Tutor Handbooks: Heuristic Texts for Negotiating Difference in a Globalized World

I would like to begin this article by telling a true story. When I was a graduate student earning my doctoral degree, I worked in a writing center on a midsized and predominantly white university campus. Every week I attended and sometimes facilitated the writing center’s tutor education workshop. At one of these meetings, an undergraduate tutor from a Euro- American background said that one of the things she liked about working at the writing center was that if she had a question about grammar during a conference with a client, she could simply lean over to the next table and ask another tutor for advice. In response to this statement, an African-American tutor said that she would never ask another tutor for grammar help because she felt that doing so would undermine her authority and lead clients to question her competence in Standard American English. At this point a bilingual Asian-American tutor said that clients often doubted her ability to tutor based solely on her appearance. For many of her American clients she was too foreign, while for many of her international clients she was not American enough. This discussion was a revelation for many of the Euro-American tutors, since it had never occurred to them that one’s physical appearance could bring his or her linguistic competence into question. All of the tutors learned a great deal from this remarkable discussion, and the theory and practice of the writing center shifted in ways that more fully accounted for the experiences of tutors from diverse backgrounds. I tell this story for two reasons.University Writing Cente

Can Modern Nuclear Hamiltonians Tolerate a Bound Tetraneutron?

I show that it does not seem possible to change modern nuclear Hamiltonians to bind a tetraneutron without destroying many other successful predictions of those Hamiltonians. This means that, should a recent experimental claim of a bound tetraneutron be confirmed, our understanding of nuclear forces will have to be significantly changed. I also point out some errors in previous theoretical studies of this problem.Comment: 4 pages, 4 figures Revision corrects a pronou

The scaling of secondary craters

Secondary craters are common features around fresh planetary-scale primary impact craters throughout most of the Solar System. They derive from the ejection phase of crater formation, thus secondary scaling relations provide constraints on parameters affecting ejection processes. Secondary crater fields typically begin at the edge of the continuous ejecta blankets (CEB) and extend out several crater radii. Secondaries tend to have rounded rims and bilateral symmetry about an axis through the primary crater's center. Prominent secondary chains can extend inward across the CEB close to the rim. A simple method for comparing secondary crater fields was employed: averaging the diameters and ranges from the center of the primary crater of the five largest craters in a secondary crater field. While not as much information is obtained about individual crater fields by this method as in more complete secondary field mapping, it facilitates rapid comparison of many secondary fields. Also, by quantifying a few specific aspects of the secondary crater field, this method can be used to construct scaling relations for secondary craters

Mechanical and thermal properties of planetologically important ices

Two squences of ice composition were proposed for the icy satellites: a dense nebula model and a solar nebula model. Careful modeling of the structure, composition, and thermal history of satellites composed of these various ices requires quantitative information on the density, compressibility, thermal expansion, heat capacity, and thermal conductivity. Equations of state were fitted to the density data of the molecular ices. The unusual thermal and mechanical properties of the molecular and binary ices suggest a larger range of phenomena than previously anticipated, sufficiently complex perhaps to account for many of the unusual geologic phenomena found on the icy satellites

Iapetus: Tectonic structure and geologic history

Many papers have been written about the surface of Iapetus, but most of these have discussed either the nature of the strongly contrasting light and dark materials or the cratering record. Little has been said about other geologic features on Iapetus, such as tectonic structures, which would provide constraints on Iapetus' thermal history. Most references have suggested that there is no conclusive evidence for any tectonic activity, even when thermal history studies indicate that there should be. However, a new study of Iapetus' surface involving the use of stereo pairs, an extensive tectonic network has been recognized. A few new observations concerning the craters and dark material were also made. Thus the geology and geologic history of Iapetus can be more fully outlined than before. The tectonic network is shown along with prominent craters and part of the dark material in the geologic/tectonic sketch map. The topology of crater rims and scarps are quite apparent and recognizable in the different image pairs. The heights and slopes of various features given are based on comparison with the depths of craters 50 to 100 km in diameter, which are assumed to have the same depths as craters of similar diameter on Rhea and Titania

Crater morphology and morphometry on the Uranian satellites

Fresh craters on the icy Uranian satellites exhibit a range of morphologies similar to craters on the icy satellites of Jupiter and Saturn. The general structural features found in the craters are described. Estimates of transition diameters from simple to complex crater morphologies are given for the five large Uranian satellites and 1985U1, and plotted with transition diameters on other bodies against surface gravity. Possible large-scale impacts are discussed

Beaming effect from increased-index photonic crystal waveguides

We study the beaming effect of light for the case of increased-index photonic crystal (PhC) waveguides, formed through the omission of low-dielectric media in the waveguide region. We employ the finite-difference time-domain numerical method for characterizing the beaming effect and determining the mechanisms of loss and the overall efficiency of the directional emission. We find that, while this type of PhC waveguides is capable of producing a highly collimated emission as was demonstrated experimentally, the inherent characteristics of the structure result in a restrictively low efficiency in the coupling of light into the collimated beam of light.Comment: 4 pages, 5 figures, submitted to Applied Physics