• International Journal of Aeronautical and Space Sciences
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• 제13권4호
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• pp.484-490
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• 2012

This paper is devoted to investigate the feasibility of using a medium power ground-based laser to produce a torque on LEO satellites of various shapes. The laser intensity delivered to a satellite is calculated using a simple model of laser propagation in which a standard atmospheric condition and linear atmospheric interaction mechanism is assumed. The laser force is formulated using a geocentric equatorial system in which the Earth is an oblate spheroid. The torque is formulated for a cylindrical satellite, spherical satellites and for satellites of complex shape. The torque algorithm is implemented for some sun synchronous low Earth orbit cubesats. Based on satellites perigee height, the results demonstrate that laser torque affecting on a cubesat has a maximum value in the order of $10^{-9}$ which is comparable with that of solar radiation. However, it has a minimum value in the order of $10^{-10}$ which is comparable with that of gravity gradient. Moreover, the results clarify the dependency of the laser torque on the orbital eccentricity. As the orbit becomes more circular it will experience less torque. So, we can conclude that the ground based laser torque has a significant contribution on the low Earth orbit cubesats. It can be adjusted to obtain the required control torque and it can be used as an active attitude control system for cubesats.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2007년도 춘계학술대회논문집
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• pp.304-304
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• 2007

• 항공우주기술
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• 제10권1호
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• pp.193-200
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• 2011

본 연구는 저궤도의 태양동기궤도 위성에 미치는 외란 토크의 크기와 영향을 해석하였다. 위성체 좌표계에서 보았을 때, 지구 지향 자세에서 최대 토크는 약 $8.3{\times}10^{-4}$ Nm로 한 궤도당 약 1.4 Nms 의 모멘텀이 축적되고, 태양지향 자세에서의 최대 토크는 약 $1.6{\times}10^{-3}$ Nm로 한 궤도당 약 3.0 Nms 의 모멘텀이 축적된다. 한 궤도당 축적되는 모멘텀의 양은 토커의 크기를 결정하는 설계 기준 자료로 사용되는데, 현재 사용 가능한 자기 토커의 한 궤도당 모멘텀 덤핑 용량을 고려했을 때, 위성의 임무 수행을 위해 적절한 선택임을 확인하였다.

• 한국기계가공학회지
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• 제11권3호
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• pp.116-121
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• 2012

In recent years, world is faced with a transportation energy dilemma, and the transportation is dependent on a single fuel - petroleum. However, Hybrid Electric Vehicle(HEV) technology holds more advantages to reduce the demand for petroleum in the transportation by efficiency improvements of petroleum consumption. Therefore, there is a trend that lower gear noise levels are demanded in HEV for drivers to avoid annoyance and fatigue during operation. And meshing transmission error(T.E.) is the excitation that leads to the tonal noise known as gear whine, and radiated gear whine is also the dominant source of noise in the whole gearbox. This paper presents a method for the analysis of gear tooth profile and lead modification, and the predictions of transmission error and load distribution are shown under one loaded torque for the 1st gear pair of HEV gearbox. The test is also obtained before tooth micro-modification under the torque. At last, the appropriate tooth modification is used to minimize the transmission error and load distribution under the loaded torque. It is a good approach which the simulated result is used to improve the design in order to minimize the radiation gear whine noise.

• 천문학회보
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• 제44권1호
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• pp.44.3-44.3
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• 2019

Massive stars, supernovae, and kilonovae are among the most luminous radiation sources in the universe. Observations usually show near- to mid-infrared (NIR-MIR, 1-5~micron) emission excess from H II regions around young massive star clusters (YMSCs) and anomalous dust extinction and polarization towards Type Ia supernova (SNe Ia). The popular explanation for such NIR-MIR excess and unusual dust properties is the predominance of small grains (size a<0.05micron) relative to large grains (a>0.1micron) in the local environment of these strong radiation sources. The question of why small grains are predominant in these environments remains a mystery. Here we report a new mechanism of dust destruction based on centrifugal stress within extremely fast rotating grains spun-up by radiative torques, namely the RAdiative Torque Disruption (RATD) mechanism, which can resolve this question. We find that RATD can destroy large grains located within a distance of ~ 1 pc from a massive star of luminosity L~ 10^4L_sun and a supernova. This increases the abundance of small grains relative to large grains and successfully reproduces the observed NIR-MIR excess and anomalous dust extinction/polarization. We show that small grains produced by RATD can also explain the steep far-UV rise in extinction curves toward starburst and high redshift galaxies, as well as the decrease of the escape fraction of Ly-alpha photons observed from HII regions surrounding YMSCs.

• 한국기계가공학회지
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• 제20권8호
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• pp.1-10
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• 2021

Gears, which rotate and transmit power by interlocking two cogwheels, were invented in BC. They have been used in various systems, including industrial machinery, transportation devices, and living facilities, through the industrial revolution. Regardless of how they are used, gears are a major source of noise and vibration. Many effective measures are being taken to reduce the radiation noise generated from gears, most commonly by lubrication. Lubrication in gear units reduces friction on interlocking gear surfaces, dampening radioactive noise. This can be very useful for quiet gear design if these lubricating damping effects can be reflected in the analytical phase for gear design. This study experimentally confirms the properties of lubricated and non-lubricated radioactive noise by designing a decelerator gearbox and analyzing the radioactive noise characteristics by torque, rotation, and the number of gears using computer analysis.

• Radiation Oncology Journal
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• 제22권4호
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• pp.316-324
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• 2004

목적 : 간 등의 상 복부에 위치한 종양의 방사선 조사 체적은 호흡에 의한 종양의 이동을 포함하기 때문에 방사선 조사 체적이 증가되어 방사선 독성 및 정상조직 선량이 증가하게 된다. 이러한 문제점을 극복하기 위해 동 팬텀과 초음파센서를 이용하여 호흡운동에 의한 환자 체표면의 움직임을 획득하고, 획득한 데이터의 역 값을 이용해 환자침대를 조절해줄 수 있는 호흡운동 조절 방사선치료 기술을 개발하고자 한다. 대상 및 방법 : 호흡운동에 의한 환자 체표면의 움직임을 평가하기 위해 제작한 팬텀은 조정기(BS II, 20 Mhz, 8K Byte), 센서(Ultra-Sonic, range $3\~3$ m), Computer (RS232C), Sewo Motor (Torque 2.3 Kg) 등으로 구성하였고, 제어와 구동을 위한 획득-보정-분석 프로그램을 작성하였다. 최대 2 cm 범위 내에서 팬텀을 움직이게 하였고, 팬텀의 움직임과 보정이 순차적으로 일어나도록 프로그램하였으며, x, y, z가 연속적으로 움직이도록 구성하였다. 임의의 움직임 데이터(유격이 2 cm이 되도록 하여 3차원 데이터 형태)를 입력하여 동 팬텀을 조정하고, 동시에 팬텀 움직임을 초음파 센서를 이용하여 획득한 후, 두 데이터간의 비교, 분석을 시행하였다. 이후 쥐(Guinea-pig, about 500g)를 이용하여 호흡운동에 의한 환자 체표면의 움직임을 획득한 후 획득한 데이터의 역 값으로 팬텀을 구동시킴으로써 실시간 호흡운동 조절 방사선치료 기술을 평가하였다. 결과 : 팬텀 실험에서 3 차원 입력데이터에 대한 팬텀 보정 데이터간의 정확성을 시간에 대한 거리 값으로 비교한 결과 ${\pm}1\%$ 이내의 정확성을 알 수 있었고, 이에 필요한 보정시간은 $2.34{times}10^{-4}$초임을 알 수 있었다. 또한 동물 실험에서도 동일한 방법으로 시간에 대한 거리 그래프와 획득-보정간의 지연 시간 등을 분석한 결과 팬텀 데이터와 같은 결과를 얻을 수 있었다. 결론 : 팬텀, 동물 실험 모두에서 시간에 대한 거리 값과 각각의 경우에 획득-보정간의 지연 시간을 분석한 결과 데이터 값은 ${\pm}1\%$ 이내에서 일치하였으며, 데이터 획득-보정 지연 시간은 2.34H10-4 초 이내 즉, 실시간으로 얻을 수 있어 새로운 호흡운동 조절 방사선치료 기술의 임상적용에의 가능성을 확인할 수 있었다.

• 항공우주기술
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• 제2권1호
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• pp.54-62
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• 2003

우주공간상의 위성체는 아주 미세한 크기에 불과하지만 여러 가지 원인에 의한 외부교란토크를 받는다. 외부교란토크는 위성체의 궤도 운동뿐만 아니라 위성체의 자세에도 큰 영향을 미친다. 저궤도위성의 자세동역학에 작용하는 외부교란토크는 다양하다. 이러한 것들 중 중요한 4가지 원인은 중력경도, 지구자기장, 태양복사압 및 대기저항 등을 들 수 있다. 본 연구에서는 저궤도위성과 같은 저궤도위성에 작용하는 외부교란토크를 상세히 분석하고 저궤도위성 자세동역학에 미치는 외부교란토크의 영향을 상세히 기술한다.

• 한국자동차공학회논문집
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• 제19권3호
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• pp.90-98
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• 2011

Noises from diesel engine are the major issues for noise pollution as well as affect customers' purchasing needs to vehicles powered by diesel engine. This study investigates to screen-out main factors that contribute to noises from diesel engine using VGT 2000cc engine developed recently. Changes of fuel temperature, intake temperature and the presence of three way catalyst don't affect the 'Engine Radiation Noise' and the solely three way catalyst influence on the 'Tail Pipe Noise'. Especially, there are no effects of the presence of three way catalyst on torque, which is main subject that should be considered in secondary study.

• 천문학회보
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• 제46권2호
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• pp.66.1-66.1
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• 2021

Extinction curves observed toward individual Active Galactic Nuclei (AGN) usually show a steep rise toward Far-Ultraviolet (FUV) wavelengths and can be described by the Small Magellanic Cloud (SMC)-like dust model. This feature suggests the dominance of small dust grains of size a < 0.1 ㎛ in the local environment of AGN, but the origin of such small grains is unclear. In this paper, we aim to explain this observed feature by applying the RAdiative Torque Disruption (RATD) to model the extinction of AGN radiation from FUV to Mid-Infrared (MIR) wavelengths. We find that in the intense radiation field of AGN, large composite grains of size a > 0.1 ㎛ are significantly disrupted to smaller sizes by RATD up to dRATD > 100 pc in the polar direction and dRATD ~ 10 pc in the torus region. Consequently, optical-MIR extinction decreases, whereas FUV-near-Ultraviolet extinction increases, producing a steep far-UV rise extinction curve. The resulting total-to selective visual extinction ratio thus significantly drops to RV < 3.1 with decreasing distances to AGN center due to the enhancement of small grains. The dependence of RV with the efficiency of RATD will help us to study the dust properties in the AGN environment via photometric observations. In addition, we suggest that the combination of the strength between RATD and other dust destruction mechanisms that are responsible for destroying very small grains of a <0.05 ㎛ is the key for explaining the dichotomy observed "SMC" and "gray" extinction curve toward many AGN.