4,121 research outputs found
Union Influence on Worker Education and Training in Canada in Tough Times
This research has focused on re-analyzing data from previous large-scale Canadian surveys that include information on education and training activities and union status, as well as other demographic and organizational factors, most prominently the 1993 and 1997 Adult Education and Training Surveys. In contrast to some recent studies, we find that union status has had consistent positive individual-level effects in Canada on participation in adult education courses and employer-sponsored courses in general, and especially for women union members. In addition, our analysis of data from the 1998 national survey on informal learning finds that in this much more extensive form of learning, unionized workers are significantly more likely than non-unionized workers to participate in more directly empowering forms of knowledge including learning about workers’ rights and political issues
Pulsar magnetic alignment and the pulsewidth-age relation
Using pulsewidth data for 872 isolated radio pulsars we test the hypothesis
that pulsars evolve through a progressive narrowing of the emission cone
combined with progressive alignment of the spin and magnetic axes. The new data
provide strong evidence for the alignment over a time-scale of about 1 Myr with
a log standard deviation of around 0.8 across the observed population. This
time-scale is shorter than the time-scale of about 10 Myr found by previous
authors, but the log standard deviation is larger. The results are inconsistent
with models based on magnetic field decay alone or monotonic counter-alignment
to orthogonal rotation. The best fits are obtained for a braking index
parameter n_gamma approximately equal to 2.3, consistent the mean of the six
measured values, but based on a much larger sample of young pulsars. The
least-squares fitted models are used to predict the mean inclination angle
between the spin and magnetic axes as a function of log characteristic age.
Comparing these predictions to existing estimates it is found that the model in
which pulsars are born with a random angle of inclination gives the best fit to
the data. Plots of the mean beaming fraction as a function of characteristic
age are presented using the best-fitting model parameters.Comment: 13 pages, 11 figures, Accepted for publication in MNRA
3D virtual worlds as environments for literacy learning
Background: Although much has been written about the ways in which new technology might transform educational practice, particularly in the area of literacy learning, there is relatively little empirical work that explores the possibilities and problems - or even what such a transformation might look like in the classroom. 3D virtual worlds offer a range of opportunities for children to use digital literacies in school, and suggest one way in which we might explore changing literacy practices in a playful, yet meaningful context. Purpose: This paper identifies some of the key issues that emerged in designing and implementing virtual world work in a small number of primary schools in the UK. It examines the tensions between different discourses about literacy and literacy learning and shows how these were played out by teachers and pupils in classroom settings.Sources of evidence: Case study data are used as a basis for exploring and illustrating key aspects of design and implementation. The case study material includes views from a number of perspectives including classroom observations, chatlogs, in-world avatar interviews with teachers and also pupils, as well as the author’s field notes of the planning process with accompanying minutes and meeting documents.Main argument: From a Foucauldian perspective, the article suggests that social control of pedagogical practice through the regulation of curriculum time, the normalisation of teaching routines and the regimes of individual assessment restricts teachers’ and pupils’ conceptions of what constitutes literacy. The counternarrative, found in recent work in new litearcies (Lankshear & Knobel, 2006) provides an attractive alternative, but a movement in this direction requires a fundamental shift of emphasis and a re-conceptualisation of what counts as learning.Conclusions: This work on 3D virtual worlds questions the notion of how transformative practice can be achieved with the use of new technologies. It suggests that changes in teacher preparation, continuing professional development as well as wider educational reform may be needed
Stimulating the innovation potential of 'routine' workers through workplace learning
Governments worldwide seek to upgrade the ‘basic skills' of employees deemed to have low literacy and numeracy, in order to enable their greater productivity and participation in workplace practices. A longitudinal investigation of such interventions in the United Kingdom has examined the effects on employees and on organizations of engaging in basic skills programmes offered in and through the workplace. ‘Tracking’ of employees in selected organizational contexts has highlighted ways in which interplay between formal and informal workplace learning can help to create the environments for employees in lower grade jobs to use and expand their skills. This workplace learning is a precondition, a stimulus and an essential ingredient for participation in employee-driven innovation, as workers engage with others to vary, and eventually to change, work practices. © 2010, SAGE Publications. All rights reserved
X-ray Phase-Resolved Spectroscopy of PSRs B0531+21, B1509-58, and B0540-69 with RXTE
The Rossi X-ray Timing Explorer ({\sl RXTE}) has made hundreds of
observations on three famous young pulsars (PSRs) B0531+21 (Crab), B1509-58,
and B0540-69. Using the archive {\sl RXTE} data, we have studied the
phase-resolved spectral properties of these pulsars in details. The variation
of the X-ray spectrum with phase of PSR B0531+21 is confirmed here much more
precisely and more details are revealed than the previous studies: the spectrum
softens from the beginning of the first pulse, turns to harden right at the
pulse peak and becomes the hardest at the bottom of the bridge, softens
gradually until the second peak, and then softens rapidly. Different from the
previous studies, we found that the spectrum of PSR B1509-58 is significantly
harder in the center of the pulse, which is also in contrast to that of PSR
B0531+21. The variation of the X-ray spectrum of PSR B0540-69 seems similar to
that of PSR B1509-58, but with a lower significance. Using the about 10 years
of data span, we also studied the real time evolution of the spectra of these
pulsars, and no significant evolution has been detected. We have discussed
about the constraints of these results on theoretical models of pulsar X-ray
emission.Comment: 42 pages, 24 figure
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