• Applied Science and Convergence Technology
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• 제26권2호
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• pp.21-25
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• 2017

The shape of the reflection spectrum is complex and appears to overlap with several signals, because the surface state is uneven due to the natural oxide film, so that the spectrum becomes a complicated signal shape divided into regions 1 and 2 due to diffuse reflection. On the other hand, it is seen that the reflection spectrum after PEO surface treatment is overlapped with several signals. In addition, the reflectance of the energy band varies from 1.32 to 1.46 eV. Usually, the MgO-type oxide film was observed at an energy band of ~4.2 eV. The thickness of the oxide film was increased as the DC voltage was increased by the thin film thickness meter (QuaNix; 7500M) after Plasma Electrolytic Oxidation (; PEO) surface treatment. This is because the higher the DC voltage, the easier the binding of the $OH^-$ ions in the solution solution and the $Mg^+$ ions of the magnesium alloy. An important part of the bonding of ordinary ions is the energy source (plasma) which can promote bonding. However, when a certain threshold voltage or more is applied, the material is adversely affected. The oxide film of the surface may be destroyed without increasing the thickness of the oxide film, that is, whitening of the material may occur.

• 한국정보통신학회논문지
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• 제9권8호
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• pp.1780-1786
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• 2005

디지털 신호의 전송 성능은 전송 시스템의 위상 에러에 지배적으로 영향을 받고 있으며, 위상 에러는 랜덤 특성을 갖는 위상 잡음과 도플러에 의한 추적 위상 에러에 의해 발생된다. 도플러 현상이 나타나는 움직임을 갖는 이동형 위성통신 시스템에서는 랜덤 위상 잡음과 추적 위상 오차에 의한 전송 신호의 영향을 해석하여 이동형 위성통신 시스템에 적합한 시스템 요구 위상 잡음 스펙트럼을 설계해야 한다. 본 논문에서는 이동형 양방향 위성통신 시스템의 비대칭 이동 서비스에 대한 도플러 영향과 위상 에러를 해석하여 요구되는 전송 시스템의 위상 잡음 스펙트럼을 설계하고, 움직임을 갖는 단말국의 도플러 영향을 최소화하는 전송서비스를 해석한다. 제안한 위상 잡음 스펙트럼은 요구 전송 시스템에 대한 주파수 발생 부 주파수 특성으로 설계할 수 있다.

• 한국정보통신학회논문지
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• 제11권7호
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• pp.1247-1253
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• 2007

본 논문에서는 통신해양기상위성 센서 데이터 송수신 시스템의 요구 시스템 위상 잡음 스펙트럼 분포도를 제안하였다. 위상 잡음 영향을 최소화하기 위한 해석된 수신 설계 파라미터를 기반으로 센서 측정 신호인 raw, LRIT 및 HRIT 데이터 전송에 적합한 위상 잡음 특성을 제시하였다. 제안된 위상 잡음 특성은 전송 채널상에서 발생하는 주파수 신호 자원의 위상 잡음 영향을 최소화하며, 서비스 단말에 양호한 전송 성능을 제공한다. 또한 제안된 위상 잡음 스펙트럼은 센서 데이터 송수신 시스템의 주파수 발생원의 신호 특성으로 설계할 수 있도록 한다.

• Earthquakes and Structures
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• 제17권4호
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• pp.365-372
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• 2019

Post-earthquake crisis management is a key capability for a country to be able to recover after a major seismic event. Instrumental seismic data transmitted and processed in a very short time can contribute to better management of the emergency and can give insights on the earthquake's impact on a specific area. Romania is a country with a high seismic hazard, mostly due to the Vrancea intermediate-depth earthquakes. The elastic acceleration response spectrum of a seismic motion provides important information on the level of maximum acceleration the buildings were subjected to. Based on new data analysis and knowledge advancements, the acceleration elastic response spectrum for horizontal ground components recommended by the Romanian seismic codes has been evolving over the last six decades. This study aims to propose a framework for post-earthquake warning based on code spectrum exceedances. A comprehensive background analysis was undertaken using strong motion data from previous earthquakes corroborated with observational damage, to prove the method's applicability. Moreover, a case-study for two densely populated Romanian cities (Focsani and Bucharest) is presented, using data from a $5.5M_W$ earthquake (October 28, 2018) and considering the evolution of the three generations of code-based spectral levels for the two cities. Data recorded in free-field and in buildings were analyzed and has confirmed that no structural damage occurred within the two cities. For future strong seismic events, this tool can provide useful information on the effect of the earthquake on structures in the most exposed areas.

• 한국정보전자통신기술학회논문지
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• 제12권1호
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• pp.78-82
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• 2019

본 논문에서는 수배전반 내 코로나 및 직렬아크 발생 시 나타나는 초음파 신호의 측정 및 분석에 대해 기술하였다. 휴대용 초음파 감지기는 전기 시스템에서 발생하는 코로나와 같은 방전 현상 감지에 유용하다. 그러나 일반적인 휴대용 초음파 감지기는 방전 여부에 대한 판단 결과가 사용자의 주관적 반응에 영향을 미치며, 음향 특성을 듣고 결과를 예측함으로써 문제 유형을 판별하는 것이 어렵다는 단점을 가지고 있다. 따라서 초음파 특성을 구별하는 새로운 분석 방법이 필요하다. 본 논문에서는 초음파 감지기로 측정 한 초음파 음향을 시각화하기 위한 초음파 분석 사례를 연구하였다. 실험 결과 초음파탐지계통은 외부소음의 영향을 받지 않고 배전반에서 코로나 및 직렬 아크 방전을 검출할 수 있었다.

• Journal of Power Electronics
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• 제19권1호
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• pp.278-287
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• 2019

In this study, a zero-crossing spike current issue in a totem-pole bridgeless power factor correction (PFC) converter is comprehensively investigated for the first time. Spike current occurs when input voltage crosses zero, becomes a noise source, and causes severe common mode emission issues. A generation mechanism for electromagnetic interference (EMI) is presented to investigate the EMI problem caused by zero-crossing issue, and a noise spectrum due to this issue is predicted by a theoretical analysis based on the Fourier coefficient of an approximate spike current waveform. Furthermore, a noise reduction method is proposed and then improved to reduce the spike current. Experimental measurements are implemented on a GaN-based totem-pole bridgeless PFC converter, and the spike current can be effectively suppressed through the proposed method. Furthermore, the noise spectrums measured without and with the reduced zero-crossing spike current are compared. Experimental results validate the analysis of the noise spectrum caused by the zero-crossing spike current issue.

• 천문학회보
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• 제40권1호
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• pp.75.3-75.3
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• 2015

Large area infrared surveys are often accompanied with follow-up optical spectroscopic surveys that has a significant legacy value even for other areas of research. Using these spectral database, we have performed a search for MgII absorption lines in the optical spectrum of background quasar. Over the ~4deg2 of AKARI North Ecliptic Pole survey field and Spitzer First Look Survey field, 18 and 16 MgII absorber systems are identified respectively. The redshift range for the background quasars was 1.0<$z_{qso}$<3.4, while the redshift range for the absorber was 0.6<$z_{abs}$<1.6. Galaxies responsible for MgII absorptions are identified in the deep optical images (CFHT r-band), yet the identification still remains ambiguous for 60% of the systems due to the limited image depth and the source crowdedness. The impact parameter ranges 20-60kpc, and the rest-frame equivalent width of MgII absorption ranges $0.7-4{\AA}$. The most critical part in the identification of MgII absorber galaxies is the existence of deep optical images in addition to the high S/N quasar spectrum with R>3000.

• 한국전기전자재료학회논문지
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• 제26권4호
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• pp.294-297
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• 2013

ZnO crystals with octahedral shape were synthesized by thermal evaporation technique. $ZnF_2$ powder was used as the source material. The thermal evaporation and oxidation of $ZnF_2$ powder was carried out for 1 hr at $1,000^{\circ}C$ in air under atmospheric pressure. SEM images showed that the ZnO crystals produced by oxidizing $ZnF_2$ vapor possessed a characteristic octahedral shape. XRD spectrum revealed that the ZnO octahedron had hexagonal wurtzite structure. In the room temperature photoluminescence spectrum, a strong green emission peak at around 510 nm was observed.

• 한국방송∙미디어공학회:학술대회논문집
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• 한국방송공학회 2013년도 하계학술대회
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• pp.29-31
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• 2013

본 논문에서는 기존라디오(primary) 네트워크와 스펙트럼을 공유하는(spectrum sharing) 인지라디오(cognitive radio) 네트워크에서 비재생적(non-regenerative) 다중안테나 중계 (relay) 시스템을 위한 소스(source) 및 중계기 프리코딩(precoding) 기법을 제안한다. 제안된 기법은 소스와 중계기 프리코딩 행렬의 최적해를 구하기 위해 QCQP(Quadratically Constrained Quadratic Programming) 문제를 통해 구한다. 제안된 기법은 기존라디오 수신기에서의 간섭세기 제한을 만족하면서 낮은 MSE(Mean squared error)와 높은 MI(Mutual Information)를 달성함을 모의실험결과를 통해 보인다. 또한 아주 빠른 속도로 최적해로 수렴함을 보이고 있다.

• Journal of Astronomy and Space Sciences
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• 제33권2호
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• pp.93-99
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• 2016

A redback system is a binary system composed of a pulsar and a main sequence star. The inverse Compton (IC) scattering between the stellar soft photons and the relativistic pulsar wind will generate orbital-modulating GeV photons. We look for these IC emissions from redback systems. A multi-wavelength observation of an unassociated gamma-ray source, 3FGL J2039.6-5618, by Salvetti et al. (2015) detected an orbital modulation with a period of 0.2 days in both X-ray and optical cases. They suggested 3FGL J2039.6-5618 to be a new redback candidate. We analyzed the gamma-ray emission of 3FGL J2039.6-5618 using the data from the Fermi large area telescope (Fermi-LAT) and obtained the spectrum in different orbital phases. We propose that the spectrum has orbital dependency and estimate the characteristic energy of the IC emission from the stellar-pulsar wind interaction.