• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2013년도 제45회 하계 정기학술대회 초록집
• /
• pp.222-222
• /
• 2013

GaN 기반 반도체는 넓은 bandgap을 가지고 있어 가시광부터 자외선까지 다양한 광전소자에 유용하게 사용된다. 광전소자중 발광다이오드의 경우 대부분 사파이어 기판위에 성장된다. 하지만 사파이어와 GaN의 격자 불일치 및 열팽창 계수의 차이로 인해 고품질의 GaN를 성장하기가 어렵다. 특히 열팽창 계수의 차이는 GaN 성장 공정이 고온에서 이루어지기 때문에 성장후 상온으로 온도가 떨어질 때 웨이퍼의 bowing을 발생시키고 동시에 dislocation이나 crack과 같은 결함이 생성되 GaN 성장막의 품질을 떨어트린다. 웨이퍼의 크기가 커지면 커질수록 웨이퍼 bowing은 커져 이에 대한 연구는 중요하다. 본 논문에서 2인치 사파이어 기판위에 성장된 GaN의 bow특성을 알아보기 위해 먼저 simulation을 하였고 실제로 성장된 GaN 웨이퍼와 비교를 하였다. c-plane 사파이어 기판위에 성장된 c-plane GaN의 bow특성을 알아보기 위해 성장 온도 $1,100^{\circ}C$에서 GaN두께를 1 ${\mu}m$에서 10 ${\mu}m$까지 1 ${\mu}m$씩 변화시켜 가며 simulation을 하였다. GaN두께가 1 ${\mu}m$일때는 bow가 11 ${\mu}m$, 6 ${\mu}m$ 일때는 54.7 ${\mu}m$, 10 ${\mu}m$ 일때는 108 ${\mu}m$를 얻어 GaN두께가 1 ${\mu}m$씩 증가할 때 마다 bow가 약 10 ${\mu}m$씩 증가하였다. 성장온도에 대한 영향을 알아보기 위해 $700^{\circ}C$에서 $1,200^{\circ}C$까지 $100^{\circ}C$씩 증가시켜며 bow특성 simulation을 하였다. 6 ${\mu}m$성장된 GaN의 경우 성장온도가 $100^{\circ}C$ 씩 증가할 때 bow는 약 6 ${\mu}m$ 증가하였다. 실제 성장된 c-plane GaN웨이퍼와 비교하기 위해 GaN을 각각 3 ${\mu}m$와 6 ${\mu}m$를 성장시켰고 high resolution x-ray diffraction장비를 사용하여 bow를 측정한 결과 각각 28 ${\mu}m$와 61 ${\mu}m$ 였고 simulation결과는 각각 33 ${\mu}m$와 65.5 ${\mu}m$를 얻어 비슷한 결과를 보였다. c-plane 사파이어 기판위에 성장된 c-plane GaN는 방향에 무관하게 동일한 bow 특성을 가지는 반해 r-plane 사파이어 기판위에 성장된 a-plane GaN는 방향에 따라 다른 bow특성을 보인다. a-plane GaN 이방향성적인 bow 특성을 알아보기 위해 simulation을 하였다. $1,100^{\circ}C$에서 a-plane GaN을 성장할 때 두께가 1 ${\mu}m$ 증가할 때마다 bow가 c축 방향으로는 21.7 ${\mu}m$씩 증가하였고 m축 방향으로는 11.8 ${\mu}m$ 씩 증가하여 매우 큰 이방향성적인 bow 특성을 보였다. 실제 r-plane 사파이어 기판위에 성장된 a-plane GaN의 bow를 측정하였고 simulation 결과와 비교해 보았다.

• 한국군사과학기술학회지
• /
• 제15권3호
• /
• pp.266-271
• /
• 2012

The rescue methods for the marine casualties are limited due to the characteristics of operation environment of the vessel. Especially the most of marine accidents have been occurred at the bow structure of ship. Moreover the failure of bow structure may lead to catastrophic mishaps. In this paper, the extents of damage of a bow structure fracture subject to collision accident was investigated by using numerical method. The computer simulation approach by using Finite Element Method was employed to accomplish this goal. A finite element model, a 3D model of ship, has been utilized to evaluate damage of bow structure according to collision scenario. In conclusion, we have demonstrated that the plastic deformation occurred at the bow structure. Also it was shown that the collision angle clearly plays a role in determining amount of damage of ship structures.

• Journal of Astronomy and Space Sciences
• /
• 제16권2호
• /
• pp.139-148
• /
• 1999

Bow shock formation, in case the supersonic solar wind flow is hindered by the atmosphere of Mars, is investigated. The atoms newly ionized from the extensive neutral atmosphere of Mars are loaded to the solar wind. By the conservation of momentum, the solar wind velocity is decreased. Then the supersonic flow velocity drops to the subsonic flow velocity in front of Mars at certain region, which is called the bow shock. The location of Mars subsolar bow shock is highly varying in the range of 1.3 to 2.5 Rm. Martian bow shock location is estimated by one-dimensional flux tube equations reduced from full three-dimensional MHD equations. The variability of Mars bow shock location effected by the solar wind conditions is studied. It is evident that the solar wind dynamic pressure change is able to make the Mars bow shock location variable.

• 한국해양공학회지
• /
• 제14권2호
• /
• pp.28-35
• /
• 2000

In this paper a complicated structural behavior in collision and its effect of energy transmission to the collision bulkhead was examined through a methodology of the numerical simulation to obtain a ideal bow construction and a location of collision bulkhead against heat on collision. At present the bow structure is normally designed in consideration of its specific structural arrangement and internal and external loads in these areas such as hydrostatic and dynamic pressure wave impact and bottom slamming in accordance with the Classification rules and the specific location of collision bulkhead by SOLAS requirement. By these studies the behavior of the bow collapse due to collision was synthetically evaluated for the different size of tankers and its operational speed limits and by the results of these simulation it provides the optimal design concept for the bow construction to prevent the subsequent plastic deformation onto or near to the collision bulkhead boundary and to determine the rational location of collision bulkhead.

• 해양환경안전학회:학술대회논문집
• /
• 해양환경안전학회 2018년도 공동국제학술발표회
• /
• pp.155-155
• /
• 2018

• 한국전자파학회:학술대회논문집
• /
• 한국전자파학회 2001년도 종합학술발표회 논문집 Vol.11 No.1
• /
• pp.127-131
• /
• 2001

본 논문에서는 공진 주파수가 2 GHz 이며 크기가 작고, 광대역 특성을 갖는 Taper 형태의 급전선로를 갖는 마이크로스트립 Bow-tie 슬롯 안테나를 제안하였다. 이 구조에서는 대역폭을 향상시키기 위하여 마이크로스트립 슬롯 안테나 방사 슬롯을 변형된 bow-tie 모양으로 설계하여 기존의 Bow-tie 슬롯 안테나와 다른 구조를 제안하였고 Electromagnetic coupling를 좋게 하기 위하여 급전선로에 Taper를 첨가하여 급전기와 안테나의 정합을 이루어 광대역 특성을 갖도록 하였다.

• Journal of the Optical Society of Korea
• /
• 제16권2호
• /
• pp.162-165
• /
• 2012

Bow-tie modes were proposed in a grooved rectangular resonator and their lasing characteristics were investigated in semiconductor microcavities. The observed spacing between two adjacent lasing peaks from the grooved cavity was reduced compared to that of 4-bounce whispering gallery modes (WGMs) from the same-sized simple rectangular cavity due to increased round-trip path length of the bow-tie modes. The lasing spectra of bow-tie modes obtained from two adjacent corners showed highly correlated patterns while those of 4-bounce WGMs did not.

• International Journal of Naval Architecture and Ocean Engineering
• /
• 제11권2호
• /
• pp.723-735
• /
• 2019

This paper employs computational tools to investigate the cause of resistance reductions in calm water and waves of the sharp bow form compared to the blunt bow in 66,000 DWT bulk carriers. A more slender shape at the fore-shoulder without a bulbous bow is a prominent feature of the sharp bow. The blunt bow incorporates a bulbous shape. A two-phase unsteady Reynolds averaged Navier-Stokes equations have been solved; and a realizable k-ε model has been applied for the turbulent closure. The free-surface is obtained by solving a VOF equation. The computational results have been validated with model tests carried out at a towing tank. The pressure component of resistance in the sharp bow is reduced by 8.9% in calm water, and 6.4-12.7% in regular head waves. The frictional components of resistance in the sharp and blunt bows are largely the same.

• 대한조선학회지
• /
• 제13권1호
• /
• pp.11-16
• /
• 1976

The effect of the bow shape on the ship motion response in longitudinal regular waves of water of finite depth is investigated by employing the strip theory. The two-dimensional hydrodynamic forces(added mass and damping) were calculated by close-fit method for water of finite depth. The models for investigation are U and V bow ship forms of block coefficient 0.8 with constant after body which were used by Yourkov [2] and recently by Kim [3] for their deep water investigations. The following results are obtained by the present numerical experiments. (1) It is confirmed that the damping coefficient of the V-bow ship is greater than that of U-bow ship and in consquence the amplitude of heave and pitch of V-bow ship is smaller than that of U-bow ship among longitudinal regular head waves in water of finite depth (2) The merit of the V-bow ship on the motion damping is more significant in heave than in pitch, and is decreasing with the shallowness of water depth. (3) The change of bow form gives little effect on the wave exciting force and moment compared with the motion responce.

• 대한조선학회지
• /
• 제12권1호
• /
• pp.47-58
• /
• 1975

The effect of the bow shape on the ship motion response among longitudinal regular waves, is investigated employing the strip theory. The two dimensional hydrodynamic forces such as added mass and damping are calculated by the integral equation method for arbitrary sections. Nine ship models are selected for investigation. They are U, UV and V bow ship forms of different block coefficient of 0.6, 0.7 and 0.8 with constant after body. The heave amplitude of the V bow ship is smaller than that of the U bow ship in the whole range of wave length except extremely short wave as were stated by the earlier investigators. This results holds also in the case of bow vertical motions such as vertical relative displacement, velocity and acceralation. As to the pitch amplitudes, the V bow ship gives smaller value in long waves but larger value in short waves. However, heave and pitch phase angles are practically not influenced by the form of the fore body sections. In the bow motions, a little difference in phase angle is appeared in the vicinity of the wave which has same ship length. With respect to the wave exiting force and moment unfovourable effects could be expected in V bow ships. And these tendency hold also in the wave bending moment.