• 지구물리
• /
• 제9권2호
• /
• pp.135-145
• /
• 2006

미국 해양대기청의 CCM3 기후모델을 이용하여 마지막최대빙하기 (Last Glacial Maximum(LGM)의 기온 및 물. 이용된 수치모델의 수평해상도는 약 75 km로 비교적 상세한 기후 기작들이 표현된다. LGM 실험은 CLIMAP 프로젝트에서 복원된 표층해수가 경계조건으로 이용되었으며 , LGM에 낮았던 대기 이산화탄소농도(200 pm) 이 적용되었고, 대륙빙하를 포함한 LGM 지표지형이 표현되었다 . LGM 경계조건하에서 전구온도는 겨울철 6.1도 여름철 5.6도 그리고 연평균 6도정도 감소한 것으로 시뮬레이션 된다 . 표층 기온의 감소는 14% 감소하고 여름에 17% 그리고 연간 13% 감소한다. 하지만, 미국, 남부유럽, 동아프리카, 남아메리카 등은 겨울에 현재보다 더 습하게 나타나며 , 캐나다 와 중동 지방은 여름철에 습윤하게 시뮬레이션 된다 . 이런 결과들은 호수면 변화기록으로부터 복원한 고기후 프락시 물수지 자료들과도 대체로 잘 일치한다 . 전체적으로 고해상도 기후모델은 지상에서 나타나는 세부적인 특징들을 잘 재현해내고 있다 .

• International Journal of Oral Biology
• /
• 제46권3호
• /
• pp.105-110
• /
• 2021

The physicochemical properties of crystalline titanium dioxide nanoparticles (TiO₂ NPs) were investigated by comparing amorphous (amTiO₂), anatase (aTiO₂), metaphase of anatase-rutile (arTiO₂), and rutile (rTiO₂) NPs, which were prepared at various calcination temperatures (100℃, 400℃, 600℃, and 900℃). X-ray diffraction (XRD) and scanning electron microscopy (SEM) analyses confirmed that the phase-transformed TiO₂ had the characteristic features of crystallinity and average size. The surface chemical properties of the crystalline phases were different in the spectral analysis. As anatase transformed to the rutile phase, the band of the hydroxyl group at 3,600-3,100 cm^-1 decreased gradually, as assessed using Fourier transform infrared spectroscopy (FT-IR). For ultraviolet-visible (UV-Vis) spectra, the maximum absorbance of anatase TiO₂ NPs at 309 nm was blue-shifted to 290 nm at the rutile phase with reduced absorbance. Under the electric field of capillary electrophoresis (CE), TiO₂ NPs in anatase migrated and detected as a broaden peak, whereas the rutile NPs did not. In addition, anatase showed the highest photocatalytic activity in an UV-irradiated dye degradation assay in the following order: aTiO₂ > arTiO₂ > rTiO₂. Overall, the phases of TiO₂ NPs showed characteristic physicochemical properties regarding size, surface chemical properties, UV absorbance, CE migration, and photocatalytic activity.

• 대한원격탐사학회지
• /
• 제34권6_2호
• /
• pp.1239-1249
• /
• 2018

광학 위성영상은 레이더 영상에 비해 시각적으로 친숙한 영상을 제공한다. 하지만해빙종류에 대한 구분은 분광학적으로 쉽지 않아 기존 기계학습에서 주로 사용하는 분광정보를 이용한 분류기법을 이용했을 경우 광학영상에서 해빙종류의 구분은 매우 어렵다. 본 연구에서는 분광정보 기반의 분류모델이 아닌 딥러닝 기반 분류기법인 semantic segmentation을 이용하여 계층적, 공간적 패턴을 학습하여 해빙종류 분류를 수행하였다. 또한 주기적으로 획득되는 광학위성자료에 비해 감독분류에서 매우 중요한 양질의 레이블 자료는 수집하는데 있어 높은 시간 및 노동 비용이 소모된다. 본 연구에서는 부족한 레이블 자료로 인해 어려운 다중영상에 대한 감독분류 문제를 준지도학습과 능동학습의 결합을 통해 해결을 시도 하였다. 이를 통해 레이블 되지 않은 새로운 영상자료로부터 추가적인 레이블을 스스로 학습하여 분류모델을 강화할 수 있었으며, 이는 향후 광학영상 기반의 운영 가능한 해빙종류 산출물 개발에도 적용될 수 있을 것으로 기대된다.

• International Journal of Computer Science & Network Security
• /
• 제22권4호
• /
• pp.193-202
• /
• 2022

The classification of hyperspectral imagery (HSI) is essential in the surface of earth observation. Due to the continuous large number of bands, HSI data provide rich information about the object of study; however, it suffers from the curse of dimensionality. Dimensionality reduction is an essential aspect of Machine learning classification. The algorithms based on feature extraction can overcome the data dimensionality issue, thereby allowing the classifiers to utilize comprehensive models to reduce computational costs. This paper assesses and compares two HSI classification techniques. The first is based on the Joint Spatial-Spectral Stacked Autoencoder (JSSSA) method, the second is based on a shallow Artificial Neural Network (SNN), and the third is used the SVM model. The performance of the JSSSA technique is better than the SNN classification technique based on the overall accuracy and Kappa coefficient values. We observed that the JSSSA based method surpasses the SNN technique with an overall accuracy of 96.13% and Kappa coefficient value of 0.95. SNN also achieved a good accuracy of 92.40% and a Kappa coefficient value of 0.90, and SVM achieved an accuracy of 82.87%. The current study suggests that both JSSSA and SNN based techniques prove to be efficient methods for hyperspectral classification of snow features. This work classified the labeled/ground-truth datasets of snow in multiple classes. The labeled/ground-truth data can be valuable for applying deep neural networks such as CNN, hybrid CNN, RNN for glaciology, and snow-related hazard applications.

• 농업과학연구
• /
• 제49권3호
• /
• pp.495-510
• /
• 2022

In this study, fluorescence hyperspectral imaging (FHSI) was used for the rapid, non-destructive detection of fake, manmade eggs from real eggs. To identify fake eggs, protoporphyrin IX (PpIX)-a natural pigment present in real eggshells-was utilized as the main indicator due to its strong fluorescence emission effect. The fluorescence images of real and fake eggs were acquired using a line-scan-based FHSI system, and their fluorescence features were analyzed based on spectroscopic techniques. To improve the detection performance and accuracy, an optimal waveband combination was investigated with analysis of variance (ANOVA), and its fluorescence ratio images (588/645 nm) were created for visualization of the real eggs between two different egg groups. In addition, real and fake eggs were scanned using a one-waveband (645 nm) handheld fluorescence imager that can perform real-time scanning for on-site applications. Then, the results of the two methods were compared with one another. The outcome clearly shows that the newly developed FHSI system and the fluorescence handheld imager were both able to distinguish real eggs from fake eggs. Consequently, FHSI showed a better performance (clearer images) compared to the fluorescence handheld imager, and the outcome provided valuable information about the feasibility of using FHSI imaging with ANOVA for the discrimination of real and fake eggs.

• 한국지구과학회지
• /
• 제43권3호
• /
• pp.351-366
• /
• 2022

우리는 CFHT에 부착된 OASIS 분광기, MR 1 그리즘으로 관측한 방출선 중, H𝛽와 [O III] 5007 방출선을 분석하여, 제 2형 세이퍼트 은하 Mrk 1의 운동학적 특성을 파악하였다. [O III] 금지선의 가우시안 선 윤곽 분석을 통해 초과하는 청색 이동 성분의 방출 영역이 비대칭적으로 보이는데, (1) 은하 중심부 약 960 pc거리에서 플럭스는 최대를 보이고, (2) 은하 중심부에서 NS 방향으로 ~900 km s^-1인 큰 선폭 지역이 있음을 확인하였다. 두 원소의 분광 영상에서 보이는 시선 속도의 특징은 NE 방향에서 접근하는 가스의 흐름이, SW 방향으로 적색 이동, 즉 멀어지는 가스의 흐름이 나타나 반시계 방향 은하의 회전 경향성을 보여준다. 시선 속도 자료로부터 은하 중심은 우리를 향해 접근하는 먼지 가스가 가리고 있음을 파악하였다.

• Nuclear Engineering and Technology
• /
• 제55권9호
• /
• pp.3268-3276
• /
• 2023

The practice of identifying the potential zones for mineral exploration in a speedy and low-cost method includes the use of satellite imagery analysis as a part of remote sensing techniques. It is challenging to explore the iron mineralization of a region through conventional methods which are a time-consuming process. The current study utilizes the Hyperion satellite imagery for mapping the iron mineralization and associated geological features in the Irikkur region, Kannur, Kerala. Along with the remote sensing results, the field study and laboratory-based analysis were conducted to retrieve the ground truth point and geochemical proportion to verify the iron ore mineralization. The MC simulation showed for shielding properties indicate an increase in the linear attenuation coefficient with raising the Fe₂O₃+SiO₂ concentrations in the investigated rocks where it is varied at 0.662 MeV in the range 0.190 cm^-1 - 0.222 cm^-1 with rising the Fe₂O₃+SiO₂ content from 57.86 wt% to 71.15 wt%. The analysis also revealed that when the γ-ray energy increased from 0.221 MeV to 2.506 MeV, sample 1 had the largest linear attenuation coefficient, ranging from 9.33 cm1 to 0.12 cm^-1. Charnockite rocks were found to have exceptional shielding qualities, making them an excellent natural choice for radiation shielding applications.

• 한국정보통신학회:학술대회논문집
• /
• 한국정보통신학회 2022년도 춘계학술대회
• /
• pp.453-455
• /
• 2022

메타데이터는 데이터에 대한 속성이나 특징을 설명하는 구조화된 데이터를 말한다. 그중에서 비디오 메타데이터는 정확한 콘텐츠 기반 검색을 위해 비디오를 구성하는 정보에서 추출한 데이터를 의미한다. 최근 영상 콘텐츠를 이용하는 사용자들이 늘어나면서 자연스럽게 OTT 제공 업체들 역시 늘어나고 있으며, OTT 제공 업체에서 많은 양의 영상 콘텐츠를 개인 사용자에게 추천 또는 알맞은 검색을 위해 메타데이터의 역할이 중요해지고 있다. 본 논문에서는 영상의 효과음을 통해 분위기 속성에 대한 메타데이터를 자동으로 추출하는 방법에 관해 연구를 진행하였다. 영상의 효과음에 대한 분류와 분위기 속성에 대한 메타데이터 생성을 위해 분위기에 대한 용어사전을 구축하고 지도학습을 통해 정보를 추출하는 방법을 제안하고자 한다.

• 천문학회보
• /
• 제46권2호
• /
• pp.66.3-67
• /
• 2021

Low-mass stars form by the gravitational collapse of dense molecular cores. Observations and theories of low-mass protostars both suggest that accretion bursts happen in timescales of ~100 years with high accretion rates, so called episodic accretion. One mechanism that triggers accretion bursts is infalling fragments from the outer disk. Such fragmentation happens when the disk is massive enough, preferentially activated during the embedded phase of star formation (Class 0 and I). Most observations and models focus on the gas structure of the protostars undergoing episodic accretion. However, the dust and ice composition are poorly understood, but crucial to the chemical evolution through thermal and energetic processing via accretion burst. During the burst phase, the surrounding material is heated up, and the chemical compositions of gas and ice in the disk and envelope are altered by sublimation of icy molecules from grain surfaces. Such alterations leave imprints in the ice composition even when the temperature returns to the pre-burst level. Thus, chemical compositions of gas and ice retain the history of past bursts. Infrared spectral observations of the Spitzer and AKARI revealed a signature caused by substantial heating, toward many embedded protostars at the quiescent phase. We present the AKARI IRC 2.5-5.0 ㎛ spectra for embedded protostars to trace down the characteristics of accretion burst across the evolutionary stages. The ice compositions obtained from the absorption features therein are used as a clock to measure the timescale after the burst event, comparing the analyses of the gas component that traced the burst frequency using the different refreeze-out timescales. We discuss ice abundances, whose chemical change has been carved in the icy mantle, during the different timescales after the burst ends.

• 천문학회보
• /
• 제45권1호
• /
• pp.30.1-30.1
• /
• 2020

The ASKAP-EMU survey is a deep wide-field radio continuum survey designed to cover the entire southern sky and a significant fraction of the northern sky up to +30°. Here, we report a discovery of a radio relic in the merging cluster SPT-CL J2023-5535 at z=0.23 from the ASKAP-EMU pilot 300 square degree survey (800-1088 MHz). The deep high-resolution data reveal a ~2 Mpc-scale radio halo elongated in the east-west direction, coincident with the intracluster gas. The radio relic is located at the western edge of this radio halo stretched ~0.5 Mpc in the north-south orientation. The integrated spectral index of the radio relic within the narrow bandwidth is α1088MHz800MHz = -0.76 ± 0.06. Our weak-lensing analysis shows that the system is massive (M200 = 1.04 ± 0.36 × 1015M⊙) and composed of at least three subclusters. We suggest a scenario, wherein the radio features arise from the collision between the eastern and middle subclusters. Furthermore, the direct link between the local AGN and the relic along with the discontinuities in X-ray observation hint us that we are looking at the site of re-acceleration.