• 대한전자공학회논문지TC
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• 제45권7호
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• pp.53-61
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• 2008

본 논문에서 줄기 노드는 mesh 토폴로지의 중추 망을 이루고 각 줄기 노드는 주변의 잎 노드와 함께 별 토폴로지의 부속망을 형성하는 무선 센서 망을 고려한다. 이러한 무선 센서 망에서 잎 노드로부터 줄기 노드로의 패킷 전달을 지원하는 MAC 방식을 설계할 때 반드시 다음 사항을 유념해야 한다. 첫째, 잎 노드는 일반적으로 배터리로부터 전력을 공급받는데 이러한 배터리를 교체하거나 충전하기가 어렵다. 둘째, 무선 센서 망은 흔히 주기적으로 데이타를 수집하여 갱신하기 위해 파송된다. 데이타 조각의 전달이 지연되면 싱크 노드의 데이타 처리가 지연되고 결과적으로 데이타 조각 자체를 폐기해야 할 수도 있다. 셋째, 무선 센서 망에서는 시그널링이 극도로 제약되고 복잡한 계산이 곤란하다. 이러한 점을 고려할 매 MAC 방식은 에너지를 절약하고 패킷 전달에서 적시성을 지원할 수 있어야 하며 동시에 단순하고 로버스트해야 한다. 본 논문에서는 무선 센서망의 MAC 방식으로 ALOHA의 수정판을 제안한다. ALOHA 제안 판은 ALOHA 원판의 단순함과 로버스트함을 보전하면서 매번 패킷의 전달을 시도하기에 앞서 잎 노드가 중지 혹은 계속을 결정하는 특징을 갖는다. 이러한 결정을 위해 본 논문에서는 Bayes 중지 규칙을 제안한다. Bayes 중지 규칙은 에너지, 적시성 고리고 throughput 손실이 반영된 Bayes 위험을 최소화하는 중지 규칙으로 잎 노드가 오직 전달 시도에 관한 선험적 지식과 자신의 전달 시도 경험에만 의존하여 중지 혹은 계속을 결정하므로 실용적이다. 계량적 결과로부터 Bayes 중지 규칙이 도입된 ALOHA 제안 판은 무선 센서 망의 열악한 환경에서 유용함을 확인한다.

• 한국음향학회:학술대회논문집
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• 한국음향학회 2002년도 하계학술발표대회 논문집 제21권 1호
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• pp.469-474
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• 2002

In recent years, modularization of engine parts has increased the application of plastic products in air intake systems. Plastic intake manifolds provide many advantages including reduced weight, contracted cost, and lower intake air temperatures. These manifolds, however, have some weakness when compared with customary aluminium intake manifolds, in that they have low sound transmission loss because of their lower material density. This low transmission loss of plastic intake manifolds causes several problems related to flow noise, especially when the throttle is opened quickly. The physical processes, responsible for this flow noise, include turbulent fluid motion and relative motion of the throttle to the airflow. The former is generated by high-speed airflow in the splits between the throttle valve and the inner-surface of the throttle body and surge-tank, which can be categorized into the quadrupole source. The latter induces the unsteady force on the flow, which can be classified into the dipole source. In this paper, the mechanism of noise generation from the turbulence is only investigated as a preliminary study. Stochastic noise source synthesis method is adopted for the analysis of turbulence-induced, i.e. quadrupole noise by throttle at quick opening state. The method consists of three procedures. The first step corresponds to the preliminary time-averaged Navier-Stokes computation with a $k-\varepsilon$ turbulence model providing mean flow field characteristics. The second step is the synthesis of time-dependent turbulent velocity field associated with quadrupole noise sources. The final step is devoted to the determination of acoustic source terms associated with turbulent velocity. For the first step, we used market available analysis tools such as STAR-CD, the trade names of fluid analysis tools available on the market. The steady state flows at three open angle of throttle valve, i.e. 20, 35 and 60 degree, are numerically analyzed. Then, time-dependent turbulent velocity fields are produced by using the stochastic model and the flow analysis results. Using this turbulent velocity field, the turbulence-originated noise sources, i.e. the self-noise and shear-noise sources are synthesized. Based on these numerical results, it is found that the origin of the turbulent flow and noise might be attributed to the process of formulation and the interaction of two vortex lines formed in the downstream of the throttle valve. These vortex lines are produced by the non-uniform splits between the throttle valve and inner cylinder surface. Based on the analysis, we present the low-noise design of the inner geometry of throttle body.

• 천문학논총
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• 제30권2호
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• pp.559-563
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• 2015

Monitor of All-sky X-ray Image (MAXI) is a Japanese X-ray all-sky surveyer mounted on the International Space Station (ISS). It has been scanning the whole sky since 2009 during every 92-minute ISS rotation. X-ray transients are quickly found by the real-time nova-search program. As a result, MAXI has issued 133 Astronomer's Telegrams and 44 Gamma-ray burst Coordinated Networks so far. MAXI has discovered six new black holes (BH) in 4.5 years. Long-term behaviors of the MAXI BHs can be classified into two types by their outbursts; a fast-rise exponential-decay type and a fast-rise flat-top one. The slit camera is suitable for accumulating data over a long time. MAXI issued a 37-month catalog containing 500 sources above a ~0.6 mCrab detection limit at 4-10 keV in the region ${\mid}{b}{\mid}$ > $10^{\circ}$. The SSC instrument utilizing an X-ray CCD has detected diffuse soft X-rays extending over a large solid angle, such as the Cygnus super bubble. MAXI/SSC has also detcted a Ne emission line from the rapid soft X-ray nova MAXI J0158-744. The overall shapes of outbursts in Be X-ray binaries (BeXRB) are precisely observed with MAXI/GSC. BeXRB have two kinds of outbursts, a normal outburst and a giant one. The peak dates of the subsequent giant outbursts of A0535+26 repeated with a different period than the orbital one. The Be stellar disk is considered to either have a precession motion or a distorted shape. The long-term behaviors of low-mass X-ray binaries (LMXB) containing weakly magnetized neutron stars are investigated. Transient LMXBs (Aql X-1 and 4U 1608-52) repeated outbursts every 200-1000 days, which is understood by the limit-cycle of hydrogen ionization states in the outer accretion disk. A third state (very dim state) in Aql X-1 and 4U 1608-52 was interpreted as the propeller effect in the unified picture of LMXB. Cir X-1 is a peculiar source in the sense that its long-term behavior is not like typical LMXBs. The luminosity sometimes decreases suddenly at periastron. It might be explained by the stripping of the outer accretion disk by a clumpy stellar wind. MAXI observed 64 large flares from 22 active stars (RS CVns, dMe stars, Argol types, young stellar objects) over 4 years. The total energies are $10^{34}-10^{36}$ erg $s^{-1}$. Since MAXI can measure the spectrum (temperature and emission measure), we can estimate the size of the plasma and the magnetic fields. The size sometimes exceeds the size of the star. The magnetic field is in the range of 10-100 gauss, which is a typical value for solar flares.

• 천문학논총
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• 제30권2호
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• pp.665-669
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• 2015

The Kepler mission has shown that small planets are extremely common. It is likely that nearly every star in the sky hosts at least one rocky planet. We just need to look hard enough-but this requires vast amounts of telescope time. MINERVA (MINiature Exoplanet Radial Velocity Array) is a dedicated exoplanet observatory with the primary goal of discovering rocky, Earth-like planets orbiting in the habitable zone of bright, nearby stars. The MINERVA team is a collaboration among UNSW Australia, Harvard-Smithsonian Center for Astrophysics, Penn State University, University of Montana, and the California Institute of Technology. The four-telescope MINERVA array will be sited at the F.L. Whipple Observatory on Mt Hopkins in Arizona, USA. Full science operations will begin in mid-2015 with all four telescopes and a stabilised spectrograph capable of high-precision Doppler velocity measurements. We will observe ~100 of the nearest, brightest, Sun-like stars every night for at least five years. Detailed simulations of the target list and survey strategy lead us to expect $15{\pm}4$ new low-mass planets.

• 천문학회보
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• 제37권2호
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• pp.97.2-97.2
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• 2012

The main payload of Science and Technology Satellite 3 (STSAT-3), Multipurpose InfraRed Imaging System (MIRIS) is the first Korean infrared space mission to explore the near-infrared sky with a small astronomical instrument developed by KASI. The 8-cm passively cooled telescope with a wide field of view (3.67 deg. ${\times}$ 3.67 deg.) will be operated in the wavelength range from 0.9 to $2{\mu}m$. It will carry out wide-band imaging and the Paschen-${\alpha}$ emission line survey. After the calibration of MIRIS in our laboratory, MIRIS has been delivered to SaTReC and successfully assembled into the STSAT-3. The main purposes of MIRIS are to perform the observation of Cosmic Infrared Background (CIB) at two wide spectral bands (I and H band) and to survey the Galactic plane at $1.88{\mu}m$ wavelength, the Paschen-${\alpha}$ emission line. CIB observation enables us to reveal the nature of degree-scale CIB fluctuation detected by the IRTS (Infrared Telescope in Space) mission and to measure the absolute CIB level. The MIRIS will continuously monitor the seasonal variation of the zodiacal light towards the both north and south ecliptic poles for the purpose of calibration as well as the effective removal of zodiacal light. The Pashen-${\alpha}$ emission line survey of Galactic plane helps us to understand the origin of Warm Ionized Medium (WIM) and to find the physical properties of interstellar turbulence related to star formation. Here, we also discuss the observation plan with MIRIS.

• Journal of Ginseng Research
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• 제41권1호
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• pp.60-68
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• 2017

Background: Various Panax ginseng cultivars exhibit a range of diversity for morphological and physiological traits. However, there are few studies on diversity of metabolic profiles and genetic background to understand the complex metabolic pathway in ginseng. Methods: To understand the complex metabolic pathway and related genes in ginseng, we tried to conduct integrated analysis of primary metabolite profiles and related gene expression using five ginseng cultivars showing different morphology. We investigated primary metabolite profiles via gas chromatography-mass spectrometry (GC-MS) and analyzed transcriptomes by Illumina sequencing using adventitious roots grown under the same conditions to elucidate the differences in metabolism underlying such genetic diversity. Results: GC-MS analysis revealed that primary metabolite profiling allowed us to classify the five cultivars into three independent groups and the grouping was also explained by eight major primary metabolites as biomarkers. We selected three cultivars (Chunpoong, Cheongsun, and Sunhyang) to represent each group and analyzed their transcriptomes. We inspected 100 unigenes involved in seven primary metabolite biosynthesis pathways and found that 21 unigenes encoding 15 enzymes were differentially expressed among the three cultivars. Integrated analysis of transcriptomes and metabolomes revealed that the ginseng cultivars differ in primary metabolites as well as in the putative genes involved in the complex process of primary metabolic pathways. Conclusion: Our data derived from this integrated analysis provide insights into the underlying complexity of genes and metabolites that co-regulate flux through these pathways in ginseng.

• 한국컴퓨터정보학회논문지
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• 제12권1호
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• pp.177-188
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• 2007

스타 스키마는 중앙에 사실테이블이 있고 이 주변에 여러 개의 차원테이블이 감싸고 있는 형태로 되어있다. 사실테이블에서의 각 행은 여러 외래키로 구성된 하나의 복합키와 이 복합키와 관련된 여러 측정값으로 구성된다 복합키의 구성원인 각 외래키는 각 하나씩의 차원테이블과 관련을 맺고 있다. 그런데 문제가 되는 것은 OLAP 스키마에서는 사실테이블에서의 복합키와 측정값이 1 : 1의 관계를 맺고 있는 것으로 되어있는데 비해서 실제의 애플리케이션 특히 금융 애플리케이션에 있어서는 복합키와 측정값이 1 : N의 관계를 맺게 된다는 점이다. 따라서 1 : N의 관계를 1 : 1로 만들기 위해서 예를 들면 SQL 데이터베이스에서 미리 필요한 처리를 한 다음 이 선처리 결과를 OLAP 데이터베이스에 입력하는 방법을 취하게 되는데, 이 방법에도 여러 문제가 있는 것으로 알려져 있다. 특히 어떤 경우에는 결과 값이 틀리게 나오기도 한다. 본 연구에서는 1 : N의 관계를 사실테이블에 유지를 하면서도 어떠한 선처리도 하지 않고 정확한 결과값을 산출할 수 있는 사실테이블의 모델링과 MDX 쿼리문 작성법을 제안하고 있다.

• 천문학회보
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• 제36권1호
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• pp.83.1-83.1
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• 2011

We report multi-epoch, simultaneous 22 GHz water and 44 GHz Class I methanol maser line survey towards 180 intermediate-mass young stellar objects, including 14 Class 0, 19 Class I objects, and 147 Herbig Ae/Be stars. We detected $H_2O$ and $CH_3OH$ maser emission towards 16 (9%) and 10 (6%) sources with one new $H_2O$ and six new $CH_3OH$ maser sources. The detection rates of both masers rapidly decrease as the central (proto)stars evolve, which is contrary to the trends in high-mass star-forming regions. This suggests that the excitations of the two masers are closely related to the evolutionary stage of the central (proto)stars and the circumstellar environments. $H_2O$ maser velocities deviate on average 9 km s-1 from the ambient gas velocities whereas $CH_3OH$ maser velocities well match with. For both maser emissions, large velocity difference (${\mid}v_{H2O}-v_{sys}{\mid}\;>\; 10kms^{-1}\; and\;{\mid}v_{CH3OH}-v_{sys}{\mid}\;>\;1kms^{-1}$) is mostly confined to Class 0 objects. The formation and disappearance of $H_2O$ maser lines are frequent and the integrated intensities of them change up to two orders of magnitude. In contrast, $CH_3OH$ maser lines usually show no significant change in the intensity, shape, and velocity. This consistent with the previous suggestion that $H_2O$ maser emission originates from the base of an outflow while 44 GHz Class I $CH_3OH$ maser emission arises from the interaction region of the outflow with the ambient gas. The isotropic maser luminosities are well correlated with the bolometric luminosities of the central the objects. The fitted relations are $L_{H2O}=1.71{\ast}10^{-9}(L_{bol})^{0.97}$ and $L_{CH3OH}=1.71{\ast}10^{-10}(L_{bol})^{1.22}$.

• 한국문헌정보학회지
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• 제13권
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• pp.39-71
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• 1986

Interlibrary loan has been a very common library service in the developed countries but it is yet to be actualized formerly in Korea. As Korea is moving toward an information society where all the individual user's request in the library should be met, we need to understand, in detail, the theory and practice of interlibrary loan service. As various information technology has been applied to the libraries, the libraries became the open system. Thus, the libraries become more cooperative, form networks, and make interlibrary loan service available. This study is based on the following three hypothesis formulated from the systems theory. 1. If libraries cooperate each other and form some kind of networks by mail, computers or telecommunications, they become the open system. 2. If a library develops as the open system, interlibrary loan becomes available in the library. 3. If the interlibrary loan system works, the role of the librarians will be changed. The research was carried out by analyzing the various studies about interlibrary loan service and by examining the interlibrary loan systerns presently working in the U.S.. The conclusions are reached deductively from the data. Some of the terminology used are defined as follows: System: a network of interrelated procedures that are joined together to perform an activity or to accomplish a specific objective. It is, in effect, all the ingredient which make up the whole. Cooperation: Working together to benefit participant libraries. Network: a much more structured type of cooperation in which definite regions or areas are connected by electronic or other means to promote interlibrary loaning of materials, in-service traing & other sharing of resources. Interlibrary loan: the lending of books between libraries. The model of cooperation or networks was used to be (1) a star type, (2) a hieranchical type, (3) a distributed type or (4) the combination of aforementioned three. However, the development of the telecommunications and computers enables all kinds of libraires cooperate together. Interlibrary loan service starts with the needs of user's information. The information have to be logically accessed through bibliographies, computers, electronic mails and satellite communications. And the logical access requires the information technology and the libraries become cooperative. The physical access to the information follows next but only traditional method of mail and some commercial service are currently available for this purpose. Therefore, researches are needed to develop this physical access. If the libraries form networks, the microaspect of library changes accordingly as the macroaspect changes. If the libraries . cooperate to become one large world library, the librarians plan, organize, control library operations and report the results. And the librarians work inside and outside of the library to cooperate with other libraries. Only the cooperation of the libraries will enhance interlibrary loan and the Korean librarians have to be prepared to accept the new role of librarianship for the interlibrary loan service.

• 한국미생물·생명공학회지
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• 제40권3호
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• pp.274-277
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• 2012

본 연구에서는 다제내성을 보이는 인체 병원균의 하나인 S. aureus에서 유래된 FtsZ 단백질의 유전자를 클로닝하고 대장균에 형질전환하여 재조합 단백질을 만들고, in vitro 상에서 폴리머 형성 활성을 측정하였다. Bradford 방법을 이용하여 SA FtsZ단백질의 농도를 측정한 후, SA FtsZ단백질의 폴리머 형성 활성을 확인하기 위해 형광계를 이용하여 excitation 방향과 $90^{\circ}$의 방향에서 산란되는 빛의 양을 측정하는 방법을 사용하였을 때에 대조군에서는 빛이 산란되지 않았고, SA FtsZ 단백질에 GTP와 $Mg^{2+}$를 처리한 실험군에서만 빛이 산란되는 현상을 관찰하였다. 1분여의 시간이 지난 이후에는 다시 산란되는 빛이 줄어드는 것을 볼 수 있는데, 이것은 SA FtsZ 단백질의 아미노말단 도메인의 GTPase 활성에 의해서 GTP가 분해되어서 SA FtsZ 단백질의 폴리머가 단량체로 분해되었기 때문이라고 예측된다. 본 연구를 통하여 확립된 SA FtsZ 활성 측정 방법은 향후 SA FtsZ 단백질의 폴리머 형성을 저해하는 방식으로 S. aureus를 표적으로 하는 항생제 후보물질 도출을 위한 스크리닝 방법으로 사용될 수 있을 것이다.