Digital control of diode laser for atmospheric spectroscopy

A system is described for remote absorption spectroscopy of trace species using a diode laser tunable over a useful spectral region of 50 to 200 cm(-1) by control of diode laser temperature over range from 15 K to 100 K, and tunable over a smaller region of typically 0.1 to 10 cm(-1) by control of the diode laser current over a range from 0 to 2 amps. Diode laser temperature and current set points are transmitted to the instrument in digital form and stored in memory for retrieval under control of a microprocessor during measurements. The laser diode current is determined by a digital to analog converter through a field effect transistor for a high degree of ambient temperature stability, while the laser diode temperature is determined by set points entered into a digital to analog converter under control of the microprocessor. Temperature of the laser diode is sensed by a sensor diode to provide negative feedback to the temperature control circuit that responds to the temperature control digital to analog converter

Discovering Software Process Deviations Using Visualizations

Peer reviewe

Judgements of Solomon: anxieties and defences of social workers involved in care proceedings

Evidence from focus group discussions with social workers in child care and child protection was collected for a research project exploring decision-making in care proceedings and seeking a better understanding of the causes of delay in the process. Here this material is used to examine social workers’ feelings about their work and to explore the anxieties they expressed. Isabel Menzies’s work on containing anxiety in institutions is used to provide a conceptual framework for thinking about the ways in which individuals’ unconscious defences against anxiety may affect the structure, policies and practices of the organization in which they work. It is suggested that this dimension needs to be taken into account in understanding difficulties which arise in putting policy into practice

Time is not enough : promoting strategic engagement with writing for publication

Research, scholarship and publication are central to the work of higher education. However, even academics with the necessary research and writing skills can struggle to publish as often as they would like. Research suggests that a writing retreat is one solution; there is a process going on there that addresses the problem, but how it does so has not been fully explained. We used a novel approach, containment theory, to explain why the functions of a structured retreat work. We argue that a retreat does more than simply provide time to write; it is a model for academics to meet the demands of research assessment. Finally, we conceptualise this as strategic engagement - a model for producing regular writing for publication while continuing to meet other professional demands

Spitzer Space Telescope spectral observations of AGB stars in the Fornax dwarf spheroidal galaxy

We have observed five carbon-rich AGB stars in the Fornax dwarf spheroidal (dSph) galaxy, using the Infrared Spectrometer on board the Spitzer Space Telescope. The stars were selected from a near-infrared survey of Fornax and include the three reddest stars, with presumably the highest mass-loss rates, in that galaxy. Such carbon stars probably belong to the intermediate-age population (2-8 Gyr old and metallicity of [Fe/H] -1) of Fornax. The primary aim of this paper is to investigate mass-loss rate, as a function of luminosity and metallicity, by comparing AGB stars in several galaxies with different metallicities. The spectra of three stars are fitted with a radiative transfer model. We find that mass-loss rates of these three stars are 4-7x10^-6 Msun yr-1. The other two stars have mass-loss rates below 1.3x10^-6 Msun yr-1. We find no evidence that these rates depend on metallicity, although we do suggest that the gas-to-dust ratio could be higher than at solar metallicity, in the range 240 to 800. The C2H2 bands are stronger at lower metallicity because of the higher C/O ratio. In contrast, the SiC fraction is reduced at low metallicity, due to low silicon abundance. The total mass-loss rate from all known carbon-rich AGB stars into the interstellar medium of this galaxy is of the order of 2x10^-5 Msun yr-1. This is much lower than that of the dwarf irregular galaxy WLM, which has a similar visual luminosity and metallicity. The difference is attributed to the younger stellar population of WLM. The suppressed gas-return rate to the ISM accentuates the difference between the relatively gas-rich dwarf irregular and the gas-poor dwarf spheroidal galaxies. Our study will be useful to constrain gas and dust recycling processes in low metallicity galaxies.Comment: MNRAS accepte

Occurrence of a Carboxin-Resistant Strain of Ustilago nuda in Italy

Loose smut of barley, caused by Ustilago nuda (Jens.) Rostr., is commonly controlled through the use of systemic seed-treatment fungicides. The most widely used active ingredient in these fungicides has been carboxin. However, isolates of U. nuda resistant to carboxin have been reported in France. In 1996 and 1997, unsatisfactory levels of loose smut of barley were observed near Perugia (central Italy), despite the treatment of the barley seed with a carboxin-based fungicide. An isolate of U. nuda (97-255) was collected from this field to determine if the pathogen had developed resistance to carboxin. Germination tests on carboxin-amended agar media indicated that isolate 97- 255 was more resistant to carboxin than a wild type isolate of U. nuda collected in Canada. In tests in which isolate 97-255 was inoculated onto barley cv. Regal, the percentage of smutted plants arising from the inoculated seed was not reduced by a carboxin seed treatment. This is the first report of resistance to carboxin in populations of U. nuda from Italy