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J. C. Kurtz N. D. Detenbeck V. D. Engle K. Ho L. M. Smith S. J. Jordan D. Campbell 《Estuaries and Coasts》2006,29(1):107-123
Coastal ecosystems are ecologically and commercially valuable, productive habitats that are experiencing escalating compromises
of their structural and functional integrity. The Clean Water Act (USC 1972) requires identification of impaired water bodies
and determination of the causes of impairment. Classification simplifies these determinations, because estuaries within a
class are more likely to respond similarly to particular stressors. We reviewed existing classification systems for their
applicability to grouping coastal marine and Great Lakes water bodies based on their responses to aquatic stressors, including
nutrients, toxic substances, suspended sediments, habitat alteration, and combinations of stressors. Classification research
historically addressed terrestrial and freshwater habitats rather than coastal habitats. Few efforts focused on stressor response,
although many well-researched classification frameworks provide information pertinent to stressor response. Early coastal
classifications relied on physical and hydrological properties, including geomorphology, general circulation patterns, and
salinity. More recent classifications sort ecosystems into a few broad types and may integrate physical and biological factors.
Among current efforts are those designed for conservation of sensitive habitats based on ecological processes that support
patterns of biological diversity. Physical factors, including freshwater inflow, residence time, and flushing rates, affect
sensitivity to stressors. Biological factors, such as primary production, grazing rates, and mineral cycling, also need to
be considered in classification. We evaluate each existing classification system with respect to objectives, defining factors,
extent of spatial and temporal applicability, existing sources of data, and relevance to aquatic stressors. We also consider
classification methods in a generic sense and discuss their strengths and weaknesses for our purposes. Although few existing
classifications are based on responses to stressors, may well-researched paradigms provide important information for improving
our capabilities for classification, as an investigative and predictive management tool. 相似文献
3.
ABSTRACTOil spill forecast modelling is typically used immediately after a spill to predict oil dispersal and promote mobilisation of more effective response operations. The aim of this work was to map oil dispersal after the grounding of the MV Rena on Astrolabe Reef and to verify the results against observations. Model predictions were broadly consistent with observed distribution of oil contamination. However, some hot spots of oil accumulation, likely due to surf-zone and rip current circulation, were not well represented. Additionally, the model was run with 81 differing wind conditions to show that the events occurring during the grounding represented the typical likely behaviour of an oil spill on Astrolabe Reef. Oil dispersal was highly dependent on prevailing wind patterns; more accurate prediction would require better observations of local wind patterns. However, comparison of predictions with observations indicated that the GNOME model was an effective low-cost approach. 相似文献
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We present numerical models based on realistic treatment of the intensity spectrum (from model atmospheres), and demonstrate that they are consistent with Kurtz and Medupe's recent formula in showing that limb darkening is too small an effect to explain the observed sharp decline of pulsation light amplitude with wavelength in rapidly oscillating Ap stars. Kurtz and Medupe's formula is shown to be a special form of Watson's earlier general formula for non-radial light variations of a star pulsating in any mode ( l m ). Using a technique suggested by Kurtz and Medupe we derive temperature semi-amplitude as a function of depth in the atmospheres of α Cir and HR 3831, assuming that we can neglect non-adiabatic effects. 相似文献
7.
Various waterborne anthropogenic contaminants disrupt the endocrine systems of wildlife and humans, targeting reproductive pathways, among others. Very little is known, however, regarding the occurrence of endocrine disruptive activity in South African freshwater ecosystems, and coastal ecosystems have not been studied in this regard. In a first attempt to investigate endocrine disruptive activity in South African coastal waters, surface water samples collected from harbours, river mouths and estuaries in three metropolitan municipalities, eThekwini (which includes Durban), Nelson Mandela (specifically Port Elizabeth Harbour) and City of Cape Town, were screened for (anti) oestrogenicity and (anti)androgenicity using recombinant yeast bioassays. Moreover, levels of the female hormone 17β-(o)estradiol (E2) were determined in all samples, as well as a selection of hydrocarbons in the eThekwini samples. A high proportion of samples collected from eThekwini were oestrogenic, whereas none from Port Elizabeth Harbour and only a single river mouth sampled in the City of Cape Town were oestrogenic. E2 was detected in all the samples tested, but at higher concentrations at the eThekwini and City of Cape Town localities than Port Elizabeth Harbour. In addition, the recombinant yeast assays revealed that anti-androgenicity was widespread, being detected in the majority of samples screened apart from those representing Port Elizabeth Harbour. Conversely, no anti-oestrogenic or androgenic activity was detected. Anti-androgenicity did not associate with hydrocarbon loads, providing evidence that other anti-androgens were responsible for the observed activity. The present data suggest potential reproductive disruption in marine and estuarine fauna inhabiting the eThekwini and City of Cape Town regions. 相似文献
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S. V. Kalenskii S. Kurtz V. I. Slysh P. Hofner C. M. Walmsley L. E. B. Johansson P. Bergman 《Astronomy Reports》2010,54(10):932-939
We present the results of VLA observations of a maser candidate in the low-mass star formation region L1157 in the 70-61
A
+ transition at 44 GHz. The line is emitted by a compact, undoubtedly maser source associated with clump B0a, which is seen
in maps of L1157 in thermal lines of methanol and other molecules. A much weaker compact source is associated with clump B1a,
which is brighter than B0a in thermal methanol lines. The newly detected masers may form in thin layers of turbulent post-shock
gas. In this case, the maser emission may be beamed, so that only an observer located in or near the planes of the layers
can observe strong masers. On the other hand, the maser lines are double with a “red” asymmetry, indicating that the masers
may form in collapsing clumps. A detailed analysis of collapsing-cloud maser models and their applicability to the masers
in L1157 will be developed in subsequent papers. 相似文献
9.
The rapidly oscillating Ap (roAp) stars currently represent the only main sequence stars other than the Sun which exhibit non-radial acoustic pulsations of high overtone. This makes them excellent subjects for asteroseismology, an approach which promises to yield accurate knowledge of the interior structures of stars. Of the 27 known roAp stars, 24 were discovered in Sutherland despite extensive searches conducted elsewhere. This paper reviews the discovery of the roAp phenomenon and describes the factors that contribute to the high discovery rate for these stars at Sutherland. Two long-term observational projects in progress at Sutherland are discussed,viz. the Cape roAp Star Survey and long-term monitoring of frequency variations in roAp stars. 相似文献
10.
Guenther Eichhorn Alberto Accomazzi Carolyn S. Grant Michael J. Kurtz Stephen S. Murray 《Astrophysics and Space Science》2002,282(1):299-340
The Astrophysics Data System (ADS) provides access to the astronomical literature through the World Wide Web. It is a NASA
funded project and access to all the ADS services is free to everybody world-wide. The ADS Abstract Service allows the searching
of four databases with abstracts in Astronomy, Instrumentation, Physics/Geophysics, and the LANL Preprints with a total of
over 2.2 million references. The system also provides access to reference and citation information, links to on-line data,
electronic journal articles, and other on-line information. The ADS Article Service contains the full articles for most of
the astronomical literature back to volume 1. It contains the scanned pages of all the major journals (Astrophysical Journal,
Astronomical Journal, Astronomy & Astrophysics, Monthly Notices of the Royal Astronomical Society, and Solar Physics), as
well as most smaller journals back to volume 1.The ADS can be accessed through any web browser without signup or login. Alternatively
an email interface is available that allows our users to execute queries via email and to retrieve scanned articles via email.
This might be interesting for users on slow or unreliable links, since the email system will retry sending information automatically
until the transfer is complete. There are now 9 mirror sites of the ADS available in different parts of the world to improve
access. The ADS is available at: http://ads.harvard.edu
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献