• 한국안전학회지
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• 제36권4호
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• pp.20-28
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• 2021

With an increase in the commercialization of electricity, and the development of advanced and large electric devices and various wireless radio wave services, concerns over the effects of electromagnetic fields on human health have increased. Accordingly, the World Health Organization encouraged the development of international standards by establishing the 'International Electromagnetic Fields Project' in 1996 based on studies on the harmful effects of electromagnetic fields on the human body. Moreover, the National Institute of Environmental Health Sciences (NIEHS) classified electromagnetic fields as possible carcinogens under Group 2B category, even though they have been found to have a weak correlation with those effects on human health. Mid-to-large-sized electric facilities used at industrial sites mostly adopt a commercial frequency of 60 Hz, and workers handling these facilities are exposed to such extremely low frequency (ELF) fields for a long time. A previous study suggested that exposure to ELF electromagnetic fields with frequency ranges from 0 to 300 Hz, even for a short time, at densities higher than 100 μT may have harmful effects on human body as it affects the activation of nerve cells in the central nervous system by inducing an electric field and current and stimulating muscles and the nervous system in the body. Such studies, however, focused on home appliances used by ordinary people, and research on facilities utilizing high-capacity current and operated by workers at industrial sites is lacking. Therefore, in this study, a 3000 kilowatt generator, which is a high-capacity electric facility employed at industrial sites, was investigated, and the size of the magnetic fields generated during its no-load and high-load operations per distance to produce a map was measured to reveal spots deemed hazardous according to domestic and international exposure standards. The findings of this study is expected to alleviate workers' anxiety about the harmful effects of magnetic fields on their body and to minimize the level of exposure during operations.

• 항공우주정책ㆍ법학회지
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• 제24권1호
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• pp.119-152
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• 2009

한국은 우주 탐사 프로그램에 대한 포부와 함께 급속하게 확장내지 발전하고 있다. 정부는 항공우주산업에 우선권을 주고 있으며, 더 좋은 기반위에, I987년의 항공우주산업개발촉진법, 2005년의 우주개발진흥법과 2007년의 우주손해배상법을 제정하여 시행 해오고 있다. 필자는 위성의 발사허가, 우주물체의 등록, 위성정보의 이용, 우주비행사의 구조, 손해배상, 지상 제3자에 대한 책임보험, 우주개발지원계획 등이 포함된 전기 세 가지 우주관계법의 입법경위, 주요내용 및 논평을 하고자 한다. 더욱이 필자는 한국의 우주산업을 효율적으로 개발하기 위하여 일본의 우주항공연구개발기구(JAXA), 영국의 국립우주센터(BNSC), 국립우주연구센터(CNES), 독일의 항공우주센터(DLR), 스웨덴의 우주공사(SSC), 중국의 항천과공집단공사(CASIC) 등과 유사한 한국의 새로운 우주항공개발공사 (KADA: 가칭)의 창설할 수 있는 입법이 필요로 하며 또한 정부기구로서 캐나다의 우주청(CSA), 러시아의 우주청(RSA), 이탈리아의 우주청(ISA), 이스라엘의 우주청(ISA), 인도의 우주성(IDS), 미국의 항공우주청(NASA)과 중국의 국가항천국(CNSA)등과 유사한 한국의 새로운 우주청(KSA: 가칭)을 창설할 수 있는 입법조치가 필요하다. 만약 한국 정부가 장차 정부 조직으로 한국의 우주청을 설립시키려면 정부조직법의 개정이 필요하다. 동양적인 사고와 창의력에 근거하여 아시아 여러 나라들 간에 우주산업을 발전시키기 위하여 연구협력을 증진시킬 수 있는 "아시아우주기구(ASA)" 의 설립이 필요하다.

• 천문학회보
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• 제43권1호
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• pp.42.1-42.1
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• 2018

Deep Ecliptic Patrol of the Southern Sky (DEEP-South) observation is being made during the off-season for exoplanet survey, using Korea Microlensing Telescope Network (KMTNet). An optimal combination of its prime focus optics and the 0.3 billion pixel CCD provides a four square degrees field of view with 0.4 arcsec/pixel plate scale which is also best suited for small body studies. Normal operation of KMTNet started in October 2015, and a significant portion of the allocated telescope time for DEEP-South is dedicated to targeted observation, Opposition Census (OC), of near-Earth asteroids for physical and taxonomic characterization. This is effectively achieved through multiband, time series photometry using Johnson-Cousins BVRI filters. Uninterrupted monitoring of the southern sky with KMTNet is optimized for spin characterization of a broad spectrum of asteroids ranging from the near-Earth space to the main-belt, including binaries, asteroids with satellites, slow/fast- and non-principal axis-rotators, and thus is expected to facilitate the debiasing of previously reported lightcurve observations. Our software subsystem consists of an automated observation scheduler, a pipelined data processing system for differential photometry, and an easy-to-use lightcurve analysis toolkit. Lightcurves, spin periods and provisional determination of class of asteroids to which the lightcurve belongs will be presented, using the dataset from first year operation of KMTNet. Our new taxonomic classification scheme for asteroids will also be summarized.

• 항공우주시스템공학회지
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• 제16권6호
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• pp.24-34
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• 2022

본 연구에서는 우주 그물의 우주 물체 포획 성능을 향상시키기 위하여 충격 흡수의 이점을 가지는 거미집 구조의 생체 모방 우주 그물을 이용한 우주 물체 포획 시뮬레이션을 수행하였다. 포획 시뮬레이션은 비선형 구조 동역학 해석 프로그램인 ABAQUS를 이용하여 수행하였다. 우주 물체는 12U 크기의 CubeSat을 강체로 모델링하였다. 거미집 구조의 우주 그물은 대각선 길이가 2.828 m이며, 탄성보 요소를 이용하여 구현하였다. 동일 중량의 정사각형 우주 그물의 포획 시뮬레이션 결과와 비교하여 생체 모방 우주 그물의 포획의 우수성을 확인하였다. 또한, 거미집 구조의 우주 그물을 이용하여 우호적 및 비우호적으로 운동하는 우주 물체를 포획하는 수치 시뮬레이션을 수행하였으며, 우주 물체의 포획 성공 및 실패 사례를 조사하였다.

• 한국의류학회지
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• 제18권5호
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• pp.602-614
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• 1994

The purpose of this study was to suggest the proper ease of total crotch length concerning both appearance and comfort. The research processes as follows. 1) For the purpose of obtaining the necessary ease of slacks in body movement, experimental slacks of no ease of total crotch length were made. Three college girls putting on these experimental slacks were examined on their back middle waist lines using cross-cut method. 2) Experimental slacks for suggesting the proper ease consist of 7 types; slacks CO, Wl, W3, W5, W7, C3, C5. The sensory evaluation for appearance and comfort was applied to evaluate the 7 slacks. The results can be summarized as follows. 1. As the leg-movement angle increased, the vertical space increased and the horizontal space decreased. There was negative relationship between vertical and horizontal space. And as the leg.movement angle increased, the area of space increased. The shapes of space showed the amounts of space and the direction of force by the movements. 2. The appearances of slacks C3, W3, C5 were better than the other slacks. The eases of the crotch were better than those of the waist line in appearance. And slakcs W7 was better than any other , ;lacks in comfort. When the amount of each part of eases was same, the comfort in eases of crotch was not as good as that of waist line. 3. In slacks, the proper ease of total crotch length was 3% and 5% of total crotch length.

• 로봇학회논문지
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• 제2권4호
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• pp.297-303
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• 2007

In this paper, we discuss a service to give alarm in the case of emergency for the old and the weak by human behavior recognition in Intelligent Space. Our Intelligent Space consists of mobile robots, sensors and agents. And these components are connected to network framework. Agent analyzes data acquired from networked sensors and determines task of robots and a space to provide a service for humans. In our emergency alarm service, human behavior recognition service module analyzes accelerometer data obtained from body-attached human behavior sensing platform, and classifies into four basic human behavior such as walking, running, sitting and falling-down. For the old and the weak, falling-down behavior may bring about dangerous situations. On such an occasion, agent executes emergency alarm service immediately. And then a selected mobile robot approaches fallen person and sends images of the person to guardians. In this paper, we set up a scenario to verify the emergency alarm service in Intelligent Space, and show feasibility of the service from our simulation experiments.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권2호
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• pp.24.2-24.2
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• 2009

We present the results of new CCD photometry for the contact binary BX Peg, made during three successive months beginning on September 2008. As do historical light curves, our observations display an O'Connell effect and the November data by themselves indicate clear evidence for very short-time brightness disturbance. For these variations, model spots are applied separately to the two data set of Group I (Sep.--Oct.) and Group II (Nov.). The former is described by a single cool spot on the secondary photosphere and the latter by a two-spot model with a cool spot on the cool star and a hot one on either star. These are generalized manifestations of the magnetic activity of the binary system. Twenty light-curve timings calculated from Wilson-Devinney code were used for a period study, together with all other minimum epochs. The complex period changes of BX Peg can be sorted into a secular period decrease caused dominantly by angular momentum loss due to magnetic stellar wind braking, a light-travel-time (LTT) effect due to the gravitational effect of a low-mass third companion, and a previously unknown short-term oscillation. This last period modulation could be produced either by a second LTT orbit with a period of about 16 yr due to the existence of a fourth body or by the effect of magnetic activity with a cycle length of about 12 yr.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권2호
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• pp.24.1-24.1
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• 2009

V994 Her(ADS 11373 AB, HIP 90483) has been recently known as a quadruple system which consists of double eclipsing and double double-lined spectroscopic binaries (Lee et al. 2008). BV CCD photometric observations of the intricate star system were made during the observing seasons from 2007 to 2008 with the 35cm reflector of the Campus station of the Chungbuk National University Observatory. From the observations a total of 10 times of minimum lights were newly determined. All timings collected, including ours, were intensively analyzed to yield new interesting findings: 1) two eclipsing binaries with the orbital periods of 2.d08326 and 1.d42001 in V994 Her system show possibly apsidal motions with different apsidal periods of 46.y4 and 15.y3, and eccentricities of 0.058 and 0.082, respectively. 2) a light-time effect with a period of 0.y93 may be possible, implying that a third-body be revolving around the binary with the orbital period of 2.d08326.

• 한국콘텐츠학회논문지
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• 제13권7호
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• pp.91-101
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• 2013

불확실성의 시대에 현대건축은 다양한 미디어의 발전으로 인해 표현 양상과 전개 및 방법론에 있어 과거에 비해 훨씬 자유로워지면서 건축의 표현 양상에도 많은 변화가 시도되고 있다. 특히 현상학이 대두되면서 건축공간에 현상학적 표현의 방법이 다각도로 진행되고 있으며 건축의 형태에서 벗어나 본질적이며 인간과 상호 소통하고 체험할 수 있는 공간에 대한 탐색이 활발히 진행되고 있다. 본 연구는 건축적 형태(Figure)와 공간(Space)을 지각하고 인식하게 되는 방법으로써의 현상학적 이해를 통해 기존의 물적 구조체로서의 건축에 대한 이해를 현상을 품은 콘텐츠의 주체로써 이해하여 다각적인 공간 디자인의 방법을 모색하고 적용하는데 있다. 건축의 표현양식에 있어서 현상적적 접근은 빛을 건축공간에 접목하여 발표한 건축들을 중심으로 살펴보았다.

• 천문학회보
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• 제41권1호
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• pp.61.3-62
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• 2016

An asteroid family is a group of asteroidal objects in the proper orbital element space (a, e, and i), considered to have been produced by a disruption of a large parent body through a catastrophic collision. Family members usually have similar surface properties such as spectral taxonomy types, colors, and visible geometric albedo with a same dynamical age. Therefore an asteroid family could be called as a natural Solar System laboratory and is also regarded as a powerful tool to investigate space weathering and non-gravitational phenomena such as the Yarkovsky/YORP effects. We carry out time series photometric observations for a number of asteroid families to obtain their physical properties, including sizes, shapes, rotational periods, spin axes, colors, and H-G parameters based on nearly round-the-clock observations, using several 0.5-2 meter class telescopes in the Northern hemisphere, including BOAO 1.8 m, LOAO 1.0 m, SOAO 0.6 m facilities in KASI, McDonald Observatory 2.1 m instrument, NARIT 2.4 m and TUG 1.0 m telescopes. This study is expected to find, for the first time, some important clues on the collisional history in our Solar System and the mechanisms where the family members are being transported from the resonance regions in the Main-belt to the near Earth space.