• 한국전자파학회논문지
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• 제19권2호
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• pp.271-279
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• 2008

본 논문에서는 FHSS 방식의 소출력 무선기기와 DSSS 방식의 소출력 무선기기가 동일 주파수 대역에 존재하는 경우 업무간 간섭을 분석하였다. 분석 방법은 몬테 카를로 방법을 이용하여 DSSS 방식의 소출력 무선기기의 불요 방사가 FHSS 방식의 소출력 무선기기에 미치는 영향을 간섭 확률 측면에서 계산하였다. 간섭 시뮬레이션은 DSSS 방식의 소출력 무선기기의 대역폭과 충격 계수에 따른 간섭량을 계산하였고, 전파 모델은 자유 공간으로 가정하였다. 그리고 간섭원과 피간섭원 사이의 거리에 따른 영향을 수신기에서의 BER 측면에서 분석하였다. 간섭 분석 결과, 간섭원의 대역폭보다는 충격 계수가 시스템 양립성에 많은 영향을 주는 것을 확인할 수 있었고, 단일 간섭원과 다중 간섭원이 존재하는 경우 BER 기준을 만족하는 이격 거리를 확인할 수 있었다.

• 한국음향학회지
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• 제35권5호
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• pp.368-374
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• 2016

본 논문은 기존의 DPSK(Differential Phase-Shift Keying) 방식 수중음향통신에 직접 수열 대역확산 기법을 적용하여 송수신단을 구성하는 내용을 다루었다. DPSK방식의 수신기에서는 인접 비트 간 위상차만 알고 있으면 복조가 가능하기 때문에 수신기 구조가 간단해지는 장점이 있다. 기존의 DPSK 수신단에서는 역확산 전 신호의 두 심볼씩 전이 상관기로 입력되면 상관 결과의 최대값을 비교하여 데이터를 검출하는데 이 때 채널에 따른 낮은 SNR(Signal to Noise Ratio) 또는 높은 도플러 천이 주파수 때문에 전이 상관기 출력의 최대값 오류율이 증가할 수 있다. 본 논문에서는 전이 상관기에서 생성되는 다수 출력들의 크기뿐만 아니라 간격을 추가적으로 이용하여 더욱 정확한 검출 결과를 얻을 수 있도록 하는 방법을 제안하였다. 제안된 방법의 성능은 모의 및 호수실험을 통해 획득한 데이터를 이용하여 분석되었다.

• 대한조선학회논문집
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• 제48권4호
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• pp.299-307
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• 2011

The offshore plants such as FPSO are subjected to combination loading of environmental conditions (swell, wave, wind and current). Therefore the fatigue damage is occurred in the operation time because the units encounter the environmental phenomena and the structural configurations are complicated. This paper is a research for frequency domain fatigue analysis of wide-band random loading focused on accuracy of fatigue damage estimation regarding the proposed methods. We selected ideal bi-modal spectrum. And comparison between time-domain fatigue analysis and frequency-domain fatigue analyses are conducted through the fatigue damage ratio. Fatigue damage ratios according to Vanmarcke's bandwidth parameter are founded for wide-band. Considering safety, we recommend that Jiao-Moan and Tovo-Benasciutti methods are optimal way at the fatigue design for wide-band response. But, it is important that these methods based on frequency-domain unstably change the accuracy according to the material parameter of S-N curve. This study will be background and guidance for the new frequency-domain fatigue analysis development in the future.

• 천문학회보
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• 제36권2호
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• pp.73.2-73.2
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• 2011

We present a new database of absorption and emission-line measurements based on the entire spectral atlas from the Sloan Digital Sky Survey (SDSS) 7th data release of galaxies within a redshift of 0.2. Our work makes use of the publicly available penalized pixel-fitting(pPXF) and gas and absorption line fitting (gandalf) IDL codes, aiming to improve the existing measurements for stellar kinematics, the strength of various absorption-line features, and the flux and width of the emissions from different species of ionized gas. Our fit to the stellar continuum uses both standard stellar population models and empirical templates obtained by combining a large number of stellar spectra in order to fit a subsample of high-quality SDSS spectra for quiescent galaxies. Furthermore, our fit to the nebular spectrum includes an exhaustive list of both recombination and forbidden lines. Foreground Galactic extinction is implicitly treated in our models, whereas reddening in the SDSS galaxies is included in the form of a simple dust screen component affecting the entire spectrum that is accompanied by a second reddening component affecting only the ionised gas emission. Most notable of our work is that, we provide quality of the fit to assess reliability of the measurements. The quality assessment can be highly effective for finding new classes of objects. For example, based on the quality assessment around the Ha and [NII] nebular lines, we found approximately 1% of the SDSS spectra which classified as "galaxies" by the SDSS pipeline are in fact type I Seyfert AGN.

• Restorative Dentistry and Endodontics
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• 제41권4호
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• pp.271-277
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• 2016

Objectives: In this study, we evaluated the influence of different radiant exposures provided by single-peak and polywave light-curing units (LCUs) on the degree of conversion (DC) and the mechanical properties of resin cements. Materials and Methods: Six experimental groups were established for each cement (RelyX ARC, 3M ESPE; LuxaCore Dual, Ivoclar Vivadent; Variolink, DMG), according to the different radiant exposures (5, 10, and $20J/cm^2$) and two LCUs (single-peak and polywave). The specimens were made (7 mm in length ${\times}$ 2 mm in width ${\times}$ 1 mm in height) using silicone molds. After 24 hours of preparation, DC measurement was performed using Fourier transform infrared spectrometry. The same specimens were used for the evaluation of mechanical properties (flexural strength, FS; elastic modulus, E) by a three-point bending test. Data were assessed for normality, after which two-way analysis of variance (ANOVA) and post hoc Tukey's test were performed. Results: No properties of the Variolink cement were influenced by any of the considered experimental conditions. In the case of the RelyX ARC cement, DC was higher when polywave LCU was used; FS and E were not influenced by the conditions evaluated. The LuxaCore cement showed greater sensitivity to the different protocols. Conclusions: On the basis of these results, both the spectrum of light emitted and the radiant exposure used could affect the properties of resin cements. However, the influence was material-dependent.

• 한국초전도ㆍ저온공학회논문지
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• 제21권4호
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• pp.9-12
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• 2019

We performed Raman spectroscopy on two different over-doped Bi₂Sr₂CaCu₂O_8+x (BSCCO), of which superconducting transition temperatures are 89 K and 77 K. Line-shape analysis of the Raman-spectrum was done, focused on B_1g bond buckling mode which have drawn a lot of attention, since photoemission studies showed an evidence for strong coupling between the mode and electron. The line-shapes show asymmetry and are well fitted by the Fano line-shape formula. Remarkably, we found that the peak line-widths from B_1g bond buckling mode in BSCCO show much broader than those in YBa₂Cu₃O_7-x. The broad line width can be attributed to the superstructure modulation of BSCCO. Our results imply that B_1g bond buckling mode may have close relation to the origin of superconductivity or to boosting the superconducting transition temperature in BSCCO.

• 한국광학회지
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• 제16권1호
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• pp.1-6
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• 2005

우리는 Rb원자의 5S$_{1}$2-/5P$_{3}$2-/5D$_{5}$2/ 전이선에서 조사광과 곁합광의 편광조합 그리고 결합광 세기에 따른 사다리형 전자기 유도 투과(EIT) 현상을 조사하였다. 우리는 5D$_{5}$2/ 전이선에서 초미세구조를 가진 사다리형 EIT 스펙트럼을 얻었고, EIT 스펙트럼의 최소 선폭은 6.5 MHz로 측정되었다. 우리는 EIT 초미세구조의 상대적인 크기가 레이저의 편광조합 뿐만 아니라 결합광의 세기에 따라서 변하는 것을 실험적으로 관측하였고, 결합광의 세기에 따라 신호의 크기가 달라지는 이유는 광의 세기에 대하여 원자계가 비선형적으로 상호작용하기 때문이라는 사식을 밝혔다.

• Geomechanics and Engineering
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• 제14권2호
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• pp.107-113
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• 2018

Coal samples with different joints morphology were subjected to uniaxial compression experiments, cracks evolution was recorded by Nikon D5300 and acoustic emission (AE) energy signals were collected by AEwin Test for Express-8.0. During loading process, coal samples deformed elastically with no obvious cracks changes, then they expanded gradually along the trace of the original cracks, accompanied by the formation of secondary cracks, and eventually produced a large-scale fracture. It was more interesting that the failure mode of samples were all shear shape, whatever the original cracks morphology was. With cracks and damage evolution, AE energy radiated regularly. At the early loading stage, micro damage and small scale fracture events only induced a few AE events with less energy, while large scale fracture leaded to a number of AE events with more energy at the later stage. Based on the multifractal theory, the multifractal spectrum could explain AE energy signals frequency responses and the causes of AE events with load. Multifractal spectrum width (${\Delta}{\alpha}$), could reflect the differences between the large and small AE energy signals. And another parameter (${\Delta}f$) could reflect the relationship between the frequency of the least and greatest signals in the AE energy time series. This research is helpful for us to understand cracks evolution and AE energy signals causes.

• 대한의용생체공학회:의공학회지
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• 제43권6호
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• pp.409-416
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• 2022

Since the detection of cervical intraepithelial neoplasia (CIN) is increasing due to regular cervical cancer screening, there is a high demand for simpler tools to diagnose and treat CIN in the clinic. In this study, we proposed an electric property of cervical tissue to verify treatment using a laser. At first, we observed the depth and width of ablated cervical tissues for 29 samples according to four different pulse energy of the fractional CO₂ laser to find enough pulse energy to reach the basement layer for initiated CIN. And then, the relative frequency differences in impedance spectrum before and after laser irradiation for ten non-CIN samples were collected using bioimpedance spectroscopy with a multi-electrode probe. As a result, the laser ablated the cervical tissues with a depth of more than 300 ㎛ at 100 mJ pulse energy. Also, we confirmed that the relative changes of electrical property for cervical tissue increased as the pulse energy of laser output increased, and the variation between samples decreased. Since the relative change in electrical properties of cervical tissue can be easily and quickly measured, the proposed technique paves the way for further verification and follow-up study of laser treatment for CIN.

• Nuclear Engineering and Technology
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• 제55권3호
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• pp.1021-1030
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• 2023

We propose an overall procedure for measuring and unfolding fast neutron spectra using a trans-stilbene scintillation detector. Detector characterization was described, including the information on energy calibration, detector resolution, and nonproportionality response. The digital charge comparison method was used for the investigation of neutron-gamma Pulse Shape Discrimination (PSD). A pair of values of 600 ns pulse width and 24 ns delay time was found as the optimized conditions for PSD. A fitting technique was introduced to increase the trans-stilbene Proton Response Function (PRF) by 28% based on comparison of the simulated and experimental electron-equivalent distributions by the Cf-252 source. The detector response matrix was constructed by Monte-Carlo simulation and the spectrum unfolding was implemented using the iterative Bayesian method. The unfolding of simulated and measured spectra of Cf-252 and AmBe neutron sources indicates reliable, stable and no-bias results. The unfolding technique was also validated by the measured cosmic-ray induced neutron flux. Our approach is promising for fast neutron detection and spectroscopy.