• 천문학회보
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• 제36권1호
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• pp.85.1-85.1
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• 2011

Recently, Faraday rotation measure (RM) at high Galactic latitude has been investigated, partly to explore the Galactic magnetic fields and partly to study the extragalactic magnetic fields. The Galactic contribution to RM comes from the global component as well as the turbulent component. So far the turbulent field was used to be analytically modeled with a Kolmogorov-type power spectrum. Here, we present the initial results of the work where the turbulent field is modeled using data of MHD turbulence simulations. Our work is intended to be applied to simulations of RM surveys with LOFAR, ASKAP, MeerKAT, and SKA.

• 한국자기학회지
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• 제8권2호
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• pp.74-78
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• 1998

LPE법으로 양질의 단결정 Bi, Gd:YIG 막을 GCMZGG 기판상에 성장시켜 자기, 광자기 및 센서특성을 조사했다. 제조한 막은 히스테리시스가 거의 없는 직선성이 양호한 연자성 특성을 나타냈고, 상온에서의 포화 Faraday 회전각은 45$^{\circ}$, 포화자장은 약 1.1kOe, 베르데 상수는 5.6$^{\circ}$/(cm,Oe0이었으며, 베르데상수의 온도의존성은 $0^{\circ}C$-10$0^{\circ}C$에서 약0.0056$^{\circ}$/(Oe, cm, $^{\circ}C$)로 우수한 특성을 나타냈다. 또한, 제조한 막을 사용하여 센서특성을 특정한 결과 전류의 세기가 3A-300A에서 양호한 적선성이 얻었졌다.

• 조명전기설비학회논문지
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• 제17권6호
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• pp.47-53
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• 2003

본 논문은 자기광학효과에 의한 초고압 전력설비에서의 광전류 센서의 특성에 대한 기초 연구를 하였다. 광원은 He-Ne laser(633[nm])를 사용하고, 수신부는 PIN-Photodiode를 사용하였다. Faraday 효과에 의한 편광면의 회전각은 도체에 인가된 전류에 비례하므로 광섬유를 도체 주위에 감아서 센싱부를 구성하였다. 광섬유센서를 통과한 광신호를 입력편광에 대하여 $\theta$방향으로 정렬된 검광자를 통과시켜 그 회 각을 분석하여 l00[A] 에서 1000[A] 까지의 광 CT 동작특성과 60[Hz] 교류전류측정을 하였다. 측정 결과에서는 전류에 따른 출력 신호가 선형적으로 증가함을 알 수 있었고 파이버의 권수에 따른 출력차이를 통해 파이버의 권수가 많을수록 강도가 커진다는 것을 알 수 있었다. 또한 자장과 감긴 파이버 사이의 매질에 따라 출력의 차이뿐만 아니라 선형성까지도 차이가 난다는 것을 알 수 있었다. 기준값과 광전류 센서의 출력 강도와의 오차율을 구했을 때 약 $\pm$7% 이하의 오차가 나왔고 이는 매질과 권수에 따라 그 오차율이 점점 나아질 수 있다는 것을 확인 시켜주었다.

• 한국통신학회논문지
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• 제19권3호
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• pp.573-581
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• 1994

Feed horn polarizer나 F.R.R.S(Fraday Rotation Rotary Switch)에 비해 소형이고 GaAs MESFET소자 스위칭으로 좌수와 우수 원형편파의 선택적 수신이 가능한 이중편파 마이크로스트립 안테나를 설계하였다. 원형편과 마이크로스트립 안테나의 공진 주파수, 입력 임피던스, 빔 패턴 등은 FDTD 방법을 이용하여 정확하게 계산하였으며, 급전 회로의 GaAs MESFET 증폭기 스위칭 회로가 ON 상태일 경우의 증폭기 이득을 포함한 안테나 이득은 16.6dB 이고, OFF 상태일 경우의 격리 특성은 -24dB로 나타남을 실험으로 확인하였다. 또한, 제작된 이중편과 마이크로스트립 안테나의 3dB 이하 축비는 11.813GHz에서 30 이하로 나타났다.

• 천문학회지
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• 제37권5호
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• pp.501-507
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• 2004

The uniquely large dimensions of Giant radio galaxies (GRGs) make it possible to probe for stringent limits on total energy content, Faraday rotation, Alfven speeds, particle transport and radiation loss times. All of these quantities are more stringently limited or specified for GRG's than in more 'normal' FRII radio sources. I discuss how both global and detailed analyses of GRG's lead to constraints on the CR electron acceleration mechanisms in GRG's and by extension in all FRII radio sources. The properties of GRG's appear to rule out large scale Fermi-type shock acceleration. The plasma parameters in these systems set up conditions that are favorable for magnetic reconnection, or some other very efficient process of conversion of magnetic to particle energy. We conclude that whatever mechanism operates in GRG's is probably the primary extragalactic CR acceleration mechanism in the Universe.

• 천문학회지
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• 제37권5호
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• pp.355-359
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• 2004

Differential Faraday Rotation measurements between the images of same background source, of multiply-imaged gravitational lens systems can be effectively used to provide a valuable probe to establish the existence of large-scale ordered magnetic fields in lensing galaxies as well as galaxy clusters. Estimates of the magnetic field in lens galaxies, based on the radio polarization measurements do not appear to show any clear evidence for evolution with redhsift of the coherent large scale magnetic field between redshift of 0.9 and the present epoch. However, our method clearly establishes the presence of coherent large scale magnetic field in giant ellitpical galaxies.

• 한국고분자학회:학술대회논문집
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• 한국고분자학회 2006년도 IUPAC International Symposium on Advanced Polymers for Emerging Technologies
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• pp.23-24
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• 2006

Magnetic and magneto-optical properties of regioregular (>99%) poly(3-dodecylthiopenes are investigated. Faraday rotation of spin-coated films show extremely large Verdet constants, falling strongly with decreasing regioregularity. EPR spectroscopy at room temperature shows the presence of about 1 spin/190 monomers, indicative of delocalisation beyond a single polymer chain. SQUID measurements on the polymer give an effective magnetic moment of about 48900 mB, corrsponding to a S-value of 25.000. The Weiss-constant is 1.33 K indicating ferromagnetic coupling. Our experimental results show that organic polymer magnets can be prepared. Large MO effects allow the use of these materials in all-organic MO-sensors and devices.

• 천문학회보
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• 제39권2호
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• pp.37-37
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• 2014

Magnetic fields appear to be ubiquitous in astrophysical environments. The existence of magnetic fields in the large-scale structure of the universe has been established through observations of Faraday rotation and synchrotron emission, as well as through recent gamma-ray observations. Yet, the nature and origin of the magnetic fields remains controversial and largely unknown. In this talk, I briefly summarize recent developments in our understanding of the nature and origin of magnetic fields. I also describe a plausible scenario for the origin of the magnetic fields; seed fields were created in the early universe and subsequently amplified during the formation of the large-scale structure of the universe. I then discuss the prospect of observation of magnetic fields in the large-scale structure of the universe.

• International Journal of Precision Engineering and Manufacturing
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• 제3권1호
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• pp.20-25
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• 2002

Electrical damages to critical parts in rotating machinery have caused many machinery failures and hours of costly downtime. The problem of shaft currents generated in non-electrical machines has puzzled both users and manufacturers of these machines. The main solution for preventing electromagnetic 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 electromagnetic shaft currents is needed. In this paper, the self excitation theory was developed far a simple model, an 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 be 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 a way to detect small instabilities or natural frequency locations by monitoring shaft currents.

• 천문학회지
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• 제47권1호
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• pp.15-39
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• 2014

Polarization is a basic property of light and is fundamentally linked to the internal geometry of a source of radiation. Polarimetry complements photometric, spectroscopic, and imaging analyses of sources of radiation and has made possible multiple astrophysical discoveries. In this article I review (i) the physical basics of polarization: electromagnetic waves, photons, and parameterizations; (ii) astrophysical sources of polarization: scattering, synchrotron radiation, active media, and the Zeeman, Goldreich-Kylafis, and Hanle effects, as well as interactions between polarization and matter (like birefringence, Faraday rotation, or the Chandrasekhar-Fermi effect); (iii) observational methodology: on-sky geometry, influence of atmosphere and instrumental polarization, polarization statistics, and observational techniques for radio, optical, and $X/{\gamma}$ wavelengths; and (iv) science cases for astronomical polarimetry: solar and stellar physics, planetary system bodies, interstellar matter, astrobiology, astronomical masers, pulsars, galactic magnetic fields, gamma-ray bursts, active galactic nuclei, and cosmic microwave background radiation.