• 항공우주시스템공학회지
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• 제16권2호
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• pp.25-32
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• 2022

캡 루프 페어링은 상용차가 주행 시 전면부에서 발생하는 유동 박리의 저항을 제어하여 상용차 항력 계수를 줄이는 장치이다. 상용차는 구조적으로 후방의 컨테이너를 적재해야 되기 때문에 차량의 주행방향으로부터 공기역학적 저항력을 피할 수 없게 설계되어 있다. 이러한 이유 때문에 유류비, 환경오염물질과 밀접한 연관을 가진다. 본 연구에서는 랭킨 반체 이론을 바탕으로 3D 페어링 형상을 설계하고 공력 해석을 통해 설계 결과를 검증하였다.

• 한국군사과학기술학회지
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• 제19권2호
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• pp.227-235
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• 2016

Heavy-weight high speed underwater vehicle(HSUV) is launched from the submerged mother ship. For the safety point of view, it is important to confirm whether the HSUV would touch the launching mother ship. In this paper, the hydrodynamic force and moment were modeled by the polynomials of motion variables and the simple lift and drag acting on a plate and cylinder which consist of the HSUV's several parts. The mother ship was assumed as the Rankine half body to consider the flow field near the moving ship. Such hydrodynamic force and moment were included in the 6 DOF equations of motion of the HSUV and the dynamic simulations for the various conditions of the HSUV until the propeller activation were performed. Developed simulation program is expected to reduce the number of expensive sea trial test to develop safety logic of the HSUV at the initial firing stage.

• 항공우주시스템공학회지
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• 제16권6호
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• pp.64-73
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• 2022

페어링은 상용차가 주행 시 전면부에서 발생하는 유동박리의 저항을 제어하여 상용차 공기 저항력을 감소시키는 장치이다. 본 연구에서는 랭킨 반체 이론을 적용하여 3D페어링 형상을 설계하고 공력 해석을 통해 설계 결과를 검증하였다. 그리고 페어링의 구조적 안전성을 위해 상용차 과속조건과 돌풍 조건을 함께 고려하여 공력하중을 도출하였다. 이러한 공력 해석 결과를 기반으로 유리섬유/에폭시 복합재료를 적용하여 안전계수 3을 만족하는 페어링 구조 설계를 수행하였다. 최종 본 연구에서 가장 경량화된 페어링의 구조 해석을 수행하여 구조 안전성이 확인되었다.

• 천문학회보
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• 제43권1호
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• pp.51.3-52
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• 2018

Since Voyager 1 passed the Heliopause in 2012, it has provided the observations of the charged particles in the local interstellar medium. However, Voyager 1 only provides the information along with its trajectory. In order to understand the global view of the interstellar plasma flow surrounding the Heliopause, we need another tool. When the interstellar plasmas approach the Heliopause, the ions are deflected around the Heliopause due to the draping of the interstellar magnetic field. The draping of the interstellar magnetic field is strongly connected with the shape of the Heliopause. A fraction of the diverted ions exchanges their charges with the undisturbed primary interstellar neutral atoms, and then the ions become neutral atoms called the secondary interstellar neutral atoms. The newly created neutral atoms carry information on the diverted flow of the interstellar ions, and a fraction of them can travel to the Sun. Therefore, the secondary component of the interstellar neutrals is an excellent diagnostic tool to provide important information to constrain the shape of the Heliopause. The secondary interstellar neutrals are observed by Interstellar Boundary Explorer (IBEX) at Earth's orbit. Since 2009, two energetic neutral atom cameras on IBEX have measured neutral atoms and it has provided sky maps of neutral atoms. In this presentation, we will discuss the directional distribution of the secondary interstellar neutrals at Earth's orbit. In the sky maps, the primary interstellar neutral gas is seen between $200^{\circ}$ and $260^{\circ}$ in ecliptic longitude and the secondary components are seen in the longitude range of $160^{\circ}-200^{\circ}$. We also present a simplified model of the outer heliosheath to help interpret the observations of interstellar neutrals by the IBEX-Lo instruments. We extract information on the large-scale shape of the Heliopause by comparing the neutral flux measured at IBEX along four different look directions with simple models of deflected plasma flow around hypothetical obstacles of different aspect ratios to the flow. Our comparisons between the model results and the observations indicate that the Heliopause is very blunt in the vicinity of the Heliospheric nose, especially compared to a Rankine half-body or cometary shape.