Zero-G Workstation Design

Zero-g workstations were designed throughout manned spaceflight, based on different criteria and requirements for different programs. The history of design of these workstations is presented along with a thorough evaluation of selected Skylab workstations (the best zero-g experience available on the subject). The results were applied to on-going and future programs, with special emphasis on the correlation of neutral body posture in zero-g to workstation design. Where selected samples of shuttle orbiter workstations are shown as currently designed and compared to experience gained during prior programs in terms of man machine interface design, the evaluations were done in a generic sense to show the methods of applying evaluative techniques

COMPASS: a 2.6m telescope for CMBR polarization studies

COMPASS (COsmic Microwave Polarization at Small Scale) is an experiment devoted to measuring the polarization of the CMBR. Its design and characteristics are presented

Breaking the Redshift Deadlock - I: Constraining the star formation history of galaxies with sub-millimetre photometric redshifts

Future extragalactic sub-millimetre and millimetre surveys have the potential to provide a sensitive census of the level of obscured star formation in galaxies at all redshifts. While in general there is good agreement between the source counts from existing SCUBA (850um) and MAMBO (1.25mm) surveys of different depths and areas, it remains difficult to determine the redshift distribution and bolometric luminosities of the sub-millimetre and millimetre galaxy population. This is principally due to the ambiguity in identifying an individual sub-millimetre source with its optical, IR or radio counterpart which, in turn, prevents a confident measurement of the spectroscopic redshift. Additionally, the lack of data measuring the rest-frame FIR spectral peak of the sub-millimetre galaxies gives rise to poor constraints on their rest-frame FIR luminosities and star formation rates. In this paper we describe Monte-Carlo simulations of ground-based, balloon-borne and satellite sub-millimetre surveys that demonstrate how the rest-frame FIR-sub-millimetre spectral energy distributions (250-850um) can be used to derive photometric redshifts with an r.m.s accuracy of +/- 0.4 over the range 0 < z < 6. This opportunity to break the redshift deadlock will provide an estimate of the global star formation history for luminous optically-obscured galaxies [L(FIR) > 3 x 10^12 Lsun] with an accuracy of 20 per cent.Comment: 14 pages, 22 figures, submitted to MNRAS, replaced with accepted versio

Flow cone – new CPTU add-on module trialled in Halden silt

publishedVersio

An Exploratory Study Of Student Satisfaction With University Web Page Design

This exploratory study evaluates the satisfaction of students with a web-based information system at a medium-sized regional university. The analysis provides a process for simplifying data interpretation in captured student user feedback. Findings indicate that student classifications, as measured by demographic and other factors, determine satisfaction levels towards various web sources of information. Differences in satisfaction levels across student groups based on gender, age, minority status, employment, and current course load were found. Implications for university web designers and university administrators are considered and discussed

CFS/ME OG AKTIVITETSAVPASNING En litteraturstudie om mennesker med CFS/ME sine opplevelser av aktivitetsavpasning (pacing)

Problemstilling: “Hvordan oppleves aktivitetsavpasning (Pacing) som en mestringsstrategi for personer med mild-moderat CFS/ME?”. Formål: Formålet med denne oppgaven er å undersøke hva forskning sier om pasienter med Chronic fatigue syndrome/Myalgic encephalomyelitis (CFS/ME) sine opplevelser knyttet til aktivitetsavpasning. Metode: Foretatt systematisk litteratursøk for å finne kvalitative studier som viser hvilke opplevelser mennesker med CFS/ME har til aktivitetsavpasning. De vitenskapelige artiklene som blir brukt i litteraturgjennomgangen er presentert i ulike databaser: EBSCO (Academic search elite), Pubmed og EMBASE. Aveyards tematiske analysemodell beskrevet i Thidemann ble benyttet for å analysere resultatene. Resultat: Aktivitetsavpasning ble i stor grad ansett som positivt, hvor denne mestringsstrategien ble brukt for å forhindre forverring av symptomer. Det gav et endret aktivitetsmønster, bevissthet på gjennomførelse av aktiviteter, energinivå og å få en positiv tankegang, samt motivasjon. Samtidig finnes det også utfordringer for å kunne ta i bruk aktivitetsavpasning som, symptomer, manglende kontroll, følelser og personlige egenskaper. Konklusjon: Gjennom utførelsen av denne litteraturstudien kommer det frem at mennesker med CFS/ME opplever aktivitetsavpasning som en nyttig mestringsstrategi. Det er videre behov for nyere og større studier som omhandler erfaringer, men også studier som viser effekt. Det er nødvendig for å kunne gi anbefalinger i videre praksis.publishedVersio

Morphine and fentanyl exposure during therapeutic hypothermia does not impair neurodevelopment

Background Hypothermia-treated and intubated infants with moderate or severe hypoxic-ischemic encephalopathy (HIE) usually receive morphine for sedation and analgesia (SA) during therapeutic hypothermia (TH) and endotracheal ventilation. Altered drug pharmacokinetics in this population increases the risk of drug accumulation. Opioids are neurotoxic in preterm infants. In term infants undergoing TH, the long-term effects of morphine exposure are unknown. We examined the effect of opioid administration during TH on neurodevelopmental outcome and time to extubation after sedation ended. Methods In this prospectively collected population-based cohort of 282 infants with HIE treated with TH (2007–2017), the cumulative opioid dose of morphine and equipotent fentanyl (10–60 µg/kg/h) administered during the first week of life was calculated. Clinical outcomes and concomitant medications were also collected. Of 258 survivors, 229 underwent Bayley-3 neurodevelopmental assessments of cognition, language and motor function at 18–24 months. Multivariate stepwise linear regression analysis was used to examine the relation between cumulative opioid dose and Bayley-3 scores. Three severity-groups (mild-moderate-severe) were stratified by early (<6 h) amplitude-integrated electroencephalography (aEEG) patterns. Findings The cumulative dose of opioid administered as SA during TH was median (IQR) 2121 µg/kg (1343, 2741). Time to extubation was independent of SA dose (p > 0.2). There was no significant association between cumulative SA dose and any of the Bayley-3 domains when analysing the entire cohort or any of the aEEG severity groups. Interpretation Higher cumulative opioid doses in TH-treated infants with HIE was not associated with worse Bayley-3 scores at 18–24 months of age. Funding The Bristol cooling program was funded by the Children's Medical Research Charity SPARKS managing donations for our research from the UK and US, the UK Moulton Foundation, the Lærdal Foundation for Acute Medicine in Norway and the Norwegian Research Council (JKG)

New Measurements of Fine-Scale CMB Polarization Power Spectra from CAPMAP at Both 40 and 90 GHz

We present new measurements of the cosmic microwave background (CMB) polarization from the final season of the Cosmic Anisotropy Polarization MAPper (CAPMAP). The data set was obtained in winter 2004-2005 with the 7 m antenna in Crawford Hill, New Jersey, from 12 W-band (84-100 GHz) and 4 Q-band (36-45 GHz) correlation polarimeters with 3.3' and 6.5' beamsizes, respectively. After selection criteria were applied, 956 (939) hours of data survived for analysis of W-band (Q-band) data. Two independent and complementary pipelines produced results in excellent agreement with each other. A broad suite of null tests as well as extensive simulations showed that systematic errors were minimal, and a comparison of the W-band and Q-band sky maps revealed no contamination from galactic foregrounds. We report the E-mode and B-mode power spectra in 7 bands in the range 200 < l < 3000, extending the range of previous measurements to higher l. The E-mode spectrum, which is detected at 11 sigma significance, is in agreement with cosmological predictions and with previous work at other frequencies and angular resolutions. The BB power spectrum provides one of the best limits to date on B-mode power at 4.8 uK^2 (95% confidence).Comment: 19 pages, 17 figures, 2 tables, submitted to Ap