• 제목/요약/키워드: Intermediate Space

검색결과 340건 처리시간 0.029초

S 석회석광산에서의 최종 잔벽사면의 안정성 평가 (Stability Assessment on the Final Pit Slope in S Limestone Mine)

  • 선우춘;이윤수;김현우;이병주
    • 터널과지하공간
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    • 제23권2호
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    • pp.99-109
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    • 2013
  • 노천광산사면은 일반적으로 경제성 문제로 지보대책을 고려하지 않고 설계된다. 그러나 최종 잔벽사면은 장기적인 안정성이 필요하므로 경우에 따라서는 안정성을 높일 수 있는 적절한 대책이 필요하다. 본 연구를 위해 S 석회석 광산의 지질 및 불연속면 조사, 암반평가, 강도시험 등 현장조사를 수행하였다. 그리고 최종 잔벽사면에 대해 평사투영, SMR, 수치해석을 통한 안정성 평가를 실시하고, 최종 잔벽사면의 처리방안을 제안하였다. 해석결과, 사면 전체규모에서 파괴는 예상되지 않지만, 벤치규모의 사면파괴는 발생할 가능성이 있다. 최종 잔벽사면은 프리스플리팅 발파로 정리하고, 중간 소단에 폭이 넓은 berm을 설치하거나 국부적으로 지하수 유출이 있는 곳에는 수평배수공 등을 시공하여 벤치사면의 안정성을 높일 수 있을 것이다.

Solar Photovoltaics Technology: No longer an Outlier

  • Kazmerski, Lawrence L.
    • 한국진공학회:학술대회논문집
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    • 한국진공학회 2011년도 제41회 하계 정기 학술대회 초록집
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    • pp.70-70
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    • 2011
  • The prospects of current and coming solar-photovoltaic (PV) technologies are envisioned, arguing this solar-electricity source is beyond a tipping point in the complex worldwide energy outlook. Truly, a revolution in both the technological advancements of solar PV and the deployment of this energy technology is underway; PV is no longer an outlier. The birth of modern photovoltaics (PV) traces only to the mid-1950s, with the Bell Telephone Laboratories' development of an efficient, single-crystal Si solar cell. Since then, Si has dominated the technology and the markets, from space through terrestrial applications. Recently, some significant shift toward technology diversity have taken place. Some focus of this presentation will be directed toward PV R&D and technology advances, with indications of the limitations and relative strengths of crystalline (Si and GaAs) and thin-film (a-Si:H, Si, Cu(In,Ga)(Se,S)2, CdTe). Recent advances, contributions, industry growth, and technological pathways for transformational now and near-term technologies (Si and primarily thin films) and status and forecasts for next-generation PV (nanotechnologies and non-conventional and "new-physics" approaches) are evaluated. The need for R&D accelerating the now and imminent (evolutionary) technologies balanced with work in mid-term (disruptive) approaches is highlighted. Moreover, technology progress and ownership for next generation solar PV mandates a balanced investment in research on longer-term (the revolution needs revolutionary approaches to sustain itself) technologies (quantum dots, multi-multijunctions, intermediate-band concepts, nanotubes, bio-inspired, thermophotonics, ${\ldots}$ and solar hydrogen) having high-risk, but extremely high performance and cost returns for our next generations of energy consumers. This presentation provides insights to the reasons for PV technology emergence, how these technologies have to be developed (an appreciation of the history of solar PV)-and where we can expect to be by this mid-21st century.

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ACCRETION FLOW AND DISPARATE PROFILES OF RAMAN SCATTERED O VI λλ 1032, 1038 IN THE SYMBIOTIC STAR V1016 CYGNI

  • Heo, Jeong-Eun;Lee, Hee-Won
    • 천문학회지
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    • 제48권2호
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    • pp.105-112
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    • 2015
  • The symbiotic star V1016 Cygni, a detached binary system consisting of a hot white dwarf and a mass-losing Mira variable, shows very broad emission features at around 6825 Å and 7082 Å, which are Raman scattered O vi λλ 1032, 1038 by atomic hydrogen. In the high resolution spectrum of V1016 Cyg obtained with the Bohyunsan Optical Echelle Spectrograph these broad features exhibit double peak profiles with the red peak stronger than the blue counterpart. However, their profiles differ in such a way that the blue peak of the 7082 feature is relatively weaker than the 6825 counterpart when the two Raman features are normalized to exhibit an equal red peak strength in the Doppler factor space. Assuming that an accretion flow around the white dwarf is responsible for the double peak profiles, we attribute this disparity in the profiles to the local variation of the flux ratio of O vi λλ 1032, 1038 in the accretion flow. A Monte Carlo technique is adopted to provide emissivity maps showing the local emissivity of O vi λ1032 and O vi λ1038 in the vicinity of the white dwarf. We also present a map indicating the differing flux ratios of O vi λλ 1032 and 1038. Our result shows that the flux ratio reaches its maximum of 2 in the emission region responsible for the central trough of the Raman feature and that the flux ratio in the inner red emission region is almost 1. The blue emission region and the outer red emission region exhibit an intermediate ratio around 1.5. We conclude that the disparity in the profiles of the two Raman O vi features strongly implies accretion flow around the white dwarf, which is azimuthally asymmetric.

철도시스템 개발에서 시스템 안전성을 고려한 설계검증 프로세스의 개선에 관한 연구 (On the Improvement of the Design Verification Process for the Development of Railway Systems with Systems Safety Considered)

  • 심상현;이재천
    • 대한안전경영과학회지
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    • 제15권1호
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    • pp.51-60
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    • 2013
  • As the human demand or desire on brand new systems otherwise equipped with new functions grows drastically, so does the complexity of the systems. With this trend, the systems are becoming bigger in scale and at the same time the safety requirements are more stringent in the development. Typical systems examples in such a situation may include high-speed railway systems, aero and space systems, marine systems, etc. Failure of those systems can cause serious damages on both the human being and wealth with social infrastructure. As such, it is quite necessary to ensure that the safety requirements be satisfied in the system development. To achieve this need, there could be a lot of solutions to take. In this paper, regarding safety, a special attention is given to the verification phase process, which is one of the intermediate phases of whole systems development process. More specifically, the ultimate concern is placed on how to carry out the design verification while ensuring the safety requirements. To do so, some improvements in the verification phase were proposed first. Then, the outcomes were combined with the systems safety process by generating an integrated process model to reach the goal. As a case study, application to a railway system was discussed, where strict safety requirements are usually necessary. It would be expected that the potential likelihood of failure with rail systems could be reduced if the results obtained are used effectively with some enhancement from further study.

가상공동체에서 매개 변수로서의 몰입의 역할 (The Role of Cognitive Absorption as a Mediating Variable in Virtual Community)

  • 김진화;변현수
    • 경영정보학연구
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    • 제6권2호
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    • pp.47-63
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    • 2004
  • 인터넷의 발달로 인해 가상공간에서 벌어지는 현상에 관한 관심과 영향력이 증가하고 있다. 그 중에서도 현실의 실제 공동체와 비슷한 가상공동체의 중요성이 커지고 있다. 그런데 가상공간 자체는 몰입하기 쉬운 특징을 고루 지니고 있다. 본 연구에서는 가상공동체의 구성원들이 가상공동체를 이용함에 있어서 몰입이 큰 역할을 한다는 것을 알아보고자 한다. 연구 결과 도전의욕, 숙련도, 지각된 현실감, 욕구충족 등의 변수들은 몰입을 통해 가상공동체의 이용에 유의한 영향을 미치는 것을 확인하였다. 단지 상호작용성은 몰입을 거치지 않고 직접 가상공동체 이용에 영향을 미치고 있었다. 이는 몰입이 가상공동체 이용에 중요한 역할을 하는 요인이라는 것을 나타내는 것이며, 또한 가상공동체가 제대로 운영되기 위해서는 상호작용에 필요한 최소한의 구성원을 확보할 필요가 있다는 것을 의미한다. 가상공동체의 운영에 있어서, 몰입을 높이는 여러 가지 방법들을 고안해서 적용한다면 가상공동체의 활성화와 성과를 높이는데 큰 기여를 할 수 있을 것이다.

LOW FREQUENCY OBSERVATIONS OF A RADIO LOUD DWARF GALAXY

  • Park, Songyoun;Sengupta, Chandreyee;Sohn, Bong Won;Paudel, Sanjaya
    • 천문학회지
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    • 제50권5호
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    • pp.151-155
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    • 2017
  • We investigate the radio properties of the dwarf galaxy SDSS J133245.62+263449.3 which shows optical signatures of black hole activity. Dwarf galaxies are known to host intermediate mass black holes (IMBHs) with masses $M_{BH}{\sim}10^{4-6}M_{\odot}$, some of them being radio loud. Recently, Reines et al. (2013) found dwarf galaxy candidates which show signatures of being black hole hosts based on optical spectral lines. SDSS J133245.62+263449.3 is one of them; it shows a flux density of ~ 20 mJy at 1.4 GHz, which corresponds to $L_{1.4GHz}{\sim}10^{23}W\;Hz^{-1}$. This is much brighter than other black hole host dwarf galaxies. However, star formation activity can contribute to radio continuum emission as well. To understand the nature of the radio emission from SDSS J133245.62+263449.3, we imaged this radio loud dwarf galaxy at low frequencies (325 MHz and 610 MHz) using the Giant Metrewave Radio Telescope (GMRT). We present here the high resolution images from our GMRT observations. While we detect no obvious extended emission from radio jets from the central AGN, we do find the emission to be moderately extended and unlikely to be dominated by disk star formation. VLBI observations using the Korean VLBI Network (KVN) are now being planned to understand the emission morphology and radiation mechanism.

한국성년례 복식의 형태와 의미 (Korean Costume's Figure and Means in the Coming-of-age Ceremony)

  • 황미선;이은영
    • 한국의상디자인학회지
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    • 제15권1호
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    • pp.155-173
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    • 2013
  • Recently, social problem of teens becomes one of the important social issues. Adolescence is the intermediate stages of childhood and adulthood. Teens have not find their identity at this time. That reason is why teens and the old generation are disconnect. That arise from the development of industry and the nuclear family, entrance examination-oriented education system. So they are wandering in the popular culture and the cyber-space. Therefore, families, schools and state should have interesting and understanding for teens, and should strive that teens establish a self established identity. Specially, ethics education using traditional culture will help to establish their identity, and that provide self-esteem and pride about korean traditional culture. This is the reason why culture contents that is based on Korean traditional culture have to make for teens. The purpose of this study is to provide the basic data that will help in the development Korean traditional cultural contents for teens. In this study, this researchers will search the following matters; first, what is ritual for Coming-of-age, second, various forms of ritual for Coming-of-age and Korean modern ritual in order to grasp the meaning of the ritual for Coming-of-age, third, costume and meaning of costume which has in both Kwan-Ryea as Korean traditional ritual for Coming-of-age and Korean modern ritual. This study will compare Kwan-Ryea with traditional ritual of modern.

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적응형 웹 사이트 구축을 위한 연관규칙 알고리즘 개발과 적용 (Development and Application of An Adaptive Web Site Construction Algorithm)

  • 최윤희;전우천
    • 정보처리학회논문지D
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    • 제16D권3호
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    • pp.423-432
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    • 2009
  • 컴퓨터의 보급과 인터넷의 발달로 인해 데이터의 유통은 증가하고 있으나 전통적인 방법으로는 가치 있고 의미 있는 정보를 획득하는 것은 어렵다. 또한, 정보화 사회에서의 많은 정보 중에서 자신에게 알맞은 정보를 탐사하는 데이터 마이닝의 필요성이 대두되고 있다. 또한 사용자들의 편리한 인터넷 항해를 돕고 적절한 정보를 제공할 수 있는 적응형 웹 사이트에 관한 연구도 필요하다. 본 연구의 목적은 사용자들에게 연관성이 있는 웹 페이지를 연결해 주는 적응형 웹 사이트 구축을 위해 웹 로그 분석을 통한 웹 사이트 사용자들의 행동 패턴을 발견하는 연관규칙 알고리즘의 개발에 있다. 데이터 마이닝의 기법 중에서 연관규칙은 웹 사이트에 접속하는 사용자들의 행동을 파악하는데 효과적이다. 본 논문에서는 웹 사용 마이닝을 이용하여 웹 서버의 로그 데이터를 분석하여 트랜잭션을 구성하고, 사용자들의 행동 패턴을 발견하기 위한 의미 있는 문서만을 추출하여 추출된 문서를 대상으로 발견한 빈발 항목으로 연결리스트를 구성하며, 빈발 패턴을 찾아 웹 페이지에 적용하는 일련의 알고리즘을 제안한다. 제안한 알고리즘의 특징은 첫째, 빈발패턴 발견을 위해 생성하는 연결리스트 이외에는 마이닝 과정에서 다른 중간생성물이 필요하지 않으므로 공간 사용면에 있어 효율적이다. 둘째, 기존의 연관규칙 알고리즘에 비해 데이터 베이스의 스캔 횟수를 줄이고, 시간복잡도를 개선하였다.

유동장 자극이 화염의 질소산화물 배출에 미치는 영향 (Effects of Flow Excitation on the Nitrogen Oxide Emission of a Non-Premixed Flame)

  • 이기만
    • 한국화재소방학회논문지
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    • 제18권2호
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    • pp.34-40
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    • 2004
  • 층류 비예혼합 분류 화염에서 다양한 주파수와 강도로 외부에서 유동장에 자극을 주었을 때 화염의 배출특성과 거동에 대해서 실험적으로 조사하였다. 먼저 일정한 관 공명 주파수에서 가진 강도를 가변시켜 난류화염 된 부상화염에서 질소산화물 배출 지수($EINO_x$)를 측정하였다. 또한, 가진 강도가 일정한 상태에서 주파수를 0 Hz에서 높은 주파수인 2 KHz까지 다양한 주파수 조건으로 가진된 한 경우에도 질소산화물의 배출지수를 측정하였다. 큰 가진 강도의 관공명 주파수로 가진된 경우 부상된 난류화염에서 $NO_x$ 배출 특성은 다음과 같이 크게 세 가지 형태의 특성을 보였다. Group I의 화염에서는 공간적인 섭동이 크며 비교적 화염길이가 길고 높은 $NO_x$ 배출 특성을 보였으며 Group II에서는 상대적으로 짧은 길이와 좁은 폭의 화염거동에 낮은 $NO_x$배출 특성을 보였다. Group III에서는 약간 긴 화염길이에 매우 큰 화염체적으로 상당한 높이까지 시ㆍ공간적으로 섭동이 큰 운동양태로 부상되는 거동과 가장 높은 $NO_x$ 배출 특성을 보였다.

The Nature of Water in Tactic Poly (2-Hydroxyethyl Methacrylate) Hydrogels

  • Kim, Eui-Hwan;Jeon, Sang-Il;Yoon, Sung-Chul;Jhon, Mu-Shik
    • Bulletin of the Korean Chemical Society
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    • 제2권2호
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    • pp.60-66
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    • 1981
  • The hypothesis that three classes of water exist in hydrogels, namely X water (free water-like), Z-water (bound water-like), and Y water (interfacial water-like), has been verified and generally accepted. To further check the validity of this hypothesis and to study the nature of X, Y, and Z water as conformation changes, several experiments have been done using Tactic Poly(2-hydroxyethyl methacrylate) (P-HEMA) gels. Thermal expansively data for tactic P-HEMA gel was obtained. In each case of isotactic and syndiotactic P-HEMA, the higher water content gels showed an extremely sharp volume change at $0^{\circ}C$, indicating the presence of normal free water-like. Lower water content gels showed no anomalous change in thermal expansion, indicating that the water is bound water-like. The medium water content gels exhibited intermediate behavior. These results were also confirmed by bulk gel conductivity measurments. The differential scanning calorimeter(DSC) experiment was simply introduced to further verify the bound water-like quantities which was obtained by the method of dilatometry and specific conductivity. Observing the amounts of X, Y, and Z water with the change of tacticity, the similar content of bound water-like may be due to the same primary structure of isotactic and syndiotactic polymer and the difference in free and interfacial water-like content may be due to the difference in secondary and tertiary structure of tactic polymer. Therefore, as the polymer conformation varies, the free and interfacial water-like content will be varied. In order to demonstrate these concepts, Russel et al.'s CPK space-filling molecular models of isotactic and syndiotactic P-HEMA was utilized.