• 천문학회지
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• 제14권2호
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• pp.55-71
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• 1981

On the basis of observational constraints, particularly the relationship between metal abundance and cumulative stellar mass, a simple two-zone disk-halo model for the chemical evolution of our Galaxy was investigated, assuming different chemical processes in the disk and halo and the infall rates of the halo gas defined by the halo evolution. The main results of the present model calculations are: (i) The halo formation requires more than 80% of the initial galactic mass and it takes a period of $2{\sim}3{\times}10^9$ yrs. (ii) The halo evolution is divided into two phases, a fast collapse phase ($t=2{\sim}3{\times}10^8$ yrs) during which period most of the halo stars $({\sim}95%)$ are formed and a later slow collapse phase which is characterized by the chemical enrichment due to the inflow of external matter to the halo. (iii) The disk evolution is also divided into two phases, an active disk formation phase with a time-dependent initial mass function (IMF) up to $t{\approx}6{\times}10^9$ yrs and a later steady slow formation phase with a constant IMF. It is found that at the very early time $t{\approx}5{\times}10^8$ yrs, the metal abundance in the disk is rapidly increased to ${\sim}1/3$ of the present value but the total stellar mass only to ${\sim}10%$ of the present value, finally reaching about 80% of the present values toward the end of the active formation phase.

• 한국환경복원기술학회지
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• 제17권5호
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• pp.79-89
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• 2014

This study was carried out to provide basic information to improve the surrounding ecosystems with benefit analysis and monitoring in cut slopes following establishment of a test construction to improve ecological environment in slopes of an expressway. Field tests from October 2012 to May 2013 were conducted in Seosejong IC and Shinyang IC. In order to improve the view of slopes, soil condition is an important factor. The earth slope, it is possible to introduce directly the plant. Stable construction method was applied, another foundation for planting is necessary. The mixing ratio of the seeds according to the experimental results, the difference was found at an early stage plants in Site I (Seosejong IC). Trees were planted on terraced structures were well coordinated and pictures. The growth of planted trees was good in Site II (Shinyang IC). Due to the use of plants in the landscape will continue to change. Thus, long-term monitoring and landscape analysis will be needed.

• 한국해양학회지
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• 제18권2호
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• pp.142-148
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• 1983

錦江河口의 6個定點에서 大.小潮기에 Instantaneous profiling技法으로 同時 觀測한 鹽分値를 분석하여 鹽分境界層의 變化特性을 밝혔다. 錦江河口를 鹽分境界層의 變化特性으로 分流해 본 缺課 定常波型河口(standing wave type estuary)임이 再次確認(Chung, 1981)되었으며 變化의 크기는 上流로 갈수록 커짐도 아울러 밝혀 졌다. 또한 鹽分境界層의 變化는 大潮期 보다 小潮期에 큼도 밝혀 졌다. 鹽分境界層(S<10%)의 持續時間은 小潮期에 越等히 긴데, Shinri-Saugke斷面 보다 上流域에서는 6時間以上 持續되고 Sochgot-Kupo斷面 사이에서는 0-3時間童 顔 持續됨이 밝혀 졌다. 따라서 錦江河口에서의 堆積作用은 持續時間의 分布特性에 따른 區域別의 Flocculation作用의 强弱에 의해 支配되고 있음도 아울러 밝혀 졌다.

• 자원환경지질
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• 제27권4호
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• pp.335-343
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• 1994

The Eonyang amethyst deposits are composed of vug quartz emplaced in the Eonyang granites of Mesozoic Cretaceous age. The Eonyang granites are composed of biotite granite, porphyritic biotite granite, aplite and miarolitic granite. The petrochemical data of the Eonyang granites show the trend of subalkaline magma, calc-alkaline magma, I-type granitoid and magnetite series. The vug quartz show the characteristic growth zoning (white quartz-smoky quartz-amethyst) from wall side. Generally fluid inclusions in the vug quartz can be divided into four main types based on compositions (I-type: gas inclusion, II-type: liquid inclusion, III-type: polyphase inclusion, IV-type: liquid $CO_2$-bearing inclusion). Solid phase of polyphase inclusions are halite(NaCl), sylvite(KCl), hematite ($Fe_2O_3$) and unknown anisotropic solid. Homogenization temperatures inferred from the fluid inclusion study ranges from $440^{\circ}C$ to $485^{\circ}C$ in white quartz, from $227^{\circ}C$ to $384^{\circ}C$ in smoky quartz, from $133^{\circ}C$ to $186^{\circ}C$ in amethyst, respectively. Salinities of fluid inclusions in each mineralization stages ranges from 40 wt.% to 58 wt.% in white and smoky quartz, from 1.0 wt.% to 8.7 wt.% in amethyst respectively. A consideration of the pressure regime during vug quartz deposition based on the boiling evidence suggests lithostatic pressure of less than 72 bars. This range of pressure indicate that vug quartz lay at depth of 750 m below the surface at the during mineralization.

• 대한원격탐사학회지
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• 제38권5_3호
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• pp.851-861
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• 2022

본 연구는 전산유체역학(computational fluid dynamics, CFD) 모델을 이용하여 도시 지역에서 수목이 PM_2.5 저감에 미치는 영향을 조사하였다. 현실적인 수치 모의를 위해, 기상청에서 현업으로 운영 중인 국지예보시스템(LDAPS)이 예측한 기상 자료를 CFD 모델의 초기·경계 자료로 사용하였다. CFD 모델 성능 검증은 연구 대상지 내에 구축된 6개의 센서에서 측정한 PM_2.5 농도를 이용하였다. 본 연구에서는 수목이 PM_2.5 농도 분포에 미치는 영향을 분석하기 위하여, 수목이 식재 되지 않았다고 가정한 경우, 수목이 식재되어 있지만 바람에 대한 항력 효과만 존재한다고 가정한 경우, 수목의 항력 효과와 침적 효과가 모두 존재한다고 가정한 경우에 대한 수치 실험을 수행하였다. 분석대상 기간 동안 PM_2.5 저감 효과가 뚜렷하게 나타난 세 가지 영역 중 군부대 내의 PM_2.5 평균 농도를 비교한 결과, 수목이 식재되지 않은 경우는 12.8 ㎍ m^-3, 수목의 항력 효과만 고려한 경우는 12.5 ㎍ m^-3이 나타났고, 수목의 항력 효과와 침적 효과가 모두 고려한 경우는 6.8 ㎍ m^-3가 나타났다. 수목에 의한 건성 침적이 PM_2.5 농도를 감소시키는 효과가 있는 것으로 확인되었다.

• 천문학회지
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• 제36권spc1호
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• pp.125-133
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• 2003

New Jersey Institute of Technology (NJIT), in collaboration with the University of Hawaii (UH), is upgrading Big Bear Solar Observatory (BBSO) by replacing its principal, 65 cm aperture telescope with a modern, off-axis 1.6 m clear aperture instrument from a 1.7 m blank. The new telescope offers a significant incremental improvement in ground-based infrared and high angular resolution capabilities, and enhances our continuing program to understand photospheric magneto-convection and chromospheric dynamics. These are the drivers for what is broadly called space weather - an important problem, which impacts human technologies and life on earth. This New Solar Telescope (NST) will use the existing BBSO pedestal, pier and observatory building, which will be modified to accept the larger open telescope structure. It will be operated together with our 10 inch (for larger field-of-view vector magnetograms, Ca II K and Ha observations) and Singer-Link (full disk H$\alpha$, Ca II K and white light) synoptic telescopes. The NST optical and software control design will be similar to the existing SOLARC (UH) and the planned Advanced Technology Solar Telescope (ATST) facility led by the National Solar Observatory (NSO) - all three are off-axis designs. The NST will be available to guest observers and will continue BBSO's open data policy. The polishing of the primary will be done in partnership with the University of Arizona Mirror Lab, where their proof-of-concept for figuring 8 m pieces of 20 m nighttime telescopes will be the NST's primary mirror. We plan for the NST's first light in late 2005. This new telescope will be the largest aperture solar telescope, and the largest aperture off-axis telescope, located in one of the best observing sites. It will enable new, cutting edge science. The scientific results will be extremely important to space weather and global climate change research.

• 천문학회보
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• 제46권2호
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• pp.37.3-38
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• 2021

One of the key questions on star formation is how the organic molecules are synthesized and delivered to the planets and comets since they are the building blocks of prebiotic molecules such as amino acid, which is thought to contribute to bringing life on Earth. Recent astrochemical models and experiments have explained that complex organic molecules (COMs; molecules composed of six or more atoms) are produced on the dust grain mantles in cold and dense gas in prestellar cores. However, the chemical networks and the roles of physical conditions on chemistry are not still understood well. To address this question, hot (> 100 K) cores in high mass young stellar objects (M > 8 Msun) are great laboratories due to their strong emissions and larger samples than those of low-mass counterparts. In addition, CH₃OH masers, which have been mostly found in high mass star forming regions, can provide constraints due to their very unique emerging mechanisms. We investigate twelve high mass star forming regions in ALMA band 6 observation. They are associated with 44/95 GHz Class I and 6.7 GHz Class II CH3OH masers, implying that the active accretion processes are ongoing. For these previously unresolved regions, 66 continuum peaks are detected. Among them, we found 28 cores emitting COMs and specified 10 cores associated with 6.7 GHz Class II CH3OH masers. The chemical diversity of COMs is found in cores in terms of richness and complexity; we identified up to 19 COMs including oxygen- and nitrogen-bearing molecules and their isotopologues in a core. Oxygen-bearing molecules appear to be abundant and more complex than nitrogen-bearing species. On the other hand, the COMs detection rate steeply grows with the gas column density, which can be attributed to the effective COMs formation in dense cores.

• 대기
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• 제14권4호
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• pp.3-18
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• 2004

Neglecting the vertical transport from the surface, most of the previous studies on the long-range transport of pollutants have only considered the horizontal transport caused by the free atmosphere wind. I used a three dimensional numerical model, MM5 (The fifth generation Penn State Univ./NCAR Mesoscale Model) for the simulation of vertical transport of pollutants and investigated the mechanism of the vertical transport of atmospheric pollutants between planetary boundary layer(PBL) and free atmosphere by fronts. From the three dimensional simulation of MM5, the amount of pollutants transport from PBL to free atmosphere is 48% within 18 hour after the development of front, 55% within 24 hour, and 53% within 30 hour. The ratios of the vertically transported pollutant for different seasons are 62%, 60%, 54%, and 43% for spring, summer, fall, and winter, respectively. The most active areas for the vertical transport are the center of low pressure and the warm sector located east side of cold front, in which the strong upward motion slanted northward occurs. The horizontal advection of pollutants at the upper level is stronger than at the lower level simply because of the stronger wind speed. The simulation results shows the well known plum shape distribution of pollutants. The high concentration area is located in the center and north of the low pressure system, while the second highest concentration area is in the warm sector. It is shown that the most important mechanism for the vertical transport is vertical advection, while the vertical diffusion process plays an important role in the redistribution of pollutants in the PBL.

• 대한원격탐사학회지
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• 제39권6_2호
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• pp.1605-1613
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• 2023

해양 내의 다양한 물리적 변화는 수온과 염분의 지속적인 변동에 의해 결정된다. 수온과 더불어 넓은 영역의 염분 변화를 파악하기 위해서는 인공위성 자료에 의존할 수밖에 없다. 그럼에도 불구하고 염분을 관측하는 위성인 Soil Moisture Active Passive (SMAP)는 낮은 시·공간 해상도로 인해 연안 근처에서 빠르게 변화하는 해양환경을 관측하기에는 어렵다는 한계가 존재한다. 이러한 한계를 극복하기 위해 본 연구에서는 천리안 해양 관측 위성의 정지궤도 해색 센서인 Geostationary Ocean Color Imager-II (GOCI-II) 원격반사도 자료를 입력자료로 하여 고해상도 표층 염분을 산출하는 Multi-layer Perceptron Neural Network (MPNN) 기반의 알고리즘을 개발하였다. SMAP과 비교한 결과 coefficient of determination (R²)는 0.94, root mean square error (RMSE)는 0.58 psu 그리고 relative root mean square error (RRMSE)는 1.87%였으며, 공간적인 분포 또한 매우 유사한 결과를 나타냈다. R²의 공간 분포는 0.8 이상을 보여주었으며 RMSE는 전반적으로 1 psu 이하의 낮은 값을 보여주었다. 이어도 과학기지에서의 실측 염분값과도 비교하였지만 상대적으로 조금 낮은 결과를 보여주었다. 이에 대한 원인을 분석하였으며, 산출된 GOCI-II 기반 고해상도 염분 자료를 활용하여 2022년 11호 태풍 힌남노에 의한 하루 동안의 동중국해 표층 염분 변화를 표준편차로 계산하였다. 그 결과 SMAP에서 관측할 수 없는 시공간의 염분 변화를 고해상도의 GOCI-II 기반 염분 산출물을 통해 확인할 수 있었다. 따라서 본 연구를 통해 시간 단위로 변화하는 해양환경 모니터링에 큰 기여를 할 것으로 기대된다.

• 대한지하수환경학회지
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• 제5권3호
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• pp.155-161
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• 1998

토립자 표면에서의 흡착에 의한 토양에서의 중금속의 지연효과는 잘 알려진 현상이다. 본 연구에서는 배치시험과 주상시험을 수행함으로써 사질 토양에서 Zn의 이동성에 대한 지연효과를 조사하였다. 주상시험은 파과곡선(BTC)으로 알려진 시간에 따른 용액의 농도를 측정함으로써 수행되었다. 추적자로는 10 g/L 농도의 NaCl과 ZnCl$_2$를 사용하였고, 각각의 용액을 토양시료의 상부경계에 순간주입한 후 정상류 상태에서 배출구로 빠져나온 용탈수의 농도를 EC-meter와 ICP-AES를 이용하여 측정하였다. 배치시험은 표준절차에 근거하여 이루어졌으며, 토양시료로부터 선별된 미세입자들을 다양한 초기농도의 ZnCl$_2$용액과 반응시켜 평형상태의 Zn 이온의 농도를 ICP를 이용하여 분석하였다. 주상시험의 결과는 i) ICP-AES에 의해 분석된 ZnCl$_2$의 첨두농도는 NaCl이나 총전기전도도로부터 구한 값보다 상당히 낮았고, ii) 두 종류의 추적자 모두 첨두농도의 도달시간은 상당히 일치하였다. 상대적으로 낮은 Zn의 농도는 Zn과 다른 양이온들간의 이온교환반응이 일어났고, 용탈수의 pH가 높은 값의 범위(7.0~7.9)에 있는 것으로 보아 Zn(OH)$_2$의 형태로 침전되었을 가능성이 있다는 것으로 설명될 수 있다. 첨두농도의 도달시간이 일치한다는 결과는 토양시료에서 지연효과가 일어나지 않았다는 것을 지시한다. Zn 이온의 뚜렷한 감소를 설명할 수 있는 유일한 방법은 CDE 모델에 용액상태에서 Zn 이온의 절대적 감소를 고려하는 감쇄계수(decay or sink coefficient)를 적용하는 것이었다.