• 천문학회보
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• 제36권2호
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• pp.108.1-108.1
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• 2011

Turbulence is ubiquitous in astrophysical fluids such as the interstellar medium(ISM) and the intracluster medium(ICM). There are many driving mechanisms which can inject energy into the fluid in variety driving scales, But the plausible driving scale of ISM/ICM turbulence are yet unknown. Therefore, understanding different statistical properties between turbulence with single driving scale and turbulence with double driving scale is required. In this work, we performed 3-dimensional isothermal compressible, magnetohydrodynamic(MHD) turbulence simulations. We drive turbulence in the Fourier space in two ranges, 2

• 혜화의학회지
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• 제25권1호
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• pp.53-62
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• 2016

Objectives : The purpose of this study was to report a case of a patient efficacy of electromagnetic acupuncture using Whata 153 in facial nerve palsy in Herpes zoster oticus. Methods : We treated the patient with magnetic acupuncture combined with electro-acupuncture. Acupuncture points were at the face (BL2, GB14, TE23, ST4, ST6, ST3). All the acupuncture points were stimulated with magnetic field and 4 of them were combined with electro-acupuncture. Results & Conclusions : The improvement of facial movement and symptom was evaluated by Yanagihara grading system(Y-system), House-Brackmann scale(HB scale) and Sunnybrook facial grading system(SFGS). After treatment, all of the scales(Y-system, HB scale and SFGS) and symptom of the patient were improved. From the above results, we suggest that magnetic acupuncture and electro-acupuncture might be effective on facial nerve palsy in Herpes zoster oticus.

• 천문학회지
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• 제37권5호
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• pp.533-541
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• 2004

The origin of magnetic fields in the universe remains an outstanding problem in cosmology. We propose that these fields are produced by shocks during the large-scale structure formation. We discuss the mechanism of the field generation via the counter-streaming (Weibel) instability. We also show that these Weibel-generated fields are long-lived and weakly coupled to dissipation. Subsequent field amplification by the intra-cluster turbulence may also take place, thus maintaining the magnetic energy density close to equipartition.

• 천문학회보
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• 제35권2호
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• pp.74.2-74.2
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• 2010

We investigate driven magnetohydrodynamic (MHD) turbulence by including the effects of expansion and collapse of background medium. The main goal is to quantify the evolution and saturation of strength and characteristic lengths of magnetic fields in expanding and collapsing media. Our findings are as follows. First, with expansion and collapse of background medium, the magnetic energy density per comoving volume does not saturate; either it keeps decreasing or increasing with time. The magnetic energy density relative to the kinetic energy density strongly depends on the expanding or collapsing rate. Second, at scales close to the energy injection (or driving) scale, the slope of magnetic field power spectrum shallows with expansion but steepens with collapse. Third, various characteristic lengths, relative to the energy injection scale, decrease with expansion but increase with collapse. We discuss the astrophysical implications of our findings.

• 천문학회지
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• 제29권2호
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• pp.83-91
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• 1996

We present a model that rotating primordial blackholes(PBHs) produced at the end of inflation generate the random, non-oriented primordial magnetic field. PBHs are copiously produced as the Universe completes the cosmic phase transition via bubble nucleation and tunneling processes in the extended inflation hypothesis. The PBHs produced acquire angular momentum through the mutual tidal gravitational interaction. For PBHs of mass less than 1013g, one can show that the evaporation (photon) luminosity of PBHs exceeds the Eddington limit. Thus throughout the lifetime of the rotating PBH, radiation flow from the central blackhole along the Kerr-geodesic exerts torque to ambient plasma. In the process similar to the Bierman's battery mechanism electron current reaching up to the horizon scale is induced. For PBHs of Grand Unified Theories extended inflation with the symmetry breaking temperature of $T_{GUT}\;\~\;10^{10}$ GeV, which evaporate near decoupling, we find that they generate random, non-oriented magnetic fields of $\~10^{-11}G$ on the last-scattering surface on (the present comoving) scales of $\~O(10)Mpc$.

• Structural Engineering and Mechanics
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• 제69권2호
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• pp.145-153
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• 2019

Modified couple stress formulation and first order shear deformation theory are used for magneto-electro-elastic bending analysis of three-layered curved size-dependent beam subjected to mechanical, magnetic and electrical loads. The governing equations are derived using a displacement field including radial and transverse displacements of middle surface and a rotation component. Size dependency is accounted based on modified couple stress theory by employing a small scale parameter. The numerical results are presented to study the influence of small scale parameter, initial electric and magnetic potentials and opening angle on the magneto-electro-elastic bending results of curved micro beam.

• 천문학회보
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• 제36권2호
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• pp.96.2-96.2
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• 2011

We analyzed transient Ca II brightening associated with small-scale canceling magnetic features in the quiet Sun near disk center using Ca II H and NaD1 filter images of the SOT/Hinode. We found that in most Ca II brightening related to CMFs the Ca II intensity peaks after magnetic flux cancellation proceeds. Moreover, brightening tend to appear as pairs of bright points of similar size and similar brightness overlying magnetic bipoles. These results imply that magnetic reconnection taking place in the chromosphere or above may be in charge of CMFs.

• 한국정밀공학회지
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• 제22권8호
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• pp.42-49
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• 2005

Our purpose is to develop a precision magnetic displacement sensor that has sub-micron resolution and small size probe. To achieve this, we first have tried to establish mathematical models of a magnetic sensor in this paper. The inductance model that presents basic measuring principle of a magnetic sensor is based on equivalent magnetic circuit method. Especially we have concentrated on modeling of magnetic flux leakage and magnetic flux fringing. The induced model is verified by experimental results. The model, including the magnetic flux leakage and flux fringing effects, is in good agreement with the experimental data. Subsequently, based on the augmented model, we will design magnetic sensor probe in order to obtain high performances and to scale down the probe.

• 한국산학기술학회논문지
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• 제16권11호
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• pp.7367-7376
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• 2015

본 연구는 경혈점에 적용한 자장요법이 여고생의 월경통에 미치는 효과를 파악하여 여고생들에게 효율적인 자가 간호 중재로써의 활용가능성을 검증하고자 시도된 무작위 할당 대조군 전후설계이다. 자료수집기간은 2006년 3월부터 4월까지로, 보건실을 방문한 여고생에게 실험 전, 설문지에 통증척도인 도표 평정 척도(Grapic Rating Scale, GRS)와 분만어휘 평정척도(Adjective Labor Pain Rating Scale, ALPRS)를 작성하게 한 뒤 각 군에게 직경 12mm, 두께 3mm의 원형 자석에 800~1200Gauss의 자력이 있는 의료용 자석을 3시간동안 적용하였다. 설문지는 각각 자석 적용 직후 3시간과 제거 후 3시간에 설문지인 GRS와 ALPRS를 작성하게 하였다. 연구결과 경혈점에 자장요법을 적용한 실험군은 적용하지 않은 대조군보다 월경통 GRS와 ALPRS가 유의하게 감소하였다. 이상의 결과로 경혈점에 적용한 자장요법이 여고생의 월경통에 통증경감에 효과가 있는 것으로 확인되었다. 따라서 비약물요법으로서의 월경통 완화를 위한 간호중재법으로 활용할 것을 기대한다. 또한 본 연구에서 ALPRS가 월경통에 대해 타당성이 제시되었으므로 추후 연구를 통해 ALPRS의 타당도 검증을 위한 반복 연구가 필요하다. 여고생들의 월경통 경감을 위한 보완대체요법으로 적용하게 될 것을 제언한다.

• KEPCO Journal on Electric Power and Energy
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• 제5권3호
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• pp.229-233
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• 2019

Large-scale High Temperature Superconducting (HTS) wind power generators suffer from high electromagnetic force and high torque due to their high current density and low rotational speed. Therefore, the torque and Lorentz force of HTS wind power generators should be carefully investigated. In this paper, we proposed a Performance Evaluation System (PES) to physically test the structural stability of HTS coils with high torque before fabricating the generator. The PES is composed of the part of a pole-pair of the HTS generator for estimating the characteristic of the HTS coil. The 10 MW HTS generator and PES were analyzed using a 3D finite element method software. The performance of the HTS coil was evaluated by comparing the magnetic field distributions, the output power, and torque values of the 10 MW HTS generator and the PES. The magnetic flux densities, output power, and torque values of the HTS coils in the PES were the same as a pole-pair of the 10 MW HTS generator. Therefore, the PES-based evaluation method proposed in this paper can be used to estimate the critical characteristics of the HTS generator under high magnetic field and high torque before manufacturing the HTS wind turbines. These results will be used effectively to research and manufacture large-scale HTS wind turbine generators.