• Advances in materials Research
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• 제12권3호
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• pp.243-261
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• 2023

This study aims to analyze the mechanical buckling behavior of a single-walled carbon nanotube (SWCNT) integrated with a one-parameter elastic medium and modeled as a Kerr-type foundation under a longitudinal magnetic field. The structure is considered homogeneous and therefore modeled utilizing the nonlocal first shear deformation theory (NL-FSDT). This model targets thin and thick structures and considers the effect of the transverse shear deformation and small-scale effect. The Kerr model describes the elastic matrix, which takes into account the transverse shear strain and normal pressure. Using the nonlocal elastic theory and taking into account the Lorentz magnetic force acquired from Maxwell relations, the stability equation for buckling analysis of a simply supported SWCNT under a longitudinal magnetic field is obtained. Moreover, the mechanical buckling load behavior with respect to the impacts of the magnetic field and the elastic medium parameters considering the nonlocal parameter, the rotary inertia, and transverse shear deformation was examined and discussed. This study showed useful results that can be used for the design of nano-transistors that use the buckling properties of single-wall carbon nanotubes(CNTs) due to the creation of the magnetic field effect.

• 한국자기학회지
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• 제8권1호
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• pp.13-20
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• 1998

초미세결정립과 비정질을 동시에 포함하는 리본형 Fe73.9Cu1.0Nb3.5Si14.0B7.6 합금을 자기장 중 열처리한 시편의 결정？적 특성 및 고주파 연기자 특성을 인가 자기장과 열처리 온도에 따라하여 조사아였다. 제조된 리본의 표면에 석출된 Fe-Si 초미세결정립은 (400) 우선방위를 나타내는 동시에 리본길이방향으로 [011] 결정측이 형성되어 있음을 확인하엿다. 자기장을 인가하지 않거나 길이방향으로 자기장을 인가하여 열처리할 때 45$0^{\circ}C$에소 Fe-Si 초미세결정립이 석출되다, 폭방향의 자기장을 인가한 경우 초미세결정립의 석출은 지연되어 55$0^{\circ}C$에서 나타남을 확인하였다. 길이방향으로 자기장을 인가할 때 시편의 결정화 정도는 외부 자기장을 인가하지 않은 경우에 비해 조금 증가하였다. 그러나, 시편의 각도를 기울여 측정된 X-선 회절패턴으로부터 시편내부는 표면과 달리 결정화가 진행되고 있음을 확인하였다. 열처리한 시편의 포화자기유도는 1.3T로 비슷하였다. 열처리전 리본의 보자력의 크기는 1.06A/츠이었으나, 열처리한 시편은 열처리 온도가 40$0^{\circ}C$에서 55$0^{\circ}C$로 증가함에 따라 0.56A/cm에서 0.1A/cm로 감소하였다. 폭방향의 자기장을 인가한 경우 각형비는 자기장을 인가하지 않거나 길이방향으로 자기장을 인가하여 열처리한 시편의 각형비보다 작았다.

• 한국의학물리학회:학술대회논문집
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• 한국의학물리학회 2002년도 Proceedings
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• pp.109-112
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• 2002

Using Monte Carlo calculations the effects of longitudinal magnetic fields on the beam profiles produced by clinical electron beam were studied. The Monte Carlo calculations were performed using the EGS4 code system modified to account for external magnetic fields. The beam profiles for a 6 MeV electron beam with longitudinal magnetic fields of 0.5-3.0 T were calculated. As a result of these calculations we found that the penumbra widths can be reduced with increased magnetic fields. This means that the electron therapy benefits from the external magnetic fields.

• 대한기계학회논문집A
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• 제28권7호
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• pp.923-929
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• 2004

A magnetostrictive sensor is a sensor measuring elastic waves. Because of its unique non-contact measurement feature, the sensor receives more attentions in recent years. These sensors have been mainly used to measure longitudinal and torsional waves in ferromagnetic waveguides, but there increases an interest in using the sensor for flexural wave measurement. Since the performance of the sensor is strongly influenced by the applied bias magnetic field distribution, the design of the bias magnetic system providing the desired magnetic field is critical. The motivation of this investigation is to design a bias magnetic system consisting of electromagnets and yokes and the specific objective is to formulate the design problem as a bias yoke topology optimization. For the formulation, we employ linear magnetic behavior and examine the optimized results for electromagnets located at various locations. After completing the design optimization, we fabricate the prototype of the proposed bias magnetic system, and test its performance through flexural wave measurements.

• 대한전기학회논문지
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• 제40권1호
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• pp.67-72
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• 1991

For improving the magnetic properties of the amorphous Fe-B-Si alloy, we annealed the sample in a magnetic field oriented in the plane of the ribbon longitudinal to its long axis. By field annealing, coercive force and total core loss are reduced from 0.04 Oe to 0.02 Oe, and from 0.25 watt/kg to 0.15 watt/kg respectively in comparsion with non-field annealed specimen. These reductions were caused by the formation of 180 dcmain wall parallel to the annealing field due to the induced anisotropy.

• 대한전기학회:학술대회논문집
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• 대한전기학회 1996년도 하계학술대회 논문집 A
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• pp.44-46
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• 1996

Superconducting cable is using by bundling and twisting with many strands for large current capacity. As a result of the twisting, the magnetic field whose direction is parallel to a sound axis by the transport current of themselves is produced in the cable. Not only the externally exposed longitudinal field but also longitudinal component of self field make a influence on a.c loss and a.c quench current degradation. In this paper, we calculate the saturated region flowing with the critical current density in a strand in case of various twist pitch, transport current and external longitudinal field.

• Journal of Astronomy and Space Sciences
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• 제21권4호
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• pp.303-314
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• 2004

In this paper we report some properties of inner magnetospheric structure inferred from the T01_s code, one of the latest magnetospheric models by Tsyganenko. We have constructed three average storms representing moderate, strong, and severe intensity storms using 95 actual storms. The three storms are then modelled by the T01_s code to examine differences in magnetic structure among them. We find that the magnetic structure of intense storms is strikingly different from the normal structure. First, when the storm intensity is large, the field lines anchored at dayside longitudinal sectors become warped tailward to align to the solar wind direction. This is particularly so for the field lines anchored at the longitudinal sectors from postnoon through dusk. Also while for the moderate storm the equatorial magnetic field near geosynchronous altitude is found to be weakest near midnight sector, this depression region expands into even late afternoon sector during the severe storm. Accordingly the field line curvature radius at the equator in the premidnight geosynchronous region becomes unusually small, reaching down to a value less than 500 km. We attribute this strong depression and the dawn-dusk asymmetry to the combined effect from the enhanced tail current and the westward expansion/rotation of the partial ring current.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제44회 동계 정기학술대회 초록집
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• pp.394-394
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• 2013

The spin-orbit interaction has received great attention in the field of spintronics, because of its property and applicability. For instance, the spin-orbit interaction induces spin precession which is the key element of spin transistor proposed by Datta and Das, since frequency of precession can be controlled by electric field. The spin-orbit interaction is classified according to its origin, Dresselhaus and Rashba spin-orbit interaction. In particular, the Rashba spin-orbit interaction is induced by inversion asymmetry of quantum well structure and the slope of conduction band represents the strength of Rashba spin-orbit interaction. The strength of spin-orbit interaction is experimentally obtained from the Shubnikov de Hass (SdH) oscillation. The SdH oscillation is resistance change of channel for perpendicular magnetic field as a result of Zeeman spin splitting of Landau level, quantization of cyclotron motion by applied magnetic field. The frequency of oscillation is different for spin up and down due to the Rashba spin-orbit interaction. Consequently, the SdH oscillation shows the beat patterns. In many research studies, the spin-orbit interaction was treated as a tool for electrical manipulation of spin. On the other hands, it can be considered that the Rashba field, effective magnetic field induced by Rashba effect, may interact with external magnetic field. In order to investigate this issue, we utilized InAs quantum well layer, sandwiched by InGaAs/InAlAs as cladding layer. Then, the SdH oscillation was observed with tilted magnetic field in y-z plane. The y-component (longitudinal term) of applied magnetic field will interact with the Rashba field and the z-component (perpendicular term) will induce the Zeeman effect. As a result, the strength of spin-orbit interaction was increased (decreased), when applied magnetic field is parallel (anti-parallel) to the Rashba field. We found a possibility to control the spin precession with magnetic field.

• 한국초전도학회:학술대회논문집
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• 한국초전도학회 2000년도 High Temperature Superconductivity Vol.X
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• pp.21-21
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• 2000

The Josephson Plasma resonance in single crystalling Bi2Sr2CaCu2O8 has been investigated at a microwave frequency of 35 GHz in a cavity resonator. A sharp resonance is observed in a perpendicular oscillating magnetic field. The former is independent of the sample dimension, shile the latter shift to higher field as the sample size L is reduced, and it disappears when L becomes smaller than the critical length. The longitudinal plasma mode is a Nambu-Goldston mode in a superconductor, the experimental distinction between the longitudinal and the transverse mode leads to the conclusion that the existence of the Nambu-Goldston mod as predicted by Anderson was experimentally confirmed by direct observation of the Josephson plasma resonance with longitudinal excitations. The finite gap found in Josephson plasma resonance also provides a direct proof of the Anderson-Higgs mechanism within the context of the spontaneously broken phase symmetry of the Gauge-field theory in a superconductor.

• 한국의학물리학회지:의학물리
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• 제14권1호
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• pp.1-7
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• 2003

본 연구에서는 팬텀에 인가된 강한 자기장에서 전자선에 대한 선량분포 계산을 위하여 EGS4 제어코드를 개발하였다. 이를 위하여 먼저 자기장에서 전자의 운동을 고찰하고 전자의 방향변화에 관한 수학적 결과를 EGS4 제어코드에 삽입하였다. 개발된 코드를 이용하여 6 MeV 전자선에 대하여 세로자기장 1-3T가 인가된 물팬텀 속에서 팬슬빔 전자들의 경로를 계산하였고 0.6-1 T가 인가된 물팬텀 속에서 직경 1cm의 조사면의 깊이선량율과 빔측면도를 계산하였다. 전자의 경로추적 계산결과 3 T의 자기장에서 전자들의 측면변위가 현저히 감소하는 것으로 나타났다. 직경 1 cm 전자선에 대한 깊이선량율은 비정근처에서 자기장의 세기에 따라 미소한 증가를 보였으며, 반음영은 1 T에서 약 0.15 cm 감소가 나타났다. 선량분포의 변화에 관한 계산결과들은 모두 이론적 해석이 가능하였으며 이로부터 본 계산코드의 신뢰성을 평가할 수 있었다.