• 한국해양공학회지
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• 제35권1호
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• pp.75-81
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• 2021

Artificial Coral Reefs (ACRs) have been introduced to help solve coastal erosion problems, but their feasibility has not been assessed with field data. This study conducted a feasibility analysis of ACRs on their erosion mitigation effects by performing a case study of Cheonjin-Bongpo beach, South Korea. A numerical-physical combined analysis was carried out using a SWAN model simulation and physical model test with a scale of 1/25 based on field observations of Cheonjin-Bongpo beach. Both Dean's parameter and the surf-scaling parameter were applied to comparative analysis between the absence and presence conditions of the ACR. The results for this combined method indicate that ACR attenuates the wave height significantly (59~71%). Furthermore, ACR helps decrease the mass flux (~50%), undertow (~80%), and maximum wave set up (~61%). The decreases in Dean's parameter (~66%) and the surf-scaling parameter suggest that the wave properties changed from the dissipative type to the reflective type even under high wave conditions. Consequently, an ACR can enhance shoreline stability.

• 대기
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• 제31권2호
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• pp.143-156
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• 2021

This study investigates the impacts of land cover change due to urbanization on the Urban Heat Island Intensity (UHII) and the Heat Index (HI) over the Seoul metropolitan area using the Unified Model (UM) with the Met Office Reading Urban Surface Exchange Scheme (MORUSES) during the heat wave from 16, July to 5, August 2018. Two simulations are performed with the late 1980s land-use (EXP1980) and the late 2000s land-use (EXP2000). EXP2000 is verified using Automatic Weather Station (AWS) data from 85 points in the study area, and observation sites are classified into two categories according to the urban fraction change over 20 years; Category A is 0.2 or less increase, and Category B is 0.2 or more increase. The 1.5-m temperature and relative humidity in Category B increase by up to 1.1℃ and decreased by 7% at 1900 LST and 2000 LST, respectively. This means that the effect of the urban fraction changes is higher at night. UHII increases by up to 0.3℃ in Category A and 1.3℃ in Category B at 1900 LST. Analysis of the surface energy balance shows that the heat store for a short time during the daytime and release at nighttime with upward sensible heat flux. As a result of the HI, there is no significant difference between the two experiments during the daytime, but it increases 1.6℃ in category B during the nighttime (2200 LST). The results indicate that the urbanization increase both UHII, and HI, but the times of maximum difference between EXP1980 and EXP2000 are different.

• 대한금속재료학회지
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• 제49권4호
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• pp.348-354
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• 2011

Long-lasting brightness $Sr_{4}Al_{14}O_{25}$ : $Eu^{2+}$, $Dy^{3+}$, $Ag^{+}$ phosphor was synthesized by modified solid state reaction and its photoluminescence was investigated. $Sr(NO_3)_{2}$ and $Al(NO_3)_3{\cdot}9H_{2}O$ as starting materials, and $B_{2}O_{3}$ as a flux were mixed with $Eu_{2}O_{3}$ as an activator, $Dy_{2}O_{3}$ as a coactivator, and $AgNO_{3}$ as a charge compensator. The crystalline of target powder showed a single-phase $Sr_{4}Al_{14}O_{25}$ by the XRD characterization and the average particle size was about 20-30 ${\mu}m$ from the FE-SEM observation. $Ag^{+}$ ion doping effects (0-0.06 mol) on $Sr_{4}Al_{14}O_{25}:Eu^{2+},\;Dy^{3+},\;Ag^{+}$ phosphor were measured by photoluminescence spectrometer and luminescence meter. The of photoluminescence intensity of the $Sr_{3.64}Al_{14}O_{25}:Eu_{0.11},\;Dy_{0.22},\;Ag_{0.03}$ phosphor was higher than other compositions and afterglow brightness was 0.186 $cd/m^{2}$.

• 대한금속재료학회지
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• 제46권10호
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• pp.634-645
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• 2008

In this study, surface composites were fabricated with Fe-based amorphous alloy powders and VC powders by high-energy electron beam irradiation, and the correlation of their microstructure with hardness and fracture toughness was investigated. Mixture of Fe-based metamorphic powders and VC powders were deposited on a plain carbon steel substrate, and then electron beam was irradiated on these powders without flux to fabricate surface composites. The composite layers of 1.3~1.8 mm in thickness were homogeneously formed without defects and contained a large amount (up to 47 vol.%) of hard $Cr_2B$ and $V_8C_7$ crystalline particles precipitated in the solidification cell region and austenite matrix, respectively. The hardness of the surface composites was directly influenced by hard $Cr_2B$ and $V_8C_7$ particles, and thus was about 2 to 4 times greater than that of the steel substrate. Observation of the microfracture process and measurement of fracture toughness of the surface composites indicated that the fracture toughness increased with increasing additional volume fraction of $V_8C_7$ particles because $V_8C_7$ particles effectively played a role in blocking the crack propagation along the solidification cell region heavily populated with $Cr_2B$ particles. Particularly in the surface composite fabricated with Fe-based metamorphic powders and 30 % of VC powders, the hardness and fracture toughness were twice higher than those of the surface composite fabricated without mixing of VC powders.

• 천문학회보
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• 제46권2호
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• pp.50.3-51
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• 2021

The progenitor of Type Ia supernovae is largely expected as a close binary system of a carbon/oxygen white dwarf (WD) primary and its secondary non-degenerate (single degenerate; SD) or degenerate companion (double degenerate; DD). Here we present a high-cadence monitoring observation of SN 2021hpr in a spiral galaxy, NGC 3147. SN 2021hpr shows typical characteristics as a normal type Ia supernova from its photometric (Δm₁₅(B)=1.01±0.03, dust free M_B,max=-19.45±0.02) and spectroscopic data. To investigate its progenitor system, we fit the early part of BVRI-band light curve simultaneously with a combined version of ejecta-companion and simple power-law model. As a result, we found a significant feature of an early excess possibly from a 7.63±0.52R_⊙-sized companion at the optimal viewing angle while the fit is not successful at the common viewing angle. No possible red sources brighter than F555W=-7.01 AB mag is detected at the SN location in Hubble Space Telescope (HST) pre-explosion images, excluding massive stars with initial mass of >16M_⊙ as companions. We suggest the progenitor system of SN 2021hpr can be a fairly large companion such as a main sequence, a low mass subgiant, and a helium giant star. In addition, a possibility of the ejecta-Disk Originated Matter (DOM) interaction for the DD scenario considering linearly-rising early flux still remains.

• 대한원격탐사학회지
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• 제36권6_1호
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• pp.1449-1463
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• 2020

최근 지구온난화에 따른 기후변화 문제의 심각성이 커지면서 국가 온실가스 배출량을 상쇄시킬 수 있는 산림의 탄소흡수에 대한 중요성이 높아지고 있으며, 기후변화협약에 따라 국가의 산림 탄소흡수량을 국지적인 수준에서 과학적이고 정밀하게 산출할 것이 요구되고 있다. 본 연구에서는 위성영상과 일기상 자료를 함께 활용함으로써 산림 광합성의 민감한 일변화를 반영하고, 안정된 산림으로서 대표성을 가지는 광릉숲(Gwangneung Forest) 극상림(climax forest)의 플럭스관측 자료를 참조하여 GPP(gross primary production) 재현 모델을 수립하고, 수종 및 임령에 따른 탄소흡수량 조견표를 적용하여, 우리나라의 국지지역에 최적화된 Tier 2.5 수준의 일일 탄소흡수능 격자자료를 산출하였다. 2013년 1월 1일부터 2015년 12월 31일까지 1,095일간의 실험에서, 일일 기준탄소흡수능(reference amount of CO2 absorption, RACA) 산출 모델은 상관계수 0.948의 높은 정확도를 나타냈으므로, 향후 Tier 3 수준의 일일 실제탄소흡수능(actual amount of CO2 absorption, AACA)을 정확히 산출하기 위해서는 장기간의 상세산림조사 자료와의 결합이 필요할 것이다.

• 한국농림기상학회지
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• 제23권4호
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• pp.251-267
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• 2021

원격 탐사 기반의 식생지수들은 광합성을 조절하는 식물생리적 특성과 경험적 상관관계를 보이며, 여러공간 규모에서의 총일차생산량(GPP) 추정에 활용되고 있다. 하지만 시간 해상도가 높아질수록 식생지수를 이용한 GPP 추정의 불확실성이 커지는 한계가 존재한다. 또한 식생지수 관련 분석에 주로 사용되는 에디공분산법을 이용하여 추정한 GPP 역시 실제 측정한 순생태계교환량(NEE)을 GPP와 생태계 호흡(RE)으로 배분하는 데 사용하는 방법에 따라 추정값이 달라지는 불확실성이 존재한다. 본 연구에서는 플럭스 타워가 설치된 네 곳의 농림생태계를 대상으로 근지표에서 관측한 식생의 분광 특성을 이용한 다양한 식생지수를 계산하였고, 이를 다양한 시간 해상도에서 GPP 추정에 적용가능한 지를 분석하였다. 동시에 이를 이용하여 NEE 배분 방법의 불확실성을 평가하였다. 비교에 사용한 정규식생지수, 개량식생지수, 적외반사식생지수(NIRv)에 비해 적외반사식생지수와 광합성유효광(PAR)을 결합한 NIRvP이 식생 및 지형 조건에 의한 공간 이질성으로 인해 관측지에 따라 약간의 차이가 나타났지만, 농경지와 산림에서 모두 30분과 일 단위 시간 해상도에서 GPP와 높은 상관성(r² = 0.63, 0.68)을 보였다. 또한 기존 KoFlux 표준 NEE 배분방법에 비해 기계학습 기반의 NEE 배분 방법을 적용할 경우, 산림에서 30분 단위의 GPP와 NIRvP 사이의 상관성이 향상되었지만, 일 단위에는 그 차이가 크지 않았다. 하지만 광조건 이외에 다른 요인에 의해 광합성이 제한되는 경우 NIRvP와 GPP 간의 상관성이 떨어져 NIRvP를 이용해 실제 배분 결과를 직접 평가하긴 어려웠으며, 주로 광 조건에 의해 광합성이 제한되는 흐린 날의 경우 NEE 배분 정확도를 평가할 수 있는 가능성이 존재하였다. 그러나 높은 시간해상도의 Vis 기반의 GPP 추정이 의미를 가지려면, VIs와 GPP간의 경험적 관계를 넘어서는 시스템 사고 및 자기-조직화와 관련된 복잡계 기반의 분석 방법이 요구된다.

• 천문학회보
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• 제40권1호
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• pp.73.2-74
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• 2015

The gas cloud G2 falling toward Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, is supposed to provide valuable information on the physics of accretion flows and the environment of the black hole. We observed Sgr A* with four European stations of the Global Millimeter Very Long Baseline Interferometry Array (GMVA) at 86 GHz on 1 October 2013 when parts of G2 had already passed the pericenter. We searched for possible transient asymmetric structure - such as jets or winds from hot accretion flows - around Sgr A* caused by accretion of material from G2. The interferometric closure phases (which are zero if the spatial brightness distribution of the target is symmetric, and deviate from zero otherwise) remained zero within errors during the observation time. We thus conclude that Sgr A* did not show significant asymmetric (in the observer frame) outflows in late 2013. Using simulations, we constrain the size of the outflows that we could have missed to ${\approx}2.5$ mas along the major axis, ${\approx}0.4$ mas along the minor axis of the beam, corresponding to approximately 232 and 35 Schwarzschild radii, respectively; we thus probe spatial scales on which the jets of radio galaxies are suspected to convert magnetic into kinetic energy. As probably less than 0.2 Jy of the flux from Sgr A* can be attributed to accretion from G2, one finds an effective accretion rate ${\eta}M{\leq}1.5{\times}10^9kg/s{\approx}7.7{\times}10^{-9}M_{earth}/yr$ for material from G2. Exploiting the kinetic jet power-accretion power relation of radio galaxies, one finds that the rate of accretion of matter that ends up in jets is limited to $M{\leq}10^{17}kg/s{\approx}0.5M_{Earth}/yr$ less than about 20% of the mass of G2. Accordingly, G2 appears to be largely stable against loss of angular momentum and subsequent (partial) accretion at least on time scales ${\leq}1$ year.

• 한국항공우주학회지
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• 제48권5호
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• pp.355-361
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• 2020

인공위성 중 군사적 성격을 띠는 저궤도 소형 인공위성의 경우 다표적 관측을 필요로 하고 고해상도의 사진 및 영상의 수요가 증가하는 추세이다. 고해상도 영상과 다표적 관측을 위해 인공위성의 기동성이 가장 큰 변수로 작용한다. 소형 인공위성의 경우 고기동성을 갖게 되면 빠르게 자세기동을 할 수 있지만 자세 기동을 완료 후 다음 자세 기동을 할 때 잔류진동이 발생하게 된다. 이에 본 연구에서 자세 기동 후 발생하는 평판의 진동 특성을 검증하기 위하여 자세기동을 모사하기 위한 실험 치구를 제작하고 실험을 수행하였다. 추가로 이러한 진동을 저감시키기 위해 영구자석을 이용한 수동형 감쇠방법으로 와전류 브레이크 시스템을 응용한 와전류 감쇠기를 제시하였다. 와전류 감쇠기를 적용하기 위하여 수학적 모델을 정립하였으며 영구자석의 자속밀도와 공극거리에 따라 이를 실험적으로 구현하였으며, 4개의 태양전지판(평판) 중 1개 평판을 특정하여 와전류감쇠기를 적용유무에 따라 자세 기동 후 발생하는 잔류진동에 대한 저감 성능을 실험적으로 검증하였다.

• 한국대기환경학회지
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• 제14권4호
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• pp.369-377
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• 1998

To examine various aspects of Hg exchange processes, we measured Hg$^{\circ}$concentration gradients over soil surfaces in a residential area of Seoul during Sept. 1997. From these measurements, we found that Hg$^{\circ}$concentrations in lower(20 cm) and upper(200 cm) levels varied in the range of 3.15~14.38 (5.30$\pm$1.88: N=236) and 2.07~15.10ng/m$^3$(4.06$\pm$1.69: N=236), respectively. When our data were divided into emission and dry deposition, emission of Hg$^{\circ}$was overwhelmingly dominant (up to 98% in frequency) over dry deposition. The concentration gradients for emission and deposition events were 1.29$\pm$0.86(N=231) and -1.0$\pm$1.27ng/m$^3$(N=5), respectively. The observation of excessively high concentrations in both levels and development of strong gradients suggest that our study site be greatly affected by certain pollution sources of mercury. In face, those data were quite comparable to that had previously been observed from highly contaminated soil environs of Tennessee, USA. To provide some insights into the processes governing the Hg$^{\circ}$exchange processes, we have conducted correlation analyses between Hg$^{\circ}$data and other concurrently determined meteorological plus chemical data. In general, Hg$^{\circ}$concentrations of both levels exhibited similarly the existence of strong correlations with parameters like windspeed, temperature, and relative humidity. Although its concentration gradient data showed similarly strong correlations with meteorological parameters, they showed somewhat unique patterns in that their correlations with Hg$^{\circ}$concentration were noticeably stronger for the lower level than the upper level. To provide rough estimates of Hg$^{\circ}$fluxes in this study, we computed its flux using our gradient data and the predicted K values from previous studies. According to this approach, Hg$^{\circ}$emissions were generally in the range of 103$\pm$80(N=231), while its depositions, being scarcely found, were on the similar magnitude of -92$\pm$128ng/m$^2$/hr(N=5). The findings of excessive emission of Hg$^{\circ}$in residential area of Korea suggests that contamination of mercury be a significant process and hence be dealt more seriously.