• 생명과학회지
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• 제23권12호
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• pp.1415-1419
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• 2013

본 연구에서는 식물병원성 미생물들인 잿빛곰팡이와 Agrobacterium rhizogenes의 전자선에 대한 감수성을 조사하였다. 그 결과, 2 kGy의 전자선량이 잿빛곰팡이의 분생포자 및 Agrobacterium rhizgenes의 세포를 사멸시키는 데에 충분한 것으로 나타났다. 식물 종자의 전자선에 대한 저항성을 조사해 본 결과, 대파, 열무와 오이 종자는 2 kGy의 전자선 조사에서도 발아율이 전혀 영향을 받지 않았고, 쑥갓 종자의 경우에는 발아율에 있어서 근소한 감소를 보였다. 그러나 고추와 상추의 경우에는 전자선 조사에 대해서 대단히 약한 것으로 나타났다. 결과적으로 열무, 오이, 대파 및 쑥갓 종자의 경우에는 식물병원성 미생물의 살균에 필요한 2 kGy의 전자선량을 조사함으로써 발아율에 큰 영향을 미치지 않고 충분한 살균효과를 거둘 수 있을 것으로 판단된다. 그러나 고추와 상추의 경우에는 전자선을 이용한 살균 방법은 사용하기 어려운 것으로 나타났다.

• 한국식품영양과학회지
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• 제33권6호
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• pp.1068-1073
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• 2004

노루궁뎅이 버섯의 열수 추출 실험을 실시하면서 반응표면분석에 의해 추출물의 특성을 최적화하였다. 추출물의 가용성 고형분은 설정된 추출온도와 추출시간에 대해서는 영향을 받지 않는 것으로 나타났으며, 용매에 대한 시료비가 증가할수록 가용성 고형분이 증가하였으며, 페놀성 화합물과 조단백 함량도 추출온도보다는 용매에 대한 시료비가 더 큰 영향을 미치는 것으로 나타났다. 추출물의 전자공여작용은 용매에 대한 시료비와 추출온도가 증가할수록 증가하다가 최적 추출조건에서 최대점을 보이다가 이후로 감소하는 경향을 나타내었다. 이들 추출물의 특성을 모두 만족시키는 최적 추출조건은 추출온도 91.5$^{\circ}C$∼96.5$^{\circ}C$, 용매에 대한 시료비 3.5∼4.2 g/100 mL로 나타났으며 예측된 최적 추출조건의 임의의 점에서 실험한 결과, 각 반응변수들의 예측값과 실제값이 유사하였다.

• Metals and materials international
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• 제24권6호
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• pp.1359-1368
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• 2018

The mechanical properties and microstructure evolution of Mg-8Li-3Al-1Y alloy undergoing different rolling processes were systematically investigated. X-ray diffraction, optical microscope, scanning electron microscopy, transmission electron microscopy as well as electron backscattered diffraction were used for tracking the microstructure evolution. Tensile testing was employed to characterize the mechanical properties. After hot rolling, the $MgLi_2Al$ precipitated in ${\beta}-Li$ matrix due to the transformation reaction: ${\beta}-Li{\rightarrow}{\beta}-Li+MgLi_2Al+{\alpha}-Mg$. As for the alloy subjected to annealed hot rolling, ${\beta}-Li$ phase was clearly recrystallized while recrystallization rarely occurred in ${\alpha}-Mg$ phase. With regard to the microstructure undergoing cold rolling, plenty of dislocations and dislocation walls were easily observed. In addition, the microstructure of alloys subjected to annealed cold rolling revealed the formation of new fresh ${\alpha}-Mg$ grains in ${\beta}-Li$ phase due to the precipitation reaction. The mechanical properties and fracture modes of Mg-8Li-3Al-1Y alloys can be effectively tuned by different rolling processes.

• 소성∙가공
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• 제17권7호
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• pp.523-527
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• 2008

In this study, mechanical properties of Alloy 718 welded after forgings for jet propulsion component was investigated. Hot-forged and machined work-pieces($230mm\times70mm\times15mm$) which have different grain sizes are welded by electron beam welding technique. After welding, the components were solution heat-treated and aged. Samples were sectioned to analyze the microstructural evolution and formation of micro-crack. It was found that HAZ grain boundary liquation crack generally initiates in the coarse grains rather than the fine grains. Needle-like phases with high Nb contents were found at the outer part near the base metal. Vickers hardness and tensile tests were carried out at room temperature and at $649^{\circ}C$. The tensile properties of electron beam welding specimens exhibited around 100MPa and 10% decrease in strength and elongation, respectively.

• 조명전기설비학회논문지
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• 제13권3호
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• pp.40-47
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• 1999

본 연구에서는 개발하고자 하는 저에너지 대면적 전자빔 발생장치는 원리로서 발생원인 글로우 발전에 의한 플라즈마로부터 이온을 음극으로 가속, 충돌하게 하여 그때 발생하는 2차전자를 전자빔원으로 하여 전자를 가속·제어하는데 바탕을 두고 있으며, 본 연구에서는 이러한 원리를 기본으로 이론적 해석을 통한 고효율의 저에너지 대면적 전자빔 발생장치개발의 설계 및 제작에 대해서 연구하였으며, 또한 빔 에너지의 안전성과 방전조건을 고려한 최적의 방전 파라메타를 설정하여 대면적의 균일한 빔 인출을 가능케 하였다.

• Journal of Astronomy and Space Sciences
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• 제39권2호
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• pp.35-42
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• 2022

During their respective missions, the spacecraft Voyager and Cassini measured several Saturn magnetosphere parameters at different radial distances. As a result of information gathered throughout the journey, Voyager 1 discovered hot and cold electron distribution components, number density, and energy in the 6-18 Rs range. Observations made by Voyager of intensity fluctuations in the 20-30 keV range show electrons are situated in the resonance spectrum's high energy tail. Plasma waves in the magnetosphere can be used to locate Saturn's inner magnetosphere's plasma clusters, which are controlled by Saturn's spin. Electromagnetic electron cyclotron (EMEC) wave ring distribution function has been investigated. Kinetic and linear approaches have been used to study electromagnetic cyclotron (EMEC) wave propagation. EMEC waves' stability can be assessed by analyzing the dispersion relation's effect on the ring distribution function. The primary goal of this study is to determine the impact of the magnetosphere parameters which is observed by Cassini. The magnetosphere of Saturn has also been observed. When the plasma parameters are increased as the distribution index, the growth/damping rate increases until the magnetic field model affects the magnetic field at equator, as can be seen in the graphs. We discuss the outputs of our model in the context of measurements made in situ by the Cassini spacecraft.

• 천문학회보
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• 제46권1호
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• pp.36.2-36.2
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• 2021

In the outskirts of galaxy clusters, weak shocks with M_s < ~3 appear as radio relics where the synchrotron radiation is emitted from cosmic-ray (CR) electrons. To understand the production of CR electrons through the so-called diffusive shock acceleration (DSA), the electron injection into the DSA process at shocks in the hot intracluster medium (ICM) has to be described. However, the injection remains as an unsolved, outstanding problem. To explore this problem, 2D Particle-in-Cell (PIC) simulations were performed. In this talk, we present the electron preacceleration mechanism mediated by multi-scale plasma waves in the shock transition zone. In particular, we find that the electron preacceleration is effective only in the supercritical shocks, which have the sonic Mach number M_s > M_crit ≈ 2.3 in the high-beta (β~100) plasma of the ICM, because the Alfven ion cyclotron instability operates and hence multi-scale plasma waves are induced only in such supercritical shocks. Our findings will help to understand the nature of radio relics in galaxy clusters.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2016년도 제50회 동계 정기학술대회 초록집
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• pp.149-149
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• 2016

Ceramic is widely known material due to its outstanding mechanical property. Besides, Zirconia(ZrO2) has a low thermal conductivity so it is advantage in a heat insulation. Because of these superior properties, ZrO2 is attracted to many fields using ultra high temperature for example vehicle engines, aerospace industry, turbine, nuclear system and so on. However brittle fracture is a disadvantage of the ZrO2. In order to overcome this problem, we can make the ceramic materials to the forms of ceramic nanoparticles, ceramic nanowhiskers and these forms can be used to an agent of composite materials. In this work, we selected Au catalyzed Vapor-Liquid-Solid mechanism to synthesize ZrO2 nanowhiskers. The ZrO2 whiskers are grown through Hot-wall Chemical Vapor Deposition(Hot wall CVD) using ZrCl4 as a powder source and Au film as a catalyst. This Hot wall CVD method is known to comparatively cost effective. The synthesis condition is a temperature of $1100^{\circ}C$, a pressure of 760torr(1atm) and carrier gas(Ar) flow of 500sccm. To observe the morphology of ZrO2 scanning electron microscopy is used and to identify the crystal structure x-ray diffraction is used.

• 천문학논총
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• 제15권spc1호
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• pp.133-145
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• 2000

Symbiotic stars are known as binary systems with both cool and hot components with enshrounding nebulous gas. The cool component, M-type giant, is presumably loosing its mass into a hot white or main sequence companion star through the inner Lagrangian point. The lines emit from the ionized nebulous region around the hot star while the mass loss or accretion activity is believed to be the main cause of sudden variation of the continuum and line fluxes. We selected 17 symbiotics for which the emission line fluxes were measured from the IUE SWP, LWR data, to find variability of spectrum. We also investigated the periodic variation of emissions or eclipsing effect from the IUE lines. All of our symbiotics show very high electron densities in the emission regions. For other optical symbiotics, the observations had been carried in 1999 with BOAO mid-resolution spectrometer. We classified symbiotics based on their outburst activities, or emission line characteristics, i.e., $OVI{\lambda}6830.\;The\;OVI{\lambda}6830$ emission lines are also found in S-type symbiotics, which have been known as charateristics of D-types.

• 한국세라믹학회지
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• 제14권3호
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• pp.163-168
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• 1977

As a wet chemical drying process "hot petroleum drying method" was applied and developed for preparing uniformly fine oxide powder with high purity and sinterreactivity. Using this method solution of sulfates was dried in hot petroleum bath (~17$0^{\circ}C$) to sulfate powder from which corresponding mullite doped by Fe3+ ion was formed. Particle size, shape, decomposition by heat, and phase identification of sulfate andoxide powders determined by DTA, TGA, X-ray diffraction, analysis and electron microscopy: sulfate powder prepared by this drying method is an intimate mixture of the amorphous form of uniformly and finely distributed spherical particles (0.05-0.1$\mu$). Mullitization with the sulfate powder occurs at 110$0^{\circ}C$ in air. The morphology of mullite particle made by firing the sulfate powder at 135$0^{\circ}C$ in oxygen atmosphere is granular of 0.1-0.3$\mu$ in size. This drying process proved to be a very effective method for preparing fine, homogeneous, and highly sinterreactive multicomponent oxide powder without conventional ceramic process of mixing, milling, and granulating. This process can be also applied for preparing electronic ceramic materials which are requisite for high purity and homogeneity.mogeneity.