• Journal of Yeungnam Medical Science
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• 제26권1호
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• pp.30-37
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• 2009

RO는 경계가 좋은 고형종괴로써, 석회화를 포함할 수 있다. 조영전 CT 영상에서 신실질과 유사한 밀도의 균일한 종괴로 보인다. 조영 후 영상에서는 불균일하게 조영증강되는데, 역동적 조영증강 검사의 동맥강조기에서 주변부는 강하게 조영증강되었다가 시간에 따라 점차 조영이 약해지고, 중앙부는 시간에 따라 점차 조영이 증강되어 시간에 따른 조영증강의 부분적 역전현상이 관찰되었다. 이러한 영상의학적 특징이 관찰되는 경우에는 RO의 가능성을 시사할 수 있으며 이를 통해 환자의 예후를 예측하고 수술 방법을 술전에 결정하는데 도움을 줄 수 있으리라 생각한다.

• 천문학회보
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• 제40권1호
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• pp.73.1-73.1
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• 2015

Isolated galaxies in low-density regions are significant in the sense that they are least affected by the hierarchical pattern of galaxy growth and interactions with perturbers at least for the last few Gyr. To form a comprehensive picture of the star formation history of isolated galaxies, we construct a catalog of isolated galaxies and their comparison sample in relatively denser environments. The galaxies are drawn from SDSS DR7 in the redshift range of 0.025 < z < 0.044. We performed visual inspection and classified their morphology following the Hubble classification scheme. We have investigated the color-magnitude diagram and found elliptical and unbarred spiral galaxies in isolated systems are relatively fainter and bluer than those in denser regions. For the spectroscopic study, we make use of the OSSY catalog (Oh et al. 2011). Our analysis on the absorption-line properties based on the comparison with stellar population models suggests that isolated elliptical galaxies are likely to be younger and metal poorer, while isolated Sc-type galaxies seem to have older luminosity-weighted ages, than their high-density counterpart. In addition, according to the BPT diagnostics, early-type galaxies among isolated galaxies are rather evenly classified into star forming, composite, Seyfert and LINER, whereas their comparisons are mainly populated in the LINER region. On the other hand, late-type galaxies do not show any prominent difference. We discuss the evolutionary histories of isolated galaxies in the context of the standard ${\Lambda}CDM$ cosmology.

• 천문학회보
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• 제40권2호
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• pp.41.3-41.3
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• 2015

As part of the Herschel key program "Water in Star-forming Regions with Herschel (WISH)", PACS imaging spectroscopy data have been taken toward ten massive young stellar objects (YSOs): four high mass protostellar objects (HMPOs), two hot molecular cores (HMCs), and four ultracompact HII regions (UCHIIs). The spectra cover a broad range of wavelengths (55 to 210 micron) presenting various atomic and molecular lines as well as excellent dust thermal continua. By fitting the continua utilizing a modified black-body formula we estimate mass-weighted temperature and column density distributions of warm dust and find that UCHII regions are warmer and HMCs are more deeply embedded than the other types. We also estimate rotational temperature and column density distributions of warm CO gas using the rotational diagram analysis. In addition, based on the comparison of high J CO line fluxes to the RATRAN estimates of central heating envelope models, we find that majority of warm CO is originated from bipolar outflow shocks.

• 천문학회보
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• 제36권2호
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• pp.111.2-111.2
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• 2011

While many astrophysical disks are vertically stratified and obey a polytropic equation of state, most studies on gravitational instability (GI) of flattened systems consider isothermal, razor-thin disks by taking vertical averages of disk properties. We investigate local GI of rotating pressure-confined polytropic disks with resolved vertical stratification by performing linear stability analysis. We find that the GI of vertically-stratified disks is in general a combination of conventional razor-thin Jeans modes and incompressible modes. The incompressible modes that dominate in the limit of the maximal disk compression require surface distortion and are an unstable version of terrestrial water waves. Disks with a steeper equation of state are found to be more Jeans unstable because they tend to have a smaller vertical scale height as well as a steeper temperature gradient corresponding to lower pressure support. GI depends more sensitively on the vertical temperature than density distribution. The density-weighted, harmonic mean, rather than the simple mean, of the adiabatic sound speed well describes the dispersion relation of horizontal modes, and thus is appropriate in the expression for Toomre Q stability parameter of razor-thin disks. We generalize Q into vertically-stratified disks, and discuss astrophysical application of our work.

• 한국세라믹학회지
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• 제48권5호
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• pp.404-411
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• 2011

The humidity controlling ceramic materials was developed by applying the phenomena of dew condensation in the capillary. It is said that the humidity range which human feels comfortable is from 40 to 70% in relative humidity. In this study, the ceramic tile using natural soils such as diatomite for interior wall was investigated. In particular, we had introduced novel processing routes for fabricating microcellular ceramics tile using hollow microsphere as a pore former. The microcellular pores in the humidity controlling ceramic materials showed the superior properties such as light-weight, heat insulation. The cell density was ${\sim}1.0{\times}10^9$ cells/$cm^3$ and density of sample was 0.65 g/$cm^3$ in the case of 1.71 wt% hollow microsphere content. Also, it is observed that the BET surface area and the pore volume of the sintered diatomite tile have the values of 40.92 $m^2$/g and 0.173 $cm^3$/g.

• 천문학회보
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• 제44권2호
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• pp.47.2-47.2
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• 2019

Observations indicate that turbulence in molecular clouds of the interstellar medium (ISM) is highly supersonic (M >> 1) and strongly magnetized (β ≈ 0.1), while in the intracluster medium (ICM) it is subsonic (M <~1) and weakly magnetized (β ≈ 100). Here, M is the turbulent Mach number and β is the ratio of the gas to magnetic pressures. Although magnetohydrodynamic (MHD) turbulence in such environments has been previously studied through numerical simulations, some of its properties as well as its consequences are not yet fully described. In this talk, we report a study of MHD turbulence in molecular clouds and the ICM using a newly developed code based the high-order accurate, WENO (Weighted Essentially Non-Oscillatory) scheme. The simulation results using the WENO code are generally in agreement with those presented in the previous studies with, for instance, a TVD code (Porter et al. 2015 &, Park & Ryu 2019), but reveal more detailed structures on small scales. We here present and compare the properties of simulated turbulences with WENO and TVD codes, such as the spatial distribution of density, the density probability distribution functions, and the power spectra of kinetic and magnetic energies. We also describe the populations of MHD shocks and the energy dissipation at the shocks. Finally, we discuss the implications of this study on star formation processes in the ISM and shock dissipation in the ICM.

• Clinical Nutrition Research
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• 제13권1호
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• pp.74-87
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• 2024

Since the effects of cinnamon supplementation on lipid profiles are still controversial, this study conducted a meta-analysis of randomized controlled trials to assess the effect of cinnamon supplementation on lipid profiles. The study was designed and conducted according to the guidelines of the 2020 preferred reporting items for systematic reviews and meta-analysis (PRISMA) statements. A systematic and comprehensive search was performed in several databases from inception up to 11 November 2023. The meta-analysis on the impact of Cinnamon on lipid profiles indicates a non-significant overall effect on low-density lipoprotein (weighted mean differences [WMD], -2.48; 95% confidence interval [CI], -9.70, 4.72). However, significant reductions are seen with doses < 500 mg/day (-10.26), and non-significant increases with doses ≥ 500 mg/day (1.18). The overall effect on high-density lipoprotein is non-significant (WMD, 3.97; 95% CI, -7.877, 15.831), showing varying responses at different doses. Triglycerides exhibit a significant overall reduction (WMD, -6.88; 95% CI, -12.62, -1.15), particularly in the < 500 mg/day group. The overall effect on cholesterol is non-significant (WMD, -4.314; 95% CI, -15.011, 6.384), with diverse responses at different doses. High heterogeneity underlines the importance of standardized study designs and further exploration of dosage-specific effects. Findings from this study suggest that cinnamon supplements might be beneficial to modulate the blood lipid profile.

• 한국측량학회지
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• 제36권6호
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• pp.611-620
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• 2018

도시재생사업의 활성화와 함께 주요 사업대상이 되고 있는 골목상권에 대한 사회적 관심이 커지고 있다. 골목상권 재생 방안을 마련하기 위해서는 어떤 고객이 얼마나 많이 매출을 발생시키는 지를 파악하는 것이 무엇보다 중요하다. 이에 본 연구에서는 고객특성이 골목상권 매출액에 미치는 영향을 분석하고자 한다. OLS 회귀분석 결과, 종속변수인 골목상권 매출액과 독립변수인 고객특성, 입지특성, 구조특성의 관계가 상권위치에 따라 달라지는 공간적 이질성이 확인되어 본 연구에서는 대안으로 지리가중회귀분석을 수행한다. 모형 적합도를 $R^2$과 AICc를 통해 비교한 결과, 지리가중회귀분석이 OLS 회귀분석보다 더 우수한 것으로 나타났다. OLS 회귀분석을 통해 여성고객 비율과 40-50대 고객비율, 골목상권 내 종사자수, 사업체 창업률, 건축물 밀도, 골목상권 면적이 정의 영향을 주는 반면 20-30대 고객비율, 지하철역과의 거리, 버스정류장과의 거리는 부의 영향을 주는 것으로 나타났다. 지리가중회귀분석의 국지적 회귀계수 값들을 골목상권별로 비교한 결과, 여성고객 비율은 서북권 골목상권 매출액에 가장 큰 영향을 주며 서남권과 도심권, 동북권은 그 다음으로 나타났다. 20-30대 고객비율과 40-50대 고객 비율은 동남권과 동북권 골목상권 매출액에 큰 영향을 주며 서남권은 그 다음으로 나타났다. 본 연구는 고객특성 중 성별과 연령에 한정된 분석만 수행했다는 점에서 한계를 갖지만 골목상권별로 매출액 영향 요인을 식별함으로써 상권 활성화방안 수립과 도시재생사업에 도움을 줄 수 있을 것으로 기대가 된다.

• Current Research on Agriculture and Life Sciences
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• 제6권
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• pp.163-169
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• 1988

본 연구는 식품의 동결시 동결기구의 설계 및 동결에너지의 효율적인 운용등을 위하여 동결상태에서 과일쥬스의 농도 및 온도변화에 따른 밀도변화를 예측하기 위하여 수행되었다. 10, 15, 20, 25, 30, 35, 40%농도의 Orange Juice, Apple Juice, Grape Juice 및 Sucrose Solation을 시료로 하여 온도강하에 의해 동결팽창되는 부위를 제거하므로써 거기에 따른 무게변화를 $-5^{\circ}C$에서 $-40^{\circ}C$까지의 온도범위에서 $5^{\circ}C$ 간격으로 각각 측정하여 밀도를 산출하였다. 그리고, Heldman의 식을 이용하여, 위의 농도와 온도범위에서 각 과일쥬스와 Sucrose Solution의 Unfrozen water fraction을 계산하였다. 실험을 통해 측정된 밀도데이타와 Unfrozen water fraction 데이타를 최적화 컴퓨터 프로그램을 이용하여 10%에서 40%까지의 농도범위와 $-5^{\circ}C$에서 $-40^{\circ}C$까지의 온도범위에서 Orange Juice, Apple Juice, Grape Juice 및 Sucrose Solution의 밀도를 예측할 수 있는 모델을 수립하였다.

• 전자공학회논문지B
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• 제33B권4호
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• pp.209-216
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• 1996

In this paper, we propose a learning method of multi-layer perceptrons (MLPs) with 8-bit data precision. The suggested method uses the cross-entropy cost function to remove the slope term of error signal in output layer. To decrease the possibility of overflows, we use 16-bit weighted sum results into the 8-bit data with appropriate range. In the forwared propagation, the range for bit-conversion is determined using the saturation property of sigmoid function. In the backwared propagation, the range for bit-conversion is derived using the probability density function of back-propagated signal. In a simulation study to classify hadwritten digits in the CEDAR database, our method shows similar generalization performance to the error back-propagation learning with 16-bit precision.