• The Journal of Asian Finance, Economics and Business
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• 제7권7호
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• pp.519-529
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• 2020

Livelihood capitals have a clear influence on livelihood development. As for the livelihood results, it has been pointed out in the analysis of the poor households that the ability of people to escape poverty depends especially on the access to livelihood capitals. This study aims to analyze the impacts of livelihood capital on poverty among mountain people who depend on forests through human capital, social capital, natural capital, physical capital and financial capital. This research employs the model of binary regression function. Independent variables x1, x2, …, xn are targets of livelihood strategy, vulnerability context, and livelihood capitals. These variables were selected to be included in the original model with dependent variable Y as poor and non-poor households. This study surveys households living in upland areas, near forests, and households of ethnic minorities. The results show that,out of the poor household rate, nearly 4% are newly-poor households or those falling back into poverty. Therefore, the government needs to pay more attention to this disadvantaged group and implements policies such as education and training policies, credit support policies, policies to support forest development, and payment for forest environmental services in the context of emerging countries like Vietnam.

• 대한교통학회지
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• 제32권3호
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• pp.198-206
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• 2014

경찰청 통계에 따르면, 우리나라에서 신호위반사고는 심각한 안전문제로 대두되고 있다. 본 연구에서는 청주시 신호교차로에서의 신호위반사고를 다루고 있으며, 연구 목적은 신호위반사고와 비신호위반사고의 특성을 비교분석하고 이항 로지스틱 모형을 이용하여 영향요인을 파악하기 위함이다. 이를 위해 본 연구에서는 2007-2011년간 청주에서 발생한 2천246건의 신호위반사고와 3천884건의 비신호위반사고 자료를 이용하여 두 집단 간의 차이를 검증하고자 한다. 주요 연구결과는 다음과 같다. 첫째, 신호위반사고는 야간시간대 및 직진상태에서 많이 발생하였다. 둘째, 신호위반사고와 비신호위반사고에 영향을 주는 변수로는 충돌형태, 충돌전 진행방향, 운전자 연령대(30대, 50대), 음주운전 및 사고유형 등으로 나타났다. 마지막으로, 이항 로지스틱 회귀분석에 의해 통계적으로 유의한 모형식이 개발되었다(Hosmer and Lemeshow test: 7.052, p-value:0.531).

• 한국콘텐츠학회논문지
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• 제18권4호
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• pp.214-222
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• 2018

본 연구는 결혼이주여성을 특별 광역시지역과 도지역 거주자 구분하여, 거주지의 특성이 지역사회통합에 미치는 차별적 영향 변인 분석을 목적으로 하였으며, 특별 광역시지역 거주 결혼이주여성 163명, 도지역 거주 결혼이주여성 182명을 대상으로 설문조사를 실시하여 결과를 분석하였다. 이항로짓모델(binary logit model)을 주로 이용하여 분석한 결과를 보면 다음과 같다. 첫째, 모형의 적합성은 특별 광역시지역 모형과 도지역 모형 모두 적합한 것으로 나타났다. 둘째, 특별 광역시지역 모형과 도지역 모형의 영향력을 비교한 결과, 개인적 특성 및 가족적 특성은 특별 광역시 지역보다 도지역에서 지역사회통합에 강한 영향을 미치는 반면, 사회적 특성은 도지역보다 특별 광역시 지역에서 지역사회통합에 강한 영향을 미치는 것으로 나타났다. 이는 향후 정책적 개입에 있어 차별화된 전략이 요구됨을 시사한다.

• 천문학회보
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• 제43권1호
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• pp.41.2-41.2
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• 2018

EL CVn-type eclipsing binaries are composed of a massive A-type main-sequence primary star and a hotter B-type secondary one. These are worthy of particular attention because the secondary stars are rare objects to be extremely low-mass white dwarf precursors (ELM proto-WD) with the mass of ${\leq}0.2M_{\odot}$, evolving to higher effective temperatures and higher surface gravities. A few of them were discovered to show multi-periodic pulsations in one or both components. We monitored one of these rare and interesting objects, J0247-25 (=1SWASP J024743.37-251549.2), at two KMTNet sites of SAAO in South Africa and SSO in Australia. The observations were performed with the KMTNet 1.6m telescopes and pre-science 4K CCD cameras during the system test run from July to November 2014. Using the photometric data obtained for a total of 23 nights, we constructed well-defined eclipsing light curves in B/V-bands and derived absolute parameters (mass and radius, etc.) of each binary component. After subtracting model eclipsing curves from the data, we detected seven frequencies with 33~53 cycles per day (c/d) and identified them to be Delta Sct-type pulsations originated from the A-type primary component. Five frequencies were turned out to be excited by rotational splitting of non-radial pressure modes, enabled us to investigate rotational properties. We could not detect any frequency higher than 100 c/d, implying that pulsation amplitudes of the proto-WD secondary decrease greatly.

• 한국정보통신학회논문지
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• 제25권11호
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• pp.1559-1565
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• 2021

본 논문에서는 다중 사용자 거대 다중 안테나 시스템에서 안테나 선택 기법을 제안한다. 제안된 안테나 선택 기법은 심화 강화학습 네트워크를 활용함으로써 피드백 오버헤드를 획기적으로 낮추면서 기존 방식과 거의 같은 성능을 얻을 수 있다. 각 사용자는 기지국의 거대 안테나들과 형성된 채널의 이득 값을 L번째 큰 채널 이득과 비교하여 대소관계에 따라서 단일 비트의 이진수로 변환하여 피드백함으로써 기존 피드백 방식보다 오버헤드를 낮출 수 있다. 제안 방식에서는 감소한 피드백 정보로 인한 성능 저하를 방지하기 위해서 심화 강화학습 네트워크를 활용하였다. 제안 방식의 성능을 분석하기 위하여 다양한 환경에서 시뮬레이션을 수행하였으며, 제안 방식이 최적 방식에 가까운 기존 방식과 유사한 평균 전송률을 얻을 수 있음을 확인하였다.

• 천문학회보
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• 제46권1호
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• pp.55.2-56
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• 2021

The progenitor of Type Ia supernovae (SNe Ia) is mainly believed to be a close binary system of acarbon-oxygen white dwarf (CO WD) and non-degenerate companion (single degenerate) or another WD (double degenerate). However, it is unclear which system is more prevalent. Here, we present a high cadence optical/Near-IR light curve of normal but slightly faint type Ia SN 2019ein from IMSNG project. We fit the early light curve (t <+8.3 days from the first detection) with various models to find the shock-heated cooling emission from SN ejecta-companion interaction. No significant shock-heated cooling emission is found, from which we constrain the progenitor star size as the following. The upper limit (R_upper,*) of the companion size in R-band is ~0.2R_⊙ when forcing the first light time (t_fl) to have one value and ~0.9R_⊙ when using the mean value of tfl from the fitting in each band. Assuming the source of the I-band curve is almost powered from the radioactive decay, we obtained R_upper,*~1.2R_⊙. The early B-V color curve is in agreement with the model color curve of the 2M_⊙ main sequence companion. These results allow us to at least rule out large stars like red giants as a companion star of the binary progenitor system of this supernova. B-R and V-R color do not show any significant signs of a red bump, which shows a thin helium shell (MHe<0.1M_⊙) for the sub-Mch WD (double detonation model). In addition, we estimated the distance to NGC 5353 as 37.098±0.028Mpc.

• 한국연초학회지
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• 제13권2호
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• pp.34-41
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• 1991

To explore the possibility of introducing Zea mays transposable element Ac(activator) which can be used as a mutagen and gene tag in tobacco plants other than maitre, we tried to introduce a cloned Ac element into tobacco cells by an Agrobacterium tumefaciens binary vector system. Transformation of N. babacum cv. Burley 21 tissues and regeneration to whole plant were carried out. The frequency of the transformed callus induced in shoot induction media was higher than that of transformed callus induced in callus induction media. However, the calli were not grown in the second selection media, and became yellow senescent calli. Regenerated tobacco plantlets with foreign gene were also obtained in shoot induction media containing 100 $\mu\textrm{g}$/ml kanamycin and 100$\mu\textrm{g}$/ml carbenicillin. The leaf tissues of transformant was also resistant to 1000 $\mu\textrm{g}$/ml kanamycin. The chromosomal DNAs of transformant and normal plant of N. tabacum were digested by EcoR I and Hind III but not by Pst I.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2001년도 추계학술대회 논문집
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• pp.187-192
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• 2001

In this paper, a practical method to generate task strategies applicable to charmfulness and high-precision assembly, is proposed. The difficulties in devising reliable assembly strategies result form various forms of uncertainty such as imperfect knowledge on the parts being assembled and functional limitations of the assembly devices. In approach to cope with these problems, the robot is provided with the capability of learning the corrective motion in response to the force signal through iterative task execution. The strategy is realized by adopting a learning algorithm and represented in a binary tree type database. To verify the effectiveness of the proposed algorithm, a series of simulations and experiments are carried out under assimilated real production environments. The results show that the sensory signal-to-robot action mapping can be acquired effectively and, consequently, the assembly task can be performed successfully.

• Journal of Photoscience
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• 제5권3호
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• pp.125-129
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• 1998

Occurrence of an electron (or H atom equivalent to one electron plus H+) transfer from $\alpha$- tocopherol $\alpha$(TOH) to a number of photosensitizers in theri triplet states were investigated by monitoring the ESR signal of $\alpha$-chromaoxyl radical ($\alpha$(TO.) in ethanolic solutions of $\alpha$TOH and the sensitizers under continuous illumination. Every sensitizer molecule examined, such as protocholorophyllide (Pchl), hematoporphyrin and rose bengal which are generally regarded as efficient type II photosensitizers and thus have long-lived triplet states, was found to actively participate in an electro transfer reaction with $\alpha$TOH even under air-saturation conditions, generating $\alpha$TOH complex as an intermediate in a fashion of Michaelis-Menten type of reaction. For the reaction of $\alpha$TOH with triplet Pchl, the rate law was derived by applying the steady approximation for the binary complex, triplet Pchl-$\alpha$TOH , which turned out to be well consistent with the kinetic data.

• 천문학회지
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• 제34권2호
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• pp.81-97
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• 2001

Since the first proposal by Paczynski, great efforts to detect Galactic dark matter by detecting light variations of stars located in the Magellanic Clouds and Galactic bulge caused by gravitational microlensing have been and are being carried out and more than 1,000 events have been successfully detected. In this paper, we review the progress in the theoretical and experimental progresses in microlensing. We begin with basics of microlensing and summarize the results obtained from the last 8 year observations along with the implications of the results. We also discuss the usefulness of microlensing in other fields of astronomy such as the stellar atmosphere, Galactic binary systems, and extra-solar planets. We finally discuss the problems of the current experiments and the new types of observations that can overcome these problems.