• 한국재료학회지
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• 제8권6호
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• pp.526-531
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• 1998

HVPE(hydride vapor phase epitaxy)법으로 (111) $MgAl_2O_4$기판 위에 $10~240\mu{m}$두께의 GaN를 성장하고, GaN의 두께에 따 광학적 성질을 조사하였다. $MgAl_2O_4$기판 위에 성장된 GaN의 PL 특성은 결정성장온도에서 기판으로부터 Mg이 out-diffusion하여 auto-doping 됨으로써 불순물이 첨가된 GaN의 PL 특성을 나타내었다. 10K의 온도데서 측정된 PL 스펙트럼은 자유여기자와 속박여기자의 재결합천이에 의한 피크들과 불순물과 관련된 도너-억셉터 쌍 사이의 재결합 및 이의 포논 복제에 의한 발광으로 구성되었으며, 깊은 준위로부터의 발광은 나타나지 않았다. 중성 도너에 속박된 여기자 발광 에너지와 라만 $E_2$모드 주파수는 GaN의 두께가 증가함에 따라 지수 함수적으로 감소하였으며, GaN 내의 잔류 응력에 대하여 라만 E2 모드 주파수는$\Delta$$\omega$=3.93$\sigma$($cm^{-1}$/GPa)의 관계로 변화하였다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2005년도 제25회 추계학술대회논문집
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• pp.437-444
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• 2005

본 연구는 연료-공기 혼합정도가 불안정 화염 구조와 NOx 배출 특성에 미치는 영향을 조사하기 위해 대기압, 모형 가스 터빈 연소기에서 실험을 수행하였다. 선회각은 $45^{\circ}$이며, 연료-공기 혼합정도는 당량비 0.53에서 0.79 범위에서 0, 50, 100%로 변화시켰다. 화염구조를 파악하기 위해, 당량비 0.79에서 ICCD를 사용하여 위상 동기화된 OH 자발광 이미지를 취득하였다. NOx 배출은 각 상기 실험조건에서 NOx 분석기를 이용하여 취득하였다. 위상에 대한 $OH^*$ 이미지를 취득함으로써 연료-공기 혼합정도가 화염의 구조에 미치는 영향을 확인할 수 있었다. 또한 국소 열방출의 특성을 통해, 연료-공기 혼합정도에 따른 연소불안정이 발생하거나 소멸되는 영역에 대한 정보를 얻을 수 있었으며, 혼합정도에 따른 NOx 농도를 측정함으로써 희박 연소 영역에서는 $\sigma$가 커질수록 NOx 발생이 적음을 확인할 수 있었다. 이런 결과들은 연소불안정 현상의 메카니즘을 이해하는데 중요한 기초자료로 사용될 것으로 기대된다.

• 한국표면공학회:학술대회논문집
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• 한국표면공학회 2000년도 춘계학술발표회 초록집
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• pp.1-1
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• 2000

The results of the modification of metal materials treated by high temperature pulst:d plasma fluxes (HTlPPF) with a specific power of incident flux changing in the $(3...100)10^5{]\;}W/cm^2$ range and a pulse duration lying from 15 to $50{\;}\mu\textrm{s}$ have been presented. The results of HTPPF action were studied on the stainless steels of 18Cr-l0Ni, 16Cr- 15Ni, 13Cr-2Mo types; on the structural carbon steels of (13...35)Cr, St. 3, St. 20, St. 45 types; on the tool steels of U8, 65G, ShHI5 types, and others; on nickel and high nickel alloy of 20Cr-45Ni type; on zirconium- and vanadium-base alloys and other materials. The microstructure and properties (mechanical, tribological, erosion, and other properties) of modified materials and surface alloying of metals exposed to HTPPF action have been investigated. It was found that the modification of materials by HTPPF resulted in a simultaneous increase of several properties of the treated articles: microhardness of the surface and layers of 40...60 $\mu\textrm{m}$ in depth, tribological characteristics (friction coefficient, wear resistance), mechanical properties ({\sigma_y}, {\;}{\sigma_{0.2}}.{\;}{\sigma_r}) on retention of the initial plasticity ($\delta$), corrosion resistance, radistanation erosion under ion irradiation, and others. The determining factor of the changes observed is the structural-phase modification of the near-surface layers, in particular, the formation of the fine cellular structure in the near-surface layers at a depth of $20{\;}{\mu\textrm{m}}$ with dimension of cells changing in the range from 0.1 to $1., 5{\;}\mu\textrm{m}$, depending on the kind of material, its preliminary treatment, and the parameters of plasma fluxes. The remits obtained have shown the possibility of purposeful surface alloying of metals exposed to HTPPF action over a depth up to 20...45 $\mu\textrm{m}$ and the concentration of alloying element (Ni, Cr, V) up to 20 wt.%. Possible industrial brunches for using the treatment have been also considered, as well as some results on modifying the serial industrial articles by HTPPF.

• 한국표면공학회지
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• 제54권3호
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• pp.102-111
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• 2021

The corrosion behaviors of laser-welded super duplex stainless steel tubes with post-weld heat treatment(PWHT) conditions(950, 1000, 1050, 1100 ℃ for 5 and 30 min) were evaluated by electrochemical potentiodynamic polarization and critical pitting temperature measurements. This study showed that the critical metallurgical factors affecting the degradation of corrosion resistance of a steel tube in as-welded condition were the unbalanced phase fraction(ferrite:austenite = 94:4), Cr₂N precipitation, and phase transformation from the austenite phase to ɛ-martensite(via stress-induced phase transformation). The improvement in the corrosion resistance of the welded specimen depends greatly on the PWHT conditions. The specimens after PWHT conducted below 1000 ℃ showed inferior corrosion resistance, caused by precipitation of the sigma phase enriched with Cr and Mo. At 1100 ℃ for a longer duration in PWHT, the ferrite phase grows, and its fraction increases, leading to an unbalanced phase fraction in the microstructure. As a result, pitting can be initiated primarily at the interface between the ferrite/austenite phase, particularly in base metal.

• 천문학회지
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• 제38권2호
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• pp.241-244
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• 2005

We have analysed near-infrared JHKL observations of the members of the $\approx$9 Myr-old $\eta$ Chamaeleontis cluster. Using (J - H)/(K - L) and (H - K)/(K - L) IR colour-colour diagrams for the brightest 15 members of the cluster, we find the fraction of stellar systems with near-IR excess emission was 0.60 $\pm$ 0.13 (2$\sigma$). For the CTT and WTT star population, we also find a strong correlation between the IR excess and Ha emission which is also known as an accretion indicator. The (K - L) excess of these stars appears to indicate a wide range of star-disk activity; from a CTT star with high levels of accretion, to CTT - WTT transitional objects with evidence for some on-going accretion, and WTT stars with weak or absent IR excesses. Among the brightest 15 members, four stars (RECX 5, 9, 11 and ECHA J0843.3-7905) with IR excesses ${\Delta}$(K - L) > 0.4 mag and strong or variable optical emission were identified as likely experiencing on-going mass accretion from their circumstellar disks which we confirmed their accretion disks from the optical high-resolution echelle spectroscopic study. The result-ing accretion fraction of 0.27 $\pm$ 0.13 (2$\sigma$) suggests that the accretion phase, in addition to the disks themselves, can endure for at least ${\~}$10 Myr.

• 한국응용과학기술학회지
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• 제23권3호
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• pp.185-191
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• 2006

It is desirable to have an accurate expression on the temperature dependence of surface(or interfacial) tension ${\sigma}$, because most of the interfacial thermodynamic functions can be derived from it. There have been proposed several equations on the temperature dependence of the surface tension, ${\sigma}(T)$. Among them $E{\ddot{o}}tv{\ddot{o}}s$ equation and the one modified by Katayama, which is called Katayama equation, for improving accuracies of $E{\ddot{o}}tv{\ddot{o}}s$ equation close to critical points, have been most well-known. In this article Katayama equation is interpreted on the basis of the cell model to understand the nature of the equation. The cell model results in an expression very similar to Katayama equation. This implies that, although $E{\ddot{o}}tv{\ddot{o}}s$ and Katayama equations were obtained on the basis of experimental results, they have a sound theoretical background. The Katayama equation is also modified with the phase volume replaced with a critical scaling expression. The modified Katayama equation becomes a power-law equation with the exponent slightly different from the value obtained by critical-scaling theory. This implies that Katayama equation can be replaced by a critical-scaling equation which is proven to be accurate.

• Journal of Advanced Marine Engineering and Technology
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• 제27권6호
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• pp.704-713
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• 2003

The effect of partial substitution of tungsten for molybdenum on the microstructure and corrosion resistance in 22Cr-5Ni-3Mo duplex stainless steel(DSS) aging heat treated in a temperature range of 600~$1000^{\circ}C$ has been investigated. Electrochemical tests were carried out for the evaluation of corrosion resistance. Aging treatment had hardly influenced the general corrosion resistance. With the increase of aging time, the pitting corrosion resistance of the DSS had decreased, After aging for 2min at 700~$900^{\circ}C$, the pitting potential of the 3Mo steel decreased remarkably, while that of the W-substituted steel hardly changed. During aging. the intermetallic $\sigma$ and secondary austenite ($\gamma_2$) phases were precipitated. and the pitting corrosion and intergranular corrosion resistance were significantly decreased after aging at 700~$750^{\circ}C$ for 10 h, which could be caused by the $\gamma_2$ formation. The ${\gamma}$$_2$ phase could affect the depletion of molybdenum and chromium in the $\gamma_2/\alpha and \gamma_2/\sigma$ boundaries.

• 한국가스학회지
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• 제10권1호
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• pp.1-6
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• 2006

압력설비를 안전하고 효율적으로 사용하기 위하여 본 연구에서는 API-581 절차에 의한 위험기반검사에서 취성파괴에 의한 사고발생 가능성을 정량적으로 해석하였다. 그 결과, 낮은 온도/낮은 인성파괴와 뜨임취성에서는 A 충격곡선이고. 낮은 온도와 열처리 전인 상태에서 기술종속계수(TMSF)가 큰 값을 나타내었고, $855^{\circ}F$ 취성에서는 위험도가 무시할 수 있었으나, 시그마상 취성에서는 낮은 온도의 고 시그마인 경우에 TMSF가 큰 값을 나타내어 사고발생 가능성이 매우 높았다.

• 한국광학회지
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• 제7권2호
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• pp.142-149
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• 1996

대향류버너의 화염에서 연소반응의 중간단계 생성물로 존재하는 OH라디칼의 축퇴 4광자 혼합스팩트럼을 비포화영역에서 Forward Box 형태의 위상정합조건으로 측정하였다. X$^{2}$.PI..rarw.A$^{2}$.SIGMA.$^{+}$ 천이선들 중 R$_{1}$-가지 분광선들의 세기로부터 회전에너지 준위의 밀도분포를 구하고 볼쯔만분포와 비교하여 온도를 구하였다. 흡수분광스펙트럼을 측정하여 화염내에서 레이저의 흡수효과를 보정하여 주었다. 측정된 온도의 오차는 2000K 근방에서 .+-.60K로서 CARS로 얻은 온도와 오차범위내에서 일치하였다. 화염의 여러부분에서 스펙트럼을 측정하여 온도분포와 OH농도분포를 얻었다.

• 자원환경지질
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• 제19권1호
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• pp.19-24
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• 1986

The Samkwang mine is one of gold deposits distributed mainly in the southwestern province (Chungnam) of the Korean peninsula. Golds occur in quartz veins aged of $223{\pm}4MA$ according to K-Ar age dating from muscovite in a pegmatitic quartz vein. Quantz veins intrude Precambrian biotite-granite gneiss and mica schist of unknown age. Fluid inclusions in the quartz show a range of homogenization temperatures from 159 to $274^{\circ}C$. A calculated temperature from the isotopes of the galena-sphalerite pair is $375^{\circ}C$. Two phases-fluid inclusions homogenized either by liquid or vapor phase are frequently observed in specimens over $260^{\circ}C$, which may indicate the boiling of the fluids. Pressure of formation of the quartz veins inferred by the homogenization temperatures of liquid-$CO_2$ bearing fluid is 1kb. Based on these data, it is assumed that the temperature of the formation of the Samkwang mine may lie in between $350^{\circ}-230^{\circ}C$. ${\delta}^{34}S_{{\Sigma}s}$ values of sulphide minerals show narrow range of +2.1 to +4.6, and show a trend of enrichments of $^{34}S$ in the fluid from deep to the surface. ${\delta}^{34}S_{{\Sigma}s}$ in the fluid estimated is less than 3 permil, suggesting sulphur fluid originated from the magma.