• Journal of the Korean Magnetics Society
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• v.11 no.6
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• pp.272-277
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• 2001

A spin valve structure of Ta/NiFe/CoFe/Cu/CoFe/Ru/CoFe/FeMn/Ta which has a synthetic antiferromagnet (CoFe/Ru/CoFe), was fabricated by using a magnetron sputtering system. The thickness and composition of magnetic free and pinned layers affect the magnetic properties such as exchange interaction strength of each layer and so on. Even though Rutherford Backscattering Spectrometry (RBS) has advantages of quantitative and non-destructive analysis, it is almost impossible to determine the thickness and composition of magnetic thin films using lBS because of its poor mass resolution for a higher atom number (Z>20). In this study, quantitative analysis of the element composition and thickness for the spin valve sample was performed by combining both Proton Induced X-ray Emission Spectrometry (PIXE), which is one of element specific analysis techniques, and grazing-exit RBS with a highly improved depth resolution and absolute quantitative analysis. For the quantitative analysis, standardization of PIXE was carried out with NiFe, CoFe, and FeMn layers, which are one of constituent layers of spin valve films. Through PIXE standardization and the aid of PHE experimental results of the spin valve sample, ire overlapped signal in a grazing-exit RBS spectrum were successfully resolved and the thickness of the Ru layer was determined with a resolution of ∼1 .

• Proceedings of the Korean Magnestics Society Conference
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• 2004.12a
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• pp.133-134
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• 2004

• Proceedings of the Korean Magnestics Society Conference
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• 2006.06a
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• pp.42-43
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• 2006

• Proceedings of the Korean Magnestics Society Conference
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• 2011.06a
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• pp.41-41
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• 2011

• Proceedings of the Korean Magnestics Society Conference
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• 2011.12a
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• pp.74-74
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• 2011

• Proceedings of the Korean Magnestics Society Conference
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• 2005.12a
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• pp.8-9
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• 2005

• Proceedings of the Korean Magnestics Society Conference
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• 2012.05a
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• pp.74-75
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• 2012

• The Journal of the Institute of Internet, Broadcasting and Communication
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• v.18 no.2
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• pp.73-79
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• 2018

In this paper, TM(transverse magnetic) scattering problems by a conductive strip grating between a double dielectric layer are analyzed by applying the PMM(point matching method) known as a numerical method of electromagnetic fileld. The boundary conditions are applied to obtain the unknown field coefficients, the scattered electromagnetic fields are expanded in a series of Floquet mode functions, and the conductive boundary condition is applied to analysis of the conductive strip. The most normalized reflected powers of the sharp variations in minimum values are scattered in direction of the other angles except incident angle. Generally, in the case of numerical analysis except for reflection and transmission power in free space, as the dielectric constants of the double dielectric layer increases, the reflected power increases and the transmitted power decreases relatively, respectively. The numerical results for the presented structure of this paper having a grounded double dielectric layer are shown in good agreement compared to those of the existing papers.

• The Bulletin of The Korean Astronomical Society
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• v.41 no.1
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• pp.46.1-46.1
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• 2016

The formation process of a current sheet is important for solar flare from a viewpoint of a space weather prediction. We therefore derive the temporal development of the spatial and statistical distribution of electric current density distributed in a flare-producing active region to describe the formation of a current sheet. We derive time sequence distribution of electric current density by applying a nonlinear force-free approximation reconstruction to Active Region 12158 that produces an X1.6-class flare. The time sequence maps of photospheric vector magnetic field used for reconstruction are captured by a Helioseismic and Magnetic Imager (HMI) onboard Solar Dynamic Observatory (SDO) on 10th September, 2014. The spatial distribution of electric current density in NLFFF model well reproduce observed sigmoidal structure at the preflare phase, although a layer of high current density shrinks at the postflare phase. A double power-law profile of electric current density is found in statistical analysis. This may be expected to use an indicator of the occurrence of a solar flare.

• Journal of Magnetics
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• v.8 no.1
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• pp.32-35
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• 2003

Magnetic funnel Junctions (MTJs) were fabricated on thermally oxidized Si (100) wafers using DC magnetron sputtering. The film Structures were Ta(50 ${\AA}$)/CU(100 ${\AA}$)$Ni_{80}Fe_{20}(20 $ ${\AA}$)/Cu(50 ${\AA}$)/$Mn_{75}Ir_{25}(100 $ ${\AA}$)/$Co_{70}Fe_{30}(25$ ${\AA}$)/Al-O(15 ${\AA}$)/$Co_{70}Fe_{30}(25 $ ${\AA}$)/$Ni_{80}Fe_{20}(t)/Ta(50 $ ${\AA}$), with t=0 ${\AA}$, 100 and 1000 ${\AA}$, respectively. X-ray diffraction has shown improvement of (111) texture of IrMn$_3$ and Cu by annealing. The exchange-biased energy is almost inversely proportional to temperature. The difference between the coercivity H$_c$ and the exchange biased field H$_E$ for t = 0 $_3$ sample is smaller than that for t = 1000 ${\AA}$. For the pinned layer, the decreasing rate of the coercivity with the temperature is higher compared to that of the exchange field, but variation of H$_c$ is similar to that of the exchange field for free layer.