Present Trends in High-Speed and Broad-Band Communications Services in Japan

1986 ◽  
Vol 4 (4) ◽  
pp. 438-443 ◽  
Author(s):  
M. Kurachi
2013 ◽  
Vol 664 ◽  
pp. 191-196
Author(s):  
You Gang Xiao ◽  
Yu Shi

For clarifying the noise in tunnel affected by pantograph and bogie, which are the most important noise sources, the noises near pantograph and bogie in a high-speed train were tested by multi-channel noise measurement and analysis system in tunnel, and compared with those measured outside the High-speed train and on an open field. The results show that the interior vehicle noise is spatially non-homogeneous in the whole carriage, the larger sound pressure level (SPL) near pantograph are next to ceiling, and near bogie next to floor. The noise spectra show a broad band feature, and dominated by the frequency contents among 100Hz-2kHz, so the countermeasures against noise should be within these range.


2012 ◽  
Vol 233 ◽  
pp. 239-242
Author(s):  
Xiao Feng Zhang ◽  
You Gang Xiao ◽  
He Lian Deng ◽  
Jian Feng Huang

Using microphone and removable planar microphone array, the exterior and interior vehicle noise near pantograph were investigated when the train ran at 250-350km/h, the noise spectrum characters of these areas were obtained. The results show that at the pantograph seat and in the vehicle below pantograph, the noise spectrum show a broad band distribution, and the noise energy is mainly concentrated within the range of 100Hz-2kHz. Interior vehicle noise below pantograph is a non-uniform reverberant sound field, the regions with larger sound pressure level (SPL) are distributed near the roof, the floor, the side wall below the luggage. For reducing interior vehicle noise below pantograph, such measures as using low noise pantograph, adding sound insulation pad, filling sound absorption materials and improving sealing performance should be taken, and these measures should be effective at 100Hz-2kHz.


2004 ◽  
Vol 126 (6) ◽  
pp. 931-936 ◽  
Author(s):  
N. Ranc ◽  
V. Pina ◽  
G. Sutter ◽  
S. Philippon

The working processes of metallic materials at high strain rate like forging, stamping and machining often induce high temperatures that are difficult to quantify precisely. In this work we, developed a high-speed broad band visible pyrometer using an intensified CCD camera (spectral range: 0.4 μm–0.9 μm). The advantage of the visible pyrometry technique is to limit the temperature error due to the uncertainties on the emissivity value and to have a good spatial resolution (3.6 μm) and a large observation area. This pyrometer was validated in the case of high speed machining and more precisely in the orthogonal cutting of a low carbon steel XC18. The cutting speed varies between 22 ms−1 and 60 ms−1. The experimental device allows one to visualize the evolution of the temperature field in the chip according to the cutting speed. The maximum temperature in the chip can reach 730°C and minimal temperature which can be detected is around 550°C.


2011 ◽  
Vol 1323 ◽  
Author(s):  
M. Fried ◽  
G. Juhasz ◽  
C. Major ◽  
A. Nemeth ◽  
P. Petrik ◽  
...  

ABSTRACTWe have developed a prototype spectroscopic ellipsometer for imaging/mapping purposes requiring only one measurement cycle (one rotation period of a polarizer or analyzer) for the acquisition of a two-dimensional array of data points. Our new measurement technique serves as a novel form of imaging ellipsometry, using a divergent (uncollimated, diffuse) source system and a detection system consisting of an angle-of-incidence-sensitive pinhole camera. By incorporating broad-band sources and wavelength dispersion optics, the instrument provides continuous high-resolution spectra along a line image of the sample surface. As a result, information on multilayer photovoltaics stacks can be obtained over large areas (several dm2) at high speed. The technique can be expanded to even larger areas by scaling-up the optical geometry. The spatial resolution of the line image is limited by the minimum resolved-angle as determined by the detection system. Small-aperture polarizers (25 mm diameter) are incorporated into the instrument, which reduces its cost. Demonstration mapping measurements have been performed ex situ on a multilayer sample deposited on a polymer substrate, including an intentionally graded 80-350 nm thick hydrogenated amorphous silicon (a-Si:H) layer and an intended uniform 400-500 nm thick transparent conducting ZnO:Al layer, both on opaque silver. Alternative commercial instruments for ex situ SE mapping must translate the sample in two dimensions. Even a 15 x 15 cm2 sample requires > 200 measurements with cm-resolution and at least 15 min. By collecting ex situ data in parallel along one dimension through imaging, the divergent-beam system can measure with similar spatial resolution in < 2 min. In situ measurements on both roll-to-roll polymer and rigid glass will be possible in the future.


2018 ◽  
Vol 609 ◽  
pp. L1 ◽  
Author(s):  
N. Kameswara Rao ◽  
F. Sutaria ◽  
J. Murthy ◽  
S. Krishna ◽  
R. Mohan ◽  
...  

Context. NGC 40 is a planetary nebula with diffuse X-ray emission, suggesting an interaction of the high-speed wind from WC8 central star (CS) with the nebula. It shows strong C IV 1550 Å emission that cannot be explained by thermal processes alone. We present here the first map of this nebula in C IV emission using broad band filters on the Ultra-Violet Imaging Telescope (UVIT). Aim. We aim to map the hot C IV-emitting gas and its correspondence with soft X-ray (0.3–8 keV) emitting regions in order to study the shock interaction between the nebula and the ISM. We also aim to illustrate the potential of UVIT for nebular studies. Methods. We carry out a morphological study of images of the nebula obtained at an angular resolution of about 1.3″ in four UVIT filter bands that include C IV 1550 Å and [C II] 2326 Å lines as well as UV continuum. We also make comparisons with X-ray, optical, and IR images from the literature. Results. The [C II] 2326 Å images show the core of the nebula with two lobes on either side of CS similar to [N II]. The C IV emission in the core shows similar morphology and extent to that of diffuse X-ray emission concentrated in nebular condensations. A surprising UVIT discovery is the presence of a large faint far UV (FUV) halo in an FUV filter with λeff of 1608 Å. The UV halo is not present in any other UV filter. The FUV halo is most likely due to UV fluorescence emission from the Lyman bands of H2 molecules. Unlike the optical and IR halo, the FUV halo trails predominantly towards the south-east side of the nebular core, opposite to the CS’s proper motion direction. Conclusions. Morphological similarity of C IV 1550 Å and X-ray emission in the core suggests that it results mostly from the interaction of strong CS wind with the nebula. The FUV halo in NGC 40 highlights the extensive existence of H2 molecules in the regions even beyond the optical and IR halos. Thus UV studies are important to estimate the amount of H2, which is probably the most dominant molecule and significant for mass-loss studies.


Author(s):  
Ralf Methling ◽  
Nicolas Götte ◽  
Dirk Uhrlandt

Molecule radiation can be used as a tool to study colder regions in switching arc plasmas like arc fringes in contact to walls and ranges around current zero (CZ). This is demonstrated in the present study for the first time for the case of ablation-dominated high&ndash;current arcs as key elements of self&ndash;blast circuit breakers. The arc in a model circuit breaker (MCB) in CO2 with and an arc in a long nozzle under ambient conditions with peak currents between 5 and 10 kA were studied by emission and absorption spectroscopy in the visible spectral range. The nozzle material was polytetrafluoroethylene (PTFE) in both cases. Imaging spectroscopy was carried out either with high-speed cameras or with intensified CCD cameras. A pulsed high-intensity Xe lamp was applied as background radiator for the broad-band absorption spectroscopy. Emission of Swan bands from carbon dimers was observed at the edge of nozzles only or across the whole nozzle radius with highest intensity in the arc center, depending on current and nozzle geometry. Furthermore, absorption of C2 Swan bands and CuF bands were found with the arc plasma serving as background radiator. After CZ, only CuF was detected in absorption experiments.


2008 ◽  
Vol 600-603 ◽  
pp. 493-496 ◽  
Author(s):  
Dorothea Werber ◽  
Martin Aigner ◽  
D. Denoth ◽  
F. Wittmann ◽  
Gerhard Wachutka

We present an experimental equipment for studying the charge carrier distribution in the interior of bipolar 4H-SiC high power devices by means of laser absorption measurements. Since the light absorption coefficient in a semiconductor depends on the electron and hole concentration, the attenuation of a laser beam transmitted through a sample is an integral function of the local charge carrier density. In order to detect the tiny changes in the light intensity caused by the plasma-optical effect, a highly sensitive measurement set-up has been developed. Its crucial components are a low-noise blue laser and a high-speed and broad-band photo-diode amplifier circuit. Sample preparation is sophisticated and requires special care. We investigated charge carrier profiles in 4H-SiC pin-diodes in the high-injection regime at current densities between 175 A/cm² and 350 A/cm². The measured charge carrier profiles are in good agreement with computer simulations.


2013 ◽  
Author(s):  
Brad Campbell ◽  
Scott Slocum

Accurate prediction of straked riser response can be important for determining the minimum strake coverage needed to ensure adequate riser fatigue life in demanding high-speed current environments. Previously published results from ExxonMobil’s 2003 vortex-induced vibration (VIV) model tests on a long, flexible, straked cylinder showed that strakes can greatly reduce, but may not entirely eliminate flow-induced vibration. The data also showed that the low-amplitude vibrations that persist when the cylinders are straked are different in character from VIV on bare cylinders, suggesting that the strakes are effective in disrupting the alternating vortex shedding mechanism that excites bare-cylinder VIV and that other flow mechanisms may drive the straked-cylinder vibration. This further implies that classic VIV models that have been developed to predict bare-pipe response due to alternating vortex shedding may not be accurate for straked cylinders even if the excitation model (“lift curve”) is adjusted to represent lower excitation levels on strakes. Classic VIV prediction methods for bare risers rely on special-purpose theoretical models to account for the strongly nonlinear interactions between bare cylinder motion and hydrodynamic excitation. However, for the low amplitudes of vibration observed in tests with straked cylinders, the influence of the cylinder motion on the flow may be less important. In an effort to more accurately predict the performance of strakes, ExxonMobil has recently explored a new approach for predicting flow-induced vibrations for straked risers that neglects any influence of riser motion on excitation, and instead assumes that hydrodynamic excitation can be approximated to useful accuracy by excitation measured on a fixed straked cylinder. New experiments show that this excitation is stochastic, with broad band-width, and that it conforms to relatively simple scaling laws. The measured stochastic excitation data has been used with a conventional linear random vibration model to predict the response data acquired from the 2003 model tests on the long, flexible, straked cylinder. Comparison shows a dramatic improvement in prediction scatter compared to predictions using a classic bare-pipe VIV formulation with a “lift curve” model of the strake hydrodynamic excitation.


2012 ◽  
Vol 8 (S290) ◽  
pp. 133-136
Author(s):  
Paul A. Mason ◽  
Edward L. Robinson ◽  
Sebastian Gomez ◽  
Emmanuel Gonzalez ◽  
Isaac D. Lopez ◽  
...  

AbstractHigh speed photometry of several accreting binaries was obtained using the McDonald Observatory 2.1m telescope and ARGOS CCD photometer. A broad-band filter (BVR) was used in order to maximize flux and maintain a short (1-10s) integration time on faint targets. Such observations obtained over several years allow for variability study over time scales covering many orders of magnitude. Observations and analysis for several binaries are summarized.


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