POV X 3: Helping journalism students juxtapose author, actor and audience

Asking journalism students to create stories with a strong point of view means requiring them to do three things at once. Compelling news writing triangulates between the perspectives of author, actor (the person who is the subject of the piece) and audience. This article examines an in-class activity that prompts students to elaborate on a single story from multiple points of view and then reflect on the choices they have made. This mix of creative collaboration and analysis encourages learners to think and act as “reflective practitioners” (Schön, 1983) while trying on a variety of professional identities related to multiple communities of practice (Gee, 2004)

Designing Journalists: Teaching Journalism Students to Think Like Web Designers

The authors introduced 80 university-level journalism students to a web design program called Klynt and supervised the creation of multiple interactive documentaries. They discovered that fledgling reporters could effectively design interactive media while creating work that reflects their own candid and extemporaneous ethos. Building on the insight that journalism in the digital age must give rise to modified best practices, this study examines the complex production processes from which multiple i-docs emerged. The authors conclude by suggesting four tentative “new best practices” for journalists attempting to think and act like web designers

Creep Simulations of Nuclear Fuel Cladding under long term Storage Conditions with TRANSURANUS

Within a joint research project between the Institute for Energy (IE) and the Institute for Transuranium Elements (ITU) on the integrity of spent nuclear fuel cladding the ITU code TRANSURANUS was used to simulate creep of Zircaloy cladding tubes under long term storage conditions. Since TRANSURANUS is designed to model the mechanical, thermal and physical behaviour of fuel rods during reactor operation it was the objective of this study firstly to explore the limitations of the present creep models in TRANSURANUS for the simulation of long term creep processes under dry storage conditions. If the present creep models in TRANSURANUS were found to be inappropriate then the next objective was to formulate the properties of an "ideal" creep model for dry storage. The creep models were compared with creep tests on unirradiated Zircaloy cladding tubes. It turned out that the standard creep model for Zircaloy cladding in TRANSURANUS, the model of Lassmann and Moreno, underestimated the creep strains of the tests significantly. The creep model of Mayuzumi and Onchi, which was designed to model long term creep processes under dry storage conditions, lead to reasonable agreement with the creep tests for temperatures of 350 degrees Celcius and above. It turned out that for the accurate prediction under low-temperature conditions (under 350 degrees Celcius) more sophisticated creep models, which account for a shift in creep mechanisms, are necessary.JRC.F.5-Safety of present nuclear reactor

Invisible sunspots and rate of solar magnetic flux emergence

Aims. We study the visibility of sunspots and its influence on observed values of sunspot region parameters. Methods. We use Virtual Observatory tools provided by AstroGrid to analyse a sample of 6862 sunspot regions. By studying the distributions of locations where sunspots were first and last observed on the solar disk, we derive the visibility function of sunspots, the rate of magnetic flux emergence and the ratio between the durations of growth and decay phases of solar active regions. Results. We demonstrate that the visibility of small sunspots has a strong centre-to-limb variation, far larger than would be expected from geometrical (projection) effects. This results in a large number of young spots being invisible: 44% of new regions emerging in the west of the Sun go undetected. For sunspot regions that are detected, large differences exist between actual locations and times of flux emergence, and the apparent ones derived from sunspot data. The duration of the growth phase of solar regions has been, up to now, underestimated