We have mapped 1 deg2 region toward a high latitude cloud MBM 40 in the J = 1 - 0 transition of 12CO and 13CO, using the 3 mm SIS receiver on the 14 m telescope at Taeduk Radio Astronomy Observatory. We used a high resolution autocorrelator to resolve extremely narrow CO linewidths of the molecular gas. Though the linewidth of the molecular gas is very narrow (FWHP < 1 km s-1), it is found that there is an evident velocity difference between the middle upper part and the lower part of the cloud. Their spectra for both of 12CO and 13CO show blue wings, and the position-velocity map shows clear velocity difference of 0.4 km s-1 between two parts. The mean velocity of the cloud is 3.1 km s-1. It is also found that the linewidths at the blueshifted region are broader than those of the rest of the cloud. We confirmed that the visual extinction is less than 3 magnitude, and the molecular gas is translucent. We discussed three mass estimates, and took a mass of 17 solar masses from CO integrated intensity using a conversion factor 2.3 × 10 20 cm -2 (K km s-1)-1. Spatial coincidence and close morphological similarity is found between the CO emission and dust far-infrared (FIR) emission. The ratio between the 100 f.Lm intensity and CO integrated intensity of MBM 40 is 0.7 (MJy/sr)/(K km s-1), which is larger than those of dark clouds, but much smaller than those of GMCs. The low ratio found for MBM 40 probably results from the absence of internal heating sources, or significant nearby external heating sources.

고분해능 전자현미경과 컴퓨터 이미지 시뮬레이션이 La이 첨가되고 또한 첨가되지 않은 Pb(Mg/ sub 1/3/Nb23/)O3고용체의 미세구조를 연구하기 위해서 사용되었다. 불규칙격자 영역의 격자 이미지는 정방정 형태와 유사 육방정 형태를 각각 보였다. 규칙격자 영역에서 Mg과 Nb의 비화학양론적인 규칙격자 구조 현상이<111>방향에 따라 관찰되었다. 실험 격자 이미지와 컴퓨터 시뮬레이션 이미지의 비교로부터, 규칙격자 구조를 가지는 영역의 장거리 규칙도는 0.2-0.7의 값을 가지고 있었고, 또한 규칙격자는 (NH4)3FeF6결정구조를 가지고 있었다. 작은 값의 장거리 규칙도를 가지는 규칙격자를 가지는 영역에서, 변형률 파형이 관찰되지 않았다. 이것은 대부분 두 양이온이 그들의 위치에 있기 때문에, 원자 변위가 없었기 때문이다.

We have mapped 1 deg2 region toward a high latitude HII region S73 (l, b) = (37°.69, 44°.55) and associated molecular cloud in 12CO J = 1 - 0, and 13CO J = 1 - 0, using the 3 mm SIS receiver on the 14 m telescope at Taeduk Radio Astronomy Observatory. A high resolution autocorrelator is used to resolve extremely narrow CO linewidths (FWHP < 1 km/s) of the molecular cloud. Though the linewidths are very narrow, it is found that there is systematic velocity gradient in the molecular gas associated with the H II region. Both of 12CO and 13CO averaged spectra are non-gaussian, and there are obvious blue wings in the spectra. It is remarkable that the linewidths at the blueshifted region are broader than those of the rest of the cloud. The CO emission does match well with the dust emission.

Recent high resolution CO observations of normal and starburst galaxies at Owens Valley Millimeter Array are summarized. While normal disk galaxies generally show exponential distribution which follows the optical blue light, starburst galaxies are often characterized by a compact (~1 kpc) nuclear complex whose surface gas mass density is strongly correlated with the observed large infrared luminosity and thus the ongoing massive star formation.

We have observed the emission of HC3N J=4-3, 5-4,10-9 and 12-11 transitions toward the Sgr B2 central region in an area of $150 with resolutions of 16'-48'. The intensities and central velocities of line profiles show significant variations with positions. In contrast to the intensities of the low J-level transitions which gradually increase from the central source toward the outside region, the HC3N emission of the high J-level transition become stronger toward 'the central radio continuum source MD5. Systematic change in the radial velocity of each line profile occurs along north-south direction. There are a few peaks in most line profiles, and these indicate that there are multiple velocity components along the line of sight. Distributions of excitation temperature and column density which were estimated from the excitation calculations show the existence of a small (1 X 2pc), hot (Tex>50K) core which contains two temperature peaks at-15' east and north of MD5. The column density of HC3N is (1-3)X1014cm-2 Column density at distant position from MD5 is larger than that in the central region. We have deduced that this 'hot-core' has a mass of 105M⊙, which is about an order of magnitude larger than those obtained by previous studies.

고분해능 전자에너지손실 및 자외선광전자 분광법을 사용하여 단결정 NbC(111)면의 산소횹착을 연구하였다. NbC(111) 표면에는 산소가 원자 및 분자상태로 흡착되었다. 산소원자는 3-fold hollow site에 흡착되며 진동수는 548cm-1이었다. 산소분자의 신축진동수는 968cm-1로서 기체상태인 산소분자의 진동수보다 크게 낮았으며, 산소분자의 흡착으로 일함수가 증가하였다. 이는 NbC(111) 기판으로부터 산소분자의 2ppig 궤도로 전자가 이동하였음을 보여주는 증거이다.

Simultaneous observations of high resolution spectra of CaII H, K, λ 8542 a n d λ 8498 have been made over a sunspot umbra (SPO 5007) by means of Sacramento Peak Observatory's HIRKHAD program with the Echelle spectrograph at the Vacuum Tower Telescope. The observed spectra scanned by SPO's fast microphotometer have been reduced for later theoretical interpretations. The reduced profiles, sampled over a region which is thought to be coolest over the spot, are presented in units of absolute intensity. The core intensity ratios of I ( K 3 ) / I ( H 3 ) ; a n d I ( λ 8498 ) / I ( λ 8542 ) arc found to be 1.3 and 1.14, respectively.

In this study, a field study was conducted to investigate the relationship between high-resolution remote images and the volumetric moisture, and the number of compaction. Changes in the shape of the surface and soil moisture content were observed and correlated with the number of compactions using roller equipment. As the compaction is repeated, the surface is flattened and the terrain curvature decreases and converges to zero. In particular, the tangential curvature changes as the number of compactions increase. Due to soil compaction, the vegetation index changed from a positive to a negative value, and most of the test site area was homogenized with a negative index. This suggests a decrease in porosity and an increase in volumetric water content associated with increasing soil compaction. Soil moisture, measured using a frequency domain reflectometry(FDR) sensor, tends to increase proportionately with the number of vibration compactions, but the correlation between the number of compactions and soil moisture is unclear. This study suggests that while it is necessary to consider the reproducibility of the experiments performed, the compaction quality of the soil can be evaluated using high-resolution terrain factors and soil moisture.

본 연구는 합성 모데나이트(Na6.6Al6.6Si41.4O96·20.4H2O, Na-MOR)를 이용한 다양한 중금속의 포획 연 구를 하기 위한 기초 단계로, 고분해능 X-선 분말 회절을 이용하여 치환체의 격자상수 및 부피 변화를 이해 하기 위한 목적으로 실험을 진행하였다. 열중량 분석법(Thermogravimetric analysis, TGA)으로 측정한 결과, 1가 양이온 치환체(Cs-MOR, Na-MOR)는 단위포 당 19.4, 20.4개의 물분자가 존재하였으며, 2가 양이온 치환 체(Pb-MOR, Sr-MOR, Cd-MOR)는 단위포 당 21, 23.1, 23.2개가 존재하는 것을 확인하였다. 측정한 모든 물 질은 사방정계에 속하는 Cmcm의 공간군을 가지는 것으로 확인할 수 있었다. 치환 전 물질인 Na-MOR과 비 교했을 때, 치환체의 (110)면과 (200)면의 회절강도가 명확하게 변화하였으나, 전체적인 피크의 위치는 거의 유사하게 나타나는 것을 확인할 수 있었다. 또한 Na-MOR에서는 확인이 되지 않았던 (220)면의 피크가 Pb-, Cd-, Sr-MOR에서 뚜렷하게 관찰되었다. 이를 통해서 양이온 치환에 따른 원자들의 분포 변화가 주로 ab-평 면상에서 나타나지만, 격자상수의 변화는 미세할 것으로 짐작할 수 있었다. Whole profile fitting 방법을 사용 하여 치환된 모데나이트의 미세한 격자상수의 변화를 관찰하였다. 치환체의 격자상수 및 격자부피의 변화는 치환된 양이온의 반경 및 전하수에 따라 서로 다른 경향성을 보였다. 1가 양이온의 경우, 이온반경이 증가할 수록 a-축의 길이는 증가하지만, 반면에 b- 및 c-축의 길이는 감소하였다. 2가 양이온의 경우, 이온반경이 증 가할수록 대체적으로 a-축의 길이가 감소하고, b- 및 c-축의 길이는 증가하였다. 격자부피는 1가 또는 2가 양 이온 치환체들이 각각 독립된 경향성을 가지며, 이온반경에 따라 증가하는 것을 확인할 수 있었다.

This study analyzed future projections on daily mean values and extremes for temperature and daily precipitation over Seoul metropolitan city using bias-corrected high-resolution multi-regional climate models. The factors of uncertainty for the future projection of climate variables were defined. In the time series analysis of future projections for regional climate models, the average daily temperature and the number of days of the hot day-hot night were predicted to have a stable trend in the RCP2.6 scenario, and showed a tendency to increase continuously in the RCP8.5 scenario. The daily mean precipitation and RX1day (annual daily maximum precipitation) had large annual variabilities in the models. In the estimation of the fraction of total variance, the daily mean temperature was dominated by the internal variability in the early 21st century and the most contributing to the scenario uncertainty in the late 21st century. The daily mean precipitation showed a remarkable contribution from the internal variability over the entire period. The number of days of the hot day-hot night showed a similar contribution pattern to that of the daily mean temperature. For the RX1day, the internal variability dominated over the entire period, and the scenario uncertainty had little contribution. This study will help establish more scientific climate change adaptation policies by providing the uncertainty information for future climate change projection.

High-resolution meteorological simulations were conducted using a Weather Research and Forecasting (WRF) model with an Urban Canopy Model (UCM) in the Ulsan Metropolitan Region (UMR) where large-scale industrial facilities are located on the coast. We improved the land cover input data for the WRF-UCM by reclassifying the default urban category into four detailed areas (low and high-density residential areas, commercial areas, and industrial areas) using subdivided data (class 3) of the Environmental and Geographical Information System (EGIS). The urban area accounted for about 12% of the total UMR and the largest proportion (47.4%) was in the industrial area. Results from the WRF-UCM simulation in a summer episode with high temperatures showed that the modeled temperatures agreed greatly with the observations. Comparison with a standard WRF simulation (WRF-BASE) indicated that the temporal and spatial variations in surface air temperature in the UMR were properly captured. Specifically, the WRF-UCM reproduced daily maximum and nighttime variations in air temperature very well, indicating that our model can improve the accuracy of temperature simulation for a summer heatwave. However, the WRF-UCM somewhat overestimated wind speed in the UMR largely due to an increased air temperature gradient between land and sea.

This paper has identified detailed climate types and their geographical extents in the Republic of Korea using MK (Modified Korean)-PRISM (Parameter-elevation Regression on Independent Slopes Model) 1×1km high-resolution grid climate data and Trewartha climate classification. When considering 60 ASOS (The Automated Synoptic Observing Systems) stations, only four climate types were identified over South Korea. Three climate types, Dca (52%), Doa (28%) and Cfa (18%), were prevalent while Dcb type was only located at Daegwallyeong. When based on a high-resolution grid climate data, six climate types were identified including Dob and E types which were not detected with ASOS stations. High-resolution grid climate data reflected better and detailed geographical characteristics. Areas occupied by Cfa climate types were located along the narrow southern and Jeju coastal areas, dedicating only 6.9% of South Korea. Trewartha climate classification was also applied to 1km×1km RCP scenarios. The most distinct feature of future climate changes based on RCPs was a larger expansion of Cfa and Doa types with a drastic reduction of Dca and Dcb, indicating that a warmer and wetter climate would be prevalent over South Korea in the latter period of this century. Even for RCP2.6, all the coastal areas, some of Seoul metropolitan area, a large part of Daegu and Gwangju metropolitan areas would be classified as Cfa. For RCP8.5, 51.5% of South Korea would be occupied by the Cfas and 25.1% by the Doas, leaving only 23.2% of Dcas.