• Journal of the Optical Society of Korea
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• 제17권2호
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• pp.182-187
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• 2013

We present a comparative experimental analysis of the thermal spectroscopic characteristics of a phosphosilicate (P)-based ytterbium-doped fiber (YDF) against an aluminosilicate (Al)-based YDF in the temperature range of 25 to $150^{\circ}C$. We also characterize the fibers as gain media in a cladding-pumped amplifier configuration. While both fibers exhibit comparable trends in their thermal characteristics, there are noticeable distinctions in the fluorescence lifetime reduction rate and the spectral dependence of the transition cross-sections. The P- and Al-based YDFs present thermal lifetime reduction rates of $0.012%/^{\circ}C$ and $0.026%/^{\circ}C$, respectively. In particular, in the spectral region at ~940 nm, the absorption cross-section of the P-based YDF undergoes significantly less thermal change compared to that of the Al-YDF. In the cladding-pumped amplifier configuration operating at a total gain of 10 dB, the Al-based YDF generally performs betters than the P-based YDF in the temperature range of 25 to $75^{\circ}C$. However, it is highlighted that in the high temperature range of over $75^{\circ}C$, the latter shows a less gain reduction rate than the former, thereby yielding higher relative output power by 3.3% for a 1060-nm signal, for example.

• 한국근적외분광분석학회:학술대회논문집
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• 한국근적외분광분석학회 2001년도 NIR-2001
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• pp.1171-1171
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• 2001

Quantitative analysis is an important requirement in exploration, mining and processing of minerals. There is an increasing need for the use of quantitative mineralogical data to assist with bore hole logging, deposit delineation, grade control, feed to processing plants and monitoring of solid process residues. Quantitative analysis using X-Ray Powder Diffraction (XRD) requires fine grinding and the addition of a reference material, or the application of Rietveld analysis to XRD patterns to provide accurate analysis of the suite of minerals present. Whilst accurate quantitative data can be obtained in this manner, the method is time consuming and limited to the laboratory. Mid infrared when combined with multivariant analysis has also been used for quantitative analysis. However, factors such as the absorption coefficients and refractive index of the minerals requires special sample preparation and dilution in a dispersive medium, such as KBr to minimize distortion of spectral features. In contrast, the lower intensity of the overtones and combinations of the fundamental vibrations in the near infrared allow direct measurement of virtually any solid without special sample preparation or dilution. Thus Near Infrared Spectroscopy (NIR) has found application for quantitative on-line/in line analysis and control in a range of processing applications which include, moisture control in clay and textile processing, fermentation processes, wheat analysis, gasoline analysis and chemicals and polymers. It is developing rapidly in the mineral exploration industry and has been underpinned by the development of portable NIR spectrometers and spectral libraries of a wide range of minerals. For example, iron ores have been identified and characterized in terms of the individual mineral components using field spectrometers. Data acquisition time of NIR field instruments is of the order of seconds and sample preparation is minimal. Consequently these types of spectrometers have great potential for in-line or on-line application in the minerals industry. To demonstrate the applicability of NIR field spectroscopy for quantitative analysis of minerals, a specific example on the quantification of lateritic bauxites will be presented. It has been shown that the application of Partial Least Squares regression analysis (PLS) to the NIR spectra can be used to quantify chemistry and mineralogy in a range of lateritic bauxites. Important, issues such as sampling, precision, repeatability, and replication which influence the results will be discussed.

• 한국대기환경학회지
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• 제21권6호
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• pp.631-637
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• 2005

A UV-MFRSR instrument was used to measure the global and diffuse irradiances in 7 narrowband channels in the UV range 299.4, 304.4, 310.9, 317.3. 324.5, 331.3 and 367.4 nm at Gwangju ($35^{circ}\;13'N\;126^{circ}\;50'E$), Korea. Spectral UV-AOD was retrieved using the Langley plot method for data collected from April 2002 to July 2004. Temporal variation of AOD at 367.4 nm ($AOD_{367nm}$) showed a maximum in June ($0.95\pm0.43$) and a minimum in February ($0.31\pm0.14$). Clear seasonal variation of $AOD_{367nm}$ was observed with average values of $0.68\pm0.29,\;0.82\pm0.41,\;0.48\pm0.22\;and\;0.42\pm0.21$ in spring, summer, fall and winter, respectively, Average Angstrom exponent for the entire monitoring period was $2.03\pm0.75$ in the UV-A ($324.5\∼367.4$ nm) range. Seasonal variation of the Angstrom exponent showed a maximum in spring and a minimum in summer. The lowest Angstrom exponent in summer might be due to hygroscopic growth of particles under conditions of high relative humidity. UV-AOD changes under different atmospheric conditions were also analyzed. Uncertainty in retrieving spectral UV-AOD was also estimated to range between $\pm0.218\;at\;304.4\;nm\;and\;\pm0.135\;at\;367.4\;nm$. Major causes of uncertainty were total column ozone retrieval and extraterrestrial irradiance retrieval at shorter and longer wavelengths, respectively.

• 대한전자공학회논문지SD
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• 제47권7호
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• pp.17-22
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• 2010

본 논문에서는 Mach-Zehnder 광변조기의 양방향 변조를 이용하는 새로운 광섬유격자 센서 검출 방법을 제안하고 실험을 통하여 그 유용성을 밝힌다. 제안한 구조는 광대역 광원, 광섬유격자, Mach-Zehnder 광변조기, chirped 광섬유격자, 그리고 광 검출기로 구성된다. 실험을 통하여 제안한 구조의 전달함수를 구하고, 505 MHz에서 525 MHz까지 주파수 영역에서 10개의 다른 파장을 가진 광에 대한 FSR(free spectral range)의 변화로부터 시간지연을 계산한다. 구한 결과로부터 광의 파장 변화에 따른 시간지연이 12.9 ps/0.2 nm 값을 가지면서 매우 선형적임을 알 수 있다. 이러한 결과는 광섬유격자를 이용한 스트레인 또는 온도 센서에 이용할 수 있다.

• 한국태양에너지학회 논문집
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• 제30권5호
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• pp.25-31
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• 2010

A Precision Spectral Pyranometer (PSP) is mainly used as a reference to calibrate other pyranometers due to its high accuracy and sensitivity in response to the spectrum wavelength range of 0.285 ${\mu}$ to 2.8 ${\mu}$, while the sensitivity of photovoltaic-type Li-Cor pyranometer is limited within a certain spectral range from 0.4 ${\mu}$ to 1.1 ${\mu}$. In this study, two Eppley PSPs($PSP_1$ and $PSP_2$) were first compared to the calibrated Eppley PSPs from National Renewable Energy Laboratory (NREL), resulting in two linear correction factors based on the comparison between the logger output (V) from the test PSP and the solar radiation (W/m2) from the NREL PSP. The Li-Cor pyranometer used in this study was then corrected based on the comparison of measured solar radiation ($W/m^2$) from the corrected $PSP_1$ and the Li-Cor pyranometer. In addition, instrument scale corrections were also performed for the PSPs and the Li-Cor from the transmitter to the data logger. From the comparisons, a linear correction factor (1.0214) with R=0.9998 was developed for the scale correction between$PSP_1$ and $PSP_2$, while the Li-Cor pyranometer has a scale(1.0597) and offset (32.046) with R=0.9998 against$PSP_1$. As a result, it was identified that there were good agreements within ${\pm}$ 10 W/ $m^2$ between Eppley $PSP_1$ vs. $PSP_2$ solar radiation and within ${\pm}$ 20 W/$m^2$ between$PSP_1$ vs Li-Cor solar radiation after the empirical scale corrections developed in this study.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2009년도 학술대회 초록집
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• pp.28-33
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• 2009

메탄하이드레이트는 새로운 에너지원으로의 가능성뿐 아니라 지구 온난화의 원인으로도 알려져 이에 대한 연구가 활발하다. 메탄하이드레이트 부존층의 평가에 대한 연구는 BSR의 존재와 지진파 속도로부터 메탄하이드레이트 부존랑을 추정하는 연구가 주가 되고 있으나, 최근에는 지진파 감쇠특성으로부터 메탄하이드레이트의 분포를 추정하는 연구도 시도되고 있다. 본 연구에서는 일본 난카이 트러프에서 취득된 2차원 반사법 지진파 데이터로부터 지진파 감쇠지 ($Q^{-1}$)를 산출하여 메탄하이드레이트 부존층에서의 지진파 감쇠특성을 분석하였다. QVO법을 이용하여 주파수 범위 $30{\sim}70Hz$ 오프셋 범위 $125{\sim}1,575m$내에서 제로오프셋 감쇠치를 추정한 결과, BSR상부의 메탄 하이드레이트 부존층에서 지진파 감쇠지가 크게 증가하는 것을 관찰 할 수 있었다. 따라서 본 연구의 결과를 통해 위 주파수 범위내 반사법 지진파의 메탄하이드레이트 부존층내 감쇠 특성을 확인하였으며, 이를 이용한 메탄하이드레이트 농축대의 추정 가능성을 확인하였다.

• 한국광학회지
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• 제22권5호
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• pp.207-213
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• 2011

몬테카를로 방법을 기반으로 한 수치해석을 이용하여 AWG(arrayed waveguide grating)의 위상 오차를 측정하는 방법을 제안한다. 진동수 영역 측정법에서 실험치와 가장 근접한 이론치를 구하기 위해 몬테카를로 방법을 사용하며 최적화된 이론치로부터 AWG 각 도파로의 진폭과 위상값들을 결정한다. 이 방법의 타당성을 검증하기 위해 모의실험을 수행하였다. AWG의 각 도파로에 임의로 위상 오차를 설정하여 가상의 실험치를 만들고 우리의 방법을 통해 거꾸로 위상 오차를 알아냈다. 모의실험 결과 간섭계 광원의 진동수 변조 범위가 AWG FSR(free spectral range)의 1.7 배보다 클 때, 그리고 위상 오차가 ${\pm}50^{\circ}$ 이내일 때 매우 정확하게 위상 및 진폭을 측정할 수 있음을 확인하였다.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2001년도 하계학술대회 논문집
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• pp.215-218
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• 2001

A flame detector responds either to radiant energy visible to the human eye or outside the range of human vision. Such a detector is sensitive to glowing embers, coals, or flames which radiate energy of sufficient intensity and spectral quality to actuate the alarm. An infra-red detectors can respond to the total IR component of the flame alone or in combination with flame flicker in the frequency range of 5 to 30 Hz. A major problem in the use of infrared detectors receiving total IR radiation is the possible interference of solar radiation in the infrared region. When detectors are located in places shielded from the sun, such as vaults. filtering or shielding the unit from the sun's rays is unnecessary. In this study, we proposed method for redue a false alarm with using filtering & sensor technology for distinguish of causes of raise a false alarm and pure flame.

• 천문학논총
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• 제15권spc1호
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• pp.73-83
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• 2000

X-ray astronomy deals with measurements of the electromagnetic radiation in the energy range of $E\~0.1-100 keV (\lambda\~0.12-120{\AA})$. The wavelength of X-ray is comparable to the size of atoms, so that the photons in the X-ray range are usually produced and absorbed by the atomic processes. Since the launch of the first X-ray astronomy satellite 'Uhuru' in 1970, technological advances in a launch capability and a detection capability make X-ray astronomy one of the most rapidly evolving fields of astronomical research. Particularly, a spectral resolving power $E/{\Delta}E$ has been increased by an order of 2 - 3 (in the energy range of 0.1 - 10 keV) during the past 30years. In this paper, I briefly review a developing process of the resolving power and spectroscopic techniques. Then I describe important emission/absorption lines in X-ray astronomy, as well as diagnostics of gas property with line parameters.

• 연구논문집
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• 통권30호
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• pp.43-56
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• 2000

N-IR spectroscopy technology is very useful. And, the technology has wide application range. In the range, we know that single beam type silica analyzer has some handicap. So we were studied Splitted beam type silica analyzer. This dissertation have been discuss about system structure, system fundamentals and performance test. At the test, we were study in the spectral interference of NH3. We know that existing system had some problem. It is structural frailties of single beam type. Therefore we were study for Splitted beam type structure. And we obtain a good result. We have $\pm$5% accuracy and 0.5 ppb level measuring range. But, we have a question. It is ppt level measuring technology by the laser beam spectroscopy.