• 제목/요약/키워드: Spectral density

검색결과 826건 처리시간 0.025초

Comparative Analysis of Peak Impact Acceleration and Impact Shock Frequency Components According to the Type of Treadmill for Treadmill-running

  • Lee, Jae Seok;Hur, Seung Eun;Park, Seong Han;Moon, Hwang Woon;Koo, Bon Ho
    • 한국운동역학회지
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    • 제27권4호
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    • pp.263-268
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    • 2017
  • Objective: The purpose of this study was to show differences in impact variables between treadmills with (treadmills B, C, and D) and treadmills without a shock-absorbing function (treadmill A) to propose the development of a treadmill with improved or added shock-absorbing function to reduce impact shock. Method: Thirteen male students in their twenties who had habitual rear foot strike during running ran on four treadmills at 2.67 m/sec while ankle and neck acceleration data were collected. The magnitude of the ankle and neck acceleration peaks and peak positive ankle acceleration were calculated. The power spectral density of each signal was calculated to transform the ankle and neck accelerations in the frequency domain. Results: The peak positive ankle acceleration on treadmill B was significantly lesser than that on treadmills A and D, and that on treadmill C was significantly less than that on treadmill A (p < .01). Peak positive neck acceleration was not statistically different between the treadmills. The frequencies of the peak power of the ankle and neck acceleration signal within the lower and higher frequency ranges were not statistically different between the treadmills. The signal power magnitude of the ankle in higher frequency ranges on treadmill B was significantly less than that on treadmills A, C, and D (p < .01). The signal power magnitude of the ankle in higher frequency ranges was not statistically different between the treadmills. The signal power magnitudes of the neck acceleration signal within the lower and higher frequency ranges were not statistically significantly different between the treadmills. Conclusion: Our results indicate that the shock-absorbing function of a treadmill plays a role in reducing impact shock. Therefore, in future treadmill development, shock-absorbing function should be improved or incorporated to reduce impact shock to the body.

Identifying the VeLLOs in the Spitzer Gould's Belt Survey

  • Kim, Mi-Ryang;Lee, Chang-Won;Dunham, M.;Allen, L.;Myers, Philip C.;Evans, N.
    • 천문학회보
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    • 제35권2호
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    • pp.67.2-67.2
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    • 2010
  • We present results of searching for the Very Low Luminosity Objects (VeLLOs; internal luminosity : $L_{int}$ < $0.1(d/140pc)^2\;L\odot$) in the Gould's Belt clouds using observations from 3.6 to 70 micron by the Spitzer Space Telescope. The clouds are California, Chamaeleon I, III, Musca, Lupus V, VI, Scorpius, Serpens, Corona Australis, Cepheus, and IC 5146 having the properties of active low-mass star-forming such as the Taurus cloud. The observing sensitivity of the Spitzer data is estimated to be about $L_{int}\;\geq\;5\times10^{-3}(d/140pc)^2\;L\odot$, a factor of 20 better than that of the Infrared Astronomical Satellite (IRAS). The observing data were processed by the c2d Legacy pipeline. As the criteria to select the VeLLOs, we slightly modified previous ones by Dunham et al. The most important criterion is a flux density at 70 micron that is directly converted to the internal luminosity. Also, we used additional criteria to remove the contamination of evolved stars and extragalaxies which have colors or SEDs very similar to YSOs. We identified a total of 64 new embedded VeLLO candidates with $L_{int}$ < $0.1(d/140pc)^2\;L\odot$, consisting of 8 in California, 15 in Chamaeleon-Musca, 13 in Scorpius-Lupus, 20 in Serpens, 3 in Corona Australis, 3 in Cepheus, and 2 in IC 5146. The classification of the spectral index (${\alpha}$) fitted to the shape of the Ks-24 micron SEDs shows most of VeLLO candidates (89%) are in types of Class I and Flat spectrum. We plot various diagrams based on their 2MASS-Spitzer bands colors and magnitudes to discuss properties of the VeLLOs. This search will lead us new adventure toward a future systematic study of the VeLLOs.

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고속 고밀도 WDM 광전송 시스템에서의 ASK-SSB와 PSK-SSB 변조 방식의 성능 분석 (Performance Analysis of ASK-SSB and PSK-SSB Modulation Format in High-Speed and High-Density WDM Transmission Systems)

  • 박진영;최윤희;박상규
    • 대한전자공학회논문지TC
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    • 제41권12호
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    • pp.23-32
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    • 2004
  • 본 논문에서는 SSB 변조를 이용한 광전송 시스템의 주파수 효율성 및 비선형성에 대한 저항성 등을 규명하였다. 이상적인 SSB 신호를 사용하여 도달할 수 있는 성능의 한계를 확인하는 한편, 실제 제작이 가능한 SSB 변조기가 생성할 수 있는 신호에서 얻을 수 있는 성능을 컴퓨터 시뮬레이션을 통하여 살펴보았다. 이를 통해 SSB 변조된 신호는 일반적으로 DSB 변조된 신호에 비해서 광섬유의 비선형성에 취약하나 본 연구에서 목표로 삼고 있는 전송거리가 500~1000 km 미만인 12.5 GHz 채널 간격의 WDM 시스템에서는 SSB 신호가 DSB 신호에 비해 우수한 성능을 보일 수 있음을 확인하였다.

CMOS 저잡음 기가비트급 광전단 증폭기 설계 (CMOS Gigahertz Low Power Optical Preamplier Design)

  • 황용희;강진구
    • 전기전자학회논문지
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    • 제7권1호
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    • pp.72-79
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    • 2003
  • 일반적으로 p-i-n Photodiode 수신기의 광신호처리 전단증폭기의 설계에서 공통소스 입력단을 사용하는 트랜스임피던스(Transimpedance)구조로 설계한다. 본 논문에서는 공통게이트 입력단을 사용하는 전류모드 광전단증폭기를 설계하였다. 이러한 광전단증폭기로 사용되는 전류모드 공통게이트 트랜스임피던스 증폭기의 특징은 높은 이득과 높은 대역폭을 동시에 얻을 수 있다는 것이다. 본 논문에서는 광전단 증폭기 설계에서 잡음 최적화를 이용하여 설계과정을 자동화 시킴으로써 보다 단순하게 트랜스임피던스 증폭기를 설계하는 기법을 제시하였다. 그리고 커패시턴스 피킹(Capacitive Peaking) 기술을 사용하여 대역폭을 더욱 증가시킬 수 있다. 제안하는 기법을 사용하여 설계된 전류모드 광전단 증폭기에 캐패시턴스 피킹을 적용하여 0.35um CMOS 공정을 사용할 경우 대역폭이 1.57GHz이고, 트랜스임피던스 이득이 2.34k, 입력 잡음전류가 470nA이고 입력 잡음 전류의 주파수밀도(spectral density)가 6.13pA/ 인 저 잡음의 고속 전류모드 트랜스임피던스 광전단증폭기를 설계 하였다. 시뮬레이션 결과 제안된 광전단증폭기의 전력소비는 3.3V 공급전압에서16.84mW이었다.

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무선랜에서 에너지 효율적인 전송 대역폭 결정 기법 (Energy-Efficient Transmission Bandwidth Adaptation in IEEE 802.11 WLANs)

  • 황환웅;윤지훈
    • 전기전자학회논문지
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    • 제22권3호
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    • pp.651-657
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    • 2018
  • IEEE 802.11 무선랜은 20MHz부터 160MHz의 전송 대역폭을 지원한다. 일반적으로 전송 시 대역폭이 증가함에 따라 전송속도가 증가하지만, 동시에 단위 주파수당 전송파워가 낮아져 오류율이 증가하고 재전송을 유발할 수 있다. 본 논문에서는 이러한 현상이 전송 에너지 소비에 미치는 영향을 분석하기 위한 수학적 모델링을 수행한다. 그리고, 이를 바탕으로 전송 대역폭을 결정하는 기법을 제시한다. 제시된 기법은 기존 전송 결과를 기반으로 대역폭별 오류율을 추정하고 이를 바탕으로 대역폭별 에너지 소비 테이블을 업데이트 후 이들 간의 비교를 통해 최적 대역폭을 결정한다. VoIP 트래픽을 가정한 시뮬레이션을 통해 다양한 환경에서 제안한 기법의 에너지 소비 성능을 평가한다.

경도인지장애와 알츠하이머병 치매의 생물학적 표지자로서 뇌파와 사건유발전위의 임상적 의미 (Clinical Implications of EEG and ERP as Biological Markers for Alzheimer's Disease and Mild Cognitive Impairment)

  • 김창규;김현택;이승환
    • 생물정신의학
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    • 제20권4호
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    • pp.119-128
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    • 2013
  • Objectives Memory impairment is a very important mental health issue for elderly and adults. Mild cognitive impairment (MCI) is a prodromal stage of Alzheimer's disease (AD). Early detection of the prodromal stage of patients with AD is an important topic of interest for both mental health clinicians and policy makers. Methods Electroencephalograpgy (EEG) has been used as a possible biological marker for patients with MCI, and AD. In this review, we will summarize the clinical implications of EEG and ERP as a biological marker for AD and MCI. Results EEG power density, functional coupling, spectral coherence, synchronization, and connectivity were analyzed and proved their clinical efficacy in patients with the prodromal stage of AD. Serial studies on late event-related potentials (ERPs) were also conducted in MCI patients as well as healthy elders. Even though these EEG and ERP studies have some limitations for their design and method, their clinical implications are increasing rapidly. Conclusion EEG and ERP can be used as biological markers of AD and MCI. Also they can be used as useful tools for early detection of AD and MCI patients. They are useful and sensitive research tools for AD and MCI patients. However, some problems remain to be solved until they can be practical measures in clinical setting.

Fabrication and Characterization of Dye-sensitized Solar Cells based on Anodic Titanium Oxide Nanotube Arrays Sensitized with Heteroleptic Ruthenium Dyes

  • Shen, Chien-Hung;Chang, Yu-Cheng;Wu, Po-Ting;Diau, Eric Wei-Guang
    • Rapid Communication in Photoscience
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    • 제3권1호
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    • pp.16-19
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    • 2014
  • Anodic self-organized titania nanotube (TNT) arrays have a great potential as efficient electron-transport materials for dye-sensitized solar cells (DSSC). Herewith we report the photovoltaic and kinetic investigations for a series of heteroleptic ruthenium complexes (RD16-RD18) sensitized on TNT films for DSSC applications. We found that the RD16 device had an enhanced short-circuit current density ($J_{SC}/mAcm^{-2}=15.0$) and an efficiency of power conversion (${\eta}=7.2%$) greater than that of a N719 device (${\eta}=7.1%$) due to the increasing light-harvesting and the broadened spectral features with thiophene-based ligands. However, the device made of RD17 (adding one more hexyl chain) showed smaller $J_{SC}(14.1mAcm^{-2})$ and poorer ${\eta}(6.8%)$ compare to those of RD16 due to smaller amount of dye-loading and less efficient electron injection for the RD17 device than for the RD16 device. For the RD18 dye (adding one more thiophene unit and one more hexyl chain), we found that the device showed even lower $J_{SC}(13.2mAcm^{-2}) $ that led to a poorest device performance (${\eta}=6.2%$) for the RD18 device. These results are against to those obtained from the same dyes sensitized on $TiO_2$ nanoparticle films and they can be rationalized according to the electron transport kinetics measured using the methods of charge extraction and transient photovoltage decays.

이온 보조 증착한 ${Ta_2}{O_5}$ 광학 박막의 광학적 및 기계적 특성 분석 (Optical and mechnical properties of ${Ta_2}{O_5}$ optical thin films by ion assisted deposition)

  • 류태욱;김동진
    • 한국광학회지
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    • 제11권3호
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    • pp.147-151
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    • 2000
  • 전자총을 사용하여 이온 보조한 Ta2O5 박막과 이온 보조하지 않은 ${Ta_2}{O_5}$ 박막을 진공 증착하고, 증착 조건에 따른 광학적 특성과 기계적 특성을 측정하였다. 양극전압 120V, 이온빔 전류밀도 $50~500\muA/cm^2$로 산소 이온보조 증착한 박막의 경우 굴절률은 상온에서 제작한 보통 ${Ta_2}{O_5}$ 박막의 1.94보다 높은 2.15이었으며, 변형력은 $7.0\times10^8 dyne/cm^2$보다 낮은 $5.0\times10^8 dyne/cm^2$2이었다. 이는 기판온도 $230^{\circ}C$에서 증착한 박막과 광학적.기계적 특성이 유사함을 알수 있었다. 아르곤 이온 보조한 박막의 경우 인장 변형력은 감소하였으나 가시광 영역의 단파장쪽에서 흡수가 발생하였다. 그리고 X-선 회절분석 결과 모든 박막의 비정질로 나타났다.

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Study on the possibility of the aerosol and/or Yellow dust detection in the atmosphere by Ocean Scanning Multispectral Imager(OSMI)

  • Chung, Hyo-Sang;Park, Hye-Sook;Bag, Gyun-Myeong;Yoon, Hong-Joo;Jang, Kwang-Mi
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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    • pp.409-414
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    • 1998
  • To examine the detectability of the aerosol and/or Yellow dust from China crossing over the Yellow sea, three works carried out as follows , Firstly, a comparison was made of the visible(VIS), water vapor(WV), and Infrared(IR) images of the GMS-5 and NOAA/AVHRR on the cases of yellow sand event over Korea. Secondly, the spectral radiance and reflectance(%) was observed during the yellow sand phenomena on April, 1998 in Seoul using the GER-2600 spectroradiometer, which observed the reflected radiance from 350 to 2500 nm in the atmosphere. We selected the optimum wavelength for detecting of the yellow sand from this observation, considering the effects of atmospheric absorption. Finally, the atmospheric radiance emerging from the LOWTRAN-7 radiative transfer model was simulated with and without yellow sand, where we used the estimated aerosol column optical depth ($\tau$ 673 nm) in the Meteorological Research Institute and the d'Almeida's statistical atmospheric aerosol radiative characteristics. The image analysis showed that it was very difficult to detect the yellow sand region only by the image processing because the albedo characteristics of the sand vary irregularly according to the density, size, components and depth of the yellow sand clouds. We found that the 670-680 nm band was useful to simulate aerosol characteristics considering the absorption band from the radiance observation. We are now processing the simulation of atmospheric radiance distribution in the range of 400-900 nm. The purpose of this study is to present the preliminary results of the aerosol and/or Yellow dust detectability using the Ocean Scanning Multispectral Imager(OSMI), which will be mounted on KOMPSAT-1 as the ocean color monitoring sensor with the range of 400-900 nm wavelength.

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Comparative analysis of the wind characteristics of three landfall typhoons based on stationary and nonstationary wind models

  • Quan, Yong;Fu, Guo Qiang;Huang, Zi Feng;Gu, Ming
    • Wind and Structures
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    • 제31권3호
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    • pp.269-285
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    • 2020
  • The statistical characteristics of typhoon wind speed records tend to have a considerable time-varying trend; thus, the stationary wind model may not be appropriate to estimate the wind characteristics of typhoon events. Several nonstationary wind speed models have been proposed by pioneers to characterize wind characteristics more accurately, but comparative studies on the applicability of the different wind models are still lacking. In this study, three landfall typhoons, Ampil, Jongdari, and Rumbia, recorded by ultrasonic anemometers atop the Shanghai World Financial Center (SWFC), are used for the comparative analysis of stationary and nonstationary wind characteristics. The time-varying mean is extracted with the discrete wavelet transform (DWT) method, and the time-varying standard deviation is calculated by the autoregressive moving average generalized autoregressive conditional heteroscedasticity (ARMA-GARCH) model. After extracting the time-varying trend, the longitudinal wind characteristics, e.g., the probability distribution, power spectral density (PSD), turbulence integral scale, turbulence intensity, gust factor, and peak factor, are comparatively analyzed based on the stationary wind speed model, time-varying mean wind speed model and time-varying standard deviation wind speed model. The comparative analysis of the different wind models emphasizes the significance of the nonstationary considerations in typhoon events. The time-varying standard deviation model can better identify the similarities among the different typhoons and appropriately describe the nonstationary wind characteristics of the typhoons.