• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2010년도 한국우주과학회보 제19권1호
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• pp.40.4-41
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• 2010

Using magnetic field and plasma moment data obtained by THEMIS satellites(A, D, and E), we selected 203 fast flow events accompanied by dipolarization in the near-Earth region( X(GSM) = -7 ~ -12 RE) and statistically examined their properties. It was found that most of the fast flows show the maximum velocity between 1 minute before dipolarization onset and 2 minutes after onset and proceed earthward and duskward. We also found that only the flows with low velocity of less than 400 km/s are observed at X > -8 RE, while the high velocity flows(as well as low velocity flows) are observed at the further tailward region(X < -8 RE). And most of the tailward flows are slow regardless of distance at X(GSM) = -7 ~ -12 RE. On the other hand, if we consider the fast flow as a bubble (Pontius and Wolf, 1990), the entropy parameter, PV5/3 is an important factor to describe the plasma sheet dynamics. Thus we investigated the relationship between the flow velocity and the amount of change in PV5/3 before and after dipolarization onset and found out that the dipolarizations with more depleted entropy parameter tend to show higher flow velocity. Also we examined how the magnetic field at geosynchronous orbit responds to the fast flow accompanied by dipolarization in the near-earth plasma sheet, using the measurements from GOES 11 and 12 statellites. We found that most of the fast flows do not reach geosynchronous orbit as suggested by Ohtani et al. (2006).

• 천문학회지
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• 제50권2호
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• pp.29-39
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• 2017

We investigate two abnormal CME-Storm pairs that occurred on 2014 September 10 - 12 and 2015 March 15 - 17, respectively. The first one was a moderate geomagnetic storm ($Dst_{min}{\sim}-75nT$) driven by the X1.6 high speed flare-associated CME ($1267km\;s^{-1}$) in AR 12158 (N14E02) near solar disk center. The other was a very intense geomagnetic storm ($Dst_{min}{\sim}-223nT$) caused by a CME with moderate speed ($719km\;s^{-1}$) and associated with a filament eruption accompanied by a weak flare (C9.1) in AR 12297 (S17W38). Both CMEs have large direction parameters facing the Earth and southward magnetic field orientation in their solar source region. In this study, we inspect the structure of Interplanetary Flux Ropes (IFRs) at the Earth estimated by using the torus fitting technique assuming self-similar expansion. As results, we find that the moderate storm on 2014 September 12 was caused by small-scale southward magnetic fields in the sheath region ahead of the IFR. The Earth traversed the portion of the IFR where only the northward fields are observed. Meanwhile, in case of the 2015 March 17 storm, our IFR analysis revealed that the Earth passed the very portion where only the southward magnetic fields are observed throughout the passage. The resultant southward magnetic field with long-duration is the main cause of the intense storm. We suggest that 3D magnetic field geometry of an IFR at the IFR-Earth encounter is important and the strength of a geomagnetic storm is strongly affected by the relative location of the Earth with respect to the IFR structure.

• 한국세라믹학회지
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• 제31권2호
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• pp.155-160
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• 1994

PZT ceramics substituted by La3+ and Nd3+ were fabricated according to the formula: [Pb1-x(La or Nd)x][Zr0.58Ti0.42]1-x/4$\square$x/4O3(x=0.00, 0.02, 0.05, 0.08, 0.15, 0.20). The crystal structure and microstructure were investigated by XRD and SEM. It was observed that the phase transitions among rhombohedral, tetragonal, and cubic symmetry occured as the substitutional quantity increased. Dielectric constant, dissipation factor and piezoelectric coefficient (d33), of each sample were measured. The dielectric properties were changed as the substitutional quanity of rare earth ion increased. These changes could be explained by crystal structure and compositional fluctuaction. Its d33 was higher at tetragonal region near to phase boundry between rhombohedral and tetragonal, which was explained by reorientation of domain wall.

• 지구물리
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• 제9권4호
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• pp.377-386
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• 2006

인류의 문명과 토목은 불가분의 관계를 갖고 있다. 고도의 산업화 사회로 발전하면서 제한된 지형적인 여건에 따라 다양한 대형 구조물이 형성되고 있다. 그러나 대형 구조물은 인간 생활의 편리함을 제공하는 국가 시설이지만 침하 붕괴 등 예상하지 못한 재해가 발생할 수 있다. 현재 활용되고 있는 상대적 변위측정 시스템은 전체적인 변형량을 해석하기 어려운 실태이며 설계 허용 범위내에서 구조물의 변형이 일어나고 있는지를 알 수가 없다. 본 연구에서는 약13년 된 필댐을 대상체로 하여 3D Laser Scanning을 이용하여 흙댐의 3차원 공간좌표를 가지는 측점군(point-cloud)을 생성하여 대상체 표면상의 수많은 3차원 공간좌표(x,y,z)를 얻는 방법으로서 실제 댐 사면과 동일한 사면형상 데이터를 취득할 수 있다. 이것은 3차원 공간상의 모델링이 형성되며, 이 자료로부터 댐 사면의 거리, 면적과 체적 등을 측정하여 댐체와 관련된 각종 정보를 얻을 수 있다. 본 연구를 통하여 댐체의 배부름(bulging)현상을 미연에 발견하여 유지관리의 중요 자료원으로 활용 할 수 있도록 한다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2007년도 Techno-Fair 및 추계학술대회 논문집 전기물성,응용부문
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• pp.92-93
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• 2007

X7R 고압용 적층 칩 캐패시터 제작을 위한 내환원성 유전체 조성물에서 희토류인 $Er_2O_3$을 0.6 mol% 첨가한 후 유리프릿 첨가시소결특성 및 절연저항이 향상됨을 확인 할 수 있었다. 회토류인 $Er_2O_3$을 첨가시 유전율 및 절연저항이 감소하는 경향을 보이나 $85^{\circ}C$ 영역에서 온도특성을 향상시키는 것을 확인하였으며 고압 적층 칩 캐패시터 제작시 온도 특성이 우수한 재료를 개발 할 수 있었다.

• 지구물리와물리탐사
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• 제21권4호
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• pp.213-219
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• 2018

본 연구에서는 제온 파이 x200 프로세서를 이용하여 3차원 파동 전파 모델링을 수행하고 기존의 제온 CPU를 사용한 경우와 병렬 연산 성능을 비교하였다. 제온 파이 1세대 프로세서인 제온 파이 나이츠 코너 보조프로세서와 달리 제온 파이 2세대 프로세서인 x200 프로세서는 직접 운영체제 실행이 가능하므로 내장 메모리와 주메모리 사이의 추가적인 통신이 필요 없다. 또한 제온 파이 x200 프로세서는 대용량 주메모리와 고대역폭 메모리를 이용하여 대규모 컴퓨팅을 독립적으로 실행할 수 있다. 병렬 연산 성능 비교를 위해 MPI (Message Passing Interface)와 OpenMP (Open Multi-Processing)를 이용해 모델링을 수행하였다. SEG/EAGE 암염돔 모델을 이용한 수치 실험 결과 제온 파이에서 다량의 연산 코어와 고대역폭 메모리를 이용해 12 코어 CPU 대비 2.69 ~ 3.24배 우수한 모델링 성능을 얻을 수 있었다.

• 한국광물학회지
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• 제26권1호
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• pp.35-44
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• 2013

유사 올리빈 구조를 가지는 탄소코팅 합성 $Li^+Fe^{2+}(PO_4)^{3-}$ 분말시료에 대한 상온-고압실험을 대칭 다이아몬드 앤빌기기를 이용하여 35.0 GPa까지 시행하였다. $LiFePO_4$의 압축 데이터를 이용하여 계산된 체적탄성률은 $130.1{\pm}10.3$ GPa이다. 18 GPa 이상의 압력에서 d = 3.386 ${\AA}$ 위치에 새로운 피크가 관찰되고 35 GPa에서는 d = 2.854 ${\AA}$에 또 다른 피크가 관찰되고 있으나 주 결정구조는 사방정계인 것으로 판단된다. 압력에 대한 단위 포 부피의 압축은 M1($Li^+O_6$)의 수축이 두드러지고 M2($Fe^{2+}O_6$)와 사면체($PO_4$)의 수축은 상대적으로 작은 것으로 나타났다.

• Corrosion Science and Technology
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• 제17권1호
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• pp.1-5
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• 2018

As structural materials, magnesium (Mg) alloys have been widely used in the fields of aviation, automobiles, optical instruments, and electronic products. There are few studies on the effect of coating conditions on the compositional variation during the formation process of the conversion coatings. Rare-earth based conversion coating on AZ91 magnesium alloy was prepared in ceric sulfate and hydrogen peroxide contained solution. The element composition and valence as well as their distribution in the coating were analyzed with energy dispersive X-ray spectroscopy (EDS), Electron probe micro-analyzer (EPMA), X-ray photoelectron spectroscopy (XPS). The effect of treating process on the element composition were also studied. It was found that the conversion coating surface consists of Mg, Al, O, Ce, and the weight content of Ce in the coating was affected by the treating solution concentration and immersion time; the Ce element was distributed in the coating non-uniformly and existed in the form of $Ce^{+3}$ and $Ce^{+4}$, while the O element existed in the form of $OH^-$, $O^{2-}$, $H_2O$. Based on microscopic analysis results, the electrochemical deposition mechanism on the micro-anode and micro-cathode in the process of the coating growth was suggested.

• The Korean Journal of Ceramics
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• 제5권4호
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• pp.375-378
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• 1999

In tho XRD study of $56ZrF_4 \cdot34BaF_2 \cdot4AIF_3 \cdot(6-x)LaF_3 \cdotxLnF_3$ glassdLn=Ce, Nd, Gd, Th), halo pattern charactarktic fo an amorphous sample appeared. When the halo peak angle ($\theta_p$) was converted into a wavenumber with $Qp=4\pi sinG\pi/\lambda(\lambda$ is the wavolongth of the radialion used), it was found that the Qp values varied almost liuearly with the concentration 01 $LnF_3$. The emissiou spect1.a of $Ce^{3-}$-containing fluoride glasses nnder 273 nm excitation had a peak maximum at ea. 300 nm $(Ce^{3+}$ 5d-4f- transition). The maximal intensity of the fluorescence was observed when the $CeF_3$, content was extremely low (ca. 1 mol%j. DTA measurement revealed tbat these fluoride glasses had two crystallization temperatures. In $56ZrF_4. 34BaF_2. 4NF_3. (6-x)LaF_3 .xNdF_3$ glasses, the actmation energies of crystallization obtained from a Kssinger plot were 1.7 and 5.0 eV for the glass with x=2, and 1.9 and 5.6 eV for the glass with x=4.

• 한국자기학회:학술대회 개요집
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• 한국자기학회 2009년도 정기총회 및 동계학술연구발표회
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• pp.192-192
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• 2009

Magnetic and magnetotransport properties of (1-x) $La_{0.7}Sr_{0.3}MnO_3-xRE_2O_3$ (RE=La, Nd) (x = 0.025, 0.05, 0.075, 0.1, 0.2, 0.3) composite polycrystalline samples were systematically studied. Samples were prepared using conventional solid-state reaction. LSMO and $RE_2O_3$ react at high temperature and become chemically compatible. The ferromagnetic-paramagnetic transition temperatures ($T_c$) of the LSMO-$Nd_2O_3$ composite samples were decreased 313K~349K with increasing x, while the $T_c$ values of the LSMO-$La_2O_3$ composite samples were almost unaltered in the range of 355K~358K, representing that the ferromagnetism of LSMO might be more seriously degraded by Nd substitution on the ($La_{0.7}Sr_{0.3}$) site. However, LSMO-$RE_2O_3$ composite samples exhibit greatly enhanced low field magnetoresistance (LFMR) and dMR/dH value without an appreciable increase in its resistivity. Remarkably improved LFMR properties are attributed to LSMO grain boundaries acting as effective spin-dependent scattering centers. The relationship among the $RE_2O_3$ addition, microstructure, magnetic and magnetotransport properties will be discussed in this paper.