• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2006년도 Proceedings of ISRS 2006 PORSEC Volume I
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• pp.86-89
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• 2006

Ocean color remote sensing community currently uses the different solar irradiance spectra covering the visible and near-infrared in the calibration/validation and deriving products of ocean color instruments. These spectra derived from single and / or multiple measurements sets or models have significant discrepancies, primarily due to variation of the solar activity and uncertainties in the measurements from various instruments and their different calibration standards. Thus, it is prudent to examine model-to-model differences and select a standard reference spectrum that can be adopted in the future calibration and validation processes, particularly of the first Geostationary Ocean Color Imager (GOCI) onboard its Communication Ocean and Meterological Satellite (COMS) planned to be launched in 2008. From an exhaustive survey that reveals a variety of solar spectra in the literature, only eight spectra are considered here seeing as reference in many remote sensing applications. Several criteria are designed to define the reference spectrum: i.e., minimum spectral range of 350-1200nm, based completely or mostly on direct measurements, possible update of data and less errors. A careful analysis of these spectra reveals that the Thuillier 2004 spectrum seems to be very identical compared to other spectra, primarily because it represents very high spectral resolution and the current state of the art in solar irradiance spectra of exceptionally low uncertainty ${\sim}0.1%.$ This study also suggests use of the Gueymard 2004 spectrum as an alternative for applications of multispectral/multipurpose satellite sensors covering the terrestrial regions of interest, where it provides spectral converge beyond 2400nm of the Thuillier 2004 spectrum. Since the solar-activity induced spectral variation is about less than 0.1% and a large portion of this variability occurs particularly in the ultraviolet portion of the electromagnetic spectrum that is the region of less interest for the ocean color community, we disregard considering this variability in the analysis of solar irradiance spectra, although determine the solar constant 1366.1 $Wm^{-2}$ to be proposed for an improved approximation of the extraterrestrial solar spectrum in the visible and NIR region.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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• pp.319-324
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• 1998

Ocean Scanning Multispectral Imager (OSMI) is a payload on the Korean Multi-purpose SATellite (KOMPSAT) to perform worldwide ocean color monitoring for the study of biological oceanography. The instrument images the ocean surface using a whisk-broom motion with a swath width of 800 km and a ground sample distance (GSD) of < 1 km over the entire field-of-view (FOV). The instrument is designed to have an on-orbit operation duty cycle of 20% over the mission lifetime of 3 years with the functions of programmable gain/offset and on-board image data storage. The instrument also performs sun calibration and dark calibration for on-board instrument calibration. The OSMI instrument is a multi-spectral imager covering the spectral range from 400 nm to 900 nm using a CCD Focal Plane Array (FPA). The ocean colors are monitored using 6 spectral channels that can be selected via ground commands after launch. The instrument performances are fully measured for 8 basic spectral bands centered at 412nm, 443nm, 490nm, 510nm, 555nm, 670nm, 765nm and 865nm during ground characterization of instrument. In addition to the ground calibration, the on-board calibration will also be used for the on-orbit band selection. The on-orbit band selection capability can provide great flexibility in ocean color monitoring.

• 지구물리와물리탐사
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• 제7권1호
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• pp.45-50
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• 2004

This paper describes a method of detecting formation boundaries, and permeable fractures, from frequency-domain Stoneley wave logs. Field data sets were collected between the depths of 330 and 360 m in well EE-4 in the Higashi-Hachimantai geothermal field, using a monopole acoustic logging tool with a source central frequency of 15 kHz. Stoneley wave amplitude spectra were calculated by performing a fast Fourier transform on the waveforms, and the spectra were then collected into a frequency-depth distribution of Stoneley wave amplitudes. The frequency-domain Stoneley wave log shows four main characteristic peaks at frequencies 6.5, 8.8, 12, and 13.3 kHz. The magnitudes of the Stoneley wave at these four frequencies are affected by formation properties. The Stoneley wave at higher frequencies (12 and 13.3 kHz) has higher amplitudes in hard formations than in soft formations, while the wave at lower frequencies (6.5 and 8.8 kHz) has higher amplitudes in soft formations than in hard formations. The correlation of the frequency-domain Stoneley wave log with the logs of lithology, degree of welding, and P-wave velocity is excellent, with all of them showing similar discontinuities at the depths of formation boundaries. It is obvious from these facts that the frequency-domain Stoneley wave log provides useful clues for detecting formation boundaries. The frequency-domain Stoneley wave logs are also applicable to the detection of a single permeable fracture. The procedure uses the Stoneley wave spectral amplitude logs at the four frequencies, and weighting functions. The optimally weighted sum of the four Stoneley wave spectral amplitudes becomes almost constant at all depths, except at the depth of a permeable fracture. The assumptions that underlie this procedure are that the energy of the Stoneley wave is conserved in continuous media, but that attenuation of the Stoneley wave may occur at a permeable fracture. This attenuation may take place at anyone of the four characteristic Stoneley wave frequencies. We think our multispectral approach is the only reliable method for the detection of permeable fractures.

• 상하수도학회지
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• 제31권3호
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• pp.197-204
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• 2017

This study was carried out to apply the UAV(Unmanned Aerial Vehicle) coupled with Multispectral sensor for the algae bloom monitoring in river. The study acquired remote sensing data using UAV on the midstream area of Gum River, one of four major rivers in South Korea. Normalized difference vegetation index (NDVI) is used for monitoring algae change. This study conducted water sampling and analysis in the field for correlating with NDVI values. Among the samples analyzed, the chlorophyll concentration exhibited strong and significant linear relationships with NDVI, and thus NDVI was chosen for algae bloom index to identify emergence aspect of phytoplankton in river. Aerial remote sensing technology can provide more accurate, flexible, cheaper, and faster monitoring methods of detecting and predicting eutrophication and therefore cyanobacteria bloom in water reservoirs compared to currently used technology. As a result, there was high level of correlation in chlorophyll-a and NDVI. It is expected that when this remote water quality and pollution monitoring technology is applied in the field, it would be able to improve capabilities to deal with the river water quality and pollution at the early stage.

• 대한원격탐사학회지
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• 제19권4호
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• pp.329-339
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• 2003

본 연구에서는 무감독 영상분류를 위하여 특성이 다른 센서로 수집된 영상들에 대한 의사결정 수준의 영상 융합기법을 제안하였다. 제안된 기법은 공간 확장 분할에 근거한 무감독 계층군집 영상분류기법을 개개의 센서에서 수집된 영상에 독립적으로 적용한 후 그 결과로 생성되는 분할지역의 퍼지 클래스 벡터(fuzzy class vector)를 이용하여 각 센서의 분류 결과를 융합한다. 퍼지 클래스벡터는 분할지역이 각 클래스에 속할 확률을 표시하는 지시(indicator) 벡터로 간주되며 기대 최대화 (EM: Expected Maximization) 추정 법에 의해 관련 변수의 최대 우도 추정치가 반복적으로 계산되어진다. 본 연구에서는 같은 특성의 센서 혹은 밴드 별로 분할과 분류를 수행한 후 분할지역의 분류결과를 퍼지 클래스 벡터를 이용하여 합성하는 접근법을 사용하고 있으므로 일반적으로 다중센서의 영상의 분류기법에 사용하는 화소수준의 영상융합기법에서처럼 서로 다른 센서로부터 수집된 영상의 화소간의 공간적 일치에 대한 높은 정확도를 요구하지 않는다. 본 연구는 한반도 전라북도 북서지역에서 관측된 다중분광 SPOT 영상자료와 AIRSAR 영상자료에 적용한 결과 제안된 영상 융합기법에 의한 피복 분류는 확장 벡터의 접근법에 의한 영상 융합보다 서로 다른 센서로부터 얻어지는 정보를 더욱 적합하게 융합한다는 것을 보여주고 있다.

• 대한원격탐사학회지
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• 제26권6호
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• pp.605-615
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• 2010

This study demonstrates the feasibility of small satellite, namely PROBA platform with the compact high resolution imaging spectrometer (CHRIS), for aerosol retrieval in Hong Kong. The rationale of our technique is to estimate the aerosol reflectances by decomposing the Top of Atmosphere (TOA) reflectances from surface reflectance and Rayleigh path reflectances. For the determination of surface reflectances, the modified Minimum Reflectance Technique (MRT) is used on three winter ortho-rectified CHRIS images: Dec-18-2005, Feb-07-2006, Nov-09-2006. For validation purpose, MRT image was compared with ground based multispectral radiometer measurements and atmospherically corrected Landsat image. Results show good agreements between CHRIS-derived surface reflectance and both by ground measurement data as well as by Landsat image (r>0.84). The Root-Mean-Square Errors (RMSE) at 485, 551 and 660nm are 0.99%, 1.19%, and 1.53%, respectively. For aerosol retrieval, Look Up Tables (LUT) which are aerosol reflectances as a function of various AOT values were calculated by SBDART code with AERONET inversion products. The CHRIS derived Aerosol Optical Thickness (AOT) images were then validated with AERONET sunphotometer measurements and the differences are 0.05~0.11 (error=10~18%) at 440nm wavelength. The errors are relatively small compared to those from the operational moderate resolution imaging spectroradiometer (MODIS) Deep Blue algorithm (within 30%) and MODIS ocean algorithm (within 20%).

• 대한원격탐사학회지
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• 제35권4호
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• pp.545-560
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• 2019

Unlike other critical forest diseases, pine pitch canker in Korea has shown rather mild symptoms of partial loss of crown foliage and leaf discoloration. This study used high-resolution satellite images to detect and monitor canopy decline by pine pitch canker. To enhance the subtle change of canopy reflectance in pitch canker damaged tree crowns, multi-temporal analysis was applied to two KOMPSAT multispectral images obtained in 2011 and 2015. To assure the spectral consistency between the two images, radiometric corrections of atmospheric and shadow effects were applied prior to multi-temporal analysis. The normalized difference vegetation index (NDVI) of each image and the NDVI difference (${\Delta}NDVI=NDVI_{2015}-NDVI_{2011}$) between two images were derived. All negative ΔNDVI values were initially considered any pine stands, including both pitch canker damaged trees and other trees, that showed the decrease of crown foliage from 2011 to 2015. Next, $NDVI_{2015}$ was used to exclude the canopy decline unrelated to the pitch canker damage. Field survey data were used to find the spectral characteristics of the damaged canopy and to evaluate the detection accuracy from further analysis.Although the detection accuracy as assessed by limited number of field survey on 21 sites was 71%, there were also many false alarms that were spectrally very similar to the damaged canopy. The false alarms were mostly found at the mixed stands of pine and young deciduous trees, which might invade these sites after the pine canopy had already opened by any crown damages. Using both ${\Delta}NDVI$ and $NDVI_{2015}$ could be an effective way to narrow down the potential area of the pitch canker damage in Korea.

• 한국초지조사료학회지
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• 제40권4호
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• pp.196-202
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• 2020

본 연구는 동계사료작물의 무인기기반 생육모니터링을 위하여 호밀, 총체보리, IRG를 대상으로 다중분광영상으로 건물수량을 예측하기 위한 최적식생지수를 테스트하였다. 2019년 2월부터 4월까지 나주의 실경작지에서 무인기 다중분광카메라로 분광영상을 수집하여 4종류의 식생지수(Normalized Difference Vegetation Index; NDVI, Green Normalized Difference Vegetation Index; GNDVI, Normalized Green Red Difference Index; NGRDI and Normalized Difference Red Edge Index; NDREI)를 산출하고 지상에서 건물수량을 조사하여 식생지수와 건물수량의 상관관계를 조사하였다. 호밀, 총체보리, IRG에 대하여 건물수량과 NDVI의 상관관계(R2)는 0.91~0.92, GNDVI는 0.92~0.94, NGRDI는 0.71~0.85, NDREI는 0.84~0.91로 GNDVI가 가장 효과적이었다.

• 한국지리정보학회지
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• 제7권4호
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• pp.77-87
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• 2004

지형의 수리학적 해석을 위해서 수리학자들은 정확한 하천 횡단면을 파악하는 것이 중요하다. 기존에는 직접 측량법을 이용하여 하천 횡단면을 알 수 있었지만, 본 연구에서는 정확성 경제성 확보라는 차원에서 항공사진을 이용했다. 자체 제작한 고해상도 다중분광 항공촬영시스템 (PKNU2호)으로 획득한 영상을 수치지도와 GPS 측량값으로 처리하여 정사영상지도를 제작하였다. 그리고 정사처리 된 영상을 Z/I Imaging 사의 ImageStation 도화기로 하천 횡단면 획득하고, Kinematic 측량값과 비교 분석해 보았다. 연구결과 정사영상지도 제작 시 수치지도를 사용하여 처리한 것보다 GPS 측량값으로 영상을 처리한 것이 5.5788화소(약 2m) 에서 2.84화소(약 1m)로 정확도가 향상됨을 알 수 있었다. 하천 횡단면 추출 시 Kinematic 측량값은 수평 및 수직 정확도가 95% 신뢰수준에서 ${\pm}6.6cm$ 정도로 매우 좋았으며, 항공사진을 이용한 하천 횡단면 추출 결과와는 상시성 0.857으로 하천횡단면 획득을 위해 적용가능성이 매우 높았다.

• 대한원격탐사학회지
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• 제14권3호
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• pp.277-284
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• 1998

해색관측센서 (OSMI)의 월별 자료수집계획을 수립하기 위해 색소농도, 운량 및 태양반사의 세가지 영향요소에 대한 전구분포가 검토되었다. 위성의 임무 제한조건 (예, 임무주기)을 제외한 이들 세 요소들은 OSMI 자료수집에 매우 중요한 것으로 간주된다. Nimbus-7 CZCS 월평균 자료 및 ISCCP 월평균 자료가 색소농도 및 운량 분포 분석에 각각 사용되었다. 그리고 태양반사의 월별 모사분포는 OSMI 궤도예측 및 대기 상층부 태양반사 레이디언스 계산을 수행함으로 얻어졌다. 주어진 경위도 $10^{\circ}$격자에 대한 상기 각 요소의 월별 통계자료 (월평균 혹은 표준편차)를 이용해 월별 우선순위 도를 생성시켰다. 이어서 세 요소의 중복효과를 보기위해 각 달의 세 요소에 대한 우선순위 도를 중첩 시켰다. 초기결과는 하반구의 대부분이 구름과 태양반사의 계절변화로 인해 우선순위가 낮은 지역으로 분류됨을 보였다. 서로 다른 분류세트에 대한 민감도 시험을 하여 구름과 태양반사의 계절변화가 강건함을 보였다.