• 한국진공학회:학술대회논문집
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• 한국진공학회 1994년도 제6회 학술발표회 논문개요집
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• pp.50-50
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• 1994

Half-metallic Heusler alloys (NiMnSb, ppdMnSb, pptMnSb) have attracted much attention due to their unique electronic and magnetic structures. Sppin-ppolarized band structure calculation ppredicts metallic behavior for the majority sppin states and semiconductor behavior for the minority sppin states. We have studied the electronic structures of these half-metallic Heusler alloys by core-level pphotoemission sppectroscoppy of Mn 2pp and 3s XppS sppectra. We found large intensities of Mn 2pp satellites and 3s exchange spplitting comppared with other metal Mn-alloys. These satellite structure can be understood by applying Anderson imppurity model. This fact supports the calculated sppin pprojected ppartial density of states which suggests that the valence electrons be highly sppin ppolarized near Fermi level and that the electrons involved with charge-transfer be mainly minority sppin ones which have semiconducting band structure. The trend of charge transfer energies Δ from ligands (Sb 5pp) to Mn 3d, obtained from our model fitting, is consistent with that calculated from sppin pprojected ppartial density of state. Also the trend of d-d electron correlation energies U calculated from Mn Auger line L3 VV by Mg $K\alpha$ source is comppatible with that resulted from our model fitting. We fitted the Mn 3s curve in the same way as for insulating Mn comppounds by using the same pparameters calculated from Mn 2pp curve fitting exceppt for the Coulomb interaction energy Q between core hole and d-electrons. The 3s sppectra were analyzed by combing the charge transfer model and a simpple model taking into account the configuration mixing effect due to the intra-shell correlation. We found that the exchange interaction between 3s hole and 3d electrons is mainly respponsible for the satellite of Mn 3s sppectra. This is consistent with the neutron scattering data, which suggests local 3d magnetic moment. We find that the XppS analysis results of Mn 2pp and 3s satellite structures of half-metallic Heusler alloys are very similar to those of insulating transition metal comppounds.

• 한국자기학회지
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• 제20권3호
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• pp.83-88
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• 2010

Pd과 3d(V, Ti) 및 4d(Mo, Ru, Rh) 전이금속이 c($2{\times}2$) 합금을 이루고 있는 단층의 자성을 제일원리적 FLAPW 에너지띠 방법을 이용하여 연구하였다. 이들 합금과 비교를 위하여 Pd과 V, Ti 및 Mo, Ru, Rh 원자로만 이루어진 단층의 전자구조도 계산하였다. 3d 원소인 V와 Ti 만으로 이루어진 단층의 경우, V은 반강자성, Ti의 경우는 강자성상태가 안정적이었으나, 이들이 Pd와 c($2{\times}2$) 합금을 이루었을 경우 모두 자기모멘트가 반대 방향을 가지는 준강자성 상태가 안정적이었다. 반면에 4d 원자인 Mo, Ru, Rh이 Pd와 c($2{\times}2$) 합금을 이룰 경우에는 자기모멘트들이 같은 방향을 가졌다. 자기모멘트 값을 보면, Ru이나 Rh의 경우 순수단층이나 Pd과 합금을 이룬 경우 그리 큰 차이를 보이지 않았으나, Mo의 경우 $0.02\;{\mu}_B$에서 $2.98\;{\mu}_B$로 급격히 증가하였다. 합금을 이루는 두 원소사이의 전하이동은 전기음성도에 따르게 됨을 알았다.

• 천문학회보
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• 제36권2호
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• pp.99-99
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• 2011

A statistical study of coronal hole merging and splitting has been performed through Solar Cycle 23. The NOAA/SESC solar synoptic maps are examined to identify inarguably clear events of coronal hole merging and splitting. The numbers of merging events and splitting events are more or less comparable regardless of the phase in the solar cycle. The number of both events, however, definitely shows the phase dependence in the solar cycle. It apparently has a minimum at the solar minimum whereas its maximum is located in the declining phase of the sunspot activity, about a year after the second peak in Solar Cycle 23. There are more events of merging and splitting in the descending phase than in the ascending phase. Interestingly, no event is found at the local minimum between the two peaks of the sunspot activity. This trend can be compared with the variation of the average magnetic field strength and the radial field component in the solar wind through the solar cycle. In Ulysses observations, both of these quantities have a minimum at the solar minimum while their maximum is located in the descending phase, a while after the second peak of the sunspot activity. At the local minimum between the two peaks in the solar cycle, the field strength and the radial component both have a shallow local minimum or an inflection point. At the moment, the physical reason for these resembling tendencies is difficult to understand with existing theories. Seeing that merging and splitting of coronal holes are possible by passage of opposite polarity magnetic structures, we may suggest that the energizing activities in the solar surface such as motions of flux tubes are not exactly in phase with sunspot generation, but are more active some time after the sunspot maximum.

• 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).

• 전기화학회지
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• 제22권2호
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• pp.53-59
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• 2019

전해질의 미시 구조분석을 위해서는 이온-이온 및 이온-용매 상호작용을 이해하는 것이 매우 중요하다. 이 총설은 유전체 이완 분광법(Dielectric relaxation spectroscopy)의 기본 원리와, 이를 이용한 전해질 구조 연구 사례를 소개하고자 한다. 유전체 이완 분광법은 임피던스법의 일종으로서, 수십 GHz 수준의 높은 주파수 영역에 걸쳐 전해질의 유전 특성을 측정한다. 이를 통해, 유전체 이완 분광법은 전해질 내 존재하는 다양한 극성 화학 종, 즉, 쌍극자 모멘트(Dipole moment)를 갖는 자유 용매(Free solvent) 및 이온쌍(Ion pair)의 종류와 농도에 대한 정보를 제공한다. 유전체 이완 분광법이 제공하는 정보는 기존 분석 기법(적외선 분광법(Infrared), 라만 분광법(Raman) 및 핵자기 공명 분광법(Nuclear magnetic resonance) 등)이 제공하는 정보들과 상호보완적 관계에 있으며, 이러한 종합적 분석을 통해 전해질 구조에 관한 깊은 이해가 가능하다.

• Bulletin of the Korean Chemical Society
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• 제9권6호
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• pp.345-349
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• 1988

The polycrystalline powder of (CaLa) (MgMo)$O_6$ has been prepared at $1350^{\circ}C$ in $H_2/H_2O$ and $N_2$ flowing atmosphere. The powder X-ray diffraction pattern indicates that (CaLa) (MgMo)$O_6$ has a monoclinic perovskite structure with the lattice constants $a_0=b_0=7.901(1){\AA}$, $c =7.875(1){\AA}\;and\;{\gamma}=89^{\circ}$16'(1'), which can be reduced to orthorhombic unit cell, a = 5.551(1) ${\AA}$, b = 5.622(1) ${\AA}$ and c = 7.875(1) ${\AA}$. The infrared spectrum shows two strong absorption bands with their maxima at 590($ν_3$) and 380($ν_4$) cm, which are attributed to $2T_{1u}$ modes indicating the existence of highly charged molybdenum octahedron $MoO_6$ in the crystal lattice. According to the magnetic susceptibility measurement, the compound follows the Curie-Weiss law below room temperature with the effective magnetic moment 1.83(1)$_{{\mu}B}$, which is well consistent with that of spin only value (1.73 $_{\mu}_B$) for $Mo^{5+}$ with $4d^1$-electronic configuration within the limit of experimental error. From the thermogravimetric analysis, it has been confirmed that (CaLa) (MgMo)$O_6$ decomposes gradually into $CaMoO_4,\;MoO_3,\;MgO,\;La_2O_3$ and unidentified phases due to the oxidation of $Mo^{5+}$ to $Mo^{6+}$.

• 대한청각학회지
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• 제18권3호
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• pp.105-111
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• 2014

Assistive listening devices (ALDs) refer to various types of amplification equipment designed to improve the communication of individuals with hard of hearing to enhance the accessibility to speech signal when individual hearing instruments are not sufficient. There are many types of ALDs to overcome a triangle of speech to noise ratio (SNR) problems, noise, distance, and reverberation. ALDs vary in their internal electronic mechanisms ranging from simple hard-wire microphone-amplifier units to more sophisticated broadcasting systems. They usually use microphones to capture an audio source and broadcast it wirelessly over a frequency modulation (FM), infra-red, induction loop, or other transmission techniques. The seven types of ALDs are introduced including hardwire devices, FM sound system, infra-red sound system, induction loop system, telephone listening devices, television, and alert/alarm system. Further development of digital wireless technology in hearing instruments will make possible direct communication with ALDs without any accessories in the near future. There are two technology solutions for digital wireless hearing instruments improving SNR and convenience. One is near-field magnetic induction combined with Bluetooth radio frequency (RF) transmission or proprietary RF transmission and the other is proprietary RF transmission alone. Recently launched digital wireless hearing aid applying this new technology can communicate from the hearing instrument to personal computer, phones, Wi-Fi, alert systems, and ALDs via iPhone, iPad, and iPod. However, it comes with its own iOS application offering a range of features but there is no option for Android users as of this moment.

• 한국자기학회지
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• 제18권6호
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• pp.211-216
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• 2008

Si이 체심입방구조(body centered cubic; bcc) Fe에 불순물로 포함된 경우에 Fe의 전자구조와 자성에 미치는 영향을 스핀-궤도 상호작용(spin-orbit coupling, SOC)을 고려한 제일원리방법을 통하여 연구하였다. Si 불순물의 효과를 기술하기 위하여 27개의 원자가 포함된 bcc Fe 초격자 구조를 고려하였다. 제일원리방법은 전전자 총퍼텐셜선형보강평면파(all-electron full-potential linearized augmented plane wave, FLAPW) 방법을 일반기울기 근사(generalized gradient approximation, GGA) 하에서 계산하였다. 스핀-궤도 상호작용은 스핀대각항 만을 고려한 이차변분방법을 이용하여 자체충족적으로 계산하였다. SOC를 고려하지 않은 강자성(ferromagnetic, FM) 상태의 경우 Si 불순물의 경우에는 $-0.143{\mu}B$의 스핀 자기모멘트가 계산되었으며, Fe 원자가 Si 불순물에서 멀어지면서 각각 $2.214{\mu}B$, $2.327{\mu}B$, 및 $2.354{\mu}B$의 값을 얻었다. 그러나, SOC를 고려한 경우 Si 불순물의 스핀 자기모멘트는 $-0.144{\mu}B$로 계산되어 SOC의 효과가 크지 않았으나, Fe 원자의 경우 각각 $2.189{\mu}B$, $2.310{\mu}B$, 및 $2.325{\mu}B$로 계산되어 SOC를 고려한 경우 스핀 자기모멘트 값이 줄어드는 것을 알 수 있었다. 총전하 및 스핀밀도의 비교와 상태밀도의 비교를 통하여 이러한 현상은 Si 불순물에 의한 영향을 가리는데 참여하는 Fe 원자의 $t_{2g}$ 전자 궤도의 변형의 효과로서 SOC를 고려할 때만 얻을 수 있다.

• 한국전자파학회논문지
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• 제14권5호
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• pp.458-465
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• 2003

본 논문에서는 3차원 유전체로부터의 전자기 과도 응답을 해석하기 위하여 시간 영역 전장 적분방정식을 이용한 새로운 해법을 제안한다. 이를 위하여 공간 및 시간 시험 과정으로 분리한 갤러킨 방법을 적용한다. 3차원임의 형태의 유전체 표면을 삼각형으로 분할한 다음, 공간에 대한 등가 전류의 전개 및 시험 함수로서 삼각형 벡터 함수를 사용한다. 시간 영역의 미지 계수를 라게르 함수로부터 유도된 기저함수로 근사하며, 이 함수를 시간 영역의 시험 함수로도 사용한다 제안된 방법에 의하여 계산된 등가 전류 및 원거리장의 수치 결과들을 제시한다.

• The Korean Journal of Ceramics
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• 제4권2호
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• pp.83-89
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• 1998

The structure refinements and the electrical and magnetoelectric measurements were performed for BIT.1BF and BIT.2BT. The tetragonal distortion of the ab plane became lessened with the addition of $4BiFeO_3 into Bi_4Ti_3O_{12}$ significantly. However, the tilting of the outer-oxygen octahedra of the perovskite unit and the elongatin of the $(Bi_2O_2)^{2+}$ layers became more pronounced. For the both phases, the bariations of dielectric properties and electrical conductivities at high temperatures showed that the ferroelectic I-rerroelectric II phase transition existed before reaching the Curie temperature. The electrical conductivity became higher with the increase of $Fe^{3+}$ ions, implying that the electron transfer increased correspondingly. The magnetoelectric effect was observed linear up to ~8 kOe, which was stronger in BIT.1BF than BIT.2BF. This behavior indicates that the distortion of the ab plane may affect the induced polarization as well as magnetic moment.