• 한국안전학회지
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• 제30권5호
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• pp.44-51
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• 2015

As the domestic communication industry has been made rapid progresses, the construction of base stations are also expanded yearly from more than 86,000 ones in the year 2005 to over 300,000 ones in 2013. While the new construction and rebuilt works have been rapidly increased, there has been not tried about the analysis as well as the control of hazards for the construction works. This study is conducted to do not only the focus interview for 27 expert groups who are engaged in the construction works and safety, but also the questionnaires for AHP analysis which is suggested by the Korea Occupational Safety and Health Agency for 92 persons who are engaged in the construction works in order to analyze the hazards of construction works for base stations. The high ranked risk works which are acquired from the two methods are fall under installation of antennae, struck by the hand tools and construction materials under installation of antennae, fall during going up and down the steel tower and telegraph poles and the fall by electric shock during the underground cable works. The control for the above hazards are the installation of fall protection equipments, the installation of safety nets for falling objects and the installation of protection equipment of electric shock.

• 한국전자파학회논문지
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• 제18권5호
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• pp.547-552
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• 2007

본 논문에서는 두 마이크로스트립 라인으로 이루어진 헤어핀 형태의 결합 선로를 이용하여 특성이 개선된 링 하이브리드를 설계하였다. 제안한 구조는 링 하이브리드의 $\lambda/4$ 라인에 헤어핀 형태의 결합 선로를 삽입하여 두 선로가 가까워짐에 따라 선로간의 커플링으로 세 개의 감쇠극이 생겨 넓은 저지대역을 갖는 결합 선로 구조를 이용하여 구성함으로써 링 하이브리드의 크기 감소뿐만 아니라 고조파 제거 특성도 부가하였다. 중심 주파수 2.55 GHz에서 일반적인 링 하이브리드와 특성이 같고 3차 고조파를 포함한 12 GHz까지 -20 dB 이하의 고조파 저지 특성을 가지고 있다. 또한 링 부분의 크기는 기존 링 하이브리드의 1/4 크기로 줄어들었다. 제작된 링 하이브리드의 측정된 주파수 특성 결과는 시뮬레이션 결과와 잘 일치한다.

• JSTS:Journal of Semiconductor Technology and Science
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• 제14권1호
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• pp.100-108
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• 2014

Low noise amplifier (LNA) is an integral component of RF receiver and frequently required to operate at wide frequency bands for various wireless system applications. For wideband operation, important performance metrics such as voltage gain, return loss, noise figure and linearity have been carefully investigated and characterized for the proposed LNA. An inductive shunt feedback configuration is successfully employed in the input stage of the proposed LNA which incorporates cascaded networks with a peaking inductor in the buffer stage. Design equations for obtaining low and high impedance-matching frequencies are easily derived, leading to a relatively simple method for circuit implementation. Careful theoretical analysis explains that input impedance can be described in the form of second-order frequency response, where poles and zeros are characterized and utilized for realizing the wideband response. Linearity is significantly improved because the inductor located between the gate and the drain decreases the third-order harmonics at the output. Fabricated in $0.18{\mu}m$ CMOS process, the chip area of this wideband LNA is $0.202mm^2$, including pads. Measurement results illustrate that the input return loss shows less than -7 dB, voltage gain greater than 8 dB, and a little high noise figure around 6-8 dB over 1.5 - 13 GHz. In addition, good linearity (IIP3) of 2.5 dBm is achieved at 8 GHz and 14 mA of current is consumed from a 1.8 V supply.

• 천문학회보
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• 제37권2호
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• pp.97.2-97.2
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• 2012

The main payload of Science and Technology Satellite 3 (STSAT-3), Multipurpose InfraRed Imaging System (MIRIS) is the first Korean infrared space mission to explore the near-infrared sky with a small astronomical instrument developed by KASI. The 8-cm passively cooled telescope with a wide field of view (3.67 deg. ${\times}$ 3.67 deg.) will be operated in the wavelength range from 0.9 to $2{\mu}m$. It will carry out wide-band imaging and the Paschen-${\alpha}$ emission line survey. After the calibration of MIRIS in our laboratory, MIRIS has been delivered to SaTReC and successfully assembled into the STSAT-3. The main purposes of MIRIS are to perform the observation of Cosmic Infrared Background (CIB) at two wide spectral bands (I and H band) and to survey the Galactic plane at $1.88{\mu}m$ wavelength, the Paschen-${\alpha}$ emission line. CIB observation enables us to reveal the nature of degree-scale CIB fluctuation detected by the IRTS (Infrared Telescope in Space) mission and to measure the absolute CIB level. The MIRIS will continuously monitor the seasonal variation of the zodiacal light towards the both north and south ecliptic poles for the purpose of calibration as well as the effective removal of zodiacal light. The Pashen-${\alpha}$ emission line survey of Galactic plane helps us to understand the origin of Warm Ionized Medium (WIM) and to find the physical properties of interstellar turbulence related to star formation. Here, we also discuss the observation plan with MIRIS.

• 천문학회보
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• 제36권1호
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• pp.42.1-42.1
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• 2011

The main payload of the Science and Technology Satellite 3 (STSAT-3), Multipurpose Infrared Imaging System (MIRIS), will be equipped with the wide-field near-infrared camera. Its wide field-of-view ($3.67^{\circ}{\times}3.67^{\circ}$) is optimal for the observation of the zodiacal light (ZL), the sunlight scattered by the interplanetary dust (IPD). The MIRIS will continuously monitor the seasonal variation of the ZL towards both north and south ecliptic poles, which is caused by the asymmetries of the IPD distribution with respect to the Sun and the ecliptic plane. In addition to the monitoring observations, we are planning pointed observations for compelling structures in the ZL, the asteroidal dust bands and the gegenschein. This presentation proposes the zodiacal light observations with the MIRIS and discusses the expected results.

• Advances in aircraft and spacecraft science
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• 제2권1호
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• pp.95-108
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• 2015

Automatic Dependent Surveillance Broadcast (ADS-B) is quickly being adopted by aviation safety authorities around the world as the standard for aircraft tracking. The technology provides the opportunity for live tracking of aircraft positions within range of an ADS-B receiver stations. Currently these receiver stations are bound by land and local infrastructural constraints. As such there is little to no coverage over oceans and poles, over which many commercial flights routinely travel. A low cost space based ADS-B receiving system is proposed as a constellation of small satellites. The possibility for a link between aircraft and satellite is dependent primarily on proximity. Calculating the likelihood of a link between two moving targets when considering with the non-periodic and non-uniform nature of actual aircraft flight-paths is non-trivial. This analysis of the link likelihood and the performance of the tracking ability of the satellite constellation has been carried out by a direct simulation of satellites and aircraft. Parameters defining the constellation (satellite numbers, orbit size and shape, orbit configuration) were varied between reasonable limits. The recent MH370 disappearance was simulated and potential tracking and coverage was analysed using an example constellation. The trend of more satellites at a higher altitude inclined at 60 degrees was found to be the optimal solution.

• 대한원격탐사학회지
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• 제21권1호
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• pp.91-98
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• 2005

On board satellite magnetometer measures all possible magnetic components, such as the core and crustal components from the inner Earth, and magnetospheric, ionospheric and' its coupled components from the outer Earth. Due to its dipole and non-dipole features, separation of the respective component from the measurements is most difficult unless the comprehensive knowledge of each field characteristics and the consequent modeling methods are solidly constructed. Especially, regional long wavelength magnetic signals of the crust are strongly masked by the main field and dynamic external field and hence difficult to isolate in the satellite measurements. In particular, the un-modeled effects of the strong auroral external fields and the complicated behavior of the core field near the geomagnetic poles conspire to greatly reduce the crustal magnetic signal-to-noise ratio in the polar region relative to the rest of the Earth. We can, however, use spectral correlation theory to filter the static lithospheric and core field components from the dynamic external field effects that are closely related to the geomagnetic storms affecting ionospheric current disturbances. To help isolate regional lithospheric anomalies from core field components, the correlations between CHAMP magnetic anomalies and the pseudo-magnetic effects inferred from satellite gravity-derived crustal thickness variations can also be exploited, Isolation of long wavelengths resulted from the respective source is the key to understand and improve the models of the external magnetic components as well as of the lower crustal structures. We expect to model the external field variations that might also be affected by a sudden upheaval like tsunami by using our algorithm after isolating any internal field components.

• 천문학회보
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• 제40권1호
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• pp.55.1-55.1
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• 2015

The first Korean infrared space telescope MIRIS (Milti-purpose InfraRed Imaging System) was successfully launched in November 2013, as the main payload of Korean STSAT-3 (Science and Technology Satellite-3). After initial on-orbit operation for verification, the observations have been made with MIRIS for the fluctuation of Cosmic Infrared Background and the Galactic Plane survey. For the study of near-infrared background, MIRIS completed the survey of large areas (> $10^{\circ}{\times}10^{\circ}$ around the pole regions: the north ecliptic pole (NEP), the north and south Galactic poles (NGP, SGP). We are also continuously and frequently monitoring the NEP region for the instrumental calibration and the zodiacal light study. One the other hand, the Paschen-${\alpha}$ Galactic plane survey has been carried out using two narrow-band filters (at $1.88{\mu}m$ and $1.84+1.92{\mu}m$) of MIRIS. This survey is planning to cover the whole Galactic plane with the latitude of ${\pm}3^{\circ}$, and the longitude regions of $+280^{\circ}<l<360^{\circ}$ and $0^{\circ}<l<+210^{\circ}$ have been completed (~ 80%) by February 2015. The data are still under the stage of reduction and analysis, and we present some preliminary results.

• 우주기술과 응용
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• 제3권3호
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• pp.199-212
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• 2023

과거 1970년대까지의 달 표면탐사에서는 단기간 달에서의 임무 특성을 가지는 것에 비해 최근 달 표면탐사는 달에서의 장기체류와 이를 기반으로 궁극적으로 화성까지 탐사 범위를 확장하는 방향으로 진행되고 있다. 인간의 달표면 장기체류를 실현하기 위해서는 탐사 현지 자원을 활용하여 체류에 필요한 소비재나 연료 등의 현지 생산 및 사용이 중요한 전제가 된다. 국제우주탐사협의체(ISECG, International Space Exploration Coordination Group)에서 각국의 우주탐사 계획을 반영하여 제시하는 글로벌 우주탐사 로드맵에는 달표면 탐사로부터 화성탐사로 이어지는 발전 단계가 제시되며 각 단계에서 현지자원활용은 중요한 요소가 되고 있다. 본 논문에서는 국제우주탐사협의체의 현지자원활용(ISRU) 격차분석 보고서를 기반으로 현지자원활용의 기술 분야를 현지 연료 및 소비재 생산, 현지 건설, 우주상 제조, 그리고 생성 결과물의 보관 및 활용, 자원활용에 필요한 전력시스템 등과 같은 연관 분야로 분류하여 주요 분야에서의 기술 개발 및 검증 현황을 분석한다. 다수의 국가는 달 자원 중 극 지역 영구음영지역의 얼음물 이용 그리고 표토에서 산소 등의 추출에 우선 순위를 부여하고, 무인 착륙임무를 통하여 달 남극 영구음영지역 근처에서 물질 및 물 분포 확인을 준비하고 있다. 자원 활용을 위하여 수전해를 이용한 수소, 산소 등 연료 생산, 모사토를 이용한 달 표토에서 산소의 추출 등의 기술을 개발하고 있다. 자원활용 기술의 개발을 위하여 지상에 달표면 모사환경을 구현하고 기술의 개발, 시나리오의 시연 등을 통한 효율적 현지자원활용 구현 방법 등을 모색하고 있다. 지속 가능한 달 표면 탐사를 위하여 각국은 달 표면 도달, 자원의 조사, 물질의 추출 등에 서비스 구매 등 민간 영역의 능력을 활용하고 발전시키는 노력을 병행하고 있다.

• 한국응용과학기술학회지
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• 제36권4호
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• pp.1312-1326
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• 2019

본 연구는 퇴행성 무릎 관절염을 가진 노인여성을 대상으로 12주간의 노르딕 워킹을 통해 신체 기능과 관절염 통증 정도의 개선에 어떠한 효과를 미치는지 규명하는데 목적이 있다. 본 연구의 대상자는 퇴행성관절염으로 진단받은 노인여성 16명(나이: 73.00±3.70year, 신장: 154.30±4.07cm)을 대상으로 무선배정 된 노르딕 워킹 운동그룹(n=9)과 통제그룹(n=7)으로 나누었다. 운동 그룹은 노르딕 스틱을 이용하여 12주간 주 3회, 1회 30분 노르딕 워킹 운동을 실시하였고, 운동 강도는 HRR의 40-60%로 설정하였다. 통제그룹은 동일한 기간 동안 일상생활을 유지하도록 하였다. 종속변인으로 신체조성(체중, 체지방률, 근골격량)과 근력 과 유연성(상·하지 근력, 상·하지 유연성), 균형능력(정적균형, 동적균형) 및 통증정도를 측정하였다. 이러한 지표들의 측정은 운동프로그램을 진행하기 전과 후로 나누어 2번 측정하였다. 자료처리는 SPSS-PC version 25.0을 이용하여 실험집단과 통계집단간의 생리학적 특성 비교를 위해 독립표본 t-test를 사용하였으며, 노르딕 워킹 운동그룹과 통제그룹의 그룹 간, 시기간의 변화를 알아보기 위해 2×2 반복측정 이원배치분산분석을 사용하였다. 연구 결과는 첫째, 12주간의 노르딕 워킹을 통해 신체조성 기능에서 체지방률은 운동 처치 후에 감소하는 결과가 나타났으며(p=.004), 집단 간과 시기 간의 상호작용에서도 감소하는 결과가 나타났다(p=.003). 골격근량은 운동처치 후에 증가하는 결과가 나타났으며(p=.018), 집단 간과 시기 간의 상호작용에서도 증가하는 결과가 나타났다(p=.005). 둘째, 근력과 유연성은 상지근력과 하지유연성에서 집단 간과 시기 간 상호작용에서 증가하는 결과가 나타났으며(p=.009)(p=036), 하지근력에서는 운동집단과 통제집단 간 개선효과가 나타났다(p=.006). 또한, 상지유연성은 운동처치 후에 증가하는 결과가 나타났다(p=.020). 셋째, 균형능력 요인은 정적균형에서 운동처치 후 개선 효과가 나타났으며(p=.016), 동적균형에서는 차이가 나타나지 않았다(p>.05). 넷째, 통증정도는 운동처치 후 개선 효과가 나타났으며(p=.022), 운동집단과 통제집단 간에 개선 효과도 나타났다(p=.013). 결론적으로 12주간의 노르딕 워킹은 퇴행성 무릎 관절염을 가진 노인여성의 신체조성과 근력과 유연성에 긍정적인 영향을 미치는 것으로 나타났다. 따라서 노르딕 워킹은 퇴행성 무릎 관절염을 가진 노인여성에게 신체조성과 안정성, 균형성을 높여 주였으며, 무릎 관절의 통증을 낮춰주어 재활 운동 기능 개선에 효과적인 운동방법이라고 사료된다.