The KASINICS (Korea Astronomy and Space science Institute Near Infrared Camera System) is a ground-based near-infrared (NIR) imaging instrument. KASINICS has offner relay optics to reduce unwanted infrared light. For the offner optics, we adopted an ultra precision machining process which is installed at KBSI (Korea Basics Science research Institute). Since the offner relay optics is made of aluminum 6061 metal material, we did several tests to reach the specification. We found that a 0.497mm radius nose bite and 220m/min machining speed are best tool and condition to make this offner optics with the precision machine. In this paper, we report the technical method of ultra precision machining and results of the KASINICS offner optics.

  Forming central warehouses for a number of stores can save costs in the continuous review inventory model due to economy of scale and information sharing. In this paper, transportation costs are included in this inventory model. Hence, the tradeoff betw

곰소만 조간대 퇴적물의 장기적 변화를 조사하기 위하여 1991년과 2006년에 채취된 표층퇴적물 시료를 분석하고, 그 결과를 비교하였다. 만 입구 조간대에서는 실트와 점토의 함량이 감소하고 모래의 함량이 증가하였다. 만의 중부와 상부 조간대에서는 모래와 점토의 함량이 감소하고 실트의 함량이 증가하였다. 특히 점토의 함량은 주변의 다른 반폐쇄된 조간대에 비해 상대적으로 매우 낮은 함량 분포를 보였으며, 1991년에 비해서도 뚜렷하게 감소하는 경향을 보였다. 퇴적물 구성성분의 뚜렷한 함량 변화는 퇴적상의 변화를 초래하였다. 이러한 변화는 매립 및 호안건설에 의한 해안선의 변형과 간조선 부근에 빽빽하게 설치된 양식장의 구조물, 그리고 곰소만 북쪽의 새만금 방조제 건설 등에 의한 수리에너지 조건의 변화에 기인한 것으로 해석된다.

예로부터 선장은 경험적으로 기상, 선박 제원 상태 및 운항 일정을 고려하여 최적의 항로를 선택하여 항해하여 왔다. 이는 선장의 경험을 바탕으로 해류나 파랑에 대한 기상 예보 정보를 활용하여 최적항로를 결정하는 것으로 아직까지 선상에서 항로 결정을 보조해주는 디지털화한 시스템은 그 사례를 찾아보기 힘들다. 본 논문에서는 선박의 운항 효율성과 안전성의 관점에서 구성된 선상 최적 항로 안전 평가 시스템을 소개한다. 선사와 선장이 요구하는 효율적인 항해를 위해서는 도착예정시간 및 연료소모량을 최소로 하는 최적 항로를 구한다. 이는 선박의 파랑 중 부가저항에 기초를 둔 선속 저하 빚 마력 증가를 고려하여 계산한다. 안전성 관점에서는 3D 판넬법에 기초를 둔 선박의 내항 계산을 본 시스템에서 구현하여 내항 평가를 수행하며, 최종적으로 선박의 항로 안전 계획 및 평가를 위한 보조 수단이다.

Many gravitational wave detectors are now being built or under operation throughout the world. In particular, LIGO has taken scientific data several times, although current sensitivity is not sufficient to detect the weak signals routinely. However, the sensitivities have been improving steadily over past years so that the real detection will take place in the near future. Data analysis is another important area in detecting the gravitational wave signal. We have carried out the basic research in order to implement data analysis software in Korea@home environment. We first studied the LIGO Science Collaboration Algorithm Library(LAL) software package, and extracted the module that can generate the virtual data of gravitational wave detector. Since burst sources such as merging binaries of neutron stars and black holes are likely to be detected first, we have concentrated on the simulation of such signals. This module can generate pure gravitational wave forms, noise suitable for LIGO, and combination of the signal and noise. In order to detect the gravitational signal embedded in the noisy data, we have written a simple program that employs 'matched filtering' method which is very effective in detecting the signal with known waveform. We found that this method works extremely well.

This study was designed to determine the efficacy of ultrasound and laser therapy for sub-acute lower back pain. Twenty-seven patients with sub-acute low back pain were recruited, who were randomly assigned to three groups: Ultrasound group (actual ultrasound, 1.1 MHz, , duty cycle 100%, 10 min/session, n=9), laser group (actual laser, 904 nm, 155 ns, 13.5 W, 12 mW, 90 sec/point, n=9), and control group (placebo ultrasound or placebo laser, n=9). All of treatments including placebo procedures were applied to patients over a period of 2 weeks, five times a week. Visual Analogue Scale (VAS), Modified Schober's Test (MST), and Modified Oswestry Disability Questionnaire (MODQ) were used by the clinical and functional evaluations before and after intervention. At post-hoc, significant differences were observed in all groups with respect to VAS, MST (p<.05), except MODQ. VAS and MST score were more significantly improved in the ultrasound group than the laser and control group (p<.0167). However, no significant difference was present between the laser group and the control group. Therefore, this study revealed that ultrasound therapy was effective in pain relief and improvement of lumbar mobility in patients with sub-acute lower back pain. However, laser therapy did not show the effects for sub-acute lower back pain.

Ödön Lechner has been known as an architect who incorporates Hungarian folk motifs in creating a highly original Hungarian national style. Nevertheless, his work has been surprisingly neither exposed nor familiar to Korean audiences. This article attempts to reveal the unique characteristics of Lechner’s architectural thought and ideas along with his buildings in Budapest. First of all, this article presents the evolution of Lechner’s architectural thought by dividing his career into four marking periods. They are in chronological order to serve as a record of his architectural career. The authors then discuss his concern on the Hungarian ethnography in architecture while turing away from orthodox classicism. Subsequently, this article analyzes Lechner’s three major buildings located at Budapest. By doing so, it attempts to expose his underlying design ideas and to shed light on the most elegant works of the architect. Finally, it marks out Lechner's influences on young Hungarian architects.

단핵균주 간 교잡을 통해 육성된 고품질ㆍ다수확 느타리버섯“청산”의 주요특성은 다음과 같다. 가. 균사생장적온은 27∼28℃이고 버섯발생 및 생육온도는 14∼17℃이다. 나. 갓색은 진회색이고 얕은깔대기형이며 발생형태는 다발형이다. 다. 대색은 백색이고 형태는 굵고 긴형이다. 라. 버섯의 균일성에 있어서 갓색과 갓형태의 이형개체 발생은 없었고, 배양기간에서도 지역간 균일한 결과를 나타내었다. 마. 균상재배 시 초발이소요일수는 20일 내외, 자실체 생육일수는 4일이며, 수량은 농가실증시험에 평균 38 kg/3.3㎡을 나타냈다. 바. 청산느타리버섯은 균사활력이 강하며 적정생육온도에서 진회색을 띄나 적정온도이상의 재배환경에서는 갓색이 회색으로 바뀌어 품질이 저하되므로 생육온도 관리에 주의하여야 한다. 사. 발이량이 많으므로 재배 시 환기조절에 주의하여야 하며 갓이 약해 부서지기 쉬워 수확 및 포장 시 특히 주의를 요한다.

We have developed a control electronics system for an infrared detector array of KASINICS (KASI Near Infrared Camera System), which is a new ground-based instrument of the Korea Astronomy and Space science Institute (KASI). Equipped with a 512×512 InSb array (ALADDIN III Quadrant, manufactured by Raytheon) sensitive from 1 to 5μm, KASINICS will be used at J, H, Ks, and L-bands. The controller consists of DSP(Digital Signal Processor), Bias, Clock, and Video boards which are installed on a single VME-bus backplane. TMS320C6713DSP, FPGA(Field Programmable Gate Array), and 384-MB SDRAM(Synchronous Dynamic Random Access Memory) are included in the DSP board. DSP board manages entire electronics system, generates digital clock patterns and communicates with a PC using USB 2.0 interface. The clock patterns are downloaded from a PC and stored on the FPGA. UART is used for the communication with peripherals. Video board has 4 channel ADC which converts video signal into 16-bit digital numbers. Two video boards are installed on the controller for ALADDIN array. The Bias board provides 16 dc bias voltages and the Clock board has 15 clock channels. We have also coded a DSP firmware and a test version of control software in C-language. The controller is flexible enough to operate a wide range of IR array and CCD. Operational tests of the controller have been successfully finished using a test ROIC (Read-Out Integrated Circuit).

We have tested the performance of the Proto-model of Space Infrared Cryogenic System (PSICS), which is a small infrared camera, developed by Korea Astronomy and Space science Institute (KASI), Korea Basic Science Institute (KBSI), Korea Institute of Machinery and Materials (KIMM), and i3system co., as a cooperation project. The purpose of PSICS is to ensure a technology of small infrared cryogenic system for future development of space infrared (IR) cameras. PSICS consists of cryogenic part, IR sensor and electronics part, and optical part. The performance test of each part and the integrated system has been completed successfully. PSICS will be used as a guiding camera for ground-based IR telescopes and a test system for developing a space-borne instrument.

The KASINICS (KASI Near Infrared Camera System) is a ground-based Near-Infrared (NIR) imaging instrument developed by the Korea Astronomy and Space Science Institute (KASI). In this paper, we report the test results of the KASINICS camera optics system which is comprised of a 1-1 Offner relay. We measure that the surface RMS fluctuations of the Offner mirrors are at the level of 10−1−10−2 of the target wavelengths, showing that the mirrors are sufficiently smooth for NIR observations. The alignment of the Offner optics system has been checked too. Our ray-tracing simulations find that the image quality should not degrade more than the pixel size of the KASINICS ( 40μm), if a de-centering or a tilt of the Offner mirrors are within 5mm, or 2.5° . Our measurement shows that the de-centering or the tilt of the Offner mirrors are less than 1 mm or 0.5° , assuring that the KASINICS image quality are not affected by the alignment errors. We have also measured that the optics resolution is 20μm and it does not degrade more than 10% over the detector surface area of 14.3 mm / times 14.3mm. Overall, we conclude that the KASINICS optics system satisfies the design requirements for NIR imaging observations.

A Korean team (Korea Astronomy and Space Science Institute, Korea Basic Science Institute, and Kyung Hee University) takes part in an international cooperation project called CIBER (Cosmic Infrared Background ExpeRiment), which has begun with Jet Propulsion Laboratory (JPL) in USA and Institute of Space and Astronautical Science (ISAS) in Japan. CIBER is a rocket-borne instrument, of which the scientific goal is to measure the cosmic near-infrared extra-galactic background to search for signatures of primordial galaxy formation. CIBER consists of a wide-field two-color camera, a low-resolution absolute spectrometer, and a high-resolution narrow-band imaging spectrometer. The Korean team is in charge of the ground support electronics and manufacturing of optical parts of the narrow-band spectrometer, which will provide excellent opportunities for science and technology to Korean infrared groups.

High temperature dielectric constants of the various ceramic materials have been measured using cavity perturbation method. The measurements were applied to refractory, traditional and fine ceramic powder compacts from room temperature to . Calibration constant in the equation suggested by Hutcheon et al., was determined from the dielectric constants of reference specimen (teflon and alumina) at room temperature. From these results, informations on the refectory materials were obtained for the microwave kiln design and understanding of the microwave heating effects of ceramics have been improved.