilt of the heliospheric current sheet. 相似文献
980.
The central magnetic field and rotation of the solar radiative zone are responsible for corrections to the g-mode frequencies. Magnetogravitational spectra are calculated analytically in a simple one-dimensional MHD model that goes beyond the WKB approximation and avoid any cusp resonances that trap the wave within the radiative zone in the presence of a weak magnetic background. The calculations are compared with spacecraft observations of the 1% frequency shifts for candidate g-modes found in the SOHO GOLF experiment. The magnetic correction is the main contribution for a strong magnetic field satisfying the approximation used. It is shown that a constant magnetic field of 700 kG in the radiative zone provides the required frequency shift for the n = ?10 g-mode. The rotational correction, which is due to the Coriolis force in the one-dimensional model used, is much less than a percent (αΩ ≤ 0.003). 相似文献