• 대한원격탐사학회지
• /
• 제25권6호
• /
• pp.517-529
• /
• 2009

Many satellite image fusion techniques have been developed in order to produce a high resolution multispectral (MS) image by combining a high resolution panchromatic (PAN) image and a low resolution MS image. Heretofore, most high resolution image fusion techniques have used IKONOS and QuickBird images. Recently, GeoEye-1, offering the highest resolution of any commercial imaging system, was launched. In this study, we have experimented with GeoEye-1 images in order to evaluate which fusion algorithms are suitable for these images. This paper presents compares and evaluates the efficiency of five image fusion techniques, the $\grave{a}$ trous algorithm based additive wavelet transformation (AWT) fusion techniques, the Principal Component analysis (PCA) fusion technique, Gram-Schmidt (GS) spectral sharpening, Pansharp, and the Smoothing Filter based Intensity Modulation (SFIM) fusion technique, for the fusion of a GeoEye-1 image. The results of the experiment show that the AWT fusion techniques maintain more spatial detail of the PAN image and spectral information of the MS image than other image fusion techniques. Also, the Pansharp technique maintains information of the original PAN and MS images as well as the AWT fusion technique.

• Mass Spectrometry Letters
• /
• 제9권3호
• /
• pp.73-76
• /
• 2018

The number of matched peaks (NMP) is estimated as the spectral similarity measure in tandem mass spectral library searches of small molecules. In the high resolution mode, NMP provides the same reliable identification as in the case of a common dot-product function. Corresponding true positive rates are ($94{\pm}3$) % and ($96{\pm}3$) %, respectively.

• 대한원격탐사학회지
• /
• 제35권6_2호
• /
• pp.1095-1106
• /
• 2019

산불 피해는 복구, 보상 및 2차 피해 예방을 위해 빠르고 정확히 조사되어야 한다. 원격탐사 기반의 산불 피해강도 조사 방법으로 주로 산불 전과 후의 반사율 및 분광지수의 차이를 비교하고 있다. 최근 고해상도 위성영상 및 무인기 영상의 활용이 증가하고 있으나, 언제 어디에서 발생할지 예측할 수 없는 산불에 대한 발생 전 영상을 획득하는 것이 쉽지 않다. 본 연구에서는 산불 피해강도 분류에 있어 고해상도 영상과 감독분류 기법의 활용 가능성을 분석하고자 하였다. 산불 후에 촬영된 KOMPSAT-3A 영상과 무인기 다중분광영상에 반사율의 절대값을 이용하는 최대우도법과 반사율의 패턴을 이용하는 분광각매퍼의 두 가지 감독분류 기법을 적용하였다. 그 결과 분류 기법 측면에서 최대우도법이 분광각매퍼에 비해 높은 분류정확도를 보여주었으며, 이는 피해강도 등급 간에 분광반사율의 절대값은 다르지만 패턴이 유사한 등급들이 존재하기 때문인 것으로 판단된다. 공간해상도 측면에서 상대적으로 해상도가 높은 무인기 영상의 분류정확도가 위성영상보다 높게 나타났다. 그러나 무인기와 위성 영상 모두 분류정확도가 매우 높게 나타나고 있어 피해강도 분류에 활용 가능성이 높다고 할 수 있다. 따라서, 피해강도 분류에 있어 산불 후에 촬영된 고해상도 영상들을 이용할 수 있을 것으로 판단된다.

• 대한원격탐사학회:학술대회논문집
• /
• 대한원격탐사학회 2008년도 International Symposium on Remote Sensing
• /
• pp.18-21
• /
• 2008

Lee (2008) proposed the pansharpening method to reconstruct at the higher resolution the multispectral images which agree with the spectral values observed from the sensor of the lower resolution values. It outperformed over several current techniques for the statistical analysis with quantitative measures, and generated the imagery of good quality for visual interpretation. However, if a small object stretches over two adjacent pixels with different spectral characteristics at the lower resolution, the pixels of the object at the higher resolution may have different multispectral values according to their location even though they have a same intensity in the panchromatic image of higher resolution. To correct this problem, this study employed an iterative technique similar to the image restoration scheme of Point-Jacobian iterative MAP estimation. The effect of pansharpening on image segmentation/classification was assessed for various techniques. The method was applied to the IKONOS image acquired over the area around Anyang City of Korea.

• 천문학논총
• /
• 제20권1호
• /
• pp.43-48
• /
• 2005

We present a high resolution spectrum of PU Vul observed at Bohyunsan Optical Astronomy Observatory (BOAO) on April 9, 2004. Permitted emission and nebular lines of PU Vul had been significantly changed compared to all spectra observed since its eruption in 1979. Therefore all new lines should be re-identified and were done so. We do-convoluted a $H{\beta}$ line into several emission components with Gaussian functions. Then we carefully discussed the geometrical feature of PU Vul in April 2004.

• 천문학논총
• /
• 제21권2호
• /
• pp.35-42
• /
• 2006

We report a high resolution spectrum of AG Pegasi observed at Bohyunsan Optical Astronomy Observatory (BOAO) on October 2, 2004. Some of permitted emission lines, for example H I, He I, He II, Fe II and Ti II were observed in the spectrum of AG Pegasi in 2004. Lines presented in the longer wavelength region than $6500{\AA}$ are identified. And radial velocities for each element are measured. Then we carefully discuss the geometrical feature of AG Pegasi in October 2004.

• 한국감성과학회:학술대회논문집
• /
• 한국감성과학회 2002년도 춘계학술대회 논문집
• /
• pp.44-50
• /
• 2002

The fast Fourier transform (FFT) is a good method to estimate spectral density, but the frequency resolution is limited to the sampling window, and thus the precise characteristics of the spectral density for short signals are not clear. To solve the limitation, a multiple band-pass filter was introduced to estimate the precise time course of the spectral density for flash visual evoked potentials (VEPs). Signals were recorded during -200 and 600 ms using balanced noncephalic electrodes, and sampled at 1 K Hz in 12 bits. With 1 Hz and 10 ms resolutions, spectral density was estimated between 10 and 100 Hz. Background powers at the alpha-and beta-bands were high over the posterior scalp, and powers around 200ms were evoked at the same bands over the same region, corresponding to P110 and N165 of VEPs. normalized's spectral density showed evoked powers around 200 ms and suppressed powers following the evoked powers over the posterior scalp. The evoked powers above the 20Hz band were not statistically significant. However, the gamma band was significantly evoked intra-individually; details in the gamma bands were varied among the subjects. Details of spectral density were complicated even for a simple task such as watching flashes; both synchronization and desynchronization occurred with different distributions and different time courses.

• 대한공간정보학회지
• /
• 제18권2호
• /
• pp.79-86
• /
• 2010

일반적으로, 영상 융합은 서로 다른 특징을 가지는 2개 이상의 영상을 이용하여 각 영상의 장점 및 특징을 모두 가지는 하나의 영상으로 재구성하는 것을 의미한다. 특히, 원격탐사 분야에서의 영상융합은 멀티스펙트럴 영상의 공간해상도를 향상시키는 것을 의미하며 이러한 이유로 인하여 Pan-sharpening 기술로도 불리어진다. 특히, 융합영상은 변화탐지, 영상 지도 제작, 도시 분석 등 다양한 분야에 적용 가능하기 때문에 중요성이 증대되고 있다. 그러나, 기존에 제안된 알고리즘들은 멀티스펙트럴 영상의 분광정보를 왜곡시키거나, 융합 영상의 공간해상도가 흑백영상의 공간해상도에 비하여 저하되는 문제를 지닌다. 이를 위해 본 논문에서는 멀티스펙트럴 영상의 분광 및 공간특성을 고려한 새로운 융합 방법론을 제안하였다. 본 알고리즘의 평가를 위해서 KOMPSAT-2, QuickBird 위성영상에 알고리즘을 적용을 하였으며, 기존의 영상융합 알고리즘에 비하여 공간적/분광적인 측면에서 모두 향상된 결과를 보임을 확인할 수 있었다.

• 천문학회보
• /
• 제36권2호
• /
• pp.154.1-154.1
• /
• 2011

IGRINS (Immersion Grating Infrared Spectrometer) is a cross-dispersed high resolution near-infrared spectrograph whose primary disperser is a silicon immersion grating (SIG) and cross-dispersers are two volume phase holographic gratings (VPHG). IGRINS covers the full ranges of H and K astronomical wavelength bands at a single exposure with the spectral resolution of 40,000. The overall layout of the IGRINS Cryostat is a $960{\times}600{\times}380$ cubic millimeter rectangular box and the whole optical train is sitting on an $880{\times}520{\times}50\;mm^3$ rectangular Optical Bench. The total volume of the instrument has been revolutionarily reduced and remained compact for the spectral coverage and sensitivity of a high resolution spectrograph in infrared. We, in this presentation, introduce the design models, the structural and thermal analysis results of the mechanics and cryogenics of IGRINS.

• 대한원격탐사학회:학술대회논문집
• /
• 대한원격탐사학회 2003년도 Proceedings of ACRS 2003 ISRS
• /
• pp.525-527
• /
• 2003

Recently, the spatial resolution of earth observation satellites is significantly increased to a few meters. Such high spatial resolution images definitely will provide lots of information for detail-thirsty remote sensing users. However, it is more difficult to develop automated image algorithms for automated image feature extraction and pattern recognition. In this study, we propose a two-stage procedure to extract road information from high resolution satellite images. At first stage, a watershed segmentation technique is developed to classify the image into various regions. Then, a knowledge is built for road and used to extract the road regions. In this study, we use panchromatic and multi-spectral images of the IKONOS satellite as test dataset. The experiment result shows that the proposed technique can generate suitable and meaningful road objects from high spatial resolution satellite images. Apparently, misclassified regions such as parking lots are recognized as road needed further refinement in future research.