Telehealth Tool

This tool examines current knowledge regarding telehealth

Rural Characteristics Tool

This tool examines current knowledge and confidence in teaching rural characteristics

Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of December 27th, 2004 with the AMANDA-II detector

On December 27th 2004, a giant gamma flare from the Soft Gamma-ray Repeater 1806-20 saturated many satellite gamma-ray detectors. This event was by more than two orders of magnitude the brightest cosmic transient ever observed. If the gamma emission extends up to TeV energies with a hard power law energy spectrum, photo-produced muons could be observed in surface and underground arrays. Moreover, high-energy neutrinos could have been produced during the SGR giant flare if there were substantial baryonic outflow from the magnetar. These high-energy neutrinos would have also produced muons in an underground array. AMANDA-II was used to search for downgoing muons indicative of high-energy gammas and/or neutrinos. The data revealed no significant signal. The upper limit on the gamma flux at 90% CL is dN/dE < 0.05 (0.5) TeV^-1 m^-2 s^-1 for gamma=-1.47 (-2). Similarly, we set limits on the normalization constant of the high-energy neutrino emission of 0.4 (6.1) TeV^-1 m^-2 s^-1 for gamma=-1.47 (-2).Comment: 14 pages, 3 figure

Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

The IceCube neutrino detector is a cubic kilometer TeV to PeV neutrino detector under construction at the geographic South Pole. The dominant population of neutrinos detected in IceCube is due to meson decay in cosmic-ray air showers. These atmospheric neutrinos are relatively well-understood and serve as a calibration and verification tool for the new detector. In 2006, the detector was approximately 10% completed, and we report on data acquired from the detector in this configuration. We observe an atmospheric neutrino signal consistent with expectations, demonstrating that the IceCube detector is capable of identifying neutrino events. In the first 137.4 days of livetime, 234 neutrino candidates were selected with an expectation of 211 +/- 76.1(syst.) +/- 14.5(stat.) events from atmospheric neutrinos

First year performance of the IceCube neutrino telescope

The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence by surface and deep-ice detectors separated by up to 2.5 km

The ICECUBE prototype string in AMANDA

The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole Station. Each OM contains a photomultiplier tube (PMT) that detects photons of Cherenkov light generated in the ice by muons and electrons. IceCube is a cubic-kilometer-sized expansion of Amanda currently being built at the South Pole. In IceCube the PMT signals are digitized already in the optical modules and transmitted to the surface. A prototype string of 41 OMs equipped with this new all-digital technology was deployed in the Amanda array in the year 2000. In this paper we describe the technology and demonstrate that this string serves as a proof of concept for the IceCube array. Our investigations show that the OM timing accuracy is 5 ns. Atmospheric muons are detected in excellent agreement with expectations with respect to both angular distribution and absolute rate

Limits to the muon flux from neutralino annihilations in the Sun with the AMANDA detector

A search for an excess of muon-neutrinos from neutralino annihilations in the Sun has been performed with the AMANDA-II neutrino detector using data collected in 143.7 days of live-time in 2001. No excess over the expected atmospheric neutrino background has been observed. An upper limit at 90% confidence level has been obtained on the annihilation rate of captured neutralinos in the Sun, as well as the corresponding muon flux limit at the Earth, both as functions of the neutralino mass in the range 100 GeV-5000 GeV.Comment: 13 pages, 3 figures. Submitted to Astropart. Phy

Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop

On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cherenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cut-off, we determined the particle energy spectrum in the energy range 0.6 to 7.6 GeV. This is the first such spectral measurement using a single instrument with a well defined viewing direction. We compare the IceTop spectrum and its time evolution with previously published results and outline plans for improved resolution of future solar particle spectra.Comment: To appear in Astrophysical Journal Letters, 6 pages, 4 figure

The IceCube Data Acquisition System: Signal Capture, Digitization, and Timestamping

IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital Optical Modules (DOMs), detect, digitize and timestamp the signals from optical Cherenkov-radiation photons. The DOM Main Board (MB) data acquisition subsystem is connected to the central DAQ in the IceCube Laboratory (ICL) by a single twisted copper wire-pair and transmits packetized data on demand. Time calibration is maintained throughout the array by regular transmission to the DOMs of precisely timed analog signals, synchronized to a central GPS-disciplined clock. The design goals and consequent features, functional capabilities, and initial performance of the DOM MB, and the operation of a combined array of DOMs as a system, are described here. Experience with the first InIce strings and the IceTop stations indicates that the system design and performance goals have been achieved.Comment: 42 pages, 20 figures, submitted to Nuclear Instruments and Methods

Relationship-Based Care: Effects on Patient Satisfaction

The purpose of the study was to evaluate the hospitalized patients\u27 perceptions of their care from nurses on selected patient care units implementing the Relationship-Based Care (RBC) model within a tertiary acute care hospital located in a Northern Plains state. This quasi-experimental research study employed a pretest and posttest design with a control group. There were two hypotheses. The first hypothesis was that patients who are exposed to RBC will report higher perceived levels of satisfaction with their care than patients who are not exposed to RBC. The second hypothesis was that patients\u27 perceived levels of satisfaction with nursing care will improve from pre-implementation of RBC to six months post-implementation. The instrument used to measure patients\u27 perceived levels of satisfaction with nursing care was the 10 item Caring Factor Survey (CFS). The pretest CFS was administered to the experimental (wave one) units and control (waves two, three, and four) units for a one month period prior to the launch of the RBC intervention on the experimental units. The unit-specific RBC interventions occurred over a six month period on the experimental units. The posttest CFS surveys were then distributed for a one month period on both the experimental units and control units. CFS data were analyzed using ANOVA to examine both of the hypotheses. Nonparametric analysis using the Kruskal-Wallis test was also conducted due to the unequal sample sizes. There were not differences in the parametric and non-parametric results. The study had a total of 171 pretest and posttest participants, which includes 117pretest participants and 54 posttest participants on the 10 selected patient care units included in the four waves of the study. The first hypothesis examined the experimental group (wave one) compared to the control group (waves two, three, and four) differences in posttest scores. The mean CFS score (range 10-70) between the experimental group and the control group post tests only had a 2.13 difference as the control group started with a high posttest score indicating an already established caring environment within the health care organization. The first hypothesis results were not statistically significant (p = 0.21). The second hypothesis examined the experimental group (wave one) pretest and posttest scores. The mean CFS score (range 10-70) from pretest to posttest had a 5.72 difference, which is almost a six point improvement. The second hypothesis results were statistically significant (p = 0.02). The study found RBC implementation improved patients\u27 perceived levels of satisfaction from pretest to posttest. Through RBC focused interventions on acute patient care units, patients\u27 were more satisfied with their care while hospitalized. This study confirms the necessity for nurses to meet the patients\u27 and their families\u27 needs and desires while ensuring colleagues are caring for each other as well as themselves using the RBC model