7,412 research outputs found
Decision making processes in people with symptoms of acute myocardial infarction: qualitative study
Objective To identify, the themes that influence decision making processes used by patients with symptoms of acute myocardial infarction. Design Qualitative study using semistructured interviews. Setting Two district hospitals in North Yorkshire. Participants 22 patients admitted to hospital with confirmed second, third, or fourth acute myocardial infarction. Main outcome measure Patients' perceptions of their experience between the onset of symptoms and the decision to seek medical help. Results Six main themes that influence the decision making process were identified: appraisal of In symptoms, perceived risk, previous experience, psychological and emotional factors, use of the NHS, and context of the event. Conclusions Knowledge of symptoms may not be enough to promote prompt action in the event of an acute myocardial infarction. Cognitive and emotional processes, individual beliefs and values, and the influence of the context of the event should also be considered in individual interventions designed to reduce delay in the event of symptoms of acute myocardial infarction
The Effect of LHC Jet Data on MSTW PDFs
We consider the effect on LHC jet cross sections on partons distribution
functions (PDFs), in particular the MSTW2008 set of PDFs. We first compare the
published inclusive jet data to the predictions using MSTW2008, finding a very
good description. We also use the parton distribution reweighting procedure to
estimate the impact of these new data on the PDFs, finding that the combined
ATLAS 2.76 TeV and 7 TeV data, and CMS 7 TeV data have some significant impact.
We then also investigate the impact of ATLAS, CMS and D0 dijet data using the
same techniques. In this case we investigate the effect of using different
scale choices for the NLO cross section calculation. We find that the dijet
data is generally not completely compatible with the corresponding inclusive
jet data, often tending to pull PDFs, particularly the gluon distribution, away
from the default values. However, the effect depends on the dijet data set used
as well as the scale choice. We also note that conclusions may be affected by
limiting the pull on the data luminosity chosen by the best fit, which is
sometimes a number of standard deviations. Finally we include the inclusive jet
data in a new PDF fit explicitly. This enables us to check the consistency of
the exact result with that obtained from the reweighting procedure. There is
generally good, but not full quantitative agreement. Hence, the conclusion
remains that MSTW2008 PDFs already fit the published jet data well, but the
central values and uncertainties are altered and improved respectively by
significant, but not dramatic extent by inclusion of these data.Comment: 63 pages, 50 figures. Final version. Some added discussion and
improved figure
Levels of genetic polymorphism: marker loci versus quantitative traits
Species are the units used to measure ecological diversity and alleles are the units of genetic diversity. Genetic variation within and among species has been documented most extensively using allozyme electrophoresis. This reveals wide differences in genetic variability within, and genetic distances among, species, demonstrating that species are not equivalent units of diversity. The extent to which the pattern observed for allozymes can be used to infer patterns of genetic variation in quantitative traits depends on the forces generating and maintaining variability. Allozyme variation is probably not strictly neutral but, nevertheless, heterozygosity is expected to be influenced by population size and genetic distance will be affected by time since divergence. The same is true for quantitative traits influenced by many genes and under weak stabilizing selection. However, the limited data available suggest that allozyme variability is a poor predictor of genetic variation in quantitative traits within populations. It is a better predictor of general phenotypic divergence and of postzygotic isolation between populations or species, but is only weakly correlated with prezygotic isolation. Studies of grasshopper and planthopper mating signal variation and assortative mating illustrate how these characters evolve independently of general genetic and morphological variation. The role of such traits in prezygotic isolation, and hence speciation, means that they will contribute significantly to the diversity of levels of genetic variation within and among species
On the magnetospheric ULF wave counterpart of substorm onset
One nearāubiquitous signature of substorms observed on the ground is the azimuthal structuring of the onset auroral arc in the minutes prior to onset. Termed auroral beads, these optical signatures correspond to concurrent exponential increases in ground ultralow frequency (ULF) wave power and are likely the result of a plasma instability in the magnetosphere. Here, we present a case study showing the development of auroral beads from a Time History of Events and Macroscale Interactions during Substorms (THEMIS) allāsky camera with near simultaneous exponential increases in auroral brightness, ionospheric and conjugate magnetotail ULF wave power, evidencing their intrinsic link. We further present a survey of magnetic field fluctuations in the magnetotail around substorm onset. We find remarkably similar superposed epoch analyses of ULF power around substorm onset from space and conjugate ionospheric observations. Examining periods of exponential wave growth, we find the groundā and spaceābased observations to be consistent, with average growth rates of ā¼0.01 sā1, lasting for ā¼4 min. Crossācorrelation suggests that the spaceābased observations lead those on the ground by approximately 1ā1.5 min. Meanwhile, spacecraft located premidnight and ā¼10 RE downtail are more likely to observe enhanced wave power. These combined observations lead us to conclude that there is a magnetospheric counterpart of auroral beads and exponentially increasing ground ULF wave power. This is likely the result of the linear phase of a magnetospheric instability, active in the magnetotail for several minutes prior to auroral breakup
DK-1D: a drift-kinetic simulation tool for modelling the shear AlfvƩn wave and its interaction with collisionless plasma
We present a highly accurate tool for the simulation of shear Alfven waves (SAW) in collisionless plasma. SAW are important in space plasma environments because for small perpendicular scale lengths they can support an electric field parallel to the ambient magnetic field. Electrons can be accelerated by the parallel electric field and these waves have been implicated as the source of vibrant auroral displays. However, the parallel electric field carried
by SAW is small in comparison to the perpendicular electric field of the wave, making it difficult to measure directly in the laboratory, or by satellites in the near-Earth plasma environment. In this paper, we present a simulation code that provides a means to study in detail the SAW-particle interaction in both space and laboratory
plasma. Using idealised, small-amplitude propagating waves with a single perpendicular wavenumber, the simulation code accurately reproduces the damping rates and parallel electric field amplitudes predicted by linear theory for varying temperatures and perpendicular scale lengths. We present a rigorous kinetic derivation of the parallel electric field strength for small-amplitude SAW and show that commonly-used inertial and kinetic approximations are valid except for where the ratio of thermal to Alfv\'{e}n speed is between 0.7 and 1.0. We also present nonlinear simulations of large-amplitude waves and show that in cases of strong damping, the damping rates and parallel electric field strength deviate from linear predictions when wave energies are greater than only a few percent of the plasma
kinetic energy, a situation which is often observed in the
magnetosphere. The drift-kinetic code provides reliable, testable predictions of the parallel electric field strength which can be investigated directly in the laboratory, and will help to bridge the gap between studies of SAW in man-made and naturally occuring plasma
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