• 전기학회논문지
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• 제62권9호
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• pp.1260-1263
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• 2013

Plane wave scattering from a spherical resonator is calculated by solving the combined field integral equation (CFIE) with Rao-Wilton-Glisson (RWG) basis functions and the moment method. The calculations show that magnetic and electric dipoles are found at resonant modes. These characteristics are confirmed by radiation patterns in the far field region. In addition, an analysis of a magnetodielectric sphere is discussed.

• 한국지구과학회지
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• 제32권6호
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• pp.595-601
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• 2011

이 논문에서는 자력 변화율 텐서를 이용하여 자기 쌍극자의 위치 정보를 파악하는 알고리즘에 대하여 기술하였다. 수직으로 자화된 자기 쌍극자에 의한 자력 변화율 텐서에서 출발하여 자기 쌍극자의 위치 벡터를 유도하였다. 그러나 이 경우 자기 쌍극자의 모멘트에 대한 정보가 주어지지 않았으므로 자기 쌍극자의 위치 벡터가 불완전하게 유도된다. 이를 극복하기 위하여 여러 측정점에서 측정된 자력 변화율 텐서값이 있다고 가정하고 이를 이용하여 자동으로 자기 쌍극자의 위치를 찾아내는 알고리즘을 제안하였다. 시추공에서 자력 변화율 텐서가 측정되었다고 가정한 합성 모델 실험에서 자력 변화율 텐서와 자기 쌍극자 자동 탐지 알고리즘을 이용하여 자기 쌍극자의 위치를 정확하게 찾을 수 있음을 확인하였다.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 2000년도 가을 학술발표회 논문집
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• pp.231-236
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• 2000

In order to predict depth of the pile forward modeling and inversion of magnetic logging data was conducted by using a finite line of dipoles model. The horizontal component as well as the vertical component of magnetic fields can be measured in the borehole, and the magnetic anomalies can be obtained by subtracting the Earth's magnetic field from the measurement. The magnetic anomalies of the pile are considered as vector sum of induced magnetization due to the Earth's magnetic field and remnant magnetization possessed by steel strings in the pile. The magnetic anomalies are used as input data for inversion from which the length, the magnetic moment per unit length, and the dip angle of the pile can be obtained. From the inversion of synthetic noisy data, and the data obtained from the field model test it is found that the driving depth of the pile can be determined as close to the order of measuring interval (5∼10㎝). It is also found that the resultant magnetic anomalies due to an individual steel string in the pile are almost same as those due to a group of steel strings located at the center of the pile. The magnetic logging method also can be used for locating reinforced bars, pipes, and steel casings.

• 우주기술과 응용
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• 제2권1호
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• pp.41-51
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• 2022

큐브위성은 기존의 인공위성과 마찬가지로 지구 관측뿐만 아니라, 우주탐사 분야에도 폭넓게 활용되는 인공위성 플랫폼이다. 또한 우주 공간물리현상을 관측하기 위한 자기장관측 임무에서도 다양한 형태로 제작되어 활용되고 있다. 자기장 측정의 경우, 일반적으로 위성의 자기 교란을 최소화하기 위해 자기장측정기가 위성 몸체로부터 멀리 떨어져 있다. 그러나 큐브위성과 같은 작은 위성의 경우 공간적인 제약으로 인해 자기장 센서의 위치 설정이 제한적이다. 이에 이 논문에서는 큐브위성에서 생성된 자기장 간섭을 추정하여 자기장 측정의 신뢰성에 얼마나 영향을 줄 수 있는지 분석하였다. 주요 잡음원으로는 상대적으로 높은 소비전력을 가진 반작용 휠과 자기 토크로드를 대상으로 조사하였다. 이러한 부품의 자기 쌍극자 모멘트는 제조업체의 데이터 시트에 제공된 정보를 사용하였다. 외부 자기장이 없는 공간에서 3 U 큐브위성 중간에 위치한 자기 토크로드의 잔류 모멘트의 영향은 위성의 몸체 최 외곽 끝에서 약 36,000 nT까지 나타날 수 있음을 확인했다. 또한, 1 nT 미만의 정확한 자기장 측정의 임무라면, 자력계는 위성 본체에서 약 0.6 m 반경 거리 외곽에 있어야 함을 알 수 있었다. 이러한 분석 방법은 자기장 측정을 수행하기 위해 CubeSat을 설계할 때 자기 청결도 분석의 중요한 역할이 될 것으로 기대한다.

• 수산해양기술연구
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• 제22권3호
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• pp.17-22
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• 1986

This paper investigates on the performance of liquid magnetic compass measuring the concomitant angle of the directional system by the kind of compass and the coefficiant of viscosity of the liquid of ones in accordance with the turning angular velocity of the compass bowl in artificial horizontal magnetic fields. The obtained results are as follows; 1. The concomitant angle is to be in proportion to the coefficiant of viscosity of the liquid of compass and the turning angular velocity of the compass bowl, but ones is to be in contrary proportion to the magnetic moment of the magnetic needle and the horizontal geomagnetic. 2. The overdevelopment of the concomitant angle keeps on regularly at any optional degree in the turning angular velocity over$\pi$ radian per minute, but varies periodically at 180 degree below 3 $\pi$ radian per minute.

• 한국재료학회:학술대회논문집
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• 한국재료학회 2003년도 춘계학술발표강연 및 논문개요집
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• pp.19-19
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• 2003

The injection of spins into nonmagnetic semiconductors has recently attracted great interest due to the potential to create new classes of spin-dependent electronic devices. A recent strategy to achieve control over the spin degree of freedom is based on dilute ferromagnetic semiconductors. Ferromagnetism has been reported in various semiconductor groups including II-Ⅵ, III-V, IV and II-IV,-V$_2$, which will be reviewed. On the other hand, to date the low solubility of magnetic ions in non-magnetic semiconductor hosts and/or low Curie temperature have limited the opportunities. Therefore the search for other promising ferromagnetic semiconducting materials, with high magnetic moments and high Curie temperatures (Tc), is of the utmost importance. In this talk, we also introduce new pure ferromagnetic semiconductors, MnGeP$_2$ and MnGeAs$_2$, exhibiting ferromagnetism and a magnetic moment per Mn at 5K larger than 2.40 ${\mu}$B. The calculated electronic structures using the FLAPW method show an indirect energy gap of 0.24 and 0.06 eV, respectively. We have observed spin injection in MnGeP$_2$ and MnGeAs$_2$ magnetic tunnel junctions through semiconducting barriers.

• 한국전기전자재료학회논문지
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• 제23권6호
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• pp.444-448
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• 2010

Based on first-principles calculations, we study the magnetic properties of Co, Ni, Fe, V, and Mn impurities in ZnO. The stabilities of the ferromagnetic state and the magnetic moment of each impurity largely depend on the amount of doped electron or hole. For lightly doped n-type ZnO, it is found that the doping of Ni ions is the most effective for inducing ferromagnetism, while Fe ions show the most stable ferromagnetic couplings for heavily doped n-type samples. The characteristics of the magnetic interactions of Co ions are similar with those of Fe ions, but Co ions require much larger amount of doped electron than Fe ions to show the ferromagnetic couplings. The ferromagnetic coupling between Mn and V ions is unstable in n-type conditions.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1992년도 한국우주과학회보 제2권1호
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• pp.7.2-7
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• 1993

The interaction between the magnetic field and the accreting matter in the magnetic compact star has taken into account in order to find some constraints between physical paramerters in these systems. We show that the interaction radius, where the matter begins to funnel in the magnetosphere, can be described as a function of the magnetic moment acctetion rate and the width of the interaction zone. This radius, after estimated iteratively for a given parameter set has been used in order to study the radiation of X-rays in the magnetic compact star. Some results of such study in context with the interaction radius in the intermediate polar have been discussed.

• Journal of Magnetics
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• 제13권2호
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• pp.57-60
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• 2008

This study examined the effect of various types of epitaxial strain on the magnetic properties of $SrRuO_3$ thin films. Epitaxial $SrTiO_3$ (001), $SrTiO_3$ (110), and $SrTiO_3$ (111) substrates were used to apply different crystal symmetries to the grown films. The films were grown using pulsed laser deposition. The X-ray diffraction patterns of the films grown under optimum conditions showed very clear peaks for the $SrRuO_3$ film and $SrTiO_3$ substrates. The saturated magnetic moment at 5 K after 7 Tesla field cooling was $1.2-1.4\;{\mu}_B$/Ru. The magnetic easy axis for all three types of films was along the surface normal. The magnetic transition temperature for the $SrRuO_3$ film with lower symmetry was slightly larger than the $SrRuO_3$ film with higher symmetry.

• Journal of Magnetics
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• 제15권1호
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• pp.1-6
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• 2010

The magnetic properties of amorphous Fe were investigated by examining the electronic structures of structurally disordered Fe systems generated from crystalline bcc and fcc Fe using a Monte-Carlo simulation. As a rst principles band method, the real space spin-polarized tight-binding linearized-mun-tin-orbital recursion method was used in the local spin density approximation. Compared to the crystalline system, the electronic structures of the disordered systems were characterized by a broadened band width, smoothened local density of states, and reduced local magnetic moment. The magnetic structures depend on the short range configurations. The antiferromagnetic structure is the most stable for a bcc-based disordered system, whereas the noncollinear spin spiral structure is more stable for a fcc-based system.