• 제목/요약/키워드: Parallel magnetic field

검색결과 230건 처리시간 0.025초

Evaluation of thermal conductivity in REBCO coated conductor

  • Yong-Ju, Hong;Sehwan, In;Hyobong, Kim;Hankil, Yeom
    • 한국초전도ㆍ저온공학회논문지
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    • 제24권4호
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    • pp.78-83
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    • 2022
  • REBCO coated conductors are widely used for HTS power application, high magnetic field magnet application, and etc. A thermal stability of the REBCO conductor is essential for the operation of HTS-based device, and thermal conductivities of the conductor are relevant parameters for modeling cryogenic heat transfer. REBCO conductors consist of a REBCO layer, copper layers for electrical stabilization and a hastelloy substrate. At cryogenic temperature, thermal conductivity of copper and silver strongly depend on the purity of the material and the intensity of the magnetic field. In this study, thermal conductivities of the laminated composite structure of REBCO conductor are evaluated by using the thermal network model and the multidimensional heat conduction analysis. As a result, the thermal network model is applicable to REBCO conductors configured in series or parallel alone and multidimensional heat conduction analysis is necessary for complex cases of series and parallel configuration.

Magnetic Susceptibility of Anisotropically Interacting Spin-Pair Systems

  • Kim, Jin-Eun
    • Bulletin of the Korean Chemical Society
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    • 제15권5호
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    • pp.347-349
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    • 1994
  • The Oguchi theory of antiferromagnetism has been modified for antiferromagnetically interacting spin-pair systems with anisotropic exchange interaction. The parallel and perpendicular susceptibilities $({\chi}_{\parallel}\;and\;{\chi}_{\perp})$ have been expressed as functions of exchange interactions $(J_z\;and\;{\gamma}=J_x/J_z)$, anisotropic molecular field parameters $({\kappa}\;and\;{\kappa}_x)$, $g_z\;and\;g_x$. In contrast to the previous theories, the parallel susceptibilities are not the same as the perpendicular susceptibilities above Neel temperature $T_N$.

Fe-B-Si 비정질 합금의 자장중 열처리 효과 (Magnetic Annealing of Amorphous Fe-B-Si Alloy)

  • 강원구;김운동;이언용;김기욱;이원재;민복기;송재성;홍진완;윤문수
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 1990년도 하계학술대회 논문집
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    • pp.236-238
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    • 1990
  • For improving magnetic properties of the amorphous Fe-B-Si alloy, we annealed 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 comparing with non-field annealed specimen. These reductions were caused by the formation of $180^{\circ}$ domains parallel to the annealing field due to the induced anisotorpy.

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Bi-2223/Ag 초전도 선재에서 임계전류와 인덱스의 자계의존성 (Magnetic field dependence of critical current and index n in a Bi-2223/Ag superconductor tape)

  • 김정호;김규태;임준형;장석헌;노연봉;주진호;최세용;나완수;홍계원
    • Progress in Superconductivity
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    • 제6권1호
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    • pp.79-83
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    • 2004
  • We fabricated Bi-2223/Ag superconductor tape with 55 filaments and estimated the magnetic field dependence of critical current (I$_{c}$) and index n (n) up to 30 T at 4.2 K. The I$_{c}$ and n were characterized as a function of external magnetic field parallel to the tape surface on increasing and decreasing field, using a 35 T hybrid magnet. The $I_{c}$ was estimated to be 325 A, and n was 32, 22, and 26 in the electric field range of $0.1 ∼1\mu$V/cm, 1∼10 $\mu$V/cm, and 0.1∼10 $\mu$V/cm, respectively, under self-field at 4.2 K. It was observed that $I_{c}$ was dependent on magnitude of magnetic field and it decreased exponentially as the field increased; in a parallel and increasing field, It was 128 A at 30 T which is approximately 40% of critical current in self-field. In addition, the $I_{c}$ was higher on decreasing field than that on increasing one. On the other hand, n did not significantly depend on field strength up to 30 T, nor varied on whether increasing or decreasing field; n value in 0.1∼1 $\mu$V/cm was 23.0$\pm$5.2 and 27.8$\pm$8.0 on increasing and decreasing field, respectively. The n value on decreasing magnetic field was slightly higher than that on increasing field. This hysteretic behavior of n was similar to that of$ I_{c}$, which is related to the trapped flux at the grain boundary.ary.

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Improved Method for Calculating Magnetic Field of Surface-Mounted Permanent Magnet Machines Accounting for Slots and Eccentric Magnet Pole

  • Zhou, Yu;Li, Huaishu;Wang, Wei;Cao, Qing;Zhou, Shi
    • Journal of Electrical Engineering and Technology
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    • 제10권3호
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    • pp.1025-1034
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    • 2015
  • This paper presented an improved analytical method for calculating the open-circuit magnetic field in the surface-mounted permanent magnet machines accounting for slots and eccentric magnet pole. Magnetic field produced by radial and parallel permanent magnet is equivalent to that produced by surface current according to equivalent surface-current method of permanent magnet. The model is divided into two types of subdomains. The field solution of each subdomain is obtained by applying the interface and boundary conditions. The magnet field produced by equivalent surface current is superposed according to superposition principle of vector potential. The investigation shows harmonic contents of radial flux density can be reduced a lot by changing eccentric distance of eccentric magnet poles compared with conventional surface-mounted permanent-magnet machines with concentric magnet poles. The FE(finite element) results confirm the validity of the analytical results with the proposed model.

병렬 안테나에 따른 플라즈마원의 균일도 연구 (Study on the Uniformity of Plasma Density at TCP Using Parallel Antennas)

  • 배근희;서상훈;장홍영
    • 한국진공학회지
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    • 제7권3호
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    • pp.273-276
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    • 1998
  • 안테나에 따른 플라즈마 밀도의 균일도 연구를 위해 병렬 안테나를 설계하고 이중 랑뮤어 탐침과 자기장 측정 탐침을 이용하여 각각의 플라즈마 밀도와 자기장의 세기를 측정 하였다. 나비형 안테나를 사용했을 때 플라즈마 밀도가 ~$2\times10^{11}(\textrmcm^{-3})$로 다른 두 안테나를 사용했을 때보다 높았으며, 전자의 온도는 2eV 이하로 동일한 조건에서의 나선형 안테나보 다 낮게 나왔다. 또 전류의 방향이 서로 다른 두 개의 안테나선이 가까이 있거나 안테나 성 분끼리 양성 결합(positive coupling)을 하는 경우에는 동력 효율(power efficiency)이 매우 낮아졌다.

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A Comprehensive Study of Interaction of Magnetic Flux Ropes Leading to Solar Eruption

  • 이시백;최광선;전홍달;김갑성
    • 천문학회보
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    • 제44권1호
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    • pp.54.1-54.1
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    • 2019
  • Solar observations often show that interaction of more than one flux rope is involved in solar eruptions. In this regard, Lau and Finn (1996) intensively studied the interaction of two flux ropes, which reside in between two parallel planes each mimicking one polarity region of the solar photosphere. However, this geometry is quite far from the real solar situation, in which all feet of flux tubes are rooted in one surface only. In this paper, we study the interaction of two flux ropes in a semi-infinite region above a plane representing the solar photosphere. Four cases of the flux rope interaction are investigated in our MHD simulation study: (1) parallel axial fields and parallel axial currents (co-helicity), (2) antiparallel axial fields and parallel axial currents (counter-helicity), (3) parallel axial fields and antiparallel axial currents (counter-helicity), and (4) antiparallel axial fields and antiparallel axial currents (co-helicity). Each case consists of four or six subcases according to the background field direction relative to the flux ropes and the relative positions of the flux rope footpoints. In our simulations, all the cases eventually show eruptive behaviors, but their degree of explosiveness and field topological evolutions are quite different. We construct artificial emission measure maps based on the simulations and compare them with images of CME observations, which provides us with information on what field configurations may generate certain eruption features.

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Statistical Comparison of ULF wave Power of Magnetic field between the upstream solar wind and the magnetosheath: THEMIS observations

  • 박미영;김희정;이대영;김경찬
    • 천문학회보
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    • 제37권1호
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    • pp.96.2-96.2
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    • 2012
  • We statistically examined ULF Pc 3-5 wave power in the regions of undisturbed upstream solar wind, quasi-parallel shock (and foreshock), quasi-perpendicular shock, and the magnetosheath to understand how and to what extent the wave power changes as the solar wind propagates to the magnetosheath. For this study, we used the magnetic field data from the THEMIS spacecraft and Wind (as shifted to the bow shock nose) for May-November in 2008 and 2009. The statistical results show that, in the case of the Pc5 wave power, the sheath power is roughly proportional to the upstream power for both quasi-parallel (and foreshock) and quasi-perpendicular shock regions. Also we identified undisturbed upstream condition from WIND as being well away from foreshock region, and found that the sheath power can be larger for quasi-parallel shock region by a factor of 5-15 than for quasi-perpendicular shock region. In the cases of Pc 3 and Pc4 waves, we found the higher sheath power when associated with the foreshock than with the quasi-perpendicular shock region.

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Study on the Magnetic Characteristics of Anisotropic SmCo7-type Alloys Synthesized by High-energy Surfactant-assisted Ball Milling

  • Yu, N.J.;Zhang, P.Y.;Shi, Y.J.;Pan, M.X.;Zhang, S.Y.;Ge, H.L.;Lu, Y.C.
    • Journal of Magnetics
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    • 제19권4호
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    • pp.340-344
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    • 2014
  • An effective process was employed for synthesizing anisotropic magnetic $SmCo_7$-type alloy flakes with high coercivity, which is highly desirable for many applications. The highest coercivity of 16.3 kOe corresponds to a typical flake thickness of 200 nm for the 3-h ball-milled sample. The anisotropy field was calculated by measuring the parallel and perpendicular directions to the easy magnetization direction of the powders. The anisotropy field decreased with the increase of the ball milling time, thus indicating that the decrease of coercivity was mainly caused by the reduction of the anisotropy field. Microstructure analysis indicated that the morphology, grain size, and anisotropy field of these samples have a great influence on the magnetic properties.