350 research outputs found

    Review of the Crown-of-thorns Starfish Research Committee (COTSREC) Program

    Get PDF
    In December 1988, following criticism in the media of the Great Barrier Reef Marine Park Authority's handling of the crown-of-thorns starfish (COTS) issue, the then Minister for the Arts, Sport, the Environment, Tourism and Territories, Senator the Honourable Graham Richardson, requested a review of the Authority's crown-of-thorns starfish research program and policies. The research program had been recommended to the Authority by the Crown-of-thorns Starfish Advisory Committee (COTSAC), a body of experts convened by the Authority in 1984 for this purpose. Funding of $3 million over four years for the program (1985-86 to 1988-89) was provided by the Federal Government. The program was reviewed annually by another advisory body established by the Authority, the Crown-of-thorns Starfish Advisory Review Committee (COTSARC). Zann and Moran (1988), Moran and Johnson (1990) and Lassig (1991) have summarised the structure and results of this program

    Crown-of-thorns starfish, Acanthaster planci (L.): synopsis of recent research

    Get PDF

    In-plane magnetic reorientation in coupled ferro- and antiferromagnetic thin films

    Full text link
    By studying coupled ferro- (FM) and antiferromagnetic (AFM) thin film systems, we obtain an in-plane magnetic reorientation as a function of temperature and FM film thickness. The interlayer exchange coupling causes a uniaxial anisotropy, which may compete with the intrinsic anisotropy of the FM film. Depending on the latter the total in-plane anisotropy of the FM film is either enhanced or reduced. Eventually a change of sign occurs, resulting in an in-plane magnetic reorientation between a collinear and an orthogonal magnetic arrangement of the two subsystems. A canted magnetic arrangement may occur, mediating between these two extremes. By measuring the anisotropy below and above the N\'eel temperature the interlayer exchange coupling can be determined. The calculations have been performed with a Heisenberg-like Hamiltonian by application of a two-spin mean-field theory.Comment: 4 pages, 4 figure

    Topological Structure of the QCD Vacuum Revealed by Overlap Fermions

    Full text link
    Overlap fermions preserve a remnant of chiral symmetry on the lattice. They are a powerful tool to investigate the topological structure of the vacuum of Yang-Mills theory and full QCD. Recent results concerning the localization of topological charge and the localization and local chirality of the overlap eigenmodes are reported. The charge distribution is radically different, if a spectral cut-off for the Dirac eigenmodes is applied. The density q(x) is changing from the scale-a charge density (with full lattice resolution) to the ultraviolet filtered charge density. The scale-a density, computed on the Linux cluster of LRZ, has a singular, sign-coherent global structure of co-dimension 1 first described by the Kentucky group. We stress, however, the cluster properties of the UV filtered topological density resembling the instanton picture. The spectral cut-off can be mapped to a bosonic smearing procedure. The UV filtered field strength reveals a high degree of (anti)selfduality at "hot spots" of the action. The fermionic eigenmodes show a high degree of local chirality. The lowest modes are seen to be localized in low-dimensional space-time regions.Comment: 13 pages, 11 figures, accepted to appear in the Proceedings of "HLRB, KONWIHR and Linux-Cluster: Review, Results and Future Projects Workshop", Leibniz Rechenzentrum Munich, December 200

    Un nuevo Código de Corrección de Errores matricial con baja redundancia

    Get PDF
    Actualmente, y debido al continuo aumento en la escala de integración, la tasa de fallos en los sistemas de memoria de los computadores ha aumentado. Así, la probabilidad de que se produzcan Single Cell Upsets (SCUs) o Multiple Cell Upsets (MCUs) aumenta. Una solución común es el uso de Códigos de Corrección de Errores (ECCs). Sin embargo, cuando se utilizan ECCs en aplicaciones empotradas, se debe lograr un buen equilibrio entre la cobertura de errores, la redundancia introducida y la eficiencia en términos de área de silicio ocupada, potencia consumida y retardo de los circuitos de codificación y decodificación. En este sentido, existen diferentes propuestas para tolerar MCUs. Por ejemplo, los códigos matriciales utilizan códigos de Hamming y controles de paridad en un formato bidimensional para detectar y/o corregir MCUs. Sin embargo, estos códigos introducen una gran redundancia, lo que conlleva una sobrecarga excesiva con respecto al área, potencia consumida y retardo. En este trabajo presentamos un nuevo código matricial con una baja redundancia, que permite corregir diferentes patrones de MCUs y que no introduce una gran sobrecarga en los circuitos de codificación y decodificación

    Louse (Insecta : Phthiraptera) mitochondrial 12S rRNA secondary structure is highly variable

    Get PDF
    Lice are ectoparasitic insects hosted by birds and mammals. Mitochondrial 12S rRNA sequences obtained from lice show considerable length variation and are very difficult to align. We show that the louse 12S rRNA domain III secondary structure displays considerable variation compared to other insects, in both the shape and number of stems and loops. Phylogenetic trees constructed from tree edit distances between louse 12S rRNA structures do not closely resemble trees constructed from sequence data, suggesting that at least some of this structural variation has arisen independently in different louse lineages. Taken together with previous work on mitochondrial gene order and elevated rates of substitution in louse mitochondrial sequences, the structural variation in louse 12S rRNA confirms the highly distinctive nature of molecular evolution in these insects

    Emotional intelligence and British expatriates’ cross-cultural adjustment in international construction projects

    Get PDF
    © 2016 Informa UK Limited, trading as Taylor & Francis Group. Today’s internationalized business demands global mindset, intercultural sensitivity and the ability to skilfully negotiate through cross-cultural interactions. Therefore, the overall aim was to investigate the influence of emotional intelligence (EI) on cross-cultural adjustment (CCA) of British expatriates working on International Architectural, Engineering and Construction assignments in Sub-Saharan Africa, China, Middle East and Indian Sub-Continent. Specifically, the causal relationship between EI and three facets of CCA i.e. work, general and interaction adjustment was explored. A sequential exploratory mixed methods design was adopted. These include extensive review of existing literature, eighteen unstructured interviews, and questionnaire survey of 191 British expatriates operating in 29 different countries from the four regions under investigation. Structural equation modelling was used to assess the causal relationship between EI and CCA. Results show that EI accounted for 91, 64 and 24% of the variance in work, interaction and general adjustment respectively. Overall, the model was able to explain 60% variance in CCA, suggesting that EI competencies play a huge role in facilitating an expatriate understand and adapt to host country culture. The findings would help decision-makers (HR managers) during expatriate selection process, in understanding that along with technical skills, it is the emotional competencies that are crucial in assisting expatriates adjust to foreign way of life

    Low energy scattering cross section ratios of N 14 (p,p) N 14

    Get PDF
    Background: The slowest reaction in the first CNO cycle is N14(p,γ)O15, therefore its rate determines the overall energy production efficiency of the entire cycle. The cross section presents several strong resonance contributions, especially for the ground-state transition. Some of the properties of the corresponding levels in the O15 compound nucleus remain uncertain, which affects the uncertainty in extrapolating the capture cross section to the low energy range of astrophysical interest. Purpose: The N14(p,γ)O15 cross section can be described by using the phenomenological R matrix. Over the energy range of interest, only the proton and γ-ray channels are open. Since resonance capture makes significant contributions to the N14(p,γ)O15 cross section, resonant proton scattering data can be used to provide additional constraints on the R-matrix fit of the capture data. Methods: A 4 MV KN Van de Graaff accelerator was used to bombard protons onto a windowless gas target containing enriched N14 gas over the proton energy range from Ep=1.0 to 3.0 MeV. Scattered protons were detected at θlab=90, 120°, 135°, 150°, and 160° using ruggedized silicon detectors. In addition, a 10 MV FN Tandem Van de Graaff accelerator was used to accelerate protons onto a solid Adenine (C5H5N5) target, of natural isotopic abundance, evaporated onto a thin self-supporting carbon backing, over the energy range from Ep=1.8 to 4.0 MeV. Scattered protons were detected at 28 angles between θlab=30.4° and 167.7° by using silicon photodiode detectors. Results: Relative cross sections were extracted from both measurements. While the relative cross sections do not provide as much constraint as absolute measurements, they greatly reduce the dependence of the data on otherwise significant systematic uncertainties, which are more difficult to quantify. The data are fit simultaneously using an R-matrix analysis and level energies and proton widths are extracted. Even with relative measurements, the statistics and large angular coverage of the measurements result in more confident values for the energies and proton widths of several levels; in particular, the broad resonance at Ec.m.=2.21 MeV, which corresponds to the 3/2+ level at Ex=9.51 MeV in O15. In particular, the s- and d-wave angular-momentum channels are separated. Conclusion: The relative cross sections provide a consistent set of data that can be used to better constrain a full multichannel R-matrix extrapolation of the capture data. It has been demonstrated how the scattering data reduce the uncertainty through a preliminary Monte Carlo uncertainty analysis, but several other issues remain that make large contributions to the uncertainty, which must be addressed by further capture and lifetime measurements

    X-ray Survey Results on Active Galaxy Physics and Evolution

    Full text link
    This "pedagogical" review describes the key Chandra and XMM-Newton extragalactic surveys to date and details some of their implications for AGN physics and evolution. We additionally highlight two topics of current widespread interest: (1) X-ray constraints on the AGN content of luminous submillimeter galaxies, and (2) the demography and physics of high-redshift (z > 4) AGN as revealed by X-ray observations. Finally, we discuss prospects for future X-ray surveys with Chandra, XMM-Newton, and upcoming missions.Comment: 26 pages, in Physics of Active Galactic Nuclei at All Scales, eds. Alloin D., Johnson R., Lira P. (Springer-Verlag, Berlin), version with all figures at http://www.astro.psu.edu/users/niel/papers/papers.htm
    corecore