A Case Study on Factors Influencing Retention of Mental Health Clinicians in a New Hampshire Community Mental Health Center

This study examined the perspectives of master-level clinical mental health providers and members of leadership at a Community Mental Health Center (CMHC) in New Hampshire, to understand clinician and leadership perspectives as to why master-level providers choose to continue working at CMHCs. Most prior research on turnover in such organizations has focused on why so many leave their positions, however this study instead focuses on factors related to the decision to stay at a specific CMHC in an urban area of New Hampshire. A single case study method was utilized to focus on masters-level mental health care providers with additional interviews with leadership at the CMHC. Some of the findings that will be explored is what draws providers to community mental health centers, the importance of connections with colleagues and leadership, and aspects of why master-level providers stay. The study contributes to the understanding of clinician retention in community mental health centers and provides recommendations for master-level providers, CMHC leadership, and clinical mental health educators. Some of the overarching themes that surface from the data were around why clinicians remain in the CMHC, the reasons why providers do the work they do each day, the draw to CMHC, and reasons why people master-level providers consider leaving a CMHC. Connections with leadership and supervisor were very important in why clinicians want to stay at the CMHC. Licensure contracts were also an area that was explored in this research. Clinicians and members of leadership provided their perspective on licensure contracts and the implementation of the contracts. This dissertation is available in open access at AURA (https://aura.antioch.edu/) and OhioLINK ETD Center (https://etd.ohiolink.edu)

The Doha Round and Globalization: A Failure of World Economic Development?

The objective of this thesis is to analyze the WTO’s Doha Round and its numerous developmental objectives, assess the major issues that led to its stagnation, as well as examine the economic prospects for developing nations and the potential future of international trade and development

BICEP: a large angular scale CMB polarimeter

We describe the design and expected performance of BICEP, a millimeter wave receiver designed to measure the polarization of the cosmic microwave background. BICEP uses an array of polarization sensitive bolometers operating at 100 and 150 GHz to measure polarized signals over a 20 degree field of view with 1 degree resolution. BICEP is designed with particular attention to systematic effects which can potentially degrade the polarimetric fidelity of the observations. BICEP is optimized to detect the faint signature of a primordial gravitational wave background which is a generic prediction of inflationary cosmologies

CMB polarimetry with BICEP: instrument characterization, calibration, and performance

BICEP is a ground-based millimeter-wave bolometric array designed to target the primordial gravity wave signature on the polarization of the cosmic microwave background (CMB) at degree angular scales. Currently in its third year of operation at the South Pole, BICEP is measuring the CMB polarization with unprecedented sensitivity at 100 and 150 GHz in the cleanest available 2% of the sky, as well as deriving independent constraints on the diffuse polarized foregrounds with select observations on and off the Galactic plane. Instrument calibrations are discussed in the context of rigorous control of systematic errors, and the performance during the first two years of the experiment is reviewed.Comment: 12 pages, 15 figures, updated version of a paper accepted for Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, Proceedings of SPIE, 7020, 200

Absolute polarization angle calibration using polarized diffuse Galactic emission observed by BICEP

We present a method of cross-calibrating the polarization angle of a polarimeter using BICEP Galactic observations. \bicep\ was a ground based experiment using an array of 49 pairs of polarization sensitive bolometers observing from the geographic South Pole at 100 and 150 GHz. The BICEP polarimeter is calibrated to +/-0.01 in cross-polarization and less than +/-0.7 degrees in absolute polarization orientation. BICEP observed the temperature and polarization of the Galactic plane (R.A= 100 degrees ~ 270 degrees and Dec. = -67 degrees ~ -48 degrees). We show that the statistical error in the 100 GHz BICEP Galaxy map can constrain the polarization angle offset of WMAP Wband to 0.6 degrees +\- 1.4 degrees. The expected 1 sigma errors on the polarization angle cross-calibration for Planck or EPIC are 1.3 degrees and 0.3 degrees at 100 and 150 GHz, respectively. We also discuss the expected improvement of the BICEP Galactic field observations with forthcoming BICEP2 and Keck observations.Comment: 13 pages, 10 figures and 2 tables. To appear in Proceedings of SPIE Astronomical Telescopes and Instrumentation 201

Sorgo Silage, Sorgo Fodder, and Cottonseed Hulls as Roughages in Rations for Fattening Calves.

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BICEP: a large angular scale CMB polarimeter

We describe the design and expected performance of BICEP, a millimeter wave receiver designed to measure the polarization of the cosmic microwave background. BICEP uses an array of polarization sensitive bolometers operating at 100 and 150 GHz to measure polarized signals over a 20 degree field of view with 1 degree resolution. BICEP is designed with particular attention to systematic effects which can potentially degrade the polarimetric fidelity of the observations. BICEP is optimized to detect the faint signature of a primordial gravitational wave background which is a generic prediction of inflationary cosmologies

Speech Communication

Contains reports on two research projects.National Institutes of Health (Grant 2 ROl1 NS04332)National Institutes of Health (Training Grant 5 T32 NS07040)C.J. LeBel FellowshipsNational Science Foundation (Grant BNS77-26871