• 한국정보통신학회논문지
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• 제14권1호
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• pp.197-204
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• 2010

본 논문은 저 전압 및 저 왜곡 스위치형 커패시터 (switched-capacitor, SC)를 적용한 새로운 형태의 몸체효과 보상형 스위치 구조를 제안한다. 제안된 회로는 저 전압 SC회로를 위해서 rail-to-rail 스위칭을 허용하며, 기존의 부트스트랩 된 회로 (19dB)보다 더 우수한 총 고조파 왜곡을 가진다. 설계된 2-1 캐스케이드 시그마 델타 변조기는 통신 송수신 시스템내의 오디오 코덱을 위한 고해상도 아날로그-디지털변환을 수행한다. 1단 폴드형 캐스코드 연산증폭기 및 2-1 캐스케이드 시그마 델타 변조기는 0.25 마이크론 이중 폴리 3-금속 표준 CMOS 공정으로 제작되었으며, 2.7V에서 동작한다. 연산증폭기의 1% 정착시간은 16 pF의 부하 용량에 대해 560ns를 보였다. 제작된 시그마 델타 변조기에 대한 검사는 비트 스트림 검사 및 아날로그 분석기를 이용하여 수행 되었다. 다이크기는 $1.9{\times}1.5\;mm^2$였다.

• 생약학회지
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• 제17권2호
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• pp.153-160
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• 1986

We have isolated two new metabolites of territrem, designated as territrem $A'\;(TRA';\;C_{28}H_{30}O_{10})$ and $B'\;(TRB';\; C_{29}H_{34}O_{10})$ from chloroform extract of rice culture of Aspergillus terreus 23-1, using the same isolation procedure as that for territrem A, B and C(TRA, TRB, TRC). The present isolation procedure gave about 5 mg of TRA' and 10 mg of TRB' from 4 kg of rice culture per batch. Analysis of the high resolution mass spectrum showed that the molecular composition of TRA' and TRB' are $C_{28}H_{30}O_{10}$ and $C_{29}H_{34}O_{10}$ respectively, Some results of physicochemical properties were presented in this paper. Single crystal X-ray diffractometry of TRB' showed that the three dimensional structure of TRB' has not changed significantly from that of $TRB\;(C_{29}H_{34}O_9)$, except for the insertion of one oxygen atom into TRB to make additional pyran in the E-ring. It is also suggested that the aromatic moiety of TRA' is similar to that of $TRA\;(C_{28}H_{30}O_9)$ and the rest non-aromatic portions resemble to those of TRB'. The tremorgenic activity, lethality and inhibitory effect on acetylcholine esterase of TRA' and TRB' are greatly reduced comparing to that of TRA and TRB.

• 비파괴검사학회지
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• 제33권2호
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• pp.160-164
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• 2013

레이저 초음파검사 장치는 레이저 빔을 이용하여 초음파 신호를 발생시키고 측정하는 비접촉식 결함 검사 장치이다. 이 장치는 펄스 레이저 빔을 이용하여 광대역 주파수 범위를 갖는 초음파 신호를 발생시키고 작은 점으로 집속된 레이저 빔을 이용하여 초음파 신호를 측정하므로 우수한 측정 분해능을 제공한다. 본 연구에서는 이종금속 접촉부식(갈바닉 부식) 현상을 레이저를 이용한 비파괴, 비접촉 방법으로 측정하였다. 부식된 부분에 이물질이 혼합되는 경우를 가정하고, 레이저 초음파 실험을 진행하였다. 시편의 뒷면에서 펄스 레이저로 초음파를 발생시키고, 같은 위치의 앞면에서 CW 레이저와 CFPI를 이용하여 초음파 신호를 획득하였다. 이물질이 존재하는 부분의 초음파 신호 특성을 분석하여 이물질의 위치 및 크기를 측정하였다.

• 천문학회보
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• 제43권1호
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• pp.66.1-66.1
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• 2018

Turbulence is a phenomenon which largely determines the density and velocity fields in molecular clouds. Turbulence can produce density fluctuation which triggers a gravitational collapse, and it can also produce a non-thermal pressure against gravity. Therefore, turbulence controls the mode and tempo of star formation. However, despite many years of study, the properties of turbulence remain poorly understood. As part of the Taeduk Radio Astronomy Observatory (TRAO) Key Science Program (KSP), "apping Turbulent properties In star-forming MolEcular clouds down to the Sonic scale (TIMES; PI: Jeong-Eun Lee)", we have mapped two star-forming clouds, the Orion A and the ${\rho}$ Ophiuchus molecular clouds, in 3 sets of lines (13CO 1-0/C18O 1-0, HCN 1-0/HCO+ 1-0, and CS 2-1/N2H+ 1-0) using the TRAO 14-m telescope. We aim to map entire clouds with a high-velocity resolution (~0.05 km/s) to compare turbulent properties between two different star-forming environments. We will present the preliminary results using a statistical method, Principal Component Analysis (PCA), that is a useful tool to represent turbulent power spectrum.

• 천문학회지
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• 제50권6호
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• pp.157-165
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• 2017

$H_2O$ maser emission at 22 GHz in the circumstellar envelope is one of the good tracers of detailed physics and kinematics in the mass loss process of asymptotic giant branch stars. Long-term monitoring of an $H_2O$ maser spectrum with high time resolution enables us to clarify acceleration processes of the expanding shell in the stellar atmosphere. We monitored the $H_2O$ maser emission of the semi-regular variable R Crt with the Kagoshima 6-m telescope, and obtained a large data set of over 180 maser spectra over a period of 1.3 years with an observational span of a few days. Using an automatic peak detection method based on least-squares fitting, we exhaustively detected peaks as significant velocity components with the radial velocity on a $0.1kms^{-1}$ scale. This analysis result shows that the radial velocity of red-shifted and blue-shifted components exhibits a change between acceleration and deceleration on the time scale of a few hundred days. These velocity variations are likely to correlate with intensity variations, in particular during flaring state of $H_2O$ masers. It seems reasonable to consider that the velocity variation of the maser source is caused by shock propagation in the envelope due to stellar pulsation. However, it is difficult to explain the relationship between the velocity variation and the intensity variation only from shock propagation effects. We found that a time delay of the integrated maser intensity with respect to the optical light curve is about 150 days.

• Journal of Radiation Protection and Research
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• 제43권3호
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• pp.85-96
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• 2018

Background: A variety of inorganic scintillators have been developed and improved for use in radiation detection and measurement, and in situ gamma-ray spectrometry in the environment remains an important area in nuclear safety. In order to verify the feasibility of promising scintillators in an actual environment, a performance test is necessary to identify gamma-ray peaks and calculate the radioactivity from their net count rates in peaks. Materials and Methods: Among commercially available scintillators, $LaBr_3(Ce)$ scintillators have so far shown the highest energy resolution when detecting and identifying gamma-rays. However, the intrinsic background of this scintillator type affects efficient application to the environment with a relatively low count rate. An algorithm to subtract the intrinsic background was consequently developed, and the in situ calibration factor at 1 m above ground level was calculated from Monte Carlo simulation in order to determine the radioactivity from the measured net count rate. Results and Discussion: The radioactivity of six natural radionuclides in the environment was evaluated from in situ gamma-ray spectrometry using an $LaBr_3(Ce)$ detector. The results were then compared with those of a portable high purity Ge (HPGe) detector with in situ object counting system (ISOCS) software at the same sites. In addition, the radioactive cesium in the ground of Jeju Island, South Korea, was determined with the same assumption of the source distribution between measurements using two detectors. Conclusion: Good agreement between both detectors was achieved in the in situ gamma-ray spectrometry of natural as well as artificial radionuclides in the ground. This means that an $LaBr_3(Ce)$ detector can produce reliable and stable results of radioactivity in the ground from the measured energy spectrum of incident gamma-rays at 1 m above the ground.

• 센서학회지
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• 제23권2호
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• pp.110-113
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• 2014

In this paper, we propose and demonstrate a Fabry-Perot interferometer (FPI) optical fiber tip sensor fabricated by a blade-sawing technique using a fiber optic patch cord for high-resolution temperature measurement. The sensor head consists of a short air FP cavity near the tip of a single-mode fiber patch cord tip. The temperature which we can measure is determined through a phase variation of the interference fringes in the reflective spectrum of the sensor. The fiber optic FPI sensor in this work can monitor the environmental temperature very accurately from 40 to $120^{\circ}C$. As a result, the temperature sensitivity is obtained as $38.2pm/^{\circ}C$.

• 천문학회지
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• 제48권2호
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• pp.105-112
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• 2015

The symbiotic star V1016 Cygni, a detached binary system consisting of a hot white dwarf and a mass-losing Mira variable, shows very broad emission features at around 6825 Å and 7082 Å, which are Raman scattered O vi λλ 1032, 1038 by atomic hydrogen. In the high resolution spectrum of V1016 Cyg obtained with the Bohyunsan Optical Echelle Spectrograph these broad features exhibit double peak profiles with the red peak stronger than the blue counterpart. However, their profiles differ in such a way that the blue peak of the 7082 feature is relatively weaker than the 6825 counterpart when the two Raman features are normalized to exhibit an equal red peak strength in the Doppler factor space. Assuming that an accretion flow around the white dwarf is responsible for the double peak profiles, we attribute this disparity in the profiles to the local variation of the flux ratio of O vi λλ 1032, 1038 in the accretion flow. A Monte Carlo technique is adopted to provide emissivity maps showing the local emissivity of O vi λ1032 and O vi λ1038 in the vicinity of the white dwarf. We also present a map indicating the differing flux ratios of O vi λλ 1032 and 1038. Our result shows that the flux ratio reaches its maximum of 2 in the emission region responsible for the central trough of the Raman feature and that the flux ratio in the inner red emission region is almost 1. The blue emission region and the outer red emission region exhibit an intermediate ratio around 1.5. We conclude that the disparity in the profiles of the two Raman O vi features strongly implies accretion flow around the white dwarf, which is azimuthally asymmetric.

• 한국광학회지
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• 제19권1호
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• pp.36-42
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• 2008

PZT형 파장가변 필터를 이용하여 파장스윕(wavelength-swept) 광원을 구성할 때 발진파장의 변화율을 일정하게 하려면 필터의 이력(hysteresis)특성을 알아야 한다. 이력특성을 무시하고 필터를 구동할 경우 파장스윕 광원을 사용하는 optical frequency domain reflectometry(OFDR) 시스템의 분해능이 떨어진다. 광스펙트럼 분석기(OSA)를 이용하여 필터의 이력특성을 측정할 수도 있지만 측정시간이 너무 길고 실제 구동조건에서의 이력특성은 측정할 수 없다는 문제가 있어 실제 구동조건에서 필터의 이력특성을 고속으로 측정할 수 있는 OFDR의 원리에 기초한 이력 측정법을 제시하였다. 파장스윕 광원과 간섭계, 신호처리 장치, 그리고 PC 프로그램으로 구성된 고속 이력측정장치를 구현하고, 이를 사용하여 필터 구동조건에서의 이력특성을 측정하였다. 마지막으로 측정된 이력특성을 파장스윕광원의 구동에 적용하여 선형적 파장변화를 얻음으로써 새로운 이력측정법의 유효성을 검증하였다.

• 한국자기학회지
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• 제16권1호
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• pp.11-13
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• 2006

[ $M\"{o}ssbauer$ ] spectra of $Ti_{1-x-y}Co_xFe_yO_2(0.01{\leq}x,\;y{\leq}0.05)$ prepared with $^{57}Fe$ enriched iron have been taken at various temperatures ranging from 80 to 300K. The Mossbauer spectrum of $Ti0.94Co_{0.03}Fe_{0.03}O_2$ consists of a ferromagnetic (six-Lorentzian), a paramagnetic phase (doublet) and armorphous phase over all temperature ranges. Isomer shifts indicate $Fe^{3+}$ for the ferromagnetic phase and the paramagneic phase of $Ti_{1-x-y}Co_xFe_yO_2$ samples. It is noted that the magnetic hyperfine field of ferromagnetic phase had the value about 1.5 times as large as that of u-fe. The XRB data for $Ti_{1-x-y}Co_xFe_yO_2$ showed mainly rutile phase with tetragonal structures without any segregation of Co and Fe into particulates within the instrumental resolution limit. The magnetic moment per (Co+Fe) atom in $Ti0.94Co_{0.03}Fe_{0.03}O_2$, under the applied field of 1T was estimated to be about $0.332{\mu}_B$ which is ten times as large as that of $Ti0.97Co_{0.03}Fe_{0.03}O_2,\;0.024{\mu}_B$ per Co atom, suggesting a high spin configuration of Co and fe ions.