Sensitivity and cost considerations for the detection and eradication of marine pests in ports     

Hayes KR  Cannon R  Neil K  Inglis G 《Marine pollution bulletin》2005,50(8):823-834

Port surveys are being conducted in Australia, New Zealand and around the world to confirm the presence or absence of particular marine pests. The most critical aspect of these surveys is their sensitivity-the probability that they will correctly identify a species as present if indeed it is present. This is not, however, adequately addressed in the relevant national and international standards. Simple calculations show that the sensitivity of port survey methods is closely related to their encounter rate-the average number of target individuals expected to be detected by the method. The encounter rate (which reflects any difference in relative pest density), divided by the cost of the method, provides one way to compare the cost-effectiveness of different survey methods. The most cost-effective survey method is site- and species-specific but, in general, will involve sampling from the habitat with the highest expected population of target individuals. A case study of Perna viridis in Trinity Inlet, Cairns, demonstrates that plankton trawls processed with gene probes provide the same level of sensitivity for a fraction of the cost associated with the next best available method-snorkel transects in bad visibility (secchi depth=0.72 m). Visibility and the adult/larvae ratio, however, are critical to these arguments. If visibility were good (secchi depth=10 m), the two approaches would be comparable. Diver deployed quadrats were at least three orders of magnitude less cost-effective in this case study. It is very important that environmental managers and scientists perform sensitivity calculations before embarking on port surveys to ensure the highest level of sensitivity is achieved for any given budget.  相似文献   

Reviews     

A. Hubaux  Frank Simpson  Graeme Bonham-Carter 《Mathematical Geology》1970,2(4):415-420

  相似文献   

URBAN RESIDENTIAL RENOVATION AND RENEWAL: MODELING BY GRAPHIC SYNTHESIS     

Graeme H. T. Hart 《The Professional geographer》1980,32(4):439-445

Houses in inner-city areas, because of their age, suffer the depredations of functional obsolescence and decay. Some, however, have sound locations and are able to assemble economic forces that precipitate rehabilitation by both renters and owners. Accompanying restoration is a concomitant increase in market value and in population density, the corollary of which is a reduction in lot size. This process is modeled by graphically synthesizing elements of location theory, urban growth theory, and principles of economics.  相似文献   

Ca II K Emission Line Asymmetries Among Red Giants     

Graeme H. Smith 《Astrophysics and Space Science》1997,253(1):119-138

In the spectra of red giants the chromospheric emission feature found in the core of the Ca II K line often exhibits an asymmetric profile. This asymmetry can be documented by a parameter V/R which is classified as > 1, 1, or < 1 if the violet wing of the emission profile is of greater, equal, or lower intensity than the redward wing. A literature search has been conducted to compile a V/R dataset which builds on the large survey of bright field giants made by Wilson (1976). Among stars of luminosity classes II–III–IV the majority of those with V/R > 1 are found to be bluer than B-V =1.3, while those with V/R < 1 are mostly redder than this colour. Stars with nearly symmetric profiles, V/R≈ 1, are found throughout the colour range 0.8 < B-V < 1.5. There is no sharp transition line separating stars of V/R > 1 and < 1 in the colour-magnitude diagram, but rather a ‘transition zone’ centered at B-V ≈ 1.3. The center of this zone coincides closely with a ‘coronal dividing line’ identified by Haish, Schmitt and Rosso (1991) as the red envelope in the H–R diagram of giants detected in soft x-ray emission by ROSAT. It is suggested that both the transition to a Ca II K emission asymmetry of V/R < 1 and the drop in soft x-ray activity across the coronal dividing line are related to changes in the dynamical state of the chromospheres of red giants. By contrast, the onset of photometric variability due to pulsation occurs among stars of early-M spectral type, that are redward of the mid-point of the Ca II V/R ‘transition zone’, suggesting that the chromospheric motions which produce an asymmetry of V/R < 1 are established prior to the onset of pulsation. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

The rail-cutter: a simple,cheap and compact system for opening sediment cores in the lab and field     

Graeme N. D. Rogers  Karen I. Bonner  Jamie R. Wood  Janet M. Wilmshurst 《Journal of Paleolimnology》2015,53(4):433-436

  相似文献   

A Review of “Taming the Disorderly City: The Spatial Landscape of Johannesburg After Apartheid”     

Lindsay Bremner 《The Professional geographer》2013,65(1):143-144

  相似文献   

A model of plate kinematics in Gondwana breakup   总被引：2，自引：0，他引：2  

Graeme Eagles  Matthias König 《Geophysical Journal International》2008,173(2):703-717

  相似文献   

Responses of polar mesospheric cloud brightness to stratospheric gravity waves at the South Pole and Rothera,Antarctica     

Xinzhao Chu  Chihoko Yamashita  Patrick J. Espy  Graeme J. Nott  Eric J. Jensen  Han-Li Liu  Wentao Huang  Jeffrey P. Thayer 《Journal of Atmospheric and Solar》2009,71(3-4):434-445

We present the first observational proof that polar mesospheric cloud (PMC) brightness responds to stratospheric gravity waves (GWs) differently at different latitudes by analyzing the Fe Boltzmann lidar data collected from the South Pole and Rothera (67.5°S, 68.0°W), Antarctica. Stratospheric GW strength is characterized by the root-mean-square (RMS) relative density perturbation in the 30–45 km region and PMC brightness is represented by the total backscatter coefficient (TBC) in austral summer from November to February. The linear correlation coefficient (LCC) between GW strength and PMC brightness is found to be +0.09 with a 42% confidence level at the South Pole and ?0.49 with a 98% confidence level at Rothera. If a PMC case potentially affected by a space shuttle exhaust plume is removed from the Rothera dataset, the negative correlation coefficient and confidence level increase to ?0.61 and 99%, respectively. The Rothera negative correlation increases when shorter-period waves are included while no change is observed in the South Pole correlation. Therefore, observations show statistically that Rothera PMC brightness is negatively correlated with the stratospheric GW strength but no significant correlation exists at the South Pole. A positive correlation of +0.74 with a confidence level of 99.98% is found within a distinct subset of the South Pole data but the rest of the dataset exhibits a random distribution, possibly indicating different populations of ice particles at the South Pole. Our data show that these two locations have similar GW strength and spectrum in the 30–45 km region during summer. The different responses of PMC brightness to GW perturbations are likely caused by the latitudinal differences in background temperatures in the ice crystal growth region between the PMC altitude and the mesopause. At Rothera, where temperatures in this region are relatively warm and supersaturations are not as large, GW-induced temperature perturbations can drive subsaturation in the warm phase. Thus, GWs can destroy growing ice crystals or limit their growth, leading to negative correlation at Rothera. Because the South Pole temperatures in the mesopause region are much colder, GW-perturbed temperature may never be above the frost point and have less of an impact on crystal growth and PMC brightness. The observed phenomena and proposed mechanisms above need to be understood and verified through future modeling of GW effects on PMC microphysics and ray modeling of GW propagation over the South Pole and Rothera.  相似文献   

Organic matter degradation in paper sludge amendments over gold mine tailings     

Christine Cousins  Glenn H. Penner  Bruce Liu  Peter Beckett  Graeme Spiers 《Applied Geochemistry》2009

The long-term stability of paper sludge amendments as covers for reclaimed mine waste storage facilities must be assessed by the mining industry. This study examines a 6 yr old sequence of paper sludge amendments applied over wastes from historic Au mines located in Northern Ontario, Canada. As paper sludge is mostly comprised of C-rich organic compounds, elemental quantification, ¹³C cross polarization/magic angle spinning nuclear magnetic resonance (¹³C CP/MAS NMR) spectroscopy, and Fourier transform infrared (FTIR) spectroscopy were used to examine the minimal changes in the C content and speciation observed of the amendments over time. These results suggest that paper sludge covers are suitable for use in medium to long-term mining reclamation strategies.  相似文献   

Near-bed mass flux profiles in aeolian sand transport: high-resolution measurements in a wind tunnel     

Graeme R. Butterfield 《地球表面变化过程与地形》1999,24(5):393-412

Vertical profiles of the streamwise mass flux of blown sand in the near-bed (< 17 mm) region are analysed from high-resolution measurements made using an optical sensor in a wind tunnel. This analysis is complemented by detailed measurements of mass flux and mean velocity profiles throughout the boundary layer depth (0·17 m) using passive, chambered sand traps of small dimensions and armoured thermal anemometers, respectively. The data permit a preliminary analysis of the relations between the observed forms of the profiles of near-bed fluid stress and horizontal mass flux within a carefully conditioned boundary layer. Profiles of mass flux density are found to be characterized by three regions of differing gradient with transitions at about 2 mm and 19 mm above the bed. The exponential decay of mass flux with height is confirmed for elevations above 19 mm, and when plotted as a function of u_*²/g (a parameter of mean vertical trajectory height in saltation), the gradient of mass flux in this region scales with the wake-corrected friction velocity (u), where u > 0·30 m s⁻¹. A separate near-bed region of more intense transport below 19 mm is identified which carries 80 per cent of the total mass flux. This region is evident in some previous field and wind tunnel data but not in profiles simulated by numerical models. Ventilated passive sand traps underestimate mass flux in this region by 37 per cent. At slow or moderate wind speeds a third significant region below 2 mm is observed. These regions are likely to be related to grain populations in successive saltation, low-energy ejections and intermittent bed contact, respectively. Optical measurements reveal locally high grain concentrations at some elevations below 5 mm; these heights scale with transport rate, mass flux gradient and wind speed. Copyright © 1999 John Wiley & Sons, Ltd.  相似文献