Alien Registration- Macarthur, George E. (Saco, York County)

https://digitalmaine.com/alien_docs/3535/thumbnail.jp

Foam, Foam-resin composite and method of making a foam-resin composite

This invention relates to a foam, a foam-resin composite and a method of making foam-resin composites. The foam set forth in this invention comprises a urethane modified polyisocyanurate derived from an aromatic amino polyol and a polyether polyol. In addition to the polyisocyanurate foam, the composite of this invention further contains a resin layer, wherein the resin may be epoxy, bismaleimide, or phenolic resin. Such resins generally require cure or post-cure temperatures of at least 350.degree. F

Integrating Species Traits into Species Pools

Despite decades of research on the species‐pool concept and the recent explosion of interest in trait‐based frameworks in ecology and biogeography, surprisingly little is known about how spatial and temporal changes in species‐pool functional diversity (SPFD) influence biodiversity and the processes underlying community assembly. Current trait‐based frameworks focus primarily on community assembly from a static regional species pool, without considering how spatial or temporal variation in SPFD alters the relative importance of deterministic and stochastic assembly processes. Likewise, species‐pool concepts primarily focus on how the number of species in the species pool influences local biodiversity. However, species pools with similar richness can vary substantially in functional‐trait diversity, which can strongly influence community assembly and biodiversity responses to environmental change. Here, we integrate recent advances in community ecology, trait‐based ecology, and biogeography to provide a more comprehensive framework that explicitly considers how variation in SPFD, among regions and within regions through time, influences the relative importance of community assembly processes and patterns of biodiversity. First, we provide a brief overview of the primary ecological and evolutionary processes that create differences in SPFD among regions and within regions through time. We then illustrate how SPFD may influence fundamental processes of local community assembly (dispersal, ecological drift, niche selection). Higher SPFD may increase the relative importance of deterministic community assembly when greater functional diversity in the species pool increases niche selection across environmental gradients. In contrast, lower SPFD may increase the relative importance of stochastic community assembly when high functional redundancy in the species pool increases the influence of dispersal history or ecological drift. Next, we outline experimental and observational approaches for testing the influence of SPFD on assembly processes and biodiversity. Finally, we highlight applications of this framework for restoration and conservation. This species‐pool functional diversity framework has the potential to advance our understanding of how local‐ and regional‐scale processes jointly influence patterns of biodiversity across biogeographic regions, changes in biodiversity within regions over time, and restoration outcomes and conservation efforts in ecosystems altered by environmental change

"It's like being the hero of your own story": perceptions of musical skill development for the beginner cellist

Background: When children commence learning a musical instrument, they are introduced to a diverse range of skills from the cognitive, expressive and psychomotor domains. Children’s capacity to adopt and integrate these musical skills can directly affect their progress and influence ongoing interest. However, as many of these skills are unfamiliar to the beginner musician, their development requires specialised support, deliberate attention and focussed practice. The outcomes of these learning processes can also be a critical to children’s future musical engagement. Children’s lived experience of musical instrument skill acquisition is rarely examined in music education research; therefore, the current paper adopts a novel case study approach to investigate how children perceive and manage musical skill development. Intrapersonal factors and interpersonal relationships including those with the teacher, who is the principal researcher, are also examined. Aims: 1. To investigate seven-year-old children’s lived experience of cello skill development within the first 18-months of tuition. 2. To investigate how children’s musical skill development is affected by intrapersonal factors and interpersonal relationships. 3. To investigate how the experience and perceptions of skill development in early learning influences children’s longer-term musical engagement. Method: Through a longitudinal Action Research methodology, 14 seven-year-old children’s lived experiences of learning the cello were tracked across the first 18-months of tuition. Interpretative Phenomenological Analysis of interviews with the children and their parents were integrated with the teacher-researcher’s recorded observations from work with the children. Results: During the early stages of learning, children prioritised the development of skills in one of the three learning domains and this was attributed to initial competencies and affinities at the beginner level. As tuition progressed, teaching and learning challenges included ensuring that all skill sets developed according to the children’s individual, differentiated needs. Central to this developmental process was how the children’s intrapersonal factors interacted with their interpersonal relationships to shape their learning behaviour at home and in the instrumental music studio. Regardless of skill level or ability, all of the children measured their process in musical skill development through critical evaluation of their sound production. The children’s sophisticated perception of sound included discerning nuanced difference in quality of tone, intonation, volume, fluency and timbre. Production of an ideal sound that integrated these qualities was described as an aspirational goal in practice and performance. Sound was perceived also by the children as a powerful conduit for self-expression and musical communication. In this context, musical skill development fulfilled children’s creative needs and satisfied their desire to be seen and hear by others as capable musicians. This result generated growth in the children’s sense of agency and autonomy. When the complex process of skill attainment, sound production and musical expression was achieved successfully, students experienced transformed representations of their internal selves that positively impacted their emotional states. These transformative experiences were linked to a close affinity with their cello and this was evidenced by the children’s use of language devices such as metaphor, simile, analogy and imaginative narrative to describe how skill development strengthened their bond with the instrument. Further, some children ascribed anthropomorphic traits to their instruments, defining them as a person or ally and assigning names and gender pronouns. Investigation of students’ learning over time indicated that children who experienced beneficial interpersonal growth and productive interpersonal relationships through musical skill development maintained active longer-term musical engagement. These children described imagining themselves in positive performance and learning environments in their projected musical futures. Taken together, the findings from this investigation of children’s perceptions of musical skill development highlight how instrumental music learning can profoundly affect children’s inner worlds. The breadth and depth of the experience contributed to the children’s enjoyment in engagement and affected motivation to continue with their musical development. Conclusions: This research, conducted by the teacher as researcher, makes a unique contribution to the literature by identifying the importance of children’s perception of sound in the process of cognitive, physical and emotional engagement with musical skill development. It identifies how this can have a transformative effect on a child’s sense of self and influence their future musical engagement. Implications: Monitoring children’s perception of sound production and its impact on musical expression in the development of skills in the three learning domains is integral to instrumental music teaching and fosters meaningful, ongoing engagement outcomes

A Library of Integrated Spectra of Galactic Globular Clusters

We present a new library of integrated spectra of 40 Galactic globular clusters, obtained with the Blanco 4-m telescope and the R-C spectrograph at the Cerro Tololo Interamerican Observatory. The spectra cover the range ~ 3350 -- 6430 A with ~ 3.1 A (FWHM) resolution. The spectroscopic observations and data reduction were designed to integrate the full projected area within the cluster core radii in order to properly sample the light from stars in all relevant evolutionary stages. The S/N values of the flux-calibrated spectra range from 50 to 240/A at 4000 A and from 125 to 500/A at 5000 A. The selected targets span a wide range of cluster parameters, including metallicity, horizontal-branch morphology, Galactic coordinates, Galactocentric distance, and concentration. The total sample is thus fairly representative of the entire Galactic globular cluster population and should be valuable for comparison with similar integrated spectra of unresolved stellar populations in remote systems. For most of the library clusters, our spectra can be coupled with deep color-magnitude diagrams and reliable metal abundances from the literature to enable the calibration of stellar population synthesis models. In this paper we present a detailed account of the observations and data reduction. The spectral library is publicly available in electronic format from the National Optical Astronomical Observatory website.Comment: 39 Pages, including 2 tables and 15 Figures. To appear in the Astrophysical Journal, Supplement Serie

The Tully-Fisher Relation of Barred Galaxies

We present new data exploring the scaling relations, such as the Tully-Fisher relation (TFR), of bright barred and unbarred galaxies. A primary motivation for this study is to establish whether barredness correlates with, and is a consequence of, virial properties of galaxies. Various lines of evidence suggest that dark matter is dominant in disks of bright unbarred galaxies at 2.2 disk scale lengths, the point of peak rotation for a pure exponential disk. We test the hypothesis that the TF plane of barred high surface brightness galaxies is offset from the mean TFR of unbarred galaxies, as might be expected if barred galaxies are ``maximal'' in their inner parts. We use existing and new TF data to search for basic structural differences between barred and unbarred galaxies. Our new data consist of 2-dimensional Halpha velocity fields derived from SparsePak integral field spectroscopy (IFS) and V,I-band CCD images collected at the WIYN Observatory for 14 strongly barred galaxies. We use WIYN/SparsePak (2-D) velocity fields to show that long-slit (1-D) spectra yield reliable circular speed measurements at or beyond 2.2 disk scale lengths, far from any influence of the bar. This enables us to consider line width measurements from extensive TF surveys which include barred and nonbarred disks and derive detailed scaling relation comparisons. We find that for a given luminosity, barred and unbarred galaxies have comparable structural and dynamical parameters, such as peak velocities, scale lengths, or colors. In particular, the location of a galaxy in the TF plane is independent of barredness. In a global dynamical sense, barred and unbarred galaxies behave similarly and are likely to have, on average, comparable fractions of luminous and dark matter at a given radius. (abridged)Comment: Accepted for publication in the ApJ (September 1, 2003 issue, v594). Appendix figures with I-band image and superimposed 2-D velocity field plus rotation curves must be downloaded separately (due to size constraints) from http://www.astro.ubc.ca/people/courteau/public/courteau03_TFbars.ps.g

Qualitative Evaluation of Web-Based Digital Intervention to Prevent and Reduce Excessive Alcohol Use and Harm Among Young People Aged 14-15 Years: A "Think-Aloud" Study

BACKGROUND: In the United Kingdom, despite some downward trends in alcohol use among young people, over one-fifth of young people reported excessive alcohol use in the past month, which is associated with short- and long-term harm to health. Digital interventions to reduce alcohol use, such as websites, among young people present an appealing and cost-effective mode of intervention that can be integrated into the education system. However, relatively few school-based digital alcohol-focused interventions have been developed and evaluated for young people in the United Kingdom. OBJECTIVE: This study aims to develop a novel web-based intervention, Rethink Alcohol, to prevent and reduce excessive alcohol use and related harm among young people aged between 14 and 15 years, and explore the views of young people, teachers, and youth workers in relation to the content, design, and usability of the intervention. METHODS: Intervention development followed the person-based approach, using theories of social norms and social influence. Qualitative "Think-Aloud" interviews, either one-to-one or paired, were conducted while participants perused and worked through the web-based intervention, talking aloud. Participants included 20 young people (12 female, 8 male), 5 youth workers (4 female, 1 male), 3 teachers (2 male, 1 female), and 1 (male) clinical professional, recruited via youth groups and professional networks. Interviews were audio recorded, transcribed verbatim, and analyzed thematically. RESULTS: The prototype web-based intervention included normative feedback, information, a quiz, interactive activities, and scenarios. On a rating scale of impressions from poor (1) to excellent (5), participants gave an average score of 3.6/5. A total of 5 themes were identified: content, credibility of the website, making the website easy to understand, design and navigation, and suitability for the audience. These themes reflected views that the content was interesting, credible, informative, and embodied a neutral and nonjudgmental tone, but stronger messaging was needed regarding social pressures and short-term risks regarding safety and risk behavior alongside clarity around pathways of risk; credibility and trustworthiness of information were critical features, determined in part, by the professionalism of design and referencing of sources of information provided; and messages should be succinct and come to life through design and interactive features. CONCLUSIONS: Together, the data illustrated the importance and challenge of communicating nuanced alcohol-focused public health messages to young people in concise, clear, nonjudgmental, and appealing ways. Young people report interest in clear, credible, neutral, and interactive messages regarding social pressures and short-term risks of alcohol use via a web-based intervention. There is scope for optimization and feasibility testing of the Rethink Alcohol intervention

The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales

The Next Generation Virgo Cluster Survey has recently determined the luminosity function of galaxies in the core of the Virgo cluster down to unprecedented magnitude and surface brightness limits. Comparing simulations of cluster formation to the derived central stellar mass function, we attempt to estimate the stellar-to-halo-mass ratio (SHMR) for dwarf galaxies, as it would have been before they fell into the cluster. This approach ignores several details and complications, e.g., the contribution of ongoing star formation to the present-day stellar mass of cluster members, and the effects of adiabatic contraction and/or violent feedback on the subhalo and cluster potentials. The final results are startlingly simple, however; we find that the trends in the SHMR determined previously for bright galaxies appear to extend down in a scale-invariant way to the faintest objects detected in the survey. These results extend measurements of the formation efficiency of field galaxies by two decades in halo mass, or five decades in stellar mass, down to some of the least massive dwarf galaxies known, with stellar masses of $\sim 10^5 M_\odot$.Comment: 18 pages, 12 figures; published in ApJ July 1st 201