A Study of Communication Patterns of Teahers Using Teacher Aides as Compared to Those not Using Teacher Aides

Problem . The purpose of this study was to determine whether the use of teacher aides would show any change in teachers\u27 patterns of communication. Procedure Teachers of three schools, paired with three other schools by factors such as plant facilities, student enrollment and student/ teacher ratio, served as the control group. The teachers of the three other schools served as the experimental group with teacher aides employed as the criterion measure. Ten trained observers in interaction analysis recorded the verbal classroom behavior of these teachers in the fall and again in the spring of the school term to indicate whether a change in verbal behavior was found as a result of utilizing teacher aides. The data-was studied by recording the observations in ten-column by ten-row matrices. The statistical techniques employed in the analysis of the data were t tests for comparing mean changes between the fall and spring observations and analysis of covariance for differences between the control and experimental teachers. Results and Conclusions The findings of this study support the following general conclusions: 1. The employment of teacher aides causes little change in teachers\u27 classroom behavior in areas such as asking questions, lecturing, accepting feelings of students,\u27 praising or encouraging students, giving directions, allowing self-initiated student talk or in the amount of silence or confusion when tested as individual units. 2. Teachers using teacher aides allowed student talk in response to questions more than those teachers not using teacher aides. 3. An increase of indirect teacher response following student talk was found in those schools using teacher aides. 4. The amount of silence or confusion in the classroom following student or teacher talk showed no change when teacher aides were utilized. 5. No difference was found in the use of extended indirect or extended direct influence by teachers using teacher aides. 6. Direct teacher response following student talk did not change with the addition of teacher aides. 7. Differences were not found in teachers indirect/direct ratio nor in their revised indirect/direct ratio of communication when teacher aides were utilized. 8. In general, teacher aides have very little effect on changes in verbal behavior of classroom teachers. Teachers must have the desire for change and be willing to accept professional guidance in bringinging about changes in their classroom verbal behavior

Spectroscopy of Giant Stars in the Pyxis Globular Cluster

The Pyxis globular cluster is a recently discovered globular cluster that lies in the outer halo (R_{gc} ~ 40 kpc) of the Milky Way. Pyxis lies along one of the proposed orbital planes of the Large Magellanic Cloud (LMC), and it has been proposed to be a detached LMC globular cluster captured by the Milky Way. We present the first measurement of the radial velocity of the Pyxis globular cluster based on spectra of six Pyxis giant stars. The mean heliocentric radial velocity is ~ 36 km/sec, and the corresponding velocity of Pyxis with respect to a stationary observer at the position of the Sun is ~ -191 km/sec. This radial velocity is a large enough fraction of the cluster's expected total space velocity, assuming that it is bound to the Milky Way, that it allows strict limits to be placed on the range of permissible transverse velocities that Pyxis could have in the case that it still shares or nearly shares an orbital pole with the LMC. We can rule out that Pyxis is on a near circular orbit if it is Magellanic debris, but we cannot rule out an eccentric orbit associated with the LMC. We have calculated the range of allowed proper motions for the Pyxis globular cluster that result in the cluster having an orbital pole within 15 degrees of the present orbital pole of the LMC and that are consistent with our measured radial velocity, but verification of the tidal capture hypothesis must await proper motion measurement from the Space Interferometry Mission or HST. A spectroscopic metallicity estimate of [Fe/H] = -1.4 +/- 0.1 is determined for Pyxis from several spectra of its brightest giant; this is consistent with photometric determinations of the cluster metallicity from isochrone fitting.Comment: 22 pages, 5 figures, aaspp4 style, accepted for publication in October, 2000 issue of the PAS

Spectrum Modal Analysis for the Detection of Low-Altitude Windshear with Airborne Doppler Radar

A major obstacle in the estimation of windspeed patterns associated with low-altitude windshear with an airborne pulsed Doppler radar system is the presence of strong levels of ground clutter which can strongly bias a windspeed estimate. Typical solutions attempt to remove the clutter energy from the return through clutter rejection filtering. Proposed is a method whereby both the weather and clutter modes present in a return spectrum can be identified to yield an unbiased estimate of the weather mode without the need for clutter rejection filtering. An attempt will be made to show that modeling through a second order extended Prony approach is sufficient for the identification of the weather mode. A pattern recognition approach to windspeed estimation from the identified modes is derived and applied to both simulated and actual flight data. Comparisons between windspeed estimates derived from modal analysis and the pulse-pair estimator are included as well as associated hazard factors. Also included is a computationally attractive method for estimating windspeeds directly from the coefficients of a second-order autoregressive model. Extensions and recommendations for further study are included

The extent of NGC 6822 revealed by its C stars population

Using the CFH12K camera, we apply the four band photometric technique to identify 904 carbon stars in an area 28' x 42' centered on NGC 6822. A few C stars, outside of this area were also discovered with the Las Campanas Swope Telescope. The NGC 6822 C star population has an average I of 19.26 mag leading to an average absolute I magnitude of -4.70 mag, a value essentially identical to the mean magnitude obtained for the C stars in IC 1613. Contrary to stars highlighting the optical image of NGC 6822, C stars are seen at large radial distances and trace a huge slightly elliptical halo which do not coincide with the huge HI cloud surrounding NGC6822. The previously unknown stellar component of NGC 6822 has a exponential scale length of 3.0' +/- 0.1' and can be traced to five scale lengths. The C/M ratio of NGC 6822 is evaluated to br 1.0 +/- 0.2.Comment: accepted, to be published in A

The Role of Arachidonic Acid Metabolites in Mononuclear Phagocytic Cell Interactions

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/65162/1/j.1365-4362.1986.tb04543.x.pd

C‐C chemokine‐induced eosinophil chemotaxis during allergic airway inflammation

The production of eosinophil‐specific chemotactic factors during allergic airway responses may be a pivotal event resulting in eosinophil accumulation, activation, and airway damage. Recent studies have identified specific chemokines that may play crucial roles in recruitment of eosinophils to the site of allergic reactions. In this study we have utilized an established model of schistosome egg antigen (SEA)‐mediated allergic responses to examine the role of specific C‐C chemokines [macrophage inflammatory protein‐1α (MIP‐1α), RANTES, and monocyte chemoattractant protein‐1 (MCP‐1)] in eosinophil recruitment. We have previously identified a role for MIP‐1α in eosinophil accumulation in the lung and airway during allergic airway inflammation. We extend those studies using in vitro eosinophil chemotaxis to establish that both MIP‐1α and RANTES are potent eosinophil chemotactic factors in lungs during allergic airway responses. Morphometric analysis demonstrated a peribronchial accumulation of eosinophils within the lungs beginning at 8 h, peaking at 24 h, and plateauing at 48–96 h after allergen (SEA) challenge. Utilizing whole‐lung homogenates from allergen‐challenged mice, in vitro eosinophil chemotactic assays demonstrated significant increases in eosinophil chemotactic activity with 8‐h lung homogenates and peak activity with samples from 24‐h lung homogenates. These data correlated with the morphometric analysis of peribronchial eosinophil accumulation in situ. When lung homogenates from allergen‐challenged mice were preincubated in vitro with antibodies specific for MIP‐1α, RANTES, or MCP‐1, a significant reduction in eosinophil chemotaxis was observed with only MIP‐1α and RANTES neutralization. Altogether, these studies indicate that RANTES and MIP‐1α are major eosinophil chemotactic factors produced during allergic airway responses. J. Leukoc. Biol. 60:573–578; 1996.Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/141543/1/jlb0573.pd