• 한국자기학회:학술대회 개요집
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• 한국자기학회 2007년도 The 1st International Symposium on Advanced Magnetic Materials
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• pp.49.1-49.1
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• 2007

• 대한전자공학회논문지TC
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• 제46권9호
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• pp.52-59
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• 2009

본 논문에서는 차량용 위성 안테나에 적합한 평판형 도파관 안테나를 설계 제작 하였다. 제안된 안테나는 마이크로 스트립 패치 배열 안테나의 유전체 손실 및 급전 라인의 손실을 대체하고자 조립하기에 간단한 3층 구조의 급전 도파관을 이용하여 고이득의 안테나를 구현하였다. 또한 위성에서 송신한 선형 편파 신호가 전리층을 지나면서 'Faraday rotation' 현상으로 인해 송신 안테나와 수신 안테나사이에 스큐가 발생하고 이는 편파 손실을 야기시켜 신호의 세기가 감쇄되는데, 이를 제거하기 위해서 아령 모양의 선형 편파기를 제안하였다. 본 논문에서 제안된 $4{\times}16$ 배열 안테나를 제작한 결과 29.4dB의 이득을 얻었다.

• 천문학회보
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• 제35권2호
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• pp.75.1-75.1
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• 2010

The nature and origin of the intergalactic magnetic field (IGMF) are an outstanding problem of cosmology, yet they are not well understood. Measuring Faraday rotation (RM) is one of a few promising methods to explore the IGMF. We have theoretically investigated RM using a model of the IGMF based on a MHD turbulence dynamo (Ryu et al. 2008; Cho et al. 2009). In the previous KAS meeting, we reported the results for the present-day local universe; for instance, the probability distribution function (PDF) of ${\mid}RM{\mid}$ follows the lognormal distribution, the root mean square (rms) value for filaments is ~1 rad m^{-2}, and the power spectrum peaks at ~1 h^{-1} Mpc scale. In this talk, we extend our study of RM; by stacking simulation data up to redshift z=5 and taking account of the redshift distribution of radio sources, we have reproduced an observable view of RM through filaments against background radio sources. Our findings are as follows. The inducement of RM is a random walk process, so that the rms of RM increases with increasing path length. The rms value of RM for filaments reaches several rad m^{-2}. The PDF still follows the lognormal distribution, and the power spectrum of RM peaks at less than degree scale. Our predictions of RM could be tested, for instance, with LOFAR, ASKAP, MEERKAT, and SKA.

• Journal of Magnetics
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• 제12권3호
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• pp.129-132
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• 2007

Bismuth-substituted yttrium iron garnet (Bi:YIG, $Bi_{0.5}Y_{2.5}Fe_5O_{12}$) films were deposited with aerosol deposition method and their magnetic and optical properties were investigated as a function of annealing temperature. Since the ceramic films deposited with aerosol deposition method have not a perfect crystal structure due to non-uniform internal stress occurred by mechanical collision during their deposition, the post annealing could be a key process to release its internal stress and to improve its micro structure for optimizing the magnetic and magneto-optic properties of films. The crystallinity of Bi: YIG film was improved with increase of annealing temperature, and the saturation magnetization increased up to 87 emu/cc at $800^{\circ}C$. The Faraday rotation increased up to $1.4deg/{\mu}m$ by annealing at $700^{\circ}C$ around the wavelength of $0.5{\mu}m$. The optical transmittance of the Bi:YIG film was also improved in visible region.

• 한국자기학회지
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• 제19권5호
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• pp.186-190
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• 2009

본 연구에서는 수직 Bridgman 법으로 묽은 자성 반도체 Cd$_{1-x}$Mn$_x$Te 단결정을 성장시켜 Mn의 조성비 변화에 따른 자기광학적 특성과 응용성을 조사하였다. X-선 회절 실험으로부터 x < 0.82 조성에 대하여 zinc-blende 구조임을 확인하였다. 띠 간격 에너지는 온도 감소와 Mn 조성비 증가에 대하여 선형적으로 증가하였다. Faraday 회전은 광 에너지 증가 때문에 띠 간격 에너지 근처에서 증가하였고, Mn 조성비 x가 증가함에 따라 증가하였다. Cd$_{0.62}$Mn$_{0.38}$Te 결정을 이용한 광 아이솔레이트의 아이솔레이션과 삽입손실은 45와 0.35 dB이었다.

• 천문학회지
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• 제48권5호
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• pp.257-265
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• 2015

We present results of long-term multi-wavelength polarization observations of the powerful blazar 3C 279 after its γ-ray flare on 2013 December 20. We followed up this flare with single-dish polarization observations using two 21-m telescopes of the Korean VLBI Network. Observations carried out weekly from 2013 December 25 to 2015 January 11, at 22 GHz, 43 GHz, 86 GHz simultaneously, as part of the Monitoring Of GAmma-ray Bright AGN (MOGABA) program. We measured 3C 279 total flux densities of 22–34 Jy at 22 GHz, 15–28 Jy (43 GHz), and 10–21 Jy (86 GHz), showing mild variability of ≤ 50 % over the period of our observations. The spectral index between 22 GHz and 86 GHz ranged from −0.13 to −0.36. Linear polarization angles were 27°–38°, 30°–42°, and 33°–50° at 22 GHz, 43 GHz, and 86 GHz, respectively. The degree of linear polarization was in the range of 6–12 %, and slightly decreased with time at all frequencies. We investigated Faraday rotation and depolarization of the polarized emission at 22–86 GHz, and found Faraday rotation measures (RM) of −300 to −1200 rad m⁻² between 22 GHz and 43 GHz, and −800 to −5100 rad m⁻² between 43 GHz and 86 GHz. The RM values follow a power law with a mean power law index a of 2.2, implying that the polarized emission at these frequencies travels through a Faraday screen in or near the jet. We conclude that the regions emitting polarized radio emission may be different from the region responsible for the 2013 December γ-ray flare and are maintained by the dominant magnetic field perpendicular to the direction of the radio jet at milliarcsecond scales.

• 한국정밀공학회지
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• 제16권12호
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• pp.40-45
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• 1999

Electrical damages to critical parts in rotation machinery have caused may machinery failures and hours of costly downtime. The problem of shaft currents generated in non-electrical machines have puzzled both users and manufacturers of these machines. The main solution for preventing electro- magnetic type damage is to demagnetize all of the machinery parts, however this is costly and time consuming. Therefore a thorough investigation into the causes and physical characteristics of electro- magnetic shaft currents is needed. In this paper, the self excitation theory was developed for a simple model, and axial flux Faraday disk machine surrounded by a long solenoid. Experimental tests were conducted to investigate the physical characteristics on an electromagnetic self excitation rig. The theory showed that the directions of both the shaft rotation and the coil turns should e identical if self excitation is to occur. From the tests, the electromagnetic type shaft current had both AC and DC components occurred at all vibration frequencies. This could point to the way to detect small instabilities or natural frequency locations by monitoring shaft currents.

• 대한전기학회:학술대회논문집
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• 대한전기학회 1988년도 전기.전자공학 학술대회 논문집
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• pp.769-770
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• 1988

The Pockel's effect is well know as a voltage measurement method. This method is applicable to high voltage measurement equipments. We observe the Faraday rotation of the polarization plane in the current-induced magnetic field.

• 천문학회보
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• 제36권2호
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• pp.116.2-116.2
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• 2011

We investigate Faraday rotation measure (RM) toward high Galactic latitudes due to the Galactic magnetic field (GMF). The Galactic contribution to RM comes from the global component and the turbulent component of the GMF, and we newly model the latter by incorporating data of MHD turbulence simulations. We find that for the turbulent velocity of ~50 km/s, the standard deviation of the RM due to the GMF toward high Galactic latitudes is close to the observed value, several rad m^{-2}. Yet, the predicted second-order structure function (SF) has values substantially smaller than the observed ones at separation angles of <~ several degree. This suggests that the intergalactic magnetic field (IGMF) significantly contributes to RM toward high Galactic latitudes, particularly at small angular scales. Our work proposes a strategy for surveys to explore the IGMF with LOFAR, ASKAP, MeerKAT, and SKA.

• 대한전자공학회논문지
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• 제20권6호
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• pp.52-57
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• 1983

자성체 박막을 갖는 광도파판에서 전자파의 전파를 이론적으로 조사하였다. 광도파관이 갖는 혼합모드의 전계 및 자계의 분포, 또한 그들의 위상속도를 광도파관의 기본 모드의 위상차와 자성박막의 파라데이 회전각으로 나타냈으며 파라데이 효자에 의한 위상 특성곡선의 분할에 대하여 논하였다. 그리고 흔합모드의 이론으로 모드변환 행열을 도출한 결과, 전자파의 진행거리에 따른 모드변환이 광도파관에서는 bulk 매질과는 다름을 나타내었다.