• 한국진공학회지
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• 제4권S1호
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• pp.113-117
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• 1995

MOCVD of Cu films were carried out on gold-TiN(1000$\AA$)/Ti/Si wafers from hexafluoroacetylacetonate-Cu(l) vinyltrimethylsilane, Cu(l)(hafac)(vtms), in a small cold-wall type reactor. Effects of the substrate and bubbler temperatures on the film growth rate were studied, and a film with $\rho$=1.8$\pm$0.1$\mu$$\Omega$.cm could be deposited 150nm/min at Ts=200 and Tb=$30^{\circ}C$, respectively. The initial stage of the film formation was also investigated by in-situ laser reflectivity monitoring combined with SEM observations, based on which variations in the film properties depending on the growth conditions were discussed in terms of the nucleation rate and grain size.

• 한국윤활학회:학술대회논문집
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• 한국윤활학회 2002년도 proceedings of the second asia international conference on tribology
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• pp.79-80
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• 2002

This paper presents an experimental study of the effect of rolling speed and surface roughness on the mixed elastohydrodynamic (EHD) lubrication characteristics for point contact formed between a real, random, rough surface, steel ball and smooth glass disc. The Thin Film Colorimetic Interferometry measurement technique has been extended to give detailed information about in-contact deformation of the microgeometry. It has enabled to derive the amplitude reduction curve that shows progressive recovering of ball roughness features with increasing speed.

• Journal of Astronomy and Space Sciences
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• 제32권3호
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• pp.167-180
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• 2015

Herein, we discuss the in situ measurement of the electron temperature in the ionosphere/plasmasphere by means of DC Langmuir probes. Major instruments which have been reported are a conventional DC Langmuir probe, whose probe voltage is swept; a pulsed probe, which uses pulsed bias voltage; a rectification probe, which uses sinusoidal signal; and a resonance cone probe, which uses radio wave propagation. The content reviews past observations made with the instruments above. We also discuss technical factors that should be taken into account for reliable measurement, such as problems related to the contamination of electrodes and the satellite surface. Finally, we discuss research topics to be studied in the near future.

• 천문학회보
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• 제44권2호
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• pp.40.4-40.4
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• 2019

Interplanetary coronal mass ejections (ICMEs) are regarded as one of the most powerful sources of space weather disturbances observed near the Earth orbit (1 AU). In this study, we aim at investigating the relation between these disturbances and the physical properties of an ICME. Toward this end, we used an spheromak-type ICME and performed a series of three-dimensional magnetohydrodynamic (MHD) simulations with different sets of ICME parameters. The ICME is injected into the background solar wind generated from near-Sun data and interplanetary scintillation (IPS) data via an MHD-IPS tomography method. We will compare simulation results to in situ observations near the Earth and discuss how the physical properties of an ICME affect the space weather disturbances at 1 AU.

• 대한원격탐사학회지
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• 제34권6_2호
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• pp.1299-1310
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• 2018

본 연구는 북극해에 분포하는 유빙의 움직임을 이해하기 위해 현장관측 자료와 입자 추적 방법을 사용하여 분포 및 이동경향을 분석하였다. 북극해에서 유빙의 움직임은 NOAA(National Oceanic and Atmospheric Administration)에서 제공하는 ITP(Ice-Tethered Profiler)의 자료 중에서 2009년부터 2018년 자료를 이용했다. 유빙의 유동은 각 연도별로 분류하고 각각의 ITP 자료를 이용하여 위치 및 속도를 분석하였다. 입자 추적은 HYCOM(Hybrid Coordinate Ocean Model)과 ECMWF(European Centre for Medium-Range Weather Forecasts)에서 제공하는 일별 해류 및 바람 자료를 사용하여 2009년부터 2018년까지의 유빙의 움직임을 모의하였다. 북극해 전역에서 유빙의 이동경향을 분석하기 위해서 현장관측 자료인 ITP자료를 입력 자료로 이용하여 북극해에서 해류와 바람과의 관계식을 계산하여 라그랑지안 입자 추적을 수행하였다. 입자 추적 시뮬레이션은 해류에 의한, 그리고 해류와 바람에 의한 영향을 고려한 두 종류의 실험을 수행하였고, 대부분의 입자는 해류와 바람의 영향을 고려한 경우에 현장관측 자료와 동일하게 재현되었다. 북극해에서 유빙의 움직임은 바람의 영향을 고려한 관계식을 이용하여 재현되었고, 이를 이용하여 특정 연도의 유빙의 이동경향을 분석하였다. 2010년의 경우 Arctic Oscillation Index(AOI)는 음의 해로 입자들은 보퍼트 환류(Beaufort Gyre)를 따라 명확하게 움직임을 보이고, 극점 인근에서는 상대적으로 더 빠른 속도를 나타낸다. 반면에 2017년의 경우 AOI는 양의 해로 대부분의 입자들은 Gyre에 크게 영향을 받지 않는 움직임을 보이며 보퍼트 해 (Beaufort Sea) 인근에서 나타나는 이동속도 또한 상대적으로 감소하였고, 극점에서의 이동속도도 감소했다. 2010년과 2017년의 계절적 특징은 2010년도의 유빙의 이동속도는 동계(0.22 m/s)에 증가되고 춘계(0.16 m/s)에 감소되며, 2017년의 경우 하계(0.22 m/s)에 증가되고 춘계(0.13 m/s)에 감소되었다. 결과적으로 입자추적 방법은 제한된 현장관측 자료를 대신하여 북극해에서 유빙의 분포 및 이동경향을 이해할 수 있는 방법으로 위성자료와 연계하여 장기적인 유빙의 탐지 및 이동경향을 이해하는 유용한 방법이 될 것이다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제45회 하계 정기학술대회 초록집
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• pp.99-99
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• 2013

In this talk, I will present two research works in progress, which are: i) mapping of piezoelectric polarization and associated charge density distribution in the heteroepitaxial InGaN/GaN multi-quantum well (MQW) structure of a light emitting diode (LED) by using inline electron holography and ii) in-situ observation of the polarization switching process of an ferroelectric Pb(Zr1-x,Tix)O3 (PZT) thin film capacitor under an applied electric field in transmission electron microscope (TEM). In the first part, I will show that strain as well as total charge density distributions can be mapped quantitatively across all the functional layers constituting a LED, including n-type GaN, InGaN/GaN MQWs, and p-type GaN with sub-nm spatial resolution (~0.8 nm) by using inline electron holography. The experimentally obtained strain maps were verified by comparison with finite element method simulations and confirmed that not only InGaN QWs (2.5 nm in thickness) but also GaN QBs (10 nm in thickness) in the MQW structure are strained complementary to accommodate the lattice misfit strain. Because of this complementary strain of GaN QBs, the strain gradient and also (piezoelectric) polarization gradient across the MQW changes more steeply than expected, resulting in more polarization charge density at the MQW interfaces than the typically expected value from the spontaneous polarization mismatch alone. By quantitative and comparative analysis of the total charge density map with the polarization charge map, we can clarify what extent of the polarization charges are compensated by the electrons supplied from the n-doped GaN QBs. Comparison with the simulated energy band diagrams with various screening parameters show that only 60% of the net polarization charges are compensated by the electrons from the GaN QBs, which results in the internal field of ~2.0 MV cm-1 across each pair of GaN/InGaN of the MQW structure. In the second part of my talk, I will present in-situ observations of the polarization switching process of a planar Ni/PZT/SrRuO3 capacitor using TEM. We observed the preferential, but asymmetric, nucleation and forward growth of switched c-domains at the PZT/electrode interfaces arising from the built-in electric field beneath each interface. The subsequent sideways growth was inhibited by the depolarization field due to the imperfect charge compensation at the counter electrode and preexisting a-domain walls, leading to asymmetric switching. It was found that the preexisting a-domains split into fine a- and c-domains constituting a $90^{\circ}$ stripe domain pattern during the $180^{\circ}$ polarization switching process, revealing that these domains also actively participated in the out-of-plane polarization switching. The real-time observations uncovered the origin of the switching asymmetry and further clarified the importance of charged domain walls and the interfaces with electrodes in the ferroelectric switching processes.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2006년도 춘계학술대회 논문집
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• pp.341-343
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• 2006

The current spectral shape matching method (SSMM), developed by Ahn and Shanmugam (2004), relies on the assumption that the path radiance resulting from scattered photons due to air molecules and aerosols and possibly direct-reflected light from the air-sea interface is spatially homogeneous over the sub-scene of interest, enabling the retrieval of water-leaving radiances ($L_w$) from the satellite ocean color image data. This assumption remains valid for the clear atmospheric conditions, but when the distribution of aerosol loadings varies dramatically the above postulation of spatial homogeneity will be violated. In this study, we present the second version of SSMM which will take into account the horizontal variations of aerosol loading in the correction of atmospheric effects in SeaWiFS ocean color image data. The new version includes models for the correction of the effects of aerosols and Raleigh particles and a method fur computation of diffuse transmittance ($t_{os}$) as similar to SeaWiFS. We tested this method over the different optical environments and compared its effectiveness with the results of standard atmospheric correction (SAC) algorithm (Gordon and Wang, 1994) and those from in-situ observations. Findings revealed that the SAC algorithm appeared to distort the spectral shape of water-leaving radiance spectra in suspended sediments (SS) and algal bloom dominated-areas and frequently yielded underestimated or often negative values in the lower green and blue part of the electromagnetic spectrum. Retrieval of water-leaving radiances in coastal waters with very high sediments, for instance = > 8g $m^{-3}$, was not possible with the SAC algorithm. As the current SAC algorithm does not include models for the Asian aerosols, the water-leaving radiances over the aerosol-dominated areas could not be retrieved from the image and large errors often resulted from an inappropriate extrapolation of the estimated aerosol radiance from two IR bands to visible spectrum. In contrast to the above results, the new SSMM enabled accurate retrieval of water-leaving radiances in a various range of turbid waters with SS concentrations from 1 to 100 g $m^{-3}$ that closely matched with those from the in-situ observations. Regardless of the spectral band, the RMS error deviation was minimum of 0.003 and maximum of 0.46, in contrast with those of 0.26 and 0.81, respectively, for SAC algorithm. The new SSMM also remove all aerosol effects excluding areas for which the signal-to-noise ratio is much lower than the water signal.

• 한국터널지하공간학회 논문집
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• 제12권1호
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• pp.1-14
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• 2010

지금까지 Martin 등(1999)의 선형관계식에 의한 스폴링 깊이 평가법이 널리 이용되어 왔으나, 이 방법은 원형 공동에만 적용될 수 있으며 실제 스폴링 발생현장에 적용한 결과 과대평가하는 결과를 보였다. 한편, 스폴링 폭을 평가하는 방법은 아직까지 제시되어 있지 않아 적절하게 평가가 이루어지지 못했다. 그러나, 스폴링 영역에 대한 적절한 보강을 위해서는 스폴링 깊이와 스폴링 폭에 대한 정량적인 평가가 필수적이다. 본 연구에서는 스폴링 관측사례와 스폴링 발생현장의 CWFS 수치해석 사례를 통해 3가지 스폴링 평가인자의 함수로 표현되는 정규화 스폴링 깊이와 정규화 스폴링 폭의 선형회귀식을 도출하였고, 통계추론에 의한 95% 신뢰구간을 통해 회귀식의 신뢰성을 검증하였다. 제안된 선형회귀식으로부터 예측된 스폴링 깊이와 스폴링 폭은 회귀관계의 분산도를 고려한 가중치를 적용함으로써 현장관측결과를 합리적으로 예측할 수 있었다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2006년도 Proceedings of ISRS 2006 PORSEC Volume I
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• pp.122-125
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• 2006

The distribution of phytoplankton pigments were studied bimonthly at four stations from the mouth of Mahanadi River at Paradip to the 36.7km off coast in Bay of Bengal during April 2001 to December 2002. Bottom depth was shallower than 40m in all stations. The pigment concentration of Chl-a was measured. It increased from surface to bottom in the water column. The water column integrated chlorophyll-a concentration (Chl-a) varied between 6.1 and $48.5mg{\cdot}m-^2$ with peaks during monsoon period (Aug & Oct). Spatial distribution of salinity depended strongly on freshwater runoff. The salinity was 5psu at river mouth and 25.15psu at offshore in monsoon period; however it was 30psu at the river mouth in summer. We found a linear relationship between the amount of river discharge and integrated Chl-a in coastal region from 2 years observations. Extending this result, we analyzed rainfall and coastal Chl-a using satellite data. The relationship between the river discharge and monthly accumulated rainfall estimated from TRMM and others data sources was analyzed in 2001 and 2002 using Giovanni infrastructure provided by NASA. The result depended on the specified area on TRMM images; the river delta area had sharper relationship than wider rain catchments area. Moreover, the relationship between monthly averaged Chl-a derived from SeaWiFS and monthly accumulated rainfall estimated from TRMM was analyzed from 1998 to 2005. It was clear that the broom in monsoon period was strongly controlled by rainfall on river delta.

• 대기
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• 제29권4호
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• pp.355-365
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• 2019

Based on in-situ monitoring data produced by National Institute of Meteorological Sciences, we evaluated the performance of Joint UK Land Environment Simulator (JULES) on the surface energy balance for rice-paddy and cropland in Korea with the operational ancillary data used for Unified Model (UM) Local Data Assimilation and Prediction System (LDAPS) (CTL) and the high-resolution ancillary data from external sources (EXP). For these experiments, we employed the one-year (March 2015~February 2016) observations of eddy-covariance fluxes and soil moisture contents from a double-cropping rice-paddy in BoSeong and a cropland in AnDong. On the rice-paddy site the model performed better in the CTL experiment except for the sensible heat flux, and the latent heat flux was underestimated in both of experiments which can be inferred that the model represents flood-irrigated surface poorly. On the cropland site the model performance of the EXP experiment was worse than that of CTL experiment related to unrealistic surface type fractions. The pattern of the modeled soil moisture was similar to the observation but more variable in time. Our results shed a light on that 1) the improvement of land scheme for the flood-irrigated rice-paddy and 2) the construction of appropriate high-resolution ancillary data should be considered in the future research.