440 research outputs found
Color Changes in Electronic Endoscopic Images Caused by Image Compression
In recent years, recording of color still images into magnetoâoptical video disks has been
increasingly used as a method for recording electronic endoscopic images. In this case,
image compression is often used to reduce the volume and cost of recording media and
also to minimize the time required for image recording and playback. With this in mind,
we recorded 8 images into a magneto-optical video disk in 4 image compression modes
(no compression, weak compression, moderate compression, and strong compression)
using the Joint Photographic Image Coding Experts Group (JPEG) system, which is a
widely used and representative method for compressing color still images, in order to
determine the relationship between the degree of image compression and the color
information in electronic endoscopic images. The acquired images were transferred to an
image processor using an offline system. A total of 10 regions of interest (ROls) were
selected, and red (R), green (G), and blue (B) images were obtained using different
compression modes. From histograms generated for these images, mean densities of R,
G, and B in each ROI were measured and analyzed. The results revealed that color
changes were greater for B, which had the lowest density, than for R or G as the degree
of compression was increased
A Massive Jet Ejection Event from the Microquasar SS 433 Accompanying Rapid X-Ray Variability
Microquasars occasionally exhibit massive jet ejections which are distinct
from the continuous or quasi-continuous weak jet ejections. Because those
massive jet ejections are rare and short events, they have hardly been observed
in X-ray so far. In this paper, the first X-ray observation of a massive jet
ejection from the microquasar SS 433 with the Rossi X-ray Timing Explorer
(RXTE) is reported. SS 433 undergoing a massive ejection event shows a variety
of new phenomena including a QPO-like feature near 0.1 Hz, rapid time
variability, and shot-like activities. The shot-like activity may be caused by
the formation of a small plasma bullet. A massive jet may be consist of
thousands of those plasma bullets ejected from the binary system. The size,
mass, internal energy, and kinetic energy of the bullets and the massive jet
are estimated.Comment: 21 pages including 5 figures, submitted to Ap
Anomalous Metal-Insulator Transition in Filled Skutterudite CeOsSb
Anomalous metal-insulator transition observed in filled skutterudite
CeOsSb is investigated by constructing the effective tight-binding
model with the Coulomb repulsion between f electrons. By using the mean field
approximation, magnetic susceptibilities are calculated and the phase diagram
is obtained. When the band structure has a semimetallic character with small
electron and hole pockets at and H points, a spin density wave
transition with the ordering vector occurs due to the
nesting property of the Fermi surfaces. Magnetic field enhances this phase in
accord with the experiments.Comment: 4 pages, 4 figure
A Calculation of Baryon Diffusion Constant in Hot and Dense Hadronic Matter Based on an Event Generator URASiMA
We evaluate thermodynamical quantities and transport coefficients of a dense
and hot hadronic matter based on an event generator URASiMA (Ultra-Relativistic
AA collision Simulator based on Multiple Scattering Algorithm). The statistical
ensembles in equilibrium with fixed temperature and chemical potential are
generated by imposing periodic boundary condition to the simulation of URASiMA,
where energy density and baryon number density is conserved. Achievement of the
thermal equilibrium and the chemical equilibrium are confirmed by the common
value of slope parameter in the energy distributions and the saturation of the
numbers of contained particles, respectively. By using the generated ensembles,
we investigate the temperature dependence and the chemical potential dependence
of the baryon diffusion constant of a dense and hot hadronic matter.Comment: 15 pages, 5 figures, LaTeX2
Magnified Examination of Small Colorectal Polyps Using a Prototype Electronic Endoscope
Magnifying electronic endoscopes are frequently used to evaluate the pit patterns of the
colorectal mucosa, but such endoscopes suffer from a number of problems. For example, they
tend to have long, hard tips and heavy controller sections. In addition, the magnified
endoscopic images obtained are often quite coarse due to the small number of pixels in the
charge-coupled device (CCD). As a result, at higher magnification ratios, the orientation of
the field of view is easily lost. A newly developed prototype colorectal electronic endoscope
(Toshiba Corporation, Tokyo) overcomes these problems. The length of the hard tip of the
scope and the weight of the controller section are comparable to those of the TCE-3680MH
(Toshiba Corporation). High-resolution magnified images can be obtained, because a
410,000-pixel CCD is employed. Two magnification methods are available, optical
magnification and electronic zooming, permitting images to be magnified by a factor of up
to 90â120 without losing the orientation of the field of view. This newly developed magnifying
electronic endoscope was found to be very useful, allowing us to observe the pit patterns of the
colorectal mucosa in 82 small colorectal polyps measuring 7 mm or less in diameter
ASCA Detection of Pulsed X-ray Emission from PSR J0631+1036
ASCA's long look at the 288 millisecond radio pulsar, PSR J0631+1036, reveals
coherent X-ray pulsation from this source for the first time. The source was
first detected in the serendipitous Einstein observation and later identified
as a radio pulsar. Possible pulsation in the gamma-ray band has been detected
from the CGRO EGRET data (Zepka, et al. 1996). The X-ray spectrum in the ASCA
band is characterized by a hard power-law type emission with a photon index of
about 2.3, when fitted with a single power-law function modified with
absorption. An additional blackbody component of about 0.14 keV increases the
quality of the spectral fit. The observed X-ray flux is 2.1e-13 ergs/s/cm2 in
the 1-10 keV band. We find that many characteristics of PSR J0631+1036 are
similar to those of middle-aged gamma-ray pulsars such as PSR B1055-52, PSR
B0633+17 (Geminga), and PSR B0656+14.Comment: To appear in ApJ Letter
Measurement schemes for the spin quadratures on an ensemble of atoms
We consider how to measure collective spin states of an atomic ensemble based
on the recent multi-pass approaches for quantum interface between light and
atoms. We find that a scheme with two passages of a light pulse through the
atomic ensemble is efficient to implement the homodyne tomography of the spin
state. Thereby, we propose to utilize optical pulses as a phase-shifter that
rotates the quadrature of the spins. This method substantially simplifies the
geometry of experimental schemes.Comment: 4pages 2 figure
INTRINSIC MECHANISM FOR ENTROPY CHANGE IN CLASSICAL AND QUANTUM EVOLUTION
It is shown that the existence of a time operator in the Liouville space
representation of both classical and quantum evolution provides a mechanism for
effective entropy change of physical states. In particular, an initially
effectively pure state can evolve under the usual unitary evolution to an
effectively mixed state.Comment: 20 pages. For more information or comments contact E. Eisenberg at
[email protected] (internet)
Measurement induced quantum-classical transition
A model of an electrical point contact coupled to a mechanical system
(oscillator) is studied to simulate the dephasing effect of measurement on a
quantum system. The problem is solved at zero temperature under conditions of
strong non-equilibrium in the measurement apparatus. For linear coupling
between the oscillator and tunneling electrons, it is found that the oscillator
dynamics becomes damped, with the effective temperature determined by the
voltage drop across the junction. It is demonstrated that both the quantum
heating and the quantum damping of the oscillator manifest themselves in the
current-voltage characteristic of the point contact.Comment: in RevTex, 1 figure, corrected notatio
- âŠ