• 한국재료학회지
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• 제23권8호
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• pp.405-422
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• 2013

Atomic layer deposition(ALD) is a promising deposition method and has been studied and used in many different areas, such as displays, semiconductors, batteries, and solar cells. This method, which is based on a self-limiting growth mechanism, facilitates precise control of film thickness at an atomic level and enables deposition on large and three dimensionally complex surfaces. For instance, ALD technology is very useful for 3D and high aspect ratio structures such as dynamic random access memory(DRAM) and other non-volatile memories(NVMs). In addition, a variety of materials can be deposited using ALD, oxides, nitrides, sulfides, metals, and so on. In conventional ALD, the source and reactant are pulsed into the reaction chamber alternately, one at a time, separated by purging or evacuation periods. Thermal ALD and metal organic ALD are also used, but these have their own advantages and disadvantages. Furthermore, plasma-enhanced ALD has come into the spotlight because it has more freedom in processing conditions; it uses highly reactive radicals and ions and for a wider range of material properties than the conventional thermal ALD, which uses $H_2O$ and $O_3$ as an oxygen reactant. However, the throughput is still a challenge for a current time divided ALD system. Therefore, a new concept of ALD, fast ALD or spatial ALD, which separate half-reactions spatially, has been extensively under development. In this paper, we reviewed these various kinds of ALD equipment, possible materials using ALD, and recent ALD research applications mainly focused on materials required in microelectronics.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2004년도 춘계학술대회 논문집 디스플레이 광소자분야
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• pp.142-145
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• 2004

In this work, we have investigated the application of rapid thermal processing (RTP) and plasma enhanced chemical vapour deposition (PECVD) for surface passivation. Rapid thermal oxidation (RTO) has sufficiently low surface recombination velocities (SRV) $S_{eff}$ in spite of a thin oxides and short process time. The effective lifetime is increasing with an increase of the oxide thickness. In the same oxide thickness, The effective lifetime is independent on the process temperature and time. $S_{eff,max}$ is exponentially decreased with increasing oxide thickness. $S_{eff,max}$ can be reduced to 200 cm/s with only 10 nm oxide thickness. On the other hand, three different types of SiN are reviewed. SiN1 layer has a thickness of about 72 nm and a refractive index of 2.8. Also, The SiN1 has a high passivation quality. The effective lifetime and SRV of 1 $\Omega$ cm Float zone (FZ) silicon deposited with SiN1 is about 800 s and under 10 cm/s, respectively. The SiN2 is optimized for the use as an antireflection layer since a refractive index of 2.3. The SiN3 is almost amorphous silicon caused by less contents of N2 from total process. The effective lifetime on the FZ 1 ${\Omega}cm$ is over 1000 ${\mu}s$.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2014년도 제46회 동계 정기학술대회 초록집
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• pp.470.2-470.2
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• 2014

RF-PECVD 장치에 의해 증착된 실리콘 질화막(SiNx)은 결정질 실리콘 태양전지에서 반사 방지막 효과 및 우수한 표면 패시베이션 특성을 제공하는 것으로 알려져 있다. 본 논문에서는 실리콘 질화막의 패시베이션 특성을 향상시키기 위해서 공정온도를 $400^{\circ}C$로 고정하고 공정압력, 가스비, RF (radio frequency) power를 가변하였다. 이 때의 실리콘 질화막의 굴절률 및 두께는 각각 2.0, 80 nm로 증착하여 그에 따른 특성에 대해 분석하였다. 공정 압력이 감소할수록 실리콘 질화막이 증착된 결정질 실리콘 태양전지의 유효 반송자 수명이 증가함을 보였고, 반면에 증착속도는 감소하였다. 또한 RF-power 500 W에서 실리콘 질화막이 증착된 결정질 실리콘 태양전지의 유효 반송자 수명이 상대적으로 높았으며 출력이 올라갈수록 증착속도가 증가하였다. 결과적으로 결정질 실리콘 태양전지에 증착한 실리콘 질화막은 0.8torr 공정 압력과 RF-power 500 W에서 $38.8{\mu}s$로 가장 좋은 유효 반송자 수명을 확인하였다. 위의 결과를 바탕으로 결정질 실리콘 태양전지를 제작하였고 향상된 패시베이션 특성을 갖는 실리콘 질화막의 조건을 찾기 위해서 개방전압(open circuit voltage)을 비교하였다. 공정압력 0.8 torr, RF-power 500 W에서 가장 높은 결과를 보였으며 이는 유효 반송자 수명과 유사한 결과를 나타냈다. 하지만 낮은 FF (fill factor)로 인해 변환 효율이 낮은 결과를 보였다. 태양전지 제작시 낮은 fill factor를 보인 이유와 위의 단점을 보완하기 위해 추가 실험을 수행하였으며, 개선된 fill factor를 통해 18.3% 효율의 태양전지를 제작하였다.

• 한국재료학회지
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• 제26권1호
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• pp.47-53
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• 2016

Silicon nitride ($SiN_x:H$) films made by plasma enhanced chemical vapor deposition (PECVD) are generally used as antireflection layers and passivation layers on solar cells. In this study, we investigated the properties of silicon nitride ($SiN_x:H$) films made by PECVD. The passivation properties of $SiN_x:H$ are focused on by making the antireflection properties identical. To make equivalent optical properties of silicon nitride films, the refractive index and thickness of the films are fixed at 2.0 and 90 nm, respectively. This limit makes it easier to evaluate silicon nitride film as a passivation layer in realistic application situations. Next, the effects of the mixture ratio of the process gases with silane ($SiH_4$) and ammonia ($NH_3$) on the passivation qualities of silicon nitride film are evaluated. The absorption coefficient of each film was evaluated by spectrometric ellipsometry, the minority carrier lifetimes were evaluated by quasi-steady-state photo-conductance (QSSPC) measurement. The optical properties were obtained using a UV-visible spectrophotometer. The interface properties were determined by capacitance-voltage (C-V) measurement and the film components were identified by Fourier transform infrared spectroscopy (FT-IR) and Rutherford backscattering spectroscopy detection (RBS) - elastic recoil detection (ERD). In hydrogen passivation, gas ratios of 1:1 and 1:3 show the best surface passivation property among the samples.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2009년도 추계학술대회 논문집
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• pp.619-619
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• 2009

Recently, silica nanostructures are widely used in various applicationary areas such as chemical sensors, biosensors, nano-fillers, markers, catalysts, and as a substrate for quantum dots etc, because of their excellent physical, chemical and optical properties. Additionally, these days, semiconductor silica and silicon with high purity is a key challenge because of their metallurgical grade silicon (MG-Si) exhibit purity of about 99% produced by an arc discharge method with high cast. Tremendous efforts are being paid towards this direction to reduce the cast of high purity silicon for generation of photovoltaic power as a solar cell. In this direction, which contains a small amount of impurities, which can be further purified by acid leaching process. In this regard, initially the low cast rice-husk was cultivated from local rice field and washed well with high purity distilled water and were treated with acid leaching process (1:10 HCl and $H_2O$) to remove the atmospheric dirt and impurity. The acid treated rice-husk was again washed with distilled water and dried in an oven at $60^{\circ}C$. The dried rice-husk was further annealed at different temperatures (620 and $900^{\circ}C$) for the formation of silica nanospheres. The confirmation of silica was observed by the X-ray diffraction pattern and X-ray photoelectron spectroscopy. The morphology of obtained nanostructures were analyzed via Field-emission scanning electron microscope(FE-SEM) and Transmission electron microscopy(TEM) and it reveals that the size of each nanosphares is about 50-60nm. Using the Inductively coupled plasma mass spectrometry(ICP-MS), Silica was analyzed for the amount of impurities.

• 천문학회지
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• 제34권4호
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• pp.309-311
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• 2001

Strong thermal X-ray emission, called Galactic Ridge X-ray Emission, is observed along the Galactic plane (Koyama et al. 1986). The origin of hot ($\~$7 keV) component of GRXE is not known, while cool ($\~$0.8 keV) one is associated with supernovae (Kaneda et al. 1997, Sugizaki et al. 2001). We propose a possible mechanism to explain the origin; locally strong magnetic fields of $B_{local}\;\~30{\mu}G$ heat interstellar gas to $\~$7 keV via magnetic reconnection (Tanuma et al. 1999). There will be the small-scale (< 10 pc) strong magnetic fields, which can be observed as $(B)_{obs} \;\~3{\mu}G$ by integration of Faraday Rotation Measure, if it is localized by a volume filling factor of f $\~$ 0.1. In order to examine this model, we solved three-dimensional (3D) resistive magnetohydrodynamic (MHD) equations numerically to examine the magnetic reconnect ion triggered by a supernova shock (fig.l). We assume that the magnetic field is Bx = 30tanh(y/20pc) $\mu$G, By = Bz = 0, and the temperature is uniform, at the initial condition. We put a supernova explosion outside the current sheet. The supernova-shock, as a result, triggers the magnetic reconnect ion, and the gas is heatd to > 7 keV. The magnetic reconnect ion heats the interstellar gas to $\~$7 keV in the Galactic plane, if it occurs in the locally strong magnetic fields of $B_{local}\;\~30{\mu}G$. The heated plasma is confined by the magnetic field for $\~10^{5.5} yr$. The required interval of the magnetic reconnect ions (triggered by anything) is $\~$1 - 10 yr. The magnetic reconnect ion will explain the origin of X-rays from the Galactic ridge, furthermore the Galactic halo, and clusters of galaxies.

• 천문학회보
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• 제37권2호
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• pp.101.2-101.2
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• 2012

Shocks are ubiquitous in astrophysical plasmas: bow shocks are formed by the interaction of solar wind with planetary magnetic fields, and supernova explosions and jets produce shocks in interstellar and intergalactic spaces. The global morphologies of these shocks are usually described by a set of magnetohydrodynamic (MHD) equations which tacitly assumes local thermal equilibrium, and the resulting Rankine-Hugoniot shock jump conditions are applied to obtain the relationship between the upstream and downstream physical quantities. While thermal equilibrium can be achieved easily in collisional fluids, it is generally believed that collisions are infrequent in astrophysical settings. In fact, shock widths are much smaller than collisional mean free paths and a variety of kinetic phenomena are seen at the shock fronts according to in situ observations of planetary shocks. Hence, both the MHD and kinetic equations have been adopted in theoretical and numerical studies to describe different aspects of the physical phenomena associated with astrophysical shocks. In this paper, we present the results of 3D relativistic particle-in-cell (PIC) simulations for ion-electron plasmas, with focus on the shock structures: when a jet propagates into an unmagnetized ambient plasma, a shock forms in the nonlinear stage of the Weibel instability. As the shock shows the structures that resemble those predicted in MHD systems, we compare the results with those predicted in the MHD shocks. We also discuss the thermalization processes of the upstream flows based on the time evolutions of the phase space and the velocity distribution, as well as the wave spectra analyses.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제38회 동계학술대회 초록집
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• pp.177-177
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• 2010

고효율 비정질 실리콘 박막 태양전지 제작을 위해서는 광파장대에서 optical confinement 능력을 최대화할 수 있는 기술이 필수적이다. 효율적인 photon trapping을 위해서는 back reflector를 사용하거나 전면전극인 투명전도성막의 표면에 요철을 형성하여 포획된 태양광의 내부 반사를 증가시키거나 전면 투명전극에서 반사를 감소시켜 태양광의 travel length를 증가시키는 방법이 일반적이며, 이를 통해 흡수층의 효율을 최대화할 수 있다. 이 중 전면전극으로 사용되는 투명전도성막은 불소가 도핑된 tin-oxide가 주로 사용되었으나, 최근 들어 Al이 도핑된 산화아연막을 이용한 비정질 실리콘 박막 태양전지 개발에 대한 연구도 활발히 진행되고 있다. 투명전극 증착후 표면의 유효면적을 증가시키기 위해 염산 용액을 이용하여 표면 텍스쳐링을 수행한다. 그후 흡수층인 p-i-n 층을 플라즈마 화학기상증착법을 이용하여 형성하는 것이 일반적이다. 이때 표면처리 된 투명전극은 수소플라즈마에 대해 특성이 변하지 않아야 고효율 비정질 실리콘 박막 태양전지 제조에 적용될 수 있다. 본 연구에서는 표면처리 된 AZO 투명전극의 수소플라즈마에 의한 특성 변화에 대해 고찰하였다. 먼저 AZO 투명전극은 스퍼터링 공정을 적용하여 $1\;{\mu}m$두께로 증착하였고, 0.5 wt%의 HCl 용액을 이용하여 습식 식각을 수행하였다. 수소플라즈마 처리 조건은 $H_2$ flow rate 30 sccm, working pressure 20 mtorr, RF power 300 W, Temp $60^{\circ}C$ 이며 3분간 진행하였다. 표면형상은 수소플라즈마 전 후에는 큰 차이를 보이지 않았으며 AZO의 grain size는 각각 220 nm, 210 nm로 관찰되었다. 투명전극의 가장 중요한 특성인 가시광선 영역에서의 투과도는 수소플라즈마 처리전에는 90 % 이상의 투과도를 보였으나, 수소플라즈마 처리 후에는 85 %로 약간 저하된 특성을 보였다. 그러나 이는 박막 태양전지용 전면전극으로 사용하기 위한 투과도인 80 % 이상을 만족하는 결과로, 비정질 박막 실리콘 태양전지 제작에 사용될 수 있다. 또 하나의 중요한 특성인 Haze factor 역시 수소플라즈마 처리 전 후 모두 10 이상의 값을 나타냈다. 하지만 고효율 실리콘 박막 태양전지에 적용하기 위해서는 Haze factor를 증가시키는 공정 개발에 대한 추가 연구가 필요하다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제38회 동계학술대회 초록집
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• pp.141-141
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• 2010

The effect of thermal anneal on the characteristics of structural properties and the enhancement of luminescence and photovoltaic (PV) characteristics of silicon-rich silicon-nitride films were investigated. By using an ultra high vacuum ion beam sputtering deposition, B-doped silicon-rich silicon-nitride (SRSN) thin films, with excess silicon content of 15 at. %, on P-doped (n-type) Si substrate was fabricated, sputtering a highly B doped Si wafer with a BN chip by N plasma. In order to examine the influence of thermal anneal, films were then annealed at different temperature up to $1100^{\circ}C$ under $N_2$ environment. Raman, X-ray diffraction, and X-ray photoemission spectroscopy did not show any reliable evidence of amorphous or crystalline Si clusters allowing us concluding that nearly no Si nano-cluster could be formed through the precipitation of excess Si from SRSN matrix during thermal anneal. Instead, results of Fourier transform infrared and X-ray photoemission spectroscopy clearly indicated that defective, amorphous Si-N matrix of films was changed to be well-ordered thanks to high temperature anneal. The measurement of spectral ellipsometry in UV-visible range was carried out and we found that the optical absorption edge of film was shifted to higher energy as the anneal temperature increased as the results of thermal anneal induced formation of $Si_3N_4$-like matrix. These are consistent with the observation that higher visible photoluminescence, which is likely due to the presence of Si-N bonds, from anneals at higher temperature. Based on these films, PV cells were fabricated by the formation of front/back metal electrodes. For all cells, typical I-V characteristic of p-n diode junction was observed. We also tried to measure PV properties using a solar-simulator and confirmed successful operation of PV devices. Carrier transport mechanism depending on anneal temperature and the implication of PV cells based on SRSN films were also discussed.

• 자원리싸이클링
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• 제20권2호
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• pp.45-53
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• 2011

본 연구에서는 다양한 방법들을 이용하여 태양전지 폐 모듈로부터 태양전지의 주요 구성요소인 실리콘과 강화유리를 회수하는 연구를 수행하였다. 강화유리는 유기용매를 사용하여 회수하였고, EVA수지는 열처리를 통하여 완전히 제거하였다. 실리콘은 계면 활성제를 첨가한 혼산용액을 이용하여 표면물질을 제거하고 회수하였다. 90%이상의 높은 실리콘 회수율을 얻었다. 본 연구에 의하여 얻어진 강화유리와 실리콘은 태양전지 모듈의 원료로 재활용되어 실리콘 공급부족 문제해결, 태양전지 제조원가 및 폐기물 처리비용 절감에 기여할 것으로 기대된다.