• Title/Summary/Keyword: Magnetic Fields

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LARGE SCALE MAGNETIC FIELDS IN LENS GALAXIES

  • NARASIMHA D.;CHITRE S. M.
    • Journal of The Korean Astronomical Society
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    • v.37 no.5
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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.

Effect of the rotation on a non-homogeneous infinite cylinder of orthotropic material with external magnetic field

  • Hussein, Nahed S.;Bayones, F.S.;Mahmoud, S.R.
    • Structural Engineering and Mechanics
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    • v.54 no.1
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    • pp.135-148
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    • 2015
  • The present investigation is concerned with a study effect of magnetic field and non-homogenous on the elastic stresses in rotating orthotropic infinite circular cylinder. A certain boundary conditions closed form stress fields solutions are obtained for rotating orthotropic cylinder under initial magnetic field with constant thickness for three cases: (1) Solid cylinder, (2) Cylinder with a circular hole at the center, (3) Cylinder mounted on a circular rigid shaft. Analytical expressions for the components of the displacement and stress fields in different cases are obtained. The effect of rotation and magnetic field and non-homogeneity on the displacement and stress fields are studied. Numerical results are illustrated graphically for each case. The effects of rotating and magnetic field and non-homogeneity are discussed.

Measurements of the Magnetic Fields Produced by Electric Home Appliances (가정용 전기기기에서 발생하는 자장의 측정)

  • Lee, B.H.;Park, J.W.;Eom, J.H.
    • Proceedings of the KIEE Conference
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    • 2000.07c
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    • pp.2204-2206
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    • 2000
  • In this paper, the magnetic fields measured experimentally from the electric home appliances were evaluated and the data were discussed on the bases of the international institutes recommendations. It is difficult to insulate magnetic flux completely from electric home appliances and impossible to simulate theoretically because of the different directions and magnitudes of magnetic fields according to the internal current of electric home appliances. The experimental measurements of magnetic flux density were carried out according to the increment of distance in the vicinity of electric home appliances. The magnetic flux density produced by the electric home appliances was drastically dropped with the increment of distance. The measured and analysed results of electric home appliances of 15 including computer monitor, TV, etc. were presented.

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OBSERVING MAGNETIC FIELDS ON LARGE SCALES

  • RUDNICK LAWRENCE
    • Journal of The Korean Astronomical Society
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    • v.37 no.5
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    • pp.329-335
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    • 2004
  • Observations of magnetic fields on scales up to several Mpc are important for understanding cluster and large-scale structure evolution. Our current census of such structures is heavily biased - towards fields of several $\mu$G, towards fields in deep potential wells, and towards high inferred field strengths m cooling flow and other clusters from improper analysis of rotation measure data. After reviewing these biases, I show some recent results on two relics that are powered in very different ways. I describe new investigations that are now uncovering weak diffuse fields in the outskirts of clusters and other low density environments, and the good prospects for further progress.

Heat transfer enhancement in gas tungsten arc welding using azimuthal magnetic fields generated by external current

  • Kim, Yiseul;Lee, Jaewook;Liu, Xiaolong;Lee, Boyoung;Chang, Yunlong
    • Coupled systems mechanics
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    • v.6 no.2
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    • pp.113-125
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    • 2017
  • This paper proposes the idea to enhance the heat transfer in Gas Tungsten Arc Welding (GTAW) by using the azimuthal magnetic field. The azimuthal magnetic field generated by the external currents makes the Lorentz force stronger, and consequently improves the heat transfer by the faster flow movement. The enhanced heat transfer might improve the welding performance by increasing the temperature at the workpiece. To validate the proposed idea, a two-dimensional axi-symmetric model of GTAW is built, and the multiphysics simulation of GTAW is carried out. As the analysis result, the distributions of electric current, electromagnetic fields, arc flow velocity, and temperature are investigated. Then, the proposed idea for heat transfer enhancement is validated by comparing the Lorentz force, flow velocity, and temperature distribution with and without azimuthal magnetic fields.

PRE- AND POSTNATAL TOXICITY EVALUATION OF 60 Hz HORIZONTALLY POLARIZED MAGNETIC FIELDS IN RATS

  • Chung, Moon-Koo;Kim, Jong-Choon;Myung, Sung-Ho;Han, Sang-Seop
    • Proceedings of the Korean Society of Toxicology Conference
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    • 2002.05a
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    • pp.133-133
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    • 2002
  • Recently, there is an increasing nationwide concern in Korea that exposure to electric and magnetic fields (MF) in the home environment may not be safe in humans. We previously demonstrated that exposure of MF during the entire period of pregnancy did not induce any adverse effects on both pregnant dams and embryo-fetal development in rats.(omitted)

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Characteristic study of fluid flow of laminar impinging jet in an aligned magnetic field (자기장이 인가된 영역에서의 층류 충돌제트의 유동특성 변화에 대한 수치적 연구)

  • Lee, Hyun-Goo;Ha, Man-Yeong;Yoon, Hyun-Sik;Chun, Ho-Hwan
    • Proceedings of the KSME Conference
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    • 2004.04a
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    • pp.1845-1850
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    • 2004
  • The laminar impinging jet flow fields were investigated with or without magnetic fields. The transient phenomenon from steady to unsteady flow was founded at specific Reynolds number ranges. In unsteady flow region, the magnetic fields make flow stable. So the characteristics of fluid flow at impingement wall are changed

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Characteristic study of heat transfer of laminar impinging jet in an aligned magnetic field (자기장이 인가된 영역에서의 층류 충돌제트의 열전달특성 변화에 대한 수치적 연구)

  • Lee, Hyun-Goo;Ha, Man-Yeong;Yoon, Hyun-Sik;Chun, Ho-Hwan
    • Proceedings of the KSME Conference
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    • 2004.04a
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    • pp.1447-1451
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    • 2004
  • The laminar impinging jet thermal fields were investigated with or without magnetic fields. The transient phenomenon from steady to unsteady flow was founded at specific Reynolds number ranges. In unsteady flow region, the magnetic fields make flow stable. So the characteristics of heat transfer at impingement wall are changed

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Calculations on the Reduction Rate of Ground Level Magnetic Fields due to Varying Configurations of Overhead Transmission Line (가공 송전선 형상변화에 따른 지표면 자계저감율 계산)

  • Min, Suk-Won;Kim, Eung-Sik;Park, Jun-Hyeong
    • The Transactions of The Korean Institute of Electrical Engineers
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    • v.57 no.11
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    • pp.2027-2034
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    • 2008
  • There are concerns on possible health effects from exposure to electromagnetic fields. One reflection of this concerns is the considerable controversy, delay, and cost increases involved in the construction of power lines and facilities. To cope with such challenges, in this paper we investigated magnetic fields reduction techniques such as general compaction, in' span compaction, cruciform, vertical, 3 way splits phase, and 4way splits phase. As results, we found general compaction and 4 way splits phase could reduce magnetic fields up to 90%, while cruciform, vertical, and 3 way splits phase gave lower reduction rates of 30% because these configurations were similar to a current type of low reactance arrangement. We also knew 1 spacer in span compaction was appropriate in Korea in view of effectiveness and economy.

MAGNETIC FIELDS IN STARS AND DISKS

  • VISHNIAC ETHAN T.
    • Journal of The Korean Astronomical Society
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    • v.29 no.spc1
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    • pp.201-204
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    • 1996
  • Magnetic fields are thought to playa role in a wide variety of important astrophysical processes, from angular momentum transport and jet formation in accretion disks to corona formation in stars. Unfortunately, the dynamics of magnetic fields in astrophysical plasmas are extremely complicated, and the success of current theoretical models and computer simulations seems to be inversely correlated with the amount of observational detail available to us. Here I will discuss some of the more striking conflicts between numerical simulations and observations, and present an explanation for them based on an important dynamical process which is not adequately modeled in current numerical simulations. These processes will lead to the formation of flux tubes in stars and accretion disks, in accordance with observations. I will discuss some of the implications of flux tube formation for stellar and accretion disk dynamos.

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