4,770 research outputs found
Ferroelectricity in the xAg2Nb4O11–(1−x)Na2Nb4O11 solid solution
Compositions in the (AgxNa1-x)2Nb4O11 solid solution have been prepared by a conventional
solid state method. Composites containing Ag2Nb4O11 have been shown to be ferroelectric
and the Curie temperature shown to decrease from 149 °C at x = 1 to 62 °C at x = 0.7. Roomtemperature
compositions with x ≤ 0.7 are monoclinic, while those with x ≥ 0.8 are
rhombohedral with structures consistent with the relevant end-members. At x = 0.75, the
structure was mainly rhombohedral but with coexistence of the monoclinic structure,
indicating the proximity of a phase boundary
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British fair play: sport across diasporas at the BBC World Service
This chapter uses archive material to explore the role of sports broadcasting on the BBC World Service in the twentieth century.Whereas the service's early audiences were expatriate British listeners, the BBC WS recruited different diasporic audiences later into the twentieth century.This chapter looks at specific sports and at the accommodations of the tensions between the WS's links with both Empire and with discourses of impartiaility, which have led to both endurances in the postcolonialist aspects of sport as well as new opportunities for reconfigurations of diaspora
Electron diffraction of tilted perovskites
Simulations of electron diffraction patterns for each of the
known perovskite tilt systems have been performed. The
conditions for the appearance of superlattice reflections
arising from rotations of the octahedra are modified to take
into account the effects of different tilt systems for kinematical
diffraction. The use of selected-area electron diffraction as a
tool for perovskite structure determination is reviewed and
examples are included
AgNb7O18 : an ergodic relaxor ferroelectric
AgNb7O18 is an ergodic relaxor ferroelectric at room temperature with an incipient transition to the nonergodic state. Electron diffraction confirms a locally polar symmetry, while X-ray diffraction perceives a nonpolar structure. All ions are repelled away from zones where NbO6 octahedra are edge-sharing
Growth is Failing the Poor: The Unbalanced Distribution of the Benefits and Costs of Global Economic Growth
During 1990-2001, only 0.6 per cent of additional global income per capita contributed to reducing poverty below the $1-a-day line, down from 2.2 per cent during 1981-1990, and barely half the poor’s share of global income. Coupled with the constraints on global growth associated with climate change, and the disproportionately adverse net impact of climate change on the poor, this casts serious doubt on the dominant view that global growth should be the primary means of poverty reduction. Rather than growth, policies and the global economic system should focus directly on achieving social and environmental objectives.Economic growth, income distribution, world inequality, poverty, environment, climate change
Supervised exercise training and increased physical activity to reduce cardiovascular disease risk in women with polycystic ovary syndrome: Study protocol for a randomized controlled feasibility trial
Background: Polycystic ovary syndrome (PCOS) affects up to 20% of women and is characterised by higher amounts of visceral fat, obesity, insulin resistance, dyslipidemia and reproductive and cardiometabolic complications. Increased oxidised low-density lipoprotein (LDL) concentrations have been associated with an increased risk of cardiovascular disease (CVD)-related events. Oxidised LDL is rarely used as a marker for CVD risk in PCOS-related studies despite its widely accepted role in atherogenesis and the increased risk factors associated with PCOS. Additionally, prolonged periods of sedentary behaviour can negatively affect metabolic health. No studies have specifically examined the effects of reducing sedentary behaviour on CVD risk in PCOS with a lifestyle physical activity intervention. The aim of the current study is to measure the feasibility of a randomised controlled trial (RCT) examining the effects of supervised exercise and reducing sedentary behaviour in women with PCOS on CVD risk. Methods/design: A feasibility, exploratory RCT will be conducted. Fifty-one pre-menopausal females will be randomly allocated between an exercise group (EG), a lifestyle physical activity group (LPAG) and a control group. Participants in the EG will undertake a 12-week supervised aerobic exercise programme. The LPAG will aim to increase daily physical activity and reduce sedentary behaviour for 12 weeks. The control group will not take part in any intervention. Primary outcomes are feasibility and acceptability of the intervention and procedures. Secondary outcomes are oxidised LDL, aerobic fitness, blood lipid profile, fasting glucose and insulin, testosterone and inflammatory markers. Discussion: PCOS is associated with various increased risk factors for CVD, including hypertension, dyslipidemia, abdominal obesity, insulin resistance, and inflammation. Whether oxidised LDL has a role in this increased risk is not yet known. The present study aims to measure the feasibility of implementing structured exercise training and/or increased lifestyle physical activity in women with PCOS, so that a subsequent adequately powered RCT can be designed. The results from the study will be used to refine the interventions and determine the acceptability of the study design. A limitation is that some self-monitoring in the lifestyle physical activity group may not be reliable or replicable, for example inputting information about time spent cleaning/gardening
Turbulent Mixing in Stars: Theoretical Hurdles
A program is outlined, and first results described, in which fully
three-dimensional, time dependent simulations of hydrodynamic turbulence are
used as a basis for theoretical investigation of the physics of turbulence in
stars. The inadequacy of the treatment of turbulent convection as a diffusive
process is discussed. A generalization to rotation and magnetohydrodynamics is
indicated, as are connection to simulations of 3D stellar atmospheres.Comment: 5 pages, 1 figure, IAU Symposium 265, 200
Takeoff/approach noise for a model counterrotation propeller with a forward-swept upstream rotor
A scale model of a counterrotating propeller with forward-swept blades in the forward rotor and aft-swept blades in the aft rotor (designated F39/A31) has been tested in the NASA Lewis 9- by 15-Foot Anechoic Wind Tunnel. This paper presents aeroacoustic results at a takeoff/approach condition of Mach 0.20. Laser Doppler velocimeter results taken in a plane between the two rotors are also included to quantify the interaction flow field. The intention of the forward-swept design is to reduce the magnitude of the forward rotor tip vortex and/or wakes which impinge on the aft rotor, thus lowering the interaction tone levels. A reference model propeller (designated F31/A31), having aft-swept blades in both rotors, was also tested. Aeroelastic performance of the F39/A31 propeller was disappointing. The forward rotor tip region tended to untwist toward higher effective blade angles under load. The forward rotor also exhibited steady state blade flutter at speeds and loadings well below the design condition. The noise results, based on sideline acoustic data, show that the interaction tone levels were up to 8 dB higher with the forward-swept design compared to those for the reference propeller at similar operating conditions, with these tone level differences extending down to lower propeller speeds where flutter did not occur. These acoustic results are for a poorly-performing forward-swept propeller. It is quite possible that a properly-designed forward-swept propeller would exhibit substantial interaction tone level reductions
Spitzer Observations of Comet 67P/Churyumov-Gerasimenko at 5.5-4.3 AU From the Sun
We report Spitzer Space Telescope observations of comet
67P/Churyumov-Gerasimenko at 5.5 and 4.3 AU from the Sun, post-aphelion. Comet
67P is the primary target of the European Space Agency's Rosetta mission. The
Rosetta spacecraft will rendezvous with the nucleus at heliocentric distances
similar to our observations. Rotationally resolved observations at 8 and 24
microns (at a heliocentric distance, rh, of 4.8 AU) that sample the size and
color-temperature of the nucleus are combined with aphelion R-band light curves
observed at the Very Large Telescope (VLT) and yield a mean effective radius of
2.04 +/- 0.11 km, and an R-band geometric albedo of 0.054 +/- 0.006. The
amplitudes of the R-band and mid-infrared light curves agree, which suggests
that the variability is dominated by the shape of the nucleus. We also detect
the dust trail of the comet at 4.8 and 5.5 AU, constrain the grain sizes to be
less than or similar to 6 mm, and estimate the impact hazard to Rosetta. We
find no evidence for recently ejected dust in our images. If the activity of
67P is consistent from orbit to orbit, then we may expect the Rosetta
spacecraft will return images of an inactive or weakly active nucleus as it
rendezvous with the comet at rh = 4 AU in 2014.Comment: 19 pages, 2 tables, 10 figures. Accepted for publication in the
Astronomical Journa
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