2,205 research outputs found
Opening the doors of learning: Increasing access to music degrees
This article is contextualized for Music and is a response to the CHE (2013) Report that proposes a flexible curriculum structure for undergraduate degrees in South Africa, to address student under preparedness. Research states that music graduates need well developed identities in music, as well as generic, transferable skills to ensure lifelong employment and that a bachelor of music degree is best suited for this. However, in the South African context, the bachelor of music degree qualification is not accessible to the majority of prospective students as they are under prepared to study music at tertiary level. Only a minority of learners receive quality music education at school, while the majority of learners, including those from low socio-economic communities, do not receive formal music education. Under preparedness to study music, has traditionally been addressed through certificates and diploma qualifications in music. A discussion, and interpretation of the literature, has led to the researcher to develop an alternate framework to both improve student access to music degrees and manage under preparedness. The proposed approach advocates that music departments at universities adopt the framework of the national certificate vocation as an alternative to certificates and diplomas. The alternative curriculum structure for music, would be a more cost effective way to address under preparedness, improve academic success and lead to high skill levels.
The study is situated in a constructivist, interpretive worldview, with a qualitative research design. Purposive sampling in the form of the choice of literature for the theoretical framework was adopted. While this theoretical study is contextualized for music, it is applicable to other fields
Scattering of a Long Cosmic String by a Rotating Black Hole
The scattering of a straight, infinitely long string by a rotating black hole
is considered. We assume that a string is moving with velocity v and that
initially the string is parallel to the axis of rotation of the black hole. We
demonstrate that as a result of scattering, the string is displaced in the
direction perpendicular to the velocity by an amount kappa(v,b), where b is the
impact parameter. The late-time solution is represented by a kink and
anti-kink, propagating in opposite directions at the speed of light, and
leaving behind them the string in a new ``phase''. We present the results of
the numerical study of the string scattering and their comparison with the
weak-field approximation, valid where the impact parameter is large, b/M >> 1,
and also with the scattering by a non-rotating black hole which was studied in
earlier works.Comment: 27 pages, 14 figures, to be published in Classical and Quantum
Gravit
The use of the road to health card in monitoring child health
Objectives:
The Road to Health Chart (RTHC) provides a simple, cheap, practical and convenient method of monitoring child health. The RTHC could assist with vaccine compliance and early identification of growth faltering, to improve general health. The purpose of the study was to assess whether the RTHCs were adequately completed and interpreted at primary, secondary and tertiary care levels in South Africa.
Methods:
The study was carried out at a primary, secondary and tertiary care centre. A questionnaire was administered to 100 subjects from each; seeking demographic information, whether the RTHC was brought along, and if not why it was not brought.
Results:
Most children were brought by their mothers. The RTHC was not brought to 48% of the consultations; of those, about 72% thought that bringing the RTHC along was not necessary. Health workers seldom asked to see the RTHC at the primary and secondary care settings, but 50% of them did so at Ga-Rankuwa Hospital (p = 0,002). In only 8 cases overall were the children below the 3rd percentile of weight-for-age. Approximately 20% had incomplete immunisations.
Conclusions: Many parents believe that the RTHC is only required for Well-baby-clinic visits, not for consultations. The RTHC is not often asked for at consultations; the fact that this is more often done at the tertiary care centre may be that much of the service is supplied by paediatricians-in-training. Health workers should ask to see the RTHC, in order for mothers to understand the importance of the information. The study showed that the RTHC is not used to its full potential.
South African Family Practice Vol. 49 (1) 2007: pp. 1
Books
Neurobiology Neurobiology: 2 ed. Ed. by Gordon M. Shepherd. Pp. xiv + 689. Illustrared. R74,50. Oxford: Oxford Universiry Press. 1988.Medical physiology Textbook of Medical Physiology. Ed. by A. C. Guyton. Pp. xli + 1014. Illustrated. Kent: Harcourt, Brace, Jovanovich. 1991.Bilingual heart and stress booklets The Healthy HeartlDie Gesonde Hart. Ed. by G. Jackson. Coping with Stress/Oorwin Stres. Ed. by T. Trauer. pp. 77. Illustrated. RI9,95. Cape Town: Tafelberg. 1990
Die meting van die verband tussen geslag en konformiteit as groepdinamiese veranderlikes
The original publication is available at http://www.sajip.co.zaThe amount and kind of conformity induced by group pressure
depend upon the nature of the situation. The nature of the group
and the characteristics of the individual. In this particular study
the experimental measurement of conformity developed by Asch
and Crutchfield was repeated. Confirmation was found that sex
operates as one of the determinants of conformity.Publishers' Versio
GRMHD prediction of coronal variability in accreting black holes
On the basis of data from an energy-conserving 3D general relativistic MHD
simulation, we predict the statistical character of variability in the coronal
luminosity from accreting black holes. When the inner boundary of the corona is
defined to be the electron scattering photosphere, its location depends only on
the mass accretion rate in Eddington units (\dot{M}). Nearly independent of
viewing angle and \dot{M}, the power spectrum over the range of frequencies
from approximately the orbital frequency at the innermost stable circular orbit
(ISCO) to ~100 times lower is well approximated by a power-law with index -2,
crudely consistent with the observed power spectra of hard X-ray fluctuations
in AGN and the hard states of Galactic binary black holes. The underlying
physical driver for variability in the light curve is variations in the
accretion rate caused by the chaotic character of MHD turbulence, but the power
spectrum of the coronal light output is significantly steeper. Part of this
contrast is due to the fact that the mass accretion rate can be significantly
modulated by radial epicyclic motions that do not result in dissipation, and
therefore do not drive luminosity fluctuations. The other part of this contrast
is due to the inward decrease of the characteristic inflow time, which leads to
decreasing radial coherence length with increasing fluctuation frequency.Comment: Accepted for publication in ApJ, 35 pages, 11 figures (8 color and 3
greyscale), AASTEX. High-resolution versions can be found at the following
links: [PS] http://www.pha.jhu.edu/~scn/papers/grmhd_var.ps [PDF]
http://www.pha.jhu.edu/~scn/papers/grmhd_var.pd
Application of the Cubed-Sphere Grid to Tilted Black-Hole Accretion Disks
In recent work we presented the first results of global general relativistic
magnetohydrodynamic (GRMHD) simulations of tilted (or misaligned) accretion
disks around rotating black holes. The simulated tilted disks showed dramatic
differences from comparable untilted disks, such as asymmetrical accretion onto
the hole through opposing "plunging streams" and global precession of the disk
powered by a torque provided by the black hole. However, those simulations used
a traditional spherical-polar grid that was purposefully underresolved along
the pole, which prevented us from assessing the behavior of any jets that may
have been associated with the tilted disks. To address this shortcoming we have
added a block-structured "cubed-sphere" grid option to the Cosmos++ GRMHD code,
which will allow us to simultaneously resolve the disk and polar regions. Here
we present our implementation of this grid and the results of a small suite of
validation tests intended to demonstrate that the new grid performs as
expected. The most important test in this work is a comparison of identical
tilted disks, one evolved using our spherical-polar grid and the other with the
cubed-sphere grid. We also demonstrate an interesting dependence of the
early-time evolution of our disks on their orientation with respect to the grid
alignment. This dependence arises from the differing treatment of current
sheets within the disks, especially whether they are aligned with symmetry
planes of the grid or not.Comment: 15 pages, 11 figures, submitted to Ap
The adjoint mehod for automotive optimisation using a sphericity based morpher
A robust workflow for shape optimisation of internal and external flows with application to automotive design is demonstrated in this paper. A gradient based approach is presented, in which the surface sensitivity with respect to the flow variables is computed with the continuous adjoint method. For aerodynamic shape optimisation cases, mesh displacement algorithms are indispensable in order to avoid re-meshing the updated geometry in each optimisation step. Keeping the same mesh topology at every optimisation cycle secures gradient consistency and the possibility to use the previous solution as initial conditions in order to converge the CFD equations faster. Simple mesh displacement algorithms, such as the spring analogy, run into problems under complex surface deformations. Thus a mesh optimisation approach can be proved to be more robust as it copes better with complex elements optimising also the base mesh. In this paper the mesh displacement algorithm is based on sphericity, which quantifies the mesh quality. Solving an extra optimisation problem for the maximisation of the sphericity value, results in the new internal mesh nodes positions. The methodology is heuristic in nature in that it does not consider known numerical quality metrics explicitly. It has shown however to be exceptionally robust and effective allowing the maintenance of high cell quality even during extreme deformation events. The suggested method is applied to automotive test cases of internal and external aerodynamics. In such cases, the use of a robust morpher which preserves geometry features and delays mesh quality deterioration is found to be crucial
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