• 한국항공우주학회지
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• 제38권11호
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• pp.1136-1143
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• 2010

NASA가 발사한 LRO 달 탐사선의 정밀궤도 결정을 위해서 지상에서 발사한 레이저를 이용하여 단방향 거리측정 기술이 적용되었는데, 이는 실제 탐사선의 임무에 활용되는 첫번째 시도라고 할 수 있다. 본 연구에서는 LRO 달 탐사선의 레이저 거리측정을 수행하는 탑재체 및 지상 시스템, 레이저 비행시간 및 망원경 지향 오차 요소들을 분석하였다. 또한, 지상에서 발사한 레이저 펄스가 earth window내에 검출되기 위한 기술들을 분석하였다. 이러한 기술들을 적용하여 실제 LRO 달 탐사선의 레이저 추적을 통해서 관측한 데이터를 분석하고 이를 통해 성공적인 단방향 거리측정 기술이 구현될 수 있음을 확인하였다.

• 항공우주시스템공학회지
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• 제9권4호
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• pp.73-80
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• 2015

For Korean first lunar exploration program, KARI(Korea Aerospace Research Institute) has been researching in various fields and investigating cases of abroad lunar exploration spacecrafts. In the field of the flight software, KARI has been analysing some cases such as NASA LRO, and this paper describes the result of the case study on LRO flight software.

• Corrosion Science and Technology
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• 제22권3호
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• pp.214-219
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• 2023

Considering the case in the United States where most nuclear power plants with an initial design life of 40 years continue to operate until 60 or 80 years after undergoing material soundness evaluation, it is time to plan a more robust long-term operation strategy for nuclear power plants in Korea. There are some reports that SRO/LRO might be formed when Alloy 690 is heat treated for 10,000 hours to 100,000 hours at 360 to 450 ℃. The possibility of LRO formation in Alloy 690 steam generator tubings of Kori nuclear power plant unit 1 (Kori-1) was investigated using existing research papers. The mechanism in which SRO/LRO occurred was also surveyed. Alloy 690 was found to be more likely to cause ordering than Alloy 600 in terms of alloy composition. The ordering could be evaluated through changes in material properties. However, it is difficult to evaluate it from a microstructural point of view. The likelihood of LRO in Alloy 690 of the Kori-1 plant operated at 320 ℃ for 19 years seemed to be low in terms of time and exposure temperature.

• Journal of Astronomy and Space Sciences
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• 제31권2호
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• pp.131-140
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• 2014

Lava caves could be useful as outposts for the human exploration of the Moon. Lava caves or lava tubes are formed when the external surface of the lava flows cools more quickly to make a hardened crust over subsurface lava flows. The lava flow eventually ceases and drains out of the tube, leaving an empty space. The frail part of the ceiling of lava tube could collapse to expose the entrance to the lava tubes which is called a pit crater. Several pit craters with the diameter of around 100 meters have been found by analyzing the data of SELENE and LRO lunar missions. It is hard to use these pit craters for outposts since these are too large in scale. In this study, small scale pit craters which are fit for outposts have been investigated using the NAC image data of LROC. Several topographic patterns which are believed to be lunar caves have been found and the similar pit craters of the Earth were compared and analyzed to identify caves. For this analysis, the image data of satellites and aerial photographs are collected and classified to construct a database. Several pit craters analogous to lunar pit craters were derived and a morphological pit crater model was generated using the 3D printer based on this database.

• 한국항공우주학회지
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• 제46권4호
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• pp.338-344
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• 2018

달 주위를 공전하는 탐사위성이나 달착륙선 및 월면차의 열설계에 필요한 환경 인자로써 달 표면온도가 중요하며, 본 연구에서는 에너지방정식을 단순화한 집중계 해석모델을 통하여 온도를 예측하였다. 에너지방정식의 해석에 필요한 물리적 값들은 기하학적 형상을 고려하여 유도하고, 기존의 연구결과에 제시된 값들을 사용하였다. 달 표토층의 가장 중요한 열적 물성치인 면적비열은 LRO에 탑재된 Diviner의 측정온도 분석을 통하여 추출하였으며, 해석모델에 적용함으로써 값을 추정하였다. 수치적분을 통하여 예측한 달 표면온도 분포는 달탐사위성 등의 열설계에 적용할 수 있을 정도의 충분한 정확도를 갖으며, 본 연구에서 제시한 방법을 심화시킨다면 더욱 정확한 온도예측이 가능할 것이다.

• 한국해양공학회지
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• 제25권1호
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• pp.32-38
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• 2011

Galvanized steel has gone through a chemical process to keep it from corroding. The steel gets coated in layers of zinc because rust will not attack this protective metal. For countless outdoor, marine, or industrial applications, galvanized steel is an essential fabrication component. The reduction of the corrosion rate of zinc is an important topic. In the past, a very popular way to reduce the corrosion rate of zinc was to use chemical conversion layers based on $Cr^{+6}$. However, a significant problem that has arisen is that the use of chromium salts is now restricted because of environmental protection legislation. Therefore, it is very important to develop new zinc surface treatments that are environmentally friendly to improve the corrosion resistance of zinc and adhesion with a final organic protective layer. In this study, a Urethane solution (only Urethane 20 wt.%; S-700) and an organic/inorganic solution with Si (Si polysilicate 10 wt.% + Urethane 10 wt.%; LRO-317) are used. Based on the salt spray test of 72 h, S-700 and LRO-317 had a superior effect for the corrosion resistance on EGI and HDGI, respectively.

• 한국해양공학회지
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• 제24권5호
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• pp.60-66
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• 2010

Zinc has a number of characteristics that make it well suited for use as a coating to protecting iron and steel products from corrosion. Its excellent corrosion resistance in most environments accounts for its successful use as a protective coating on a variety of products and in many exposure conditions. The excellent field performance of zinc coatings results from their ability to form dense, adherent films that corrode at a rate that ranges from 1% to 10% of the corrosion rate of ferrous materials, depending on the environment. Recently, EU RoHS and EU ELV prohibited the use of materials that adversely affect the environment, such as Pb, Hg, Cd, and $Cr^{+6}$. In this study, environmentally-friendly, Cr-free solutions (epoxy solution, acrylic solution, and urethane solution S-700) and organic/inorganic solution with Si; LRO-317) were used to evaluate the corrosion resistance of zinc-coated steel subjected to a saltwater spray for 72 hours. The coating of urethane solution (S-700) was best among the three kinds of solution with heat treatment during five minutes at $190^{\circ}F$. Test specimens with S-700 and LRO-317 coating were heat treated in a drying oven at 170, 180, 190, 200, and $210^{\circ}C$ for five minutes. The results show that the optimum corrosion resistance was $190^{\circ}C$ in EGI and $170^{\circ}C$ in HDGI, respectively.

• 암석학회지
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• 제26권4호
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• pp.373-384
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• 2017

4차 산업 혁명의 시작은 우주산업의 발달을 초래하며 인류가 지구 밖으로 인류의 활동영역을 넓혀가는 첫 계기를 가져다주었다. 아폴로 프로그램이후 달 자원 탐사 및 달 기지 건설이 현실화 되고 있는 것은 미국의 LCROSS (The Lunar Crater Observation and Sensing Satellite)와 LRO (Lunar Reconnaissance Orbiter)의 보다 진보적인 과학적 발전과 중국 창어 미션 등 최근 아시아 국가들이 내놓은 과학적인 새로운 발견이 크게 관여하였다. 달의 극지 자원은 물과 함께 휘발성 물질들이며 현지에서 활용이 요구되므로 인류의 달 기지 건설에 있어서 더욱 중요하다. 헬륨-3는 화석연료가 고갈 될 쯤에는 대체에너지로 활용될 수 있다. 현재 러시아, 유럽과 미국 뿐 만아니라 아시아에서도 달 표면 착륙을 통한 달 탐사와 인류의 향후 기지 건설에 대한 준비는 지속적으로 이어 질 것으로 전망되고 있다. 이러한 시점에서 정확한 달 자원을 이해하고 달 자원 탐사와 활용을 위한 준비는 보다 중요한 현실이라는 점을 고려하여 이 논문은 달 자원 탐사와 달기지에 대하여 고찰하였다.

• 천문학회보
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• 제37권2호
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• pp.120.1-120.1
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• 2012

The Lunar Reconnaissance Orbiter (LRO) launched on June 16, 2009 has six experiments including of the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) onboard. The CRaTER instrument characterizes the radiation environment to be experienced by humans during future lunar missions. The CRaTER instrument measures the effects of ionizing energy loss in matter specifically in silicon solid-state detectors due to penetrating solar energetic protons (SEP) and galactic cosmic rays (GCRs) after interactions with tissue-equivalent plastic (TEP), a synthetic analog of human tissue. The CRaTER instrument houses a compact and highly precise microdosimeter. It measures dose rates below one micro-Rad/sec in silicon in lunar radiation environment. Forbush decrease (FD) event is the sudden decrease of GCR flux. We use the data of cosmic ray and dose rates observed by the CRaTER instrument. We also use the CME list of STEREO SECCHI inner, outer coronagraph and the interplanetary CME data of the ACE/MAG instrument.We examine the origins and the characteristics of the FD-like events in lunar radiation environment. We also compare these events with the FD events on the Earth. We find that whenever the FD events are recorded at ground Neutron Monitor stations, the FD-like events also occur on the lunar environments. The flux variation amplitude of FD-like events on the Moon is approximately two times larger than that of FD events on the Earth. We compare time profiles of GCR flux with of the dose rate of FD-like events in the lunar environment. We figure out that the distinct FD-like events correspond to dose rate events in the CRaTER on lunar environment during the event period.

• 천문학회보
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• 제37권2호
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• pp.138.2-138.2
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• 2012

Cave on the Moon is considered as the most appropriate place for human to live during the frontier lunar exploration. While the lava flows, the outer crust gets cooled and solidified. Then, the empty space is remained inside after lava flow stops. Such empty space is called the lava caves. Those lava tubes on the Earth are formed mostly by volcanic activity. However, the lava tubes on satellite like Moon and planet like Mars without volcanic activity are mostly formed by the lava flow inside of the crater made by large meteorite impact. Some part of lava tube with collapsed ceiling appears as the entrance of the cave. Such area looks like a deep crater so called a pit crater. Four large pit craters with diameter of > 60 m and depth of > 40 m are found without difficulty from Kaguya and LRO mission image archives. However, those are too deep to use as easily accessible human frontier base. Therefore, now we are going to identify some smaller lunar caves with accessible entrances using LRO camera images of 0.5 m/pixel resolution. Earth's lava caves and their entrances are well photographed by surface and aerial camera in immense volume. Thus, if the image data are sorted and archived well, those images can be used in comparison with the less distinct lunar cave and entrance images due to its smaller size. Then, we can identify the regions on the Moon where there exist caves with accessible entrances. The database will be also useful in modeling geomorphology for lunar and Martian caves for future artificial intelligence investigation of the caves in any size.