16,478 research outputs found
Cluster observations of the midaltitude cusp under strong northward interplanetary magnetic field
We report on a multispacecraft cusp observation lasting more than 100 min. We
determine the cusp boundary motion and reveal the effect on the cusp size of the
interplanetary magnetic field (IMF) changing from southward to northward. The cusp
shrinks at the beginning of the IMF rotation and it reexpands at the rate of 0.40°
invariant latitude per hour under stable northward IMF. On the basis of plasma signatures
inside the cusp, such as counterstreaming electrons with balanced fluxes, we propose
that pulsed dual lobe reconnection operates during the time of interest. SC1 and
SC4 observations suggest a long-term regular periodicity of the pulsed dual reconnection,
which we estimate to be ~1–5 min. Further, the distances from the spacecraft to
the reconnection site are estimated on the basis of observations from three satellites. The
distance determined using SC1 and SC4 observations is ~15 RE and that determined
from SC3 data is ~8 RE. The large-scale speed of the reconnection site sunward motion is
~16 km s-1. We observe also a fast motion of the reconnection site by SC1, which
provides new information about the transitional phase after the IMF rotation. Finally, a
statistical study of the dependency of plasma convection inside the cusp on the IMF clock
angle is performed. The relationship between the cusp stagnation, the dual lobe
reconnection process, and the IMF clock angle is discussed
On the size and composition of particles in polar stratospheric clouds
Attenuation measurements of the solar radiation between 1.5 and 15 micron wavelengths were performed with the airborne (DC-8) JPL MARK 4 interferometer during the 1987 Antarctic Expedition. The opacities not only provide information about the abundance of stratospheric gases but also about the optical depths of polar stratospheric clouds (PSCs) at wavelengths of negligible gas absorption (windows). The optical depth of PSCs can be determined for each window once the background attenuation, due to air-molecules and aerosol has been filtered out with a simple extinction law. The ratio of optical thicknesses at different wavelengths reveals information about particle size and particle composition. Among the almost 700 measured spectra only a few PSC cases exist. PSC events are identified by sudden reductions in the spectrally integrated intensity value and are also verified with backscattering data from an upward directed lidar instrument, that was mounted on the DC-8. For the selected case on September 21st at 14.40 GMT, lidar data indicate an optically thin cloud at 18k and later an additional optically thick cloud at 15 km altitude. All results still suffer from: (1) often arbitrary definitions of a clear case, that often already may have contained PSC particles and (2) noise problems that restrict the calculations of optical depths to values larger than 0.001. Once these problems are handled, this instrument may become a valuable tool towards a better understanding of the role PSCs play in the Antarctic stratosphere
Unbiased Comparative Evaluation of Ranking Functions
Eliciting relevance judgments for ranking evaluation is labor-intensive and
costly, motivating careful selection of which documents to judge. Unlike
traditional approaches that make this selection deterministically,
probabilistic sampling has shown intriguing promise since it enables the design
of estimators that are provably unbiased even when reusing data with missing
judgments. In this paper, we first unify and extend these sampling approaches
by viewing the evaluation problem as a Monte Carlo estimation task that applies
to a large number of common IR metrics. Drawing on the theoretical clarity that
this view offers, we tackle three practical evaluation scenarios: comparing two
systems, comparing systems against a baseline, and ranking systems. For
each scenario, we derive an estimator and a variance-optimizing sampling
distribution while retaining the strengths of sampling-based evaluation,
including unbiasedness, reusability despite missing data, and ease of use in
practice. In addition to the theoretical contribution, we empirically evaluate
our methods against previously used sampling heuristics and find that they
generally cut the number of required relevance judgments at least in half.Comment: Under review; 10 page
An X-ray and Optical Investigation of the Environments Around Nearby Radio Galaxies
Investigations of the cluster environment of radio sources have not shown a
correlation between radio power and degree of clustering. However, it has been
demonstrated that extended X-ray luminosity and galaxy clustering do exhibit a
positive correlation. This study investigates a complete sample of 25 nearby (z
less than 0.06) radio galaxies which are not cataloged members of Abell
clusters. The environment of these radio galaxies is studied in both the X-ray
and the optical by means of the ROSAT All-Sky Survey (RASS), ROSAT pointed
observations, and the Palomar optical Digitized Sky Survey (DSS). X-ray
luminosities and extents are determined from the RASS, and the DSS is used to
quantify the degree of clustering via the spatial two-point correlation
coefficient, Bgg. Of the 25 sources, 20 are greater than sigma detections in
the X-ray and 11 possessed Bgg's significantly in excess of that expected for
an isolated galaxy. Adding the criterion that the X-ray emission be resolved,
10 of the radio galaxies do appear to reside in poor clusters with extended
X-ray emission suggestive of the presence of an intracluster medium. Eight of
these galaxies also possess high spatial correlation coefficients. Taken
together, these data suggest that the radio galaxies reside in a low richness
extension of the Abell clusters. The unresolved X-ray emission from the other
galaxies is most likely associated with AGN phenomena. Furthermore, although
the sample size is small, it appears that the environments of FR I and FR II
sources differ. FR I's tend to be more frequently associated with extended
X-ray emission (10 of 18), whereas FR II's are typically point sources or
non-detections in the X-ray (none of the 7 sources exhibit extended X-ray
emission).Comment: 28 page postscript file including figures and tables, plus one
landscape table and 5 GIF figure
Low voltage control of ferromagnetism in a semiconductor p-n junction
The concept of low-voltage depletion and accumulation of electron charge in
semiconductors, utilized in field-effect transistors (FETs), is one of the
cornerstones of current information processing technologies. Spintronics which
is based on manipulating the collective state of electron spins in a
ferromagnet provides complementary technologies for reading magnetic bits or
for the solid-state memories. The integration of these two distinct areas of
microelectronics in one physical element, with a potentially major impact on
the power consumption and scalability of future devices, requires to find
efficient means for controlling magnetization electrically. Current induced
magnetization switching phenomena represent a promising step towards this goal,
however, they relay on relatively large current densities. The direct approach
of controlling the magnetization by low-voltage charge depletion effects is
seemingly unfeasible as the two worlds of semiconductors and metal ferromagnets
are separated by many orders of magnitude in their typical carrier
concentrations. Here we demonstrate that this concept is viable by reporting
persistent magnetization switchings induced by short electrical pulses of a few
volts in an all-semiconductor, ferromagnetic p-n junction.Comment: 11 pages, 4 figure
Gravitational Wave Chirp Search: Economization of PN Matched Filter Bank via Cardinal Interpolation
The final inspiral phase in the evolution of a compact binary consisting of
black holes and/or neutron stars is among the most probable events that a
network of ground-based interferometric gravitational wave detectors is likely
to observe. Gravitational radiation emitted during this phase will have to be
dug out of noise by matched-filtering (correlating) the detector output with a
bank of several templates, making the computational resources required
quite demanding, though not formidable. We propose an interpolation method for
evaluating the correlation between template waveforms and the detector output
and show that the method is effective in substantially reducing the number of
templates required. Indeed, the number of templates needed could be a factor
smaller than required by the usual approach, when the minimal overlap
between the template bank and an arbitrary signal (the so-called {\it minimal
match}) is 0.97. The method is amenable to easy implementation, and the various
detector projects might benefit by adopting it to reduce the computational
costs of inspiraling neutron star and black hole binary search.Comment: scheduled for publicatin on Phys. Rev. D 6
Orthopaedic surgeons: as strong as an ox and almost twice as clever? Multicentre prospective comparative study
Objective To compare the intelligence and grip strength of orthopaedic surgeons and anaesthetists
Changing thoughts, changing practice: examining the delivery of a group CBT-based intervention in a school setting
Promoting mental health and well-being for children and young people in the UK has attracted increasing prominence in recent years and has been a focus for government strategy within health and education. Training and practice in educational psychology has increasingly focused on developing skills and expertise to provide therapeutic support within school contexts, at an early stage of need. One approach, Cognitive Behaviour Therapy (CBT), has been heralded as an effective, evidence-based intervention for anxiety. This research examines the factors influencing the outcomes of a group CBT-based intervention, run by an Educational Psychologist (EP), in a school setting. The findings suggest that influential variables included pupil identification, measures of change applied and the role of school staff. It is concluded that EPs can play a key role in increasing access to psychological therapies, alongside considering due caution in relation to the application of traditional clinical approaches in school contexts
R-modes in Neutron Stars with Crusts: Turbulent Saturation, Spin-down, and Crust Melting
Rossby waves (r-modes) have been suggested as a means to regulate the spin
periods of young or accreting neutron stars, and also to produce observable
gravitational wave radiation. R-modes involve primarily transverse,
incompressive motions of the star's fluid core. However, neutron stars gain
crusts early in their lives: therefore, r-modes also imply shear in the fluid
beneath the crust. We examine the criterion for this shear layer to become
turbulent, and derive the rate of dissipation in the turbulent regime. Unlike
dissipation from a viscous boundary layer, turbulent energy loss is nonlinear
in mode energy and can therefore cause the mode to saturate at amplitudes
typically much less than unity. This energy loss also reappears as heat below
the crust. We study the possibility of crust melting as well as its
implications for the spin evolution of low-mass X-ray binaries. Lastly, we
identify some universal features of the spin evolution that may have
observational consequences.Comment: 12 pages, 4 figures, submitted to Ap
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