본 연구는 헤테로코어 광파이버 센서를 활용하여 콘크리트 내부에서 발생되는 변형률의 측정을 통해 콘크리트의 프리스트레스를 직접 평가할 수 있는 새로운 매립형 센서모듈 개발을 최종 목표로 하고 있다. 이를 위하여 노출형 센서모듈을 이용한 성능발현 실험결과는 가력속도 0.12, 1.80mm/min일 때 52.1, 2.6sec로 최대 약 19배의 계측 지연현상이 발생하였다. 계측 지연현상은 구조물의 실시간 변화 상태를 계측하지 못하는 경우로 실시간 계측이 가능한 센서모듈의 개발을 위해서 추가실험이 필요한 것으로 판단하였다. 계측 지연현상 원인규명 실험은 3가지의 실험을 계획하였으며, 실험결과는 마찰저항에 의한 계측 지연이 지배적으로 확인되었다. 마찰이 제거된 장치를 이용한 센서모듈의 실험결과에서는 계측 지연현상이 나타나지 않은 것으로 확인되었다.

The telescope to be onboard SPICA (Space Infrared Telescope for Cosmology and Astrophysics) has an aperture diameter of 2.5 m and its imaging performance is to be diffraction-limited at a wavelength of 20 μm at the operating temperature of <8 K. Because manufacturing precise autocollimating at mir- rors (ACFs) with sizes comparable to the SPICA telescope is not technically feasible, we plan to use sub-aperture stitching interferometry through ACFs for optical testing of the telescope. We have verified the applicability of the sub-aperture stitching technique to the SPICA telescope by performing stitching experiments in a vacuum at a room temperature, using the 800-mm telescope and a 300-mm ACF. We have also developed a new method to reduce uncertainties possibly caused by cryogenic and gravitational deformations of ACFs.

상부 탑재형 노내계측기(TM-ICI) 개발은 원자로하부헤드 대신 원자로상부헤드로 계측기를 삽입함으로써 중대사고 위험을 줄이기 위해 진행 중이다. 이 개발 과제의 일환으로, NUREG/CR-6909와 Code Case N-761의 두 방법에 따라 TM-ICI 노즐에 대한 환경피로평가가 수행되었다. TM-ICI 노즐은 level A, level B 및 시험 조건에서의 과도조건에 따른 하중을 받는데 이에 대해 피로평가를 해야 한다. 원자로냉각재환경이 고려된 TM-ICI 노즐의 누적사용계수는 1이하로 평가되었고, 이는 ASME Code 허용기준을 만족한다.

We developed the memory storage type instrumentation device for measuring trajectory of small flying object. The instrumentation device is small enough to install into the flying object and has a 6-axis MEMS sensor and 3 AD channels for measuring flying data of object. In this paper, we specially focused on the measuring of flying trajectory of the sabot using developed device. The sabot which supports missile during carriage breaks away from missile by mechanical and aerodynamic force when missile gets out of canister. The flying trajectory of sabot should be designed not to collide with any equipments around the launcher. In order to find out the flying trajectory of sabot, the developed instrumentation device was adopted in experiment. We have proved effectiveness of the developed instrumentation device by comparing acquired results using the hi-speed camera.

본 연구에서는 간척지 내에 온실을 시공할 경우, 온실 설계의 기초자료로 활용하기 위하여 최근 나무말뚝 기초를 사용하여 완공한 계화도 간척지의 1-2W형 온실을 대상으로 온실기초의 침하량을 계측하고 검토하였다. 그 결과는 다음과 같다. 지반조사 결과, 기반암인 연암층은 확인되지 않았으며 부지 조성 당시 매립한 것으로 추정되는 매립층과 그 하부에 퇴적층이 존재하는 것으로 조사되었다. 그리고 매립층과 퇴적층 하부에 풍화대가 존재하는 것으로 조사되었다. 전체 지반층의 토성은 시추 공에 관계없이 주로 점토 섞인 모래, 실트질 모래, 실트 질 점토 및 화강편마암 순으로 구성되어 있었다. 지하수 위도 시추공에 관계없이 지반에서 0.3m 아래에 있는 것으로 나타났다. 온실기초 및 나무말뚝의 침하량은 전체적으로 볼 때, 온실 내·외부나 계측지점(채널)에 관계없이 침하량에는 다소 차이가 있지만, 시간의 경과와 함께 침하량이 증가하고 있는 것으로 나타났다. 그리고 온실 내부 기둥의 경우, CH-2는 좀 예외적이긴 하지만, 온실 측벽(방풍벽 측)에 있는 지점의 데이터가 상대적으로 큰 진폭으로 흔들리는 것은 알 수 있었다. 또한 특정 시기에 침하량이 상대적으로 크게 증가한 후, 어느 정도 침하량이 회복 되는 현상을 볼 수 있었다. 이와 같은 현상 들을 포함하여 CH-1을 제외하고 현 시점에서 온실 내· 외부 전체의 지점별(CH-2~CH-10) 침하량은 1.0~7.5mm 정도의 범위에 있는 것으로 나타났다. 회귀 분석한 결과 결정계수는 지점별로 0.6362∼0.9340까지의 범위로서 상 관관계가 높은 것으로 나타났다. 그리고 온실외부의 경우는 0.6046~0.8822로서 온실내부 보다는 다소 낮지만, 상관관계가 있는 것으로 나타났다.

현재 우리나라에서 사용되고 있는 등부표의 종류는 10가지 정도이며, 부표 설계 및 개발의 대부분을 외국 기술에 의존하고 있는 실정이다. 본 연구에서는 해상 계측 등이 가능한 소형 등부표의 개발을 목표로 소형 부표의 설계안을 제시하고 그 안전성을 수치적으로 검토하였다. 구체적으로는 다양한 실제 해상환경과 유사한 조우각과 선속 변화에 따른 내항성과 관련된 응답 진폭비, 부가저항 등의 값을 수치적으로 시뮬레이션하였다. 설계된 부표의 응답해석 결과, 종요응답비가 조우주파수의 증가에 따라 전체적으로 감소하는 특성을 확인하였다. 횡파에 대한 부가저항이 가장 크게 나타나는 것으로 분석되었고, 최종적으로 제시된 부표가 일정 조건하에서 응답 특성이 확보됨을 확인하였다.

Fuel Test Loop(FTL) is a facility which could conduct a fuel irradiation test at HANARO (High-flux Advanced Neutron Application Reactor). FTL simulates commercial NPP’s operating conditions such as the pressure, temperature and neutron flux levels to conduct the irradiation and thermo- hydraulic tests. The In-Pile Test Section(IPS) installed in HANARO FTL is designed as a pressure vessel design conditions of 350℃, 17.5MPa. The instrumentation MI-cables for thermocouples, SPND and LVDT are passed through the sealing plug, which is in the pressure boundary region and is a part of instrumentation feedthrough of MI-cable. In this study, the brazing method and performance test results are introduced to the sealing plug with BNi-2 filler metal, which is selected with consideration of the compatibility for the coolant. The performance was verified through the insulation resistance test, hydrostatic test, and helium leak test.

KASI and Seoul National University developed the Fast Imaging Solar Spectrograph (FISS) as one of major scientific instruments for the 1.6 m New Solar Telescope (NST) and installed it in the Coude room of the NST at Big Bear Solar Observatory (BBSO) in May, 2010. The major objective of the FISS is to study the fine-scale structures and dynamics of plasma in the photosphere and chromosphere. To achieve it, the FISS is required to take data with a spectral resolution higher than 105 at the spectrograph mode and a temporal resolution less than 10 seconds at the imaging mode. The FISS is a spectrograph using Echelle grating and has characteristics that can observe dual bands (Hα and CaII 8542) simultaneously and perform fast imaging using fast raster scan and two fast CCD cameras. In this paper, we introduce briefly the whole process of FISS development from the requirement analysis to the first observations.

Current instrumentation activities and the open user status of Okayama Astrophysical Observatory (OAO) are reviewed. There are two telescopes in operation and one telescope under reforming at OAO. The 188cm telescope is provided for open use for more than 200 nights in a year. The typical over-subscription rate of observation proposals for the 188cm telescope is ~ 1.5 - 2. The 50cm telescope is dedicated to ɤ-ray burst optical follow-up observation and is operated in collaboration with Tokyo Institute of Technology. The 91cm telescope will become a new very wide field near-infrared camera in two years. The high-dispersion echelle spectrograph (HIDES) is the current primary instrument for the open use of the 188cm telescope. Two new instruments, an infrared multi-purpose camera (ISLE) and an optical low-dispersion spectrograph (KOOLS), are now under development. They will be open as common use instruments in 2006.

It is realized that the extraterrestrial matter is in ionized state, plasma, so the matter of this kind behaves as not expected because of its sensitiveness to electric and magnetic fields and its ability to carry electric currents. This kind of subtle change can be observed by an instrument for the magnetic field measurement, the magnetometer usually mounted on the rocket and the satellite, and based on the ground observatory. The magnetometer is a useful instrument for the spacecraft attitude control and the Earth's magnetic field measurements for the scientific purpose. In this paper, we present the preliminary design and the test results of the two onboard magnetometers of KARl's (Korea Aerospace Research Institute) sounding rocket, KSR­III, which will be launched during the period of 2001-02. The KSR-III magnetometers consist of the fluxgate magnetometer, MAG/AIM (Attitude Information Magnetometer) for acquiring the rocket flight attitude information, and of the search-coil magnetometer, MAG/SIM (Scientific Investigation Magnetometer) for the observation of the Earth's magnetic field fluctuations. With the MAG/AIM, the 3-axis attitude information can be acquired by the comparison of the resulting dc magnetic vector fields with the IGRF (International Geomagnetic Reference Field). The Earth's magnetic field fluctuations ranging from 10 to 1,000 Hz can also be observed with the MAG/SIM measurement.

The purposes of spectroscopy in astronomy are to measure the radiation flux of the spectroscopic emission or absorption line and to measure the dynamical parameters of the line profile. In order to use an appropriate instrument for the scientific purpose, we need to understand the characteristics of various spectrometers, e.g., a prism spectrometer, a grating spectrometer, and a Fabry-Perot spectrometer (FPS), which are being used in ultra-violet, optical, and infrared bands. The Fabry­Perot spectrometer is not very popular compared to the grating spectrometer, because of its complex and tricky operations. The Fabry-Perot spectrometer, however, can get a two-dimensional image at one exposure, so we can study radiation mechanisms and dynamical properties of extended sources, e.g., clusters, nebula, and galaxies.

In this study, quartile control chart method is tried to apply to determine limit values of existing dams of K-water’s instrumentation data for dam safety, show asymmetric distributed data, and the example of application is presented. The determined limit values of concrete stress meter and concrete non-stress meter by Shewhart method and quartile method show that the determined limit values by Shewhart method indicate that the majority of instrumentation are on abnormal condition, although the measured values are normal behavior. But, in case of the result of quartile method has such an error. Like this, it is judged that the determination of the limit values of dam instrumentation, show asymmetric and abnormal distributed data, by the quartile method is appropriate. Therefor The quartile method is applied to the determination of limit values of existing dam instrumentation of K-water.

Based Recently, Box type Precast segment Retaining wall with the Relieving Platform has been developed. In this study, it is going th measure that the effect of reducing the earth pressure by placing the Relieving Platform on field.

Herein, we discuss the in situ measurement of the electron temperature in the ionosphere/plasmasphere by means of DC Langmuir probes. Major instruments which have been reported are a conventional DC Langmuir probe, whose probe voltage is swept; a pulsed probe, which uses pulsed bias voltage; a rectification probe, which uses sinusoidal signal; and a resonance cone probe, which uses radio wave propagation. The content reviews past observations made with the instruments above. We also discuss technical factors that should be taken into account for reliable measurement, such as problems related to the contamination of electrodes and the satellite surface. Finally, we discuss research topics to be studied in the near future.

In this study, among the reliability assessment method for measured data of dam instrumentation, time series analysis and behavior analysis were introduced and the reliability assessment cases for seepag weir, pore-pressure meter, concrete stress meter and joint meter were presented.

In this study, quartile control chart method is tried to apply to determine limit values of dam instrumentation data for dam safety, show asymmetric distributed data, and the example of application is presented. The determined limit values of concrete stress meter and concrete non-stress meter by Shewhart method and quartile method show that the determined limit values by Shewhart method indicate that the majority of instrumentation are on abnormal condition, although the measured values are normal behavior. But, in case of the result of quartile method has such an error. Like this, it is judged that the determination of the limit values of dam instrumentation, show asymmetric and abnormal distributed data, by the quartile method is appropriate. Therefor The quartile method is applied to the determination of limit values of dam instrumentation of K-water.