Using reverse micelle processing, ZnAl2O4 nanopowders were synthesized from a mixed precursor(consisting of Zn(NO3)2 and Al(NO3)3). The ZnAl2O4 was prepared by mixing the aqueous solution at a molar ratio of Zn : Al = 1 : 2. The average size and distribution of the synthesized powders with heat treatment at 600 oC for 2 h were in the range of 10-20 nm and narrow, respectively. The average size of the synthesized powders increased with increasing water to surfactant molar ratio. The XRD diffraction patterns show that the phase of ZnAl2O4 was spinel(JCPDS No. 05-0669). The synthesized and calcined powders were characterized using a thermogravimetric - differential scanning calorimeter(TG-DSC), X-ray diffraction analysis (XRD), and high resolution transmission electron microscopy(HRTEM). The effects of the synthesis parameter, such as the molar ratio of water to surfactant, are discussed.

Effects of dynamic high-pressure (DHP) treatments with and without integration with heating on microbial stability, vitamin C concentration, color, sugar content, and pH of orange juice were studied and compared with those of the conventional thermal treatment. Freshly squeezed orange juice was heated at 90oC for 1 min or DHP-treated at 205 MPa and 20, 50, 60, or 70oC. The DHP treatment at 20oC without heating and the treatment at 50oC inactivated indigenous mesophilic aerobic microorganisms in orange juice by 4.2 and >7 log CFU/mL, respectively. The DHPtreated juice exhibited brighter color and higher vitamin C concentration and sugar content than the thermally treated juice, regardless of integration with heating. The DHP-treated juice demonstrated brighter color and higher sugar contents than untreated juice and thermally treated juice during storage at 4oC for 63 days. The results have demonstrated the potential of applying DHP treatments to pasteurize orange juice with increasing brightness and sugar content of the juice.

Perfluorinated sulfonic acid (PFSA) ionomers have been widely used as representative polymer electrolyte membrane materials for fuel cells and water/salined water electrolyses. The PFSA ionomers membranes need to satisfy complicated transport behaviors to small molecules including gases and ionic species. That is, the PFSA ionomers membranes have to transport protons as fast as possible, while the membranes should act as hydrogen barriers, since the permeated gas induces thermal degradation of cathode catalyst resulting in rapid reduction in fuel cell performances. In this study, it is disclosed that these permeation behaviors can be easily tunable by controlling membrane processing histories even though the ionomers have the same chemical architecture and equivalent weight.

MAO ceramic coatings were prepared on AZ61 magnesium alloy for various processing times ranging from 5 to 60 min, in an electrolyte solution based on silicate-fluoride. The mechanical, electrochemical and, microstructural properties and the phase compositions of the coating layers were investigated. In this work, unlike previous studies, coatings with high amounts of the Mag2SiO4 phase were formed which contained small amounts of MgO and MgF2 at a processing condition of 30 min. A microstructural analysis revealed that the porosity of the coatings was reduced considerably with an increase in the processing time, together with a change in the pore geometry from an irregular to a spherical shape. Potentiodynamic polarization and mechanical testing results showed that the coatings acquired after a processing time of 30 min were superior to all of the others.

Analyzing asphalt mixture images can provide crucial information not only for generating advanced geometry structure in several numerical computations (i.e. FEM and/or DEM) codes, but also for numerically evaluating the material microstructure. It is well known that 3D X-Ray Computer Tomography (CT) can provide accurate and realistic microstructure information of asphalt mixtures; however, this technology still presents two limitations: 1) the equipment is very expensive and, therefore, only few pavement agencies can afford it, and 2) the software required to generate realistic image of asphalt mixture with three-phase structure (aggregate, asphalt binder and air-voids) is based on a global thresholding algorithm which cannot be easily accessed and edited by users and practitioners. In this paper, accurate and realistic 2D three-phase asphalt mixture images were generated using an advanced DIP analysis code (implemented on MATLABTM) and a common flatbed scanner, which can be easily purchased at relatively low price. The threshold algorithm was developed based on the computed results of Gmm (maximum specific gravity), Gmb (bulk specific gravity), VMA (voids in mineral aggregates) of given asphalt mixtures which can be experimentally obtained in a laboratory environment. 2D three-phase images of asphalt mixtures were derived from grey scale images (color intensity from 0 to 255) obtained from original RGB (Red-Green-Blue) scale images with a dual-threshold computation techniques (i.e. one step for computing air voids phase, T1, and a second step for computing asphalt binder (and/or mastic) phase, T2). An example of DIP analysis results is shown in Figure 1. Based on the computation results, quite accurate and good visual agreement was observed between RGB scale image and DIP analyzed image. The findings indicate that this advanced DIP analysis technique can provide reliable geometry and microstructural information for several numerical simulations such as finite element method (FEM) and discrete element modeling (DEM). This research work represents a solid base for performing simple 2D microstructure analysis using 2- and 3-point correlation function and for developing the Moon Cannone Falchetto (MCF) model which will be introduced in the next annual KSRE conference.

Galaxies can be "pre-processed" in the low-density outskirts by ambient medium in the filaments or tidal interactions with other galaxies while falling into the cluster. In order to probe how early on and by which mechanisms galaxies can be affected before they enter high-density cluster environments, we are carry- ing out an atomic hydrogen (H i) imaging study of a sample of galaxies selected from three filamentary structures around the Virgo cluster. Our sample consists of 14 late-type galaxies, which are potentially interacting with their surroundings. The Hi observations have been done using the Westerbork Synthesis Radio Telescope, the Giant Metrewave Radio Telescope, and the Jansky Very Large Array with column density sensitivity of ≈ 3-5 X 1019 cm-2 in 3σ per channel, which is low enough to detect faint Hi features in the outer disks of galaxies. In this work, we present the Hi data of two galaxies that were observed with GMRT. We examine the Hi morphology and kinematics to find the evidence for gas-gas and/or tidal interactions, and discuss which mechanism(s) could be responsible for pre-processing in these cases.

The Galactic center uniquely provides opportunities to resolve how star clusters form in neutral gas overdensities engulfed in a large-scale accretion flow. We have performed sensitive Green Bank 100m Telescope (GBT), Karl G. Jansky Very Large Array (JVLA), and Submillimeter Array (SMA) mapping observations of molecular gas and thermal dust emission surrounding the Galaxy's supermassive black hole (SMBH) Sgr A*. We resolved several molecular gas streams orbiting the center on ≳10 pc scales. Some of these gas streams appear connected to the well-known 2-4 pc scale molecular circumnuclear disk (CND). The CND may be the tidally trapped inner part of the large-scale accretion flow, which incorporates in ow via exterior gas filaments/arms, and ultimately feeds gas toward Sgr A*. Our high resolution GBT+JVLA NH3 images and SMA+JCMT 0.86 mm dust continuum image consistently reveal abundant dense molecular clumps in this region. These gas clumps are characterized by ≳100 times higher virial masses than the derived molecular gas masses based on 0.86 mm dust continuum emission. In addition, Class I CH3OH masers and some H2O masers are observed to be well associated with the dense clumps. We propose that the resolved gas clumps may be pressurized gas reservoirs for feeding the formation of 1-10 solar-mass stars. These sources may be the most promising candidates for ALMA to probe the process of high-mass star-formation in the Galactic center.

Mesenchymal stem cells (MSCs) are an attractive source for cell therapy, as they have the potential for differentiation into multi-lineage cells. Adipose tissue is a safe source due to its easy extraction and abundant resource, with minimal risk to the organ donor. In this study, we attempted to correlate the harvest yield and resulting multipotency of feline adipose tissue-derived mesenchymal stem cells (fAD-MSCs) in accordance with processing time. fAD-MSCs were individually isolated from the abdominal adipose tissues of 6 felines. They were divided into two groups, based on their processing times – Group 1: 0~1 day after adipose tissue harvesting; Group 2: more than 3 days after adipose tissue harvesting. In both groups, the proliferation capacity was analyzed using the cumulative population doubling level (CPDL) calculation assay. The expression levels of MSC-specific markers and differentiation potentials into mesodermal cell lineages were also evaluated. We observed that fAD-MSC isolation yields and CPDL were excellent in Group 1 compared with Group 2. We also found that the differentiation potential-specific genes (ACAN and OPN) were strongly expressed in Group 1 compared with Group 2. These results suggest that for the clinical treatments of feline diseases, fAD-MSCs should be isolated within 1 day after adipose tissue harvesting.

본 연구에서는 파프리카 수확기 개발의 일환으로 엔드 이펙터의 정확한 제어를 위하여 스테레오 영상으로 파프리카를 인식하고 인식된 파프리카의 공간 좌표를 획득하기 위하여 영상처리 알고리즘을 개발하고자 하였다. 먼저, 색상 정보를 이용하여 파프리카 영상을 추출하기 위하여 히스토그램 분석을 수행하였고 결과에 따른 임계값 을 설정하였다. 임계값에 의해 추출된 파프리카 영역에 대해 스테레오 대응을 수행하기 위해 실험에 사용된 스테레오 영상의 F 행렬을 구하였고 이를 이용하여 에피 폴라선을 구하여 대응을 수행하였다. 대응을 수행 할 때는 색상 영상을 이용하여 강조 마스크와 컨벌루션을 통해 중심 픽셀과 수직, 수평방향 이웃 픽셀에 가중치를 적용하여 강조한 후 최소 자승 오차를 갖는 점을 대응 점으로 추출하였다. 추출 된 대응 점간의 거리를 스테레오 영상의 기하학적인 관계를 이용하여 실제 거리를 계산하였고, 계산된 거리(Z)값을 이용하여 수평(X), 수직 (Y) 방향 공간 좌표를 획득하였다. 그 결과 수평 방향 오차 평균 5.3mm, 수직 방향 오차 평균 18.8mm, 거리 오차 평균 5.4mm로 나타났으며, 거리 400~450mm 구간과 영상의 모서리 부분의 왜곡이 발생하는 부분에서 오차가 다른 구간에 비해 크게 나타나는 것을 확인 할 수 있었다.

This paper introduces a digital image processing(DIP) method as a method for measuring the displacement of pylon. The comparison of DIP results and ANSYS analysis results verified the validity of the image processing technique. Normalized cross-correlation(NCC) coefficient was used and experiments were performed three times. It shows that the displacement difference was 22% and 5% compared to ANSYS results. Therefore, the image processing method is expected to be able to measure the displacement of pylon sufficiently.