• 한국결정성장학회지
• /
• 제22권1호
• /
• pp.29-35
• /
• 2012

Special attention in the role of convection in vapor crystal growth has been paid since some single crystals under high gravity acceleration of $10g_0$ appear considerably larger than those under normal gravity acceleration ($1g_0$). With increasing the gravity acceleration from $1g_0$ up to $10g_0$, the total molar flux for ${\Delta}T$ = 30 K increases by a factor of 4, while for ${\Delta}T$ = 90, by a factor of 3. The maximum molar fluxes for three different gravity levels of $1g_0$, $4g_0$ and $10g_0$, appear approximately in the neighborhood of y = 0.5 cm, and the molar fluxes show asymmetrical patterns, which indicate the occurrence of either one single or more than one convective cell. As the gravitational level is enhanced form $1g_0$ up to $10g_0$, the intensity of convection is increased significantly through the maximum molar fluxes for ${\Delta}T$ = 30 K and 90 K. At $10g_0$, the maximum total molar flux is nearly invariant for for ${\Delta}T$ = 30 K and 90 K. The total molar flux increases with increasing the gravity acceleration, for $1g_0{\leq}g_y{\leq}10g_0$, and decreases with increasing the partial pressure of component B, a noble gas called as Kr (Krypton), $P_B$. The ${{\mid}U{\mid}}_{max}$ is directly proportional to the gravity acceleration for 20 Torr $P_B{\leq}300$ Torr. As the partial pressure of $P_B$ (Torr) decreases from 300 Torr to 20 Torr, the slopes of the ${{\mid}U{\mid}}_{max}s$ versus the gravity accelerations increase from 0.29 sec to 0.54 sec, i.e. by a factor of 2. The total molar flux of $Hg_2Cl_2$ is first order exponentially decayed with increasing the partial pressure of component B, $P_B$ (Torr) from 20 Torr up to 300 Torr.

• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2011년도 제40회 동계학술대회 초록집
• /
• pp.72-72
• /
• 2011

Recently, Zinc oxide (ZnO) nano-structures have been received attractive attention because of their outstanding optical and electrical properties. It might be a promising material considered for applications to photonic and electronic devices such as ultraviolet light emitting diode, thin film transistor, and gas sensors. ZnO nano-structures can be typically synthesized by the VLS growth mode and self-assembly. In the VLS growth mode using various growth techniques, the noble metal catalysts such as Au and Sn were used. However, the growth of ZnO nano-structures on nano-crystalline Au seeds using radio frequency (RF) magnetron sputtering might be explained by the profile coating, i.e. the ZnO nano-structures were a morphological replica of Au seeds. Ga doped ZnO (ZnO:Ga) nano-structures using this concept were synthesized and characterized by XRD, AFM, SEM, and TEM. We found that surface morphology is drastically changed from initial islands to later sun-flower typed nano-structures. We will present the structural evolution of ZnO:Ga nano-structures with increasing the film thickness.

• Journal of Radiation Protection and Research
• /
• 제41권4호
• /
• pp.354-358
• /
• 2016

Background: To find out the leak characteristic of research reactor 'HANARO' building in a typhoon condition Materials and Methods: MELCOR code which normally is used to simulate severe accident behavior in a nuclear power plant was used to simulate the leak rate of air and fission products from reactor hall after the shutdown of the ventilation system of HANARO reactor building. For the simulation, HANARO building was designed by MELCOR code and typhoon condition passed through Daejeon in 2012 was applied. Results and Discussion: It was found that the leak rate is $0.1%{\cdot}day^{-1}$ of air, $0.004%{\cdot}day^{-1}$ of noble gas and $3.7{\times}10^{-5}%{\cdot}day^{-1}$ of aerosol during typhoon passing. The air leak rate of $0.1%{\cdot}day^{-1}$ can be converted into $1.36m^3{\cdot}hr^{-1}$, but the design leak rate in HANARO safety analysis report was considered as $600m^3{\cdot}hr^{-1}$ under the condition of $20m{\cdot}sec^{-1}$ wind speed outside of the building by typhoon. Conclusion: Most of fission products during the maximum hypothesis accident at HANARO reactor will be contained in the reactor hall, so the direct radiation by remained fission products in the reactor hall will be the most important factor in designing emergency preparedness for HANARO reactor.

• Journal of Radiation Protection and Research
• /
• 제34권4호
• /
• pp.195-200
• /
• 2009

원전에서는 많은 종류의 방사성물질이 생성되어 일부는 환경으로 방사성유출물로서 배출되고 있다. 이러한 방사성유출물 중에서 탄소 동위원소인 Carbon-14는 자연에서 이미 높은 준위의 백그라운드를 형성하고 있기 때문에, 원전에서 Carbon-14가 배출되더라도 환경이나 일반인의 피폭방사선량에 미치는 영향이 미미하여 과거에는 배출감시와 환경감시를 수행하지 않았다. 그런데, 핵연료 제조기술 발달과 운전방법 개선으로 핵연료로부터 불활성기체와 입자방사성물질의 방출이 계속 감소하고 있다. 또한 방사선계측기술의 향상에 따라 삼중수소와 Carbon-14 같은 저준위 베타방사능 핵종의 검출준위가 낮아져, 이들 핵종이 일반인 선량평가에서 미치는 비율이 상대적으로 높아지고 있다. 본 논문은 원자력시설에서 발생하는 Carbon-14에 대해 미국의 기술보고서와 논문 등을 검토하여 배출관리와 환경 영향평가에 대한 방사선감시의 기술적 배경을 조사하였다. 이를 바탕으로 Carbon-14 방사성핵종의 배출감시 방안에 대한 타당성을 제시하고자 하였다.

• 암석학회지
• /
• 제23권3호
• /
• pp.261-272
• /
• 2014

지난 ~30년 동안 가속기질량분석기와 비활성기체질량분석기 기술의 진보와 함께, 우주선유발 동위원소도 지표면의 연대측정 분야에 광범위하게 적용되어 왔다. 우주선유발 동위원소를 이용한 세부적인 연대측정법으로는 단순노출연대측정, 수직단면연대측정, 매몰연대측정 등이 있어, 다양한 노출(또는 퇴적) 환경에 따라, 다른 접근법이 요구된다. 국내에 적용 가능한 대상으로는, 하안단구, 해안단구, 선상지, 화산지형, 구조지형(단층애), 다양한 암설지형(테일러스, 암괴류 등), 호안 또는 해안 파식대 그리고, 제3기의 퇴적분지층과 고고학유물층에도 적용이 가능하다. 아울러, 기존의 석영이 풍부한 화강암과 변성암 중심에서, 최근에는 석회암과 화산암에도 적용가능하게 되었다.

• 한국물환경학회지
• /
• 제34권6호
• /
• pp.621-631
• /
• 2018

In this study, catalyst was made through incipient wetness method using palladium (Pd) as noble metal, indium (In) as secondary metal, and montmorillonite (MK10) and Al pillared montmorillonite (Al-MK10) as supporters. The nitrate reduction rate of the catalysts was measured by batch experiments where H2 gas was used as reducing agent and formic acid as pH controller. Transmission electron microscopy (TEM) equipped with energy dispersive spectroscopy (EDS) and X-ray photoelectron spectroscopy (XPS) were all used to determine the elemental distribution of Pd, In, Al, and Si on catalysts. It was observed that Al pillaring increased the Al/Si elemental composition ratio and point of zero charge of MK10, but decreased its BET specific surface area and pore volume. The nitrate reduction rate of Al-MK10 Pd/In was 2.0 ~ 2.5 times higher than that of MK10 Pd/In using artificial groundwater (GW) in ambient temperature and pressure. Nitrate reduction rates in GW were 1.2 ~ 1.7 times lower than those in distilled deionized water (DDW). Nitrate reduction rates in acidic conditions were higher than those in neutral condition in both GW and DDW. The amount of produced NH3-N over degraded NO3- at acid conditions was lower than that of neutral condition. Even though the leaching of Pd after reaction was measured in DDW it was not detected when both Al-MK10 Pd/In and MK10 Pd/In were used in GW. The modification of montmorillonite as a supporter significantly increased the reductive catalytic activities of nitrates. However, the ratio of producing ammonia by-products to degraded nitrates in ambient temperature and pressure was similar.

• Bulletin of the Korean Chemical Society
• /
• 제16권10호
• /
• pp.923-929
• /
• 1995

Four crystal structures of M3-A (M3Na9-xHx-A, M=Rb or K and x=1 or 0), Rb3Na8H-A(a=12.228(1) Å and R1=0.046), Rb3Na9-A (a=12.258(3) Å and R1=0.058), K3Na8H-A (a=12.257(3) Å and R1=0.048) and K3Na9-A (a=12.257(3) Å and R1=0.052), have been determined by single crystal x-ray diffraction technique in the cubic space group Pm3^m at 21 ℃. In all structures, each unit cell contained three M+ ions all located at one crystallographically distinct position on 8-rings. Rb+ ions are 3.12 and 3.21 Å away respectively from O(1) and O(2) oxygens, about 0.40 Å away from the centers of the 8-rings, and K+ ions are 2.87 and 2.81 Å apart from the corresponding oxygens. These distances are the shortest ones among those previously found for the corresoponding ones. Eight 6-rings per unit cell are occupied by eight Na+ ions, each with a distance of 2.31 Å to three O(3) oxygens. The twelfth cation per unit cell is found as Na+ opposite 4-ring in the large cavities of M3Na9-A and assumed to be H+ for M3Na8H-A. With these noble non-framework cationic arrangements, larger M+ ions preferably on all larger 8-rings and the compact Na+ ions on all 6-rings, the bond angles in the 8-rings of M3-A, 145.1 and 161.0 respectively for (Si,Al)-O(1)-(Si,Al) and (Si,Al)-O(2)-(Si,Al), turned out to be remarkably stable and smaller, by more than 12 to 17°, than the corresponding angles found in the crystal structures of zeolites A with high concentration of M+ ions. It is to achieve these remarkably relaxed 8-rings, the main windows for the passage of gas molecules, with simultaneously maximized cavity volumes that M3-A have been selected as one of the efficient zeolite A systems for gas encapsulation.

• 자원환경지질
• /
• 제40권5호
• /
• pp.635-649
• /
• 2007

이 연구에서는 호남지역에 분포하는 5개 온천(죽림, 변산, 지리산, 덕산, 화순)에서 9개 온천시료와 인근의 지하수 시료 3개를 채취하여 수질화학 성분과 안정동위원소 $({\delta}^{18}O,\;{\delta}D,\;{\delta}^{34}S)$ 및 영족기체(He, Ne, Ar) 동위원소 분석을 통하여 온천수의 지화학적 특성, 지화학적 진화, 그리고 황, 헬륨, 아르곤의 기원을 해석하고자 하였다. 호남지역 온천수의 수온은 $23.0{\sim}30.5^{\circ}C$ 범위로 저온형 온천특성을 보이고 pH는 $7.67{\sim}9.98$ 범위로 알카리성의 특성을 보여주었다. 전기전도도는 $153{\sim}746{\mu}S/cm$ 범위로 지역에 따라서 큰 차이를 보여주었다. 온천주변 지하수의 수질특성은 온천수보다 낮은 pH와 전기전도도의 특성을 보여주었다. 온천수와 지하수의 지화학적 성분은 파이퍼도상에서 크게 3개의 유형으로 구분된다($Na-HCO_3$ 유형, Na-Cl 유형, $Ca-HCO_3$ 유형). 온천수의 지화학적 진화과정을 보면 초기에 $Ca-HCO_3$ 유형에서 출발하여 $Ca(Na)-HCO_3$ 유형을 거쳐 $Na-HCO_3$ 유형으로 진화하였으며, 일부 온천수는(JR1)의 경우 pH 9.98의 알카리성으로, $Na-HCO_3$ 유형의 종말점까지 도달하여 지화학적 진화의 최종단계에 도달되었음을 보여준다. 온천수의 산소 및 수소동위원소 조성은 순환수선을 따라 도시되며 지역에 따라 위도효과를 보인다. 황산염에 대한 황동위원소 대부분 화성기원을 보인다. 그러나 JR1 온천은 고염수에서 기원한 것으로 보이는 해양성기원을 보인다. 온천수의 $^3He/^4He$ 비와 $^4He/^{20}Ne$ 비는 $0.0143{\times}10^{-6}{\sim}0.407{\times}10^{-6}$ 범위와 $6.49{\sim}584{\times}10^{-6}$ 범위를 각각 보여주어 대기와 지각성분의 혼합선상에 도시된다. 이는 온천수내 헬륨가스의 대부분이 지각기원임을 의미한다. 죽림온천(JR1)의 경우 맨틀기원의 헬륨가스의 혼합율이 다른 온천에 비해 다소 높은 비율을 보여준다. 이들 동위원소비와 온천수의 pH와는 대체적으로 정의 상관관계가 확인되었다. 아울러 $^{40}Ar/^{36}Ar$비가 $292.3{\times}10^{-6}{\sim}304.1{\times}10^{-6}$ 범위로 대기기원임을 지시한다.

• Nuclear Engineering and Technology
• /
• 제38권2호
• /
• pp.163-174
• /
• 2006

The $Ph{\acute{e}}bus$ FP project is an international reactor safety project. Its main objective is to study the release, transport and retention of fission products in a severe accident of a light water reactor (LWR). The FPT4 test was performed with a fuel debris bed geometry, to look at late phase core degradation and the releases of low volatile fission products and actinides. Post Test Analyses results indicate that releases of noble gases (Xe, Kr) and high-volatile fission products (Cs, I) were nearly complete and comparable to those obtained during $Ph{\acute{e}}bus$ tests performed with a fuel bundle geometry (FPT1, FPT2). Volatile fission products such as Mo, Te, Rb, Sb were released significantly as in previous tests. Ba integral release was greater than that observed during FPT1. Release of Ru was comparable to that observed during FPT1 and FPT2. As in other $Ph{\acute{e}}bus$ tests, the Ru distribution suggests Ru volatilization followed by fast redeposition in the fuelled section. The similar release fraction for all lanthanides and fuel elements suggests the released fuel particles deposited onto the plenum surfaces. A blockage by molten material induced a steam by-pass which may explain some of the low releases. The revaporisation testing under different atmospheres (pure steam, $H_2/N_2$ and steam /$H_2$) and up to $1000^{\circ}C$ was performed on samples from the first upper plenum. These showed high releases of Cs for all the atmospheres tested. However, different kinetics of revaporisation were observed depending on the gas composition and temperature. Besides Cs, significant revaporisations of other elements were observed: e.g. Ag under reducing conditions, Cd and Sn in steam-containing atmospheres. Revaporisation of small amounts of fuel was also observed in pure steam atmosphere.

• 암석학회지
• /
• 제19권4호
• /
• pp.255-267
• /
• 2010

최근 많은 발전을 이룬 (U-Th)/He 온도-연령 측정법은 광물내의 빠른 He 확산 특성을 이용해 지각 천부의 열역사 혹은 매우 짧은 열적 교란 등을 규명하는데 널리 쓰이고 있다. 이번 논평에서는 이 방법이 어떻게 화성운석의 열역사, 특히 화성(Mars)에서 방출시의 열적교란을 규명하는데 이용될수 있는지에 대한 기존 연구 및 전망에 대해 기술하였다. 모든 화성운석은 화성에서 방출될 당시 충격변성작용을 겪은 것으로 알려져 있는데, 이러한 작용의 온도조건을 규명하기 위해 충격실험을 통한 암석 조직 비교, 고지자기학적 연구, $^{40}Ar/^{39}Ar$ 및 (U-Th)/He 온도-연령측정법 등이 이용되었다. 각각의 방법은 장단점이 있으며 열역사를 밝히는데 단편적인 정보만을 제공하지만, 이러한 다양한 방법들이 동시에 적용되었을때 보다 신빙성있는 열역사를 알아낼 수 있다. ALH84001 화성운석의 경우 화성에서 방출될 당시의 조건에 대해 논란이 많은데 이는 위에 언급한 방법들로부터 서로 상반된 결론이 도출되었기 때문이다. 최근 단입자 (U-Th)/He 및 $^{40}Ar/^{39}Ar$ 결과를 동시에 만족하는 열역사를 규명한 연구가 ALH84001 화성운석에 대해 이루어 졌는데, 이는 앞으로의 운석 연구에 좋은 방법론을 제시할 수 있으리라 본다.