3,646 research outputs found
A new and efficient intelligent collaboration scheme for fashion design
Technology-mediated collaboration process has been extensively studied for over a decade. Most applications with collaboration concepts reported in the literature focus on enhancing efficiency and effectiveness of the decision-making processes in objective and well-structured workflows. However, relatively few previous studies have investigated the applications of collaboration schemes to problems with subjective and unstructured nature. In this paper, we explore a new intelligent collaboration scheme for fashion design which, by nature, relies heavily on human judgment and creativity. Techniques such as multicriteria decision making, fuzzy logic, and artificial neural network (ANN) models are employed. Industrial data sets are used for the analysis. Our experimental results suggest that the proposed scheme exhibits significant improvement over the traditional method in terms of the time–cost effectiveness, and a company interview with design professionals has confirmed its effectiveness and significance
Mapping far-IR emission from the central kiloparsec of NGC 1097
Using photometry of NGC 1097 from the Herschel PACS (Photodetector Array
Camera and Spectrometer) instrument, we study the resolved properties of
thermal dust continuum emission from a circumnuclear starburst ring with a
radius ~ 900 pc. These observations are the first to resolve the structure of a
circumnuclear ring at wavelengths that probe the peak (i.e. lambda ~ 100
micron) of the dust spectral energy distribution. The ring dominates the
far-infrared (far-IR) emission from the galaxy - the high angular resolution of
PACS allows us to isolate the ring's contribution and we find it is responsible
for 75, 60 and 55% of the total flux of NGC 1097 at 70, 100 and 160 micron,
respectively. We compare the far-IR structure of the ring to what is seen at
other wavelengths and identify a sequence of far-IR bright knots that
correspond to those seen in radio and mid-IR images. The mid- and far-IR band
ratios in the ring vary by less than +/- 20% azimuthally, indicating modest
variation in the radiation field heating the dust on ~ 600 pc scales. We
explore various explanations for the azimuthal uniformity in the far-IR colors
of the ring including a lack of well-defined age gradients in the young stellar
cluster population, a dominant contribution to the far-IR emission from dust
heated by older (> 10 Myr) stars and/or a quick smoothing of local enhancements
in dust temperature due to the short orbital period of the ring. Finally, we
improve previous limits on the far-IR flux from the inner ~ 600 pc of NGC 1097
by an order of magnitude, providing a better estimate of the total bolometric
emission arising from the active galactic nucleus and its associated central
starburst.Comment: Accepted for publication in the A&A Herschel Special Editio
Pearling instability of nanoscale fluid flow confined to a chemical channel
We investigate the flow of a nano-scale incompressible ridge of
low-volatility liquid along a "chemical channel": a long, straight, and
completely wetting stripe embedded in a planar substrate, and sandwiched
between two extended less wetting solid regions. Molecular dynamics
simulations, a simple long-wavelength approximation, and a full stability
analysis based on the Stokes equations are used, and give qualitatively
consistent results. While thin liquid ridges are stable both statically and
during flow, a (linear) pearling instability develops if the thickness of the
ridge exceeds half of the width of the channel. In the flowing case periodic
bulges propagate along the channel and subsequently merge due to nonlinear
effects. However, the ridge does not break up even when the flow is unstable,
and the qualitative behavior is unchanged even when the fluid can spill over
onto a partially wetting exterior solid region.Comment: 17 pages, 12 figures, submitted to Physics of Fluids, fixed equation
numbering after Eq. (17
A well-separated pairs decomposition algorithm for k-d trees implemented on multi-core architectures
Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.Variations of k-d trees represent a fundamental data structure used in Computational Geometry with numerous applications in science. For example particle track tting in the software of the LHC experiments, and in simulations of N-body systems in the study of dynamics of interacting galaxies, particle beam physics, and molecular dynamics in biochemistry. The many-body tree methods devised by Barnes and Hutt in the 1980s and the Fast Multipole Method introduced in 1987 by Greengard and Rokhlin use variants of k-d trees to reduce the computation time upper bounds to O(n log n) and even O(n) from O(n2). We present an algorithm that uses the principle of well-separated pairs decomposition to always produce compressed trees in O(n log n) work. We present and evaluate parallel implementations for the algorithm that can take advantage of multi-core architectures.The Science and Technology Facilities Council, UK
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