In this study, ultra-fine soft-magnetic micro-powders are prepared by high-pressure gas atomization of an Fe-based alloy, Fe-Hf-B-Nb-P-C. Spherical powders are successfully obtained by disintegration of the alloy melts under high-pressure He or N2 gas. The mean particle diameter of the obtained powders is 25.7 μm and 42.1 μm for He and N2 gas, respectively. Their crystallographic structure is confirmed to be amorphous throughout the interior when the particle diameter is less than 45 μm. The prepared powders show excellent soft magnetic properties with a saturation magnetization of 164.5 emu/g and a coercivity of 9.0 Oe. Finally, a toroidal core is fabricated for measuring the magnetic permeability, and a μr of up to 78.5 is obtained. It is strongly believed that soft magnetic powders prepared by gas atomization will be beneficial in the fabrication of high-performance devices, including inductors and motors.

Measuring the exact cable tension force is important to cable supported bridge under construction and on service. This study was planned to propose EM(electro-magnetic) sensor-based method for measuring the tension force of MS(multi-strand) cable in cable-stayed and extradosed bridge. The tension force in each strand is the same due to MS cable construction using Iso-tensioning system. Therefore, In this prosed method, EM sensor was installed directly at a strand and the measurement model was established for estimating the tension force of strand via EM sensor by experiments. The measurement model was derived from the relation of tension force and magnetic permeability. Also, the magnetic permeability is shown to be different according to the magnetization characteristic of 1860MPa and 2200MPa high-strength strand. The difference is increased as tension force increases. Additional experiment was conducted to verify the measurement model. As a result, the distribution of strand tension calculated upon the EM sensor is similar to those of tension measured by load cell. This proposed approach can be an effective tool for monitoring and measuring the cable force of MS cable.

본 연구에서는 신용카드 결제에서 가장 보편적으로 사용되는 자기띠 방식 카드의 기능을 전자적으로 모사하는 동적자장모사장치의 개발을 제안한다. 동적자장모사장치를 신용카드에 활용하여 결제가 필요한 경우에만 활성화하면, 정적으로 노출되어 있는 자기띠를 사용하는 기존 카드가 개인정보의 위/변조에 취약한 단점을 극복할 수 있게 된다. 또한 일회용비밀번호(OTP) 기능과 결합하면, 결제마다 가상의 카드번호를 사용하게 되어 위/변조를 원천적으로 예방할 수도 있다. 기술의 발전으로 다양한 결제방식이 제안되고 있으나, 실제 시장 보급은 매우 느리다. 이와 같은 이유는 여러 가지가 있지만, 결제 기반체계의 교체에 천문학적인 비용이 소요되는 문제가 가장 큰 요인으로 꼽히고 있다. 동적자장모사장치가 신용카드 두께 규격을 충족하면, 기존 결 제 기반체계를 그대로 활용할 수 있어, 한 장의 카드에 여러 카드를 담는 등의 스마트 멀티카드 기술 등의 다양한 핀테크 기술의 활용이 용이해진다는 장점이 있다.

This study investigates on the tuning stainless steel(STS630) to understand for groove cutting characteristics. For this purpose, we observed the cutting force according to feed rate and cutting speed variation and performed the computational analysis due to groove cutting depth. In groove cutting of stainless steel, there were principal force, feed force and radial force by arranging the highest cutting force in order. In case of wall thicknesses of 0.3mm and 0.5mm at groove cutting, principal force increases according to the increase of feed rate but it is not related to cutting speed. We found the unstable region of cutting force that is caused to the friction resistance of cutting tool and elastic deformation of groove wall. In computational analysis, we confirmed that the more feed rate increases, the more strain increases around the tooth root.

In this study, we investigate the kinetic properties of magnetic decreases observed in the solar wind at 1 AU using the Cluster observations. We study two different magnetic decreases: one with a short observation duration of 2.5 minutes and stable structure and the other with a longer observation duration of 40 minutes and some fluctuations and substructures. Despite the contrast in durations and magnetic structures, the velocity space distributions of ions are similar in both events. The velocity space distribution becomes more anisotropic along the direction parallel to the magnetic field, which differs from observations obtained at high heliographic latitudes. On the other hand, electrons show different features from the ions. The core component of the electrons shows similar anisotropy to the ions, though the anisotropy is much weaker. However, while ions are heated in the magnetic decreases, the core electrons are slightly cooled, especially in the perpendicular direction. The halo component does not change much in the magnetic decreases from the ambient solar wind. The strahl component is observed only in one of the magnetic decreases. The results imply that the ions and electrons in the magnetic decreases can behave differently, which should be considered for the formation mechanism of the magnetic decreases.

This study investigates the influence of sintering temperature on the magnetic properties and frequency dispersion of the complex permeability of Ni–Zn–Cu ferrites used for magnetic shielding in near-field communication (NFC) systems. Sintered specimens of (Ni0.7Zn0.3)0.96Cu0.04Fe2O4 are prepared by conventional ceramic processing. The complex permeability is measured by an RF impedance analyzer in the range of 1 MHz to 1.8 GHz. The real and imaginary parts of the complex permeability depend sensitively on the sintering temperature, which is closely related to the microstructure, including grain size and pore distribution. In particular, internal pores within grains produced by rapid grain growth decrease the permeability and increase the magnetic loss at the operating frequency of NFC (13.56 MHz). At the optimized sintering temperature (1225-1250°C), the highest permeability and lowest magnetic loss can be obtained.

We developed a Amylose magnetic beads (AMBs) based detection system for high efficient separation, concentration and detection of E. coli O157:H7 in real sample. AMBs were synthesized by amylosucrase from Deinococcus geothermalis (DgAS) with iron-oxide nanoparticle (NP). The design of amylose magnetic beads (AMBs) have studied by an enzymatic synthesis with optimized reaction condition such as substrate, sucrose, and iron-oxide NP. AMBs have specific feature. AMBs decorated with functional fusion protein, which consists in a maltose binding protein (MBP) and a streptococcal protein G (SPG). Amylose chains has maltose, thus MBP-SPG binds to the AMB. In addition, SPG specifically binds to the Fc part of antibody. That was used as a linker to immobilize antibody to the surface of AMBs. The resulting AMBs were efficiently separated and concentrated target bacteria, E. coli O157:H7. Concentrated sample is qualitatively analyzed by PCR. Our studies demonstrated that AMB-based PCR significantly reduced the limitation of detection as low as 10 1 CFU/mL, compared to that of conventional PCR. The principle of this system can be served as a high efficiency for detection method of any pathogenic bacteria. In addition, AMBs and MBP-SPG cross-linker protein developed in this study is expected to be applicable to the portable food based biological processing monitoring system.

프러시안 블루 유사체(Prussian Blue Analogue : PBA)는 3차원 구조와 기공을 갖는 금속-유 기골격체이며, 유기 리간드의 종류에 따라 다양한 구조를 갖는다. PBA는 바이오센서, 광학, 촉매, 수소 저장 장치 등의 분야에서 주목 받고 있으며 화학적 안정성을 가진 환경 친화적인 물질이다. 또한 다양 한 크기의 미세기공을 조정할 수 있어 흡착분야에서 많이 활용되고 있다. 본 연구는 수열합성법을 이용 하여 금속유기골격체인 Mn3[Fe(CN)6]2를 합성하였다. 전구체로 K4[Fe(CN)6]와 MnCl2를 사용하였고, 합 성된 물질은 소성하여 망간철산화물을 생성하였다. 실험 변수로 전구용액의 pH, 전구체의 몰농도, 반응 시간을 조절하여 입자의 크기와 형태에 대한 영향을 확인하였다. 합성된 다공체는 XRD, SEM, FT-IR, UV-Vis, TG/DTA에 의해 분석하였고, 여러 염료에 대한 흡착 특성을 평가하였다.

Magnetic decreases are often observed in various regions of interplanetary space. Many studies are devoted to reveal the physical nature and generation mechanism of the magnetic decreases, but still we do not fully understand magnetic decreases. In this study, we investigate the structure of a magnetic decrease observed in a corotating interaction region using multi-spacecraft measurements. We use three spacecraft, ACE, Cluster, and Wind, which were widely separated in the x- and y-directions in the geocentric solar ecliptic (GSE) coordinates. The boundaries of the magnetic decrease are the same at the three locations and can be identified as tangential discontinuities. A notable feature is that the magnetic decrease has very large dimension, &268 RE, along the boundary, which is much larger than the size, 6 RE, along the normal direction. This suggests that the magnetic decrease has a shape of a long, thin rod or a wide slab.

This study was carried out for characterization of MIO synthesized in our laboratory by co-precipitation method and applied isotherm and kinetic models for adsorption properties. XRD analysis were conducted to find crystal structure of synthesized MIO. Further SEM and XPS analysis was performed before and after phosphate adsorption, and BET analysis for surface characterization. Phosphate stock solution was prepared by KH2PO4 for characterization of phosphate adsorption, and batch experiment was conducted using 50 ml conical tube. Langmuir and Freundlich models were applied based on adsorption equilibrium test of MIO by initial phosphate solution. Pseudo first order and pseudo second order models were applied for interpretation of kinetic model by temperature. Surface area and pore size of MIO were found 89.6 m2/g and 16 nm respectively. And, the determination coefficient (R2) value of Langmuir model was 0.9779, which was comparatively higher than that of Freundlich isotherm model 0.9340.

목 적 : Moyamoya diseases는 특별한 이유 없이 두개 내 내경동맥의 끝부분 즉, 전대뇌동맥과 중대뇌동맥 시작 부분에 협착이나 폐색이 보이고 그 부근에 이상 혈관이 관찰되는 것을 말하는 혈관성 난치병에 속한다. 이러한 혈관성 질환을 진단하기 위해 시행하는 혈관조영술은 침습적이며, 혈관조영제가 가지고 있는 특성으로 인하여 반복 사용하는 데 있어서 제한이 있다. 따라서 비침습적이고 조영제 사용이 필요 없는 MRA가 혈관질환 진단에 많이 사용하고 있으며, 그 숫자가 해마다 증가하고 있다. 최근 MRA Data를 이용하여 혈관질환의 판단을 유용하게 할 수 있는 혈류측정 장치인 NOVA에 대하여 소개하고자 한다. 대상 및 방법 : 1. 검사장비 - MRI 장비 : Discovery 750W 3.0T (GE healthcare system) - Coil : 32channel head coil - 혈류측정 장치 : Non-invasive Optimal Vessel Analysis(NOVA 7.1.1 T4, VasSol) 2. 검사대상 2014년 5월부터 2014년 12월까지 본원을 내원한 Moyamoya disease 환자 38명(남자 : 16명, 여자 : 22명, 평균연령 38.9세)을 대상으로 Q-MRA를 시행하였다. 3. 검사방법 본원의 MRI장비 Discovery 750W 3.0T에서 획득한 3D TOF를 이용하여 Both CCA, ICA, MCA, VA, ACA, STA의 Blood flow rate(ml/min)를 측정하였다. 단, Moyamoya disease의 특성상 측정하고자 하는 혈관이 협착이나 폐색등으로 보이지 않거나 불명확 할 경우 측정에서 제외하였다. 결 과 : Q-MRA는 MRI 장비에서 획득한 3D TOF를 NOVA Tech PC workstation으로 전송하여, 측정하고자 하는 혈관의 위치를 선택한다. 선택된 혈관은 다시 MRI 장비로 전송하여 PC(Phase-contrast)기법의 MRA를 획득하고 이를 NOVA Tech PC workstation에서 혈류량과 방향을 측정하였다. 혈류량과 혈류의 방향은 NOVA Tech PC에서 제공하는 Auto contours를 이용하였다(단, PC MRA를 획득하는 과정에서 두 혈관이 너무 인접해 있거나 환자의 움직임으로 인하여 Auto contours가 정확하지 못할 경우 Manual contours를 시행하여 보정하였다). 현재 본원에서는 Moyamoya disease 환자의 수술적 치료방법인 STA-MCA 직접 혈관 문합술을 시행하기 위한 환자에게 Q-MRA를 시행하고 있으며, Q-MRA의 도입 이후 검사건수와 신뢰도가 꾸준히 증가하고 있다. 결 론 : Q-MRA은 혈관의 혈류량과 방향을 정량적으로 나타내어 혈관 수술의 적합성 여부를 확인할 수 있어 불필요한 수술을 막을 수 있고, 수술 후에는 수술 전후의 혈류량의 변화를 통하여 환자의 상태와 예후도 관찰할 수 있는 장점이 있으며, Stent 삽입의 시술 후 비 침습적인 방법으로 재협착 여부 등도 진단할 수 있어 Moyamoya disease환자에서 뿐만 아니라 다른 혈관성 질환에서도 Q-MRA 검사가 유용할 것으로 사료된다.

2007년 허베이 스피리트호 해양오염사고 이후 선박의 기름유출 시 응급봉쇄를 위한 마그네틱을 활용한 봉쇄기술이 5년간 개발되었으나 사고현장에서의 실용성이 정체된 원인을 분석하고 현재까지 개발된 봉쇄장치의 활용방안에 관한 제안을 통하여 응급봉쇄장치의 활용도와 실용화율을 높여, 방제기술의 과학화 추진의 필요성을 제안하고자 함.

The galactic magnetic field (GMF) and the intergalactic magnetic field (IGMF) affect the propagation of ultra-high energy cosmic rays (UHECRs) from the source to us. Here we examine the in uences of the GMF/IGFM and the dependence of their sky distribution on galactic latitude, b. We analyze the correlation between the arrival direction (AD) of UHECRs observed by the Pierre Auger Observatory and the large-scale structure of the universe in regions of sky divided by b. Specifically, we compare the AD distribution of observed UHECRs to that of mock UHECRs generated from a source model constructed with active galactic nuclei. Our source model has the smearing angle as a free parameter that re ects the de ection angle of UHECRs from the source. The results show that larger smearing angles are required for the observed distribution of UHECRs in lower galactic latitude regions. We obtain, for instance, a 1σ credible interval for smearing angle of 0° ≤ θs ≤ 72° at high galactic latitudes, 60° < b ≤ 90°, and of 75° ≤ θs ≤ 180°, -30° ≤ b ≤ 30°, at low galactic latitudes, respectively. The results show that the in uence of the GMF is stronger than that of the IGMF. In addition, we can estimate the strength of GMFs by these values; if we assume that UHECRs would have heavier nuclei, the estimated strengths of GMF are consistent with the observational value of a few μG. More data from the future experiments may make UHECR astronomy possible.

Observations show that the accretion ows in low-luminosity active galactic nuclei (LLAGNs) probably have a two-component structure with an inner hot, optically thin, advection dominated accretion flow (ADAF) and an outer truncated cool, optically thick accretion disk. As shown by Taam et al. (2012), within the framework of the disk evaporation model, the truncation radius as a function of mass accretion rate is strongly affected by including the magnetic field. We define the parameter β as pm = B2=8π = (1 - β)ptot, (where ptot = pgas + pm, pgas is gas pressure and pm is magnetic pressure) to describe the strength of the magnetic field in accretion ows. It is found that an increase of the magnetic field (decreasing the value of β) results in a smaller truncation radius for the accretion disk. We calculate the emergent spectrum of an inner ADAF + an outer truncated accretion disk around a supermassive black hole by considering the effects of the magnetic field on the truncation radius of the accretion disk. By comparing with observations, we found that a weaker magnetic field (corresponding to a bigger value of β) is required to match the observed correlation between L2-10keV/LEdd and the bolometric correction K2-10keV, which is consistent with the physics of the accretion ow with a low mass accretion rate around a black hole.