Picturing Teacher Agency: Developing Upstanding Heuristics in a Middle Grades Social Studies Methods Course

This paper presents a multi-case study of teacher candidates in a pre-service middle grades social studies methods course. The research aimed to understand how the middle grades teacher candidates viewed their future as upstanders with agency in middle grades settings. The focus of the research was on heuristic representations that the teacher candidates created to illustrate how they understood their role in supporting the democratic aims of middle grades social studies. Qualitative data was collected and analyzed through chordal triad of agency theory (Emirbayer & Mische, 1998). The findings indicate that preservice teachers best understand their future as change agents through their role of curriculum and instruction and their impact on students, additionally their conceptualizations of their intended agency were influenced by their past and present experiences as well as their projected goals for the future. This research also suggests that heuristics may be a powerful tool in the preparation of teacher candidates, helping them to think through their role in supporting the democratic aims of social studies, middle grades education and social justice education. Important constraints about teacher candidates’ perceptions (or lack thereof) of oppressive structures within middle schools settings are considered

On stability and spiral patterns in polar disks

To investigate the stability properties of polar disks we performed two-dimensional hydrodynamical simulations for flat polytropic gaseous self-gravitating disks which were perturbed by a central S0-like component. Our disk was constructed to resemble that of the proto-typical galaxy NGC 4650A. This central perturbation induces initially a stationary two-armed tightly-wound leading spiral in the polar disk. For a hot disk (Toomre parameter Q>1.7), the structure does not change over the simulation time of 4.5 Gyr. In case of colder disks, the self-gravity of the spiral becomes dominant, it decouples from the central perturbation and grows, until reaching a saturation stage in which an open trailing spiral is formed, rather similar to that observed in NGC4650A. The timescale for developing non-linear structures is 1-2 Gyr; saturation is reached within 2-3 Gyr. The main parameter controlling the structure formation is the Toomre parameter. The results are surprisingly insensitive to the properties of the central component. If the polar disk is much less massive than that in NGC4650A, it forms a weaker tightly-wound spiral, similar to that seen in dust absorption in the dust disk of NGC2787. Our results are derived for a polytropic equation of state, but appear to be generic as the adiabatic exponent is varied between \gamma = 1 (isothermal) and \gamma = 2 (very stiff).Comment: 14 pages including 23 figures, accepted for publication in Astronomy & Astrophysic

Who Are the Givers? Briefing Paper on British Social Attitudes to Charitable Giving

This Institute for Philanthropy paper summarizes the findings of the annual British Social Attitudes Survey on the attitudes and values of Britons regarding charitable giving and philanthropy, and on their behavior. The authors differentiate the target group by age, education, religion, income, political affiliation, and newspaper readership, and determines that there are broadly three groups in British society: contributors, bystanders, and investors

The small-scale Structure of the Magellanic Stream as a Foundation for Galaxy Evolution

The Magellanic Stream (MS) is the nearest example of a gaseous trail formed by interacting galaxies. While the substantial gas masses in these kinds of circumgalactic structures are postulated to represent important sources of fuel for future star formation, the mechanisms whereby this material might be accreted back into galaxies remain unclear. Recent neutral hydrogen (HI) observations have demonstrated that the northern portion of the MS, which probably has been interacting with the Milky Way's hot gaseous halo for close to 1000~Myr, has a larger spatial extent than previously recognized, while also containing significant amounts of small-scale structure. After a brief consideration of the large-scale kinematics of the MS as traced by the recently-discovered extension of the MS, we explore the aging process of the MS gas through the operation of various hydrodynamic instabilities and interstellar turbulence. This in turn leads to consideration of processes whereby MS material survives as cool gas, and yet also evidently fails to form stars. Parallels between the MS and extragalactic tidal features are briefly discussed with an emphasis on steps toward establishing what the MS reveals about the critical role of local processes in determining the evolution of these kinds of systems

Telescience Testbed Pilot Program

The Telescience Testbed Pilot Program is developing initial recommendations for requirements and design approaches for the information systems of the Space Station era. During this quarter, drafting of the final reports of the various participants was initiated. Several drafts are included in this report as the University technical reports

Assessment in Scotland

Assessment practice will follow and reinforce the curriculum and promote high quality learning and teaching approaches. Assessment of children's and young people's progress and achievement during their broad general education to the end of S3 will be based on teachers' assessment of their knowledge and understanding, skills, attributes and capabilities, as described in the experiences and outcomes across the curriculum