2,337 research outputs found
Integrating methods for determining length-at-age to improve growth estimates for two large scombrids
Fish growth is commonly estimated from length-at-age data
obtained from otoliths. There are several techniques for estimating length-at-age from otoliths including 1) direct observed counts of annual increments; 2) age adjustment based on a categorization of otolith margins; 3) age adjustment based on known periods of spawning and annuli formation; 4) back-calculation to all annuli, and 5) back-calculation to the last annulus only. In this study we
compared growth estimates (von Bertalanffy growth functions) obtained from the above five methods for estimating length-at-age from otoliths for two large scombrids: narrow-barred Spanish mackerel (Scomberomorus
commerson) and broad-barred king mackerel (Scomberomorus semifasciatus). Likelihood ratio tests revealed that the largest differences in growth occurred between the back-calculation methods and the observed and adjusted methods for both species of mackerel. The pattern, however, was
more pronounced for S. commerson than for S. semifasciatus, because of the pronounced effect of gear selectivity
demonstrated for S. commerson. We propose a method of substituting length-at-age data from observed or adjusted methods with back-calculated length-at-age data to provide
more appropriate estimates of population growth than those obtained with the individual methods alone, particularly when faster growing young fish are disproportionately
selected for. Substitution of observed or adjusted length-at-age data with back-calculated length-at-age data provided more realistic estimates of length for younger ages than observed or adjusted methods as well as more
realistic estimates of mean maximum length than those derived from backcalculation methods alone
A developmental study of behavioural differences in adolescents with regard to the type of parental discipline.
Dept. of Psychology. Paper copy at Leddy Library: Theses & Major Papers - Basement, West Bldg. / Call Number: Thesis1981 .T635. Source: Masters Abstracts International, Volume: 40-07, page: . Thesis (M.A.)--University of Windsor (Canada), 1981
Localisation of gamma-ray interaction points in thick monolithic CeBr3 and LaBr3:Ce scintillators
Localisation of gamma-ray interaction points in monolithic scintillator
crystals can simplify the design and improve the performance of a future
Compton telescope for gamma-ray astronomy. In this paper we compare the
position resolution of three monolithic scintillators: a 28x28x20 mm3 (length x
breadth x thickness) LaBr3:Ce crystal, a 25x25x20 mm3 CeBr3 crystal and a
25x25x10 mm3 CeBr3 crystal. Each crystal was encapsulated and coupled to an
array of 4x4 silicon photomultipliers through an optical window. The
measurements were conducted using 81 keV and 356 keV gamma-rays from a
collimated 133Ba source. The 3D position reconstruction of interaction points
was performed using artificial neural networks trained with experimental data.
Although the position resolution was significantly better for the thinner
crystal, the 20 mm thick CeBr3 crystal showed an acceptable resolution of about
5.4 mm FWHM for the x and y coordinates, and 7.8 mm FWHM for the z-coordinate
(crystal depth) at 356 keV. These values were obtained from the full position
scans of the crystal sides. The position resolution of the LaBr3:Ce crystal was
found to be considerably worse, presumably due to the highly diffusive optical
in- terface between the crystal and the optical window of the enclosure. The
energy resolution (FWHM) measured for 662 keV gamma-rays was 4.0% for LaBr3:Ce
and 5.5% for CeBr3. The same crystals equipped with a PMT (Hamamatsu R6322-100)
gave an energy resolution of 3.0% and 4.7%, respectively
Assessment of novel gear designs to reduce interactions between species
This project tested modified gillnets designed by commercial net fishers in the Queensland East Coast Inshore Finfish Fishery (ECIFF) to try and identify gears that would mitigate and/or improve interactions between fishing nets and Species of Conservation Interest (SOCI). The study also documents previously unrecognised initiatives by pro-active commercial net fishers that reflect a conservation-minded approach to their fishing practices, which is the opposite of what is perceived publicly.
Between 2011 and 2014, scientists from James Cook University and the Queensland Department of Agriculture and Fisheries teamed with commercial fishers representing the Queensland Seafood Industry Association and the Moreton Bay Seafood Industry Association to conduct field trials of various modified net designs under normal fishery conditions. Trials were conducted in Moreton Bay (southern part of the fishery) and Bowling Green Bay (northern) and tested different net designs developed by fishers to improve the nature of interactions between net fishing gear and SOCI
A Sub-arcsecond Survey Toward Class 0 Protostars in Perseus: Searching for Signatures of Protostellar Disks
We present a CARMA 1.3 mm continuum survey toward 9 Class 0 protostars in the
Perseus molecular cloud at 0.3 (70 AU) resolution. This
study approximately doubles the number of Class 0 protostars observed with
spatial resolutions 100 AU at millimeter wavelengths, enabling the presence
of protostellar disks and proto-binary systems to be probed. We detect
flattened structures with radii 100 AU around 2 sources (L1448 IRS2 and
Per-emb-14) and these sources may be strong disk candidates.
Marginally-resolved structures with position angles within 30 of
perpendicular to the outflow are found toward 3 protostars (L1448 IRS3C, IRAS
03282+3035, and L1448C) and are considered disk candidates. Two others (L1448
IRS3B and IRAS 03292+3039) have resolved structure, possibly indicative of
massive inner envelopes or disks; L1448 IRS3B also has a companion separated by
0.9 (210 AU). IC348-MMS does not have well-resolved
structure and the candidate first hydrostatic core L1451-MMS is marginally
resolved on 1 scales. The strong disk candidate sources were
followed-up with CO () observations, detecting velocity
gradients consistent with rotation, but it is unclear if the rotation is
Keplerian. We compare the observed visibility amplitudes to radiative transfer
models, finding that visibility amplitude ratios suggest a compact component
(possibly a disk) is necessary for 5 of 9 Class 0 sources; envelopes alone may
explain the other 4 systems. We conclude that there is evidence for the
formation of large disks in the Class 0 phase with a range of radii and masses
dependent upon their initial formation conditions.Comment: Accepted to ApJ, 58 pages, 19 Figures, 5 Table
Evidence of the Boyer Model of Scholarship in Counselor Education
This study delineated how the Boyer (1990) model of scholarship has been implemented in counselor education. The taxonomy of scholarship was delineated: Scholarship of Discovery, Scholarship of Teaching, Scholarship of Application, and Scholarship of Integration. The Journal of Counseling and Development and Counselor Education and Supervision were examined from 2000 to 2008. Examples of scholarship from each journal were identified. Evidence of the Boyer model in premier counseling journals suggests a consistency of approach between this model and scholarly activities in counselor education. An expanded view of scholarship may have positive implications for scholarly activity in graduate education and pretenured faculty
Reflective Learning within a Counselor Education Curriculum
The literature on counselor education and supervision acknowledged the importance of self-awareness and self-reflection in supervision. As counselor educators we emphasized a need to prepare students for reflective practice prior to the practicum experience. In order to investigate how active learning and opportunities were being infused, we conducted an inquiry into the core curriculum of a Community Counseling program. Learning activities were categorized and charted according to the eight core areas of counselor education. This case study analysis provides a guide for a curriculum review of reflective learning and a catalyst for further inquiry
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