• 제목/요약/키워드: Strong magnetic field

검색결과 254건 처리시간 0.024초

Magnetic Field Analysis of the Electrode Arc Furnace in Steel Making Foundries

  • Kim, C.W.;Im, J.I.
    • Journal of Magnetics
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    • 제8권2호
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    • pp.79-84
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    • 2003
  • Finite element analysis showed that strong magnetic fields were distributed around the arc furnace where the strongest magnetic fields were generated around the three phase cables. The second and third strongest fields near the arc furnace were found to be generated around the electrodes and the mast-arms, respectively. The generated field intensities were greatly influenced by the mast arm structure of the arc furnace as well as the phase differences and operation currents of the supplied power, Magnetic field decay patterns around the arc furnace could be smoothly fitted by this equation of exponential formula, H=H$0_$+Ae$^{\frac{r}{t}}$. These results revealed that magnetic field intensities around the arc furnace could be estimated at any 3-dimensional position using finite element method (FEM).

Dependence of Alternating Magnetic Field Intensity on Proliferation Rate of Human Breast Cancer Cell

  • Park, Hyeji;Lee, Hyun Sook;Hwang, Do Guwn
    • Journal of Magnetics
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    • 제20권3호
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    • pp.290-294
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    • 2015
  • To investigate the effects of alternating magnetic field intensity and stimulation time on the proliferation of human breast cancer cells (BT-20), we cultured the cells under a magnetic field with a saw tooth waveform of 2 kHz. The field intensities varied from 3 to 7 mT, and the stimulation time varied from 24 to 72 hours. Cell proliferation decreased dramatically to 40% during magnetic stimulation for 72 hours at 5 mT. However, the cells were not affected by a strong magnetic field of 7 mT. The p-values obtained using statistical package for social science software were below 0.05 for 5-7 mT. This means that the results have statistical significance. However, it is difficult to explain our results based on the physiology of cell membranes, which have various ionic flows at ion channels.

Magnetic Property of Oxide with the Perovskite Structure, $A_2Fe(III)BO_6$ (A = Ca, Sr, Ba and B = Sb, Bi)

  • 이성옥;조태연;변송호
    • Bulletin of the Korean Chemical Society
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    • 제18권1호
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    • pp.91-97
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    • 1997
  • In the course of magnetic study on several perovskite-type oxides, A2Fe(Ⅲ)BO6 (A = Ca, Sr, Ba and B = Sb, Bi), we have observed a strong irreversibility in their dc-magnetizations. When the structural data and the Mossbauer spectra are considered, such an irreversibility is to be associated with some competitions between the nearest-neighbors (nn) and the next-nearest-neighbors (nnn) in their magnetic sublattices. Particularly, the Mossbauer spectra indicate that Sr2FeBiO6 of cubic perovskite-structure is apparently well ordered crystalline compound. Nontheless this antiferromagnet shows a magnetic property which resembles that of a spin-glass. The strong history dependence is observed below 91 K and the irreversible magnetic behavior is also observed from the measurement of hysteresis loops at 10 K after zero-field-cooled (zfc) and field-cooled (fc) processes. Considering the nn and the nnn superexchanges of almost same order in ordered perovskite, it is proposed that there exists a competition and cancellation of antiferromagnetic and ferromagnetic superexchange between the nearest-neighbors and the next-nearest-neighbors, thus introducing a certain degree of frustration.

A Study of Kinetic Effect on Relativistic Shock using 3D PIC simulation

  • 최은진;민경욱;최청림
    • 천문학회보
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    • 제37권1호
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    • pp.67.1-67.1
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    • 2012
  • Shocks are evolved when the relativistic jets in active galactic nuclei (AGNs), black hole binaries, supernova remnants (SNR) and gamma-ray bursts (GRBs) interact with the surrounding medium. The high energy particles are believed to be accelerated by the diffusive shock acceleration and the strong magnetic field is generated by Weibel instability in the shock. When ultrarelativistic electrons with strong magnetic field cool by the synchrotron emission, the radiation is observed in gamma-ray burst and the near-equipartitioned magnetic field in the external shock delays the afterglow emission. In this paper, we performed the 3D particle-in-cell (PIC) simulations to understand the characteristics of these relativistic shock and particle acceleration. Forward and reverse shocks are shaped while the unmagnetized injecting jet interacts with the unmagnetized ambient medium. Both upstream and downstream become thermalized and the particle accelerations are shown in each transition region of the shock structures.

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CONVECTION IN A HORIZONTAL POROUS LAYER UNDERLYING A FLUID LAYER IN THE PRESENCE OF NON LINEAR MAGNETIC FIELD ON BOTH LAYERS

  • Bukhari, Abdul-Fattah K.;Abdullah, Abdullah A.
    • Journal of the Korean Society for Industrial and Applied Mathematics
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    • 제11권1호
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    • pp.1-11
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    • 2007
  • A linear stability analysis applied to a system consist of a horizontal fluid layer overlying a layer of a porous medium affected by a vertical magnetic field on both layers. Flow in porous medium is assumed to be governed by Darcy's law. The Beavers-Joseph condition is applied at the interface between the two layers. Numerical solutions are obtained for stationary convection case using the method of expansion of Chebyshev polynomials. It is found that the spectral method has a strong ability to solve the multilayered problem and that the magnetic field has a strong effect in his model.

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The Design of a Device for the Generation of a Strong Magnetic Field in an Air Gap using Permanent Magnets

  • Zezulka, Vaclav;Straka, Pavel
    • Journal of Magnetics
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    • 제22권2호
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    • pp.250-256
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    • 2017
  • The article presents the principle of a relatively small device that makes it possible to generate a strong magnetic field in an air gap without electrical energy consumption. It describes the implemented design of this device, the method of the assembly of opposing linear arrays from two NdFeB magnet layers, its advantages, the possible ways of increasing the parameters further and its application in various areas.

Magnetic Reconnection and the Substorm

  • Min, Kyoung-Wook
    • 천문학논총
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    • 제2권1호
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    • pp.13-20
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    • 1985
  • Magnetic reconnect ion is studied numerically by means of a two dimensional MHD code. The initial magnetic field configuration is the two-dimensional dipole field, and the simulation model involves magnetic reconnect ion driven by the magnetized plasma flow. Strong plasma jetting, plasmoid formation and its fast ejection are observed in the downstream region. The dependence of reconnection rate on the incoming energy flux is found to be very sensitive, while the magnitude of the resistivity does not influence much on the reconnection rate. The simulation results are discussed in the context of the geomagnetic substorm.

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COLLINEARITY AND SPIN FREEZING

  • Vincze, I.;Kemeny, T.
    • 한국자기학회지
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    • 제5권5호
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    • pp.343-350
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    • 1995
  • An overview will be given on recent Mossbauer and magnetization investigation of the applied field dependence of the magnetic properties of typical systems without strong magnetic anisotropy and showing the absence of magnetic saturation in high fields (including iron-rich spin glass (amorphous $Fe_{93}Zr_{7}$, soft ferromagnets (amorphous $Fe_{88}Zr_{12}$, $Fe_{70}Ni_{20}Zr_{10}$ and $Fe_{88}B_{12}$) and pure Fe). The results emphasize that shape anisotropy due to surface irregularities causes misalignment between the magnetization and the applied field in the otherwise collinear magnetic structure.

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자장하에서 성장한 CoCr박막의 자기적 특성 및 미세구조에 관한 연구 (A Study on the Magnetic Properties and Microstructure of CoCr Thin Films Growing under Magnetic Field)

  • 이유기;장평우;이택동;이계원
    • 한국재료학회지
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    • 제4권5호
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    • pp.581-589
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    • 1994
  • 인가자장하에서 성장한 $Co_{83}Cr_{17}$ 박막의 자가적 특성 및 미세구조를 조사하였고, 인가자장을 가하지 않은 경우에 성장한 박막과 그 특성 및 미세구조를 비교 하였다. 인가자장은 박막의 포화자화와 수평방향 보자력에는 아무런 영향을 주지 못하였지만, 수직보자력과 유효수직이방성자계를 감소시켰다. 또한 천이층의 결정립경과 두께는 인가자장에 의해 영향을 받지 않았지만, C축배향성은 약간 악화되었다. 또한 TEM사진은 인가자장의 유무에 관계없이 박막의 두께가 두꺼워질수록 (002)방위의 결정립 등이 우선적으로 성장함을 보여주었다.

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Aqueous Processing of Textured Silicon Nitride Ceramics by Slip Casting in a Strong Magnetic Field

  • Zhu, Xinwen;Uchikoshi, Tetsuo;Sakka, Yoshio
    • 한국분말야금학회:학술대회논문집
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    • 한국분말야금학회 2006년도 Extended Abstracts of 2006 POWDER METALLURGY World Congress Part2
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    • pp.866-867
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    • 2006
  • This work will report a highly textured ${\beta}-Si_3N_4$ ceramic by aqueous slip casting in a magnetic field and subsequent pressureless sintering, Effects of the sintering aids, polymer dispersant, pH and stirring time on the stability of the $Si_3N_4$ slurries were studied. The textured ${\beta}-Si_3N_4$ with 97 % relative density could be obtained by slip casting in a magnetic field of 12 T and subsequent sintering at $1800^{\circ}C$ for 1 h. The textured microstructure is featured by the alignment of c-axis of ${\beta}-Si_3N_4$ crystals perpendicular to the magnetic field, and the Lotgering orientation factor, f, is determined to be 0.8.

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