• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2003년도 Proceedings of ACRS 2003 ISRS
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• pp.1400-1402
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• 2003

The objective of this paper is to determine the suitable spectral bands for monitoring growth status change during a long period. The long-term ground-level reflectance spectra as well as LAI and biomass were obtained in xiaotangshan area, Beijing, 2001. The narrow-band NDVI type spectral indices by all possible two bands were calculated their correlation coefficients R$^2$ with biomass and LAI. The best NDVIs must have higher R$^2$ with both biomass and LAI. The reasonable band centers and band widths were determined by a systematically increasing bandwidth centered over a wavelength. In addition, the first 19 bands of MODIS were simulated and investigated. Each developed spectral indices was then validated by the biomass and LAI time series using the generalized vector angle. It turned out that six new NDVI type indices within 750-1400nm were developed. NDVI(811_10,957_10) and NDVI(962_10,802_10) performed best. No satisfactory conventional NDVI formed by red and NIR bands were found effective. MODIS_NDVI(band19, band17) and MODIS_NDVI(band19, band2) were much better than MODIS_NDVI(band2,band1) for growth monitoring.

• 한국농공학회:학술대회논문집
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• 한국농공학회 2003년도 학술발표논문집
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• pp.627-630
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• 2003

This research determined the spectral reflectance characteristics and vegetation indices when intermixed with field crops and soil. Ground-level spectral reflectance were collected in the field experiment containing plots of soybean and other seven crops. The first and second derivative of reflectance spectra showed several peaks that were dependent in different degrees on leaf age and chlorophyll concentration in the crop leaves. This study evaluated a number of spectral indices for estimating chlorophyll concentrations at the leaf scale difference, using samples from field crops at various stages of senescence. Five vegetation indices were evaluated which had advantages over previous techniques. Experimental data recorded on field crops during the growing season are in good agreement with previous theoretical results.

• Journal of Photoscience
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• 제7권4호
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• pp.139-142
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• 2000

To examine applicability of some optical indices from reflectance to estimate photosynthetic light use efficiency, photosynthesis, and narrow band spectral reflectance were simultaneously measured at various intensities of light with mongolian oak leaves. Narrow band of the broad-band NDVI was better than photochemical reflectance index and simple ratio to estimate photosynthetic light use efficiency in this study. Changes in spectral reflectance were detected at several wavelengths (540nm, 690nm, 740nm, and 800nm) associated with physiological status of plant leaves that could be components for new optical indices.

• 천문학회지
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• 제29권2호
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• pp.157-170
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• 1996

In order to determine the metallicity of a globuar cluster, M3,by using the spectral indices, a kind of index grid has been establshed by stars in globular clusters, M3, M15, M71 and old open cluster, NGC 188. The indices were measured from the medium resolution spectra of about $2{\AA}$. The summed indices were used to determine metallicity in order to increase signals. It is found that the core depth index is measured more accurately and leads result more accurate than the pseudo-equivalent width index. This method can be further improved by including many more calibration globular clusters of various metallicity to make finer grids. By this method, the metallicity of M3 is determined as $[Fe/H] = -1.46\pm0.15$.

• 한국관개배수논문집
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• 제10권2호
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• pp.43-54
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• 2003

This study investigated the spectral reflectance and leaf area index (LAI) of field crops and determined vegetation indices when intermixed with field crops and soil. Ground-level spectral reflectance and leaf area index (LAJ) were collected for eight cro

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2008년도 International Symposium on Remote Sensing
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• pp.151-154
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• 2008

Information on the area and spatial distribution of crop fields is needed for biomass production, arrangement of water resources, trace gas emission estimates, and food security. The present study aims to monitor crops status during the growing season by estimating its aboveground biomass and leaf area index (LAI) from field reflectance taken with a hand-held radiometer. Field reflectance values were collected over specific spectral bandwidths using a handheld radiometer(LI-1800). A methodology is described to use spectral reflectance as indicators of the vegetative status in crop cultures. Two vegetation indices were derived from these spectral measurements. In this paper, first we analyze each spectral reflectance characteristics of vegetation in the order of growth stage. Vegetation indices (NDVI, GNDVI) were calculated from crop reflectance. And assess the nature of relationships between LAI and VI, as measured by the in situ NDVI and GNDVI. Among the two VI, NDVI showed predictive ability across a wider range of LAI than did GNDVI. Specific objectives were to determine the relative accuracy of these two vegetation indices for predicting LAI. The results of this study indicated that the NDVI and GNDVI could potentially be applied to monitor crop agriculture on a timely and frequent basis.

• 항공우주기술
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• 제10권1호
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• pp.149-155
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• 2011

세계적 기후온난화와 이상기온현상으로 최근 급변하는 농업환경에 대응하기 위해서는 농작물 작황관리 및 예측시스템의 과학화를 통한 정부차원의 대처능력 개선이 시급하다. 농업분야에서 위성정보의 활용은 고해상도 광학 및 레이더 영상의 상용화와 더불어 정밀농업이라는 새로운 가능성을 열어주고 있다. 본 연구에서는 최근 농업분야에서 주목을 받고 있는 RapidEye 위성영상을 사용하여 우리나라 농촌지역의 토지이용유형별 분광식생지수의 시계열 특성을 살펴보았다. 식생과 비식생지역 간에 뚜렷한 시계열 변화양상이 나타났으며, 식생지역 내에서도 산림 수종별, 논 그룹별로 식생지수의 시계열 변화에 차이가 관찰되었다.

• 한국지리정보학회지
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• 제15권3호
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• pp.52-65
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• 2012

작물과 산림을 포함한 식생에 대한 순1차 생산(net primary production, NPP)와 총1차 생산(gross primary production, GPP)은 바이오매스와 식생의 탄소저장과 밀접한 관련이 있으며, 원격탐사를 이용해 바이오매스를 추정하는 많은 노력이 이루어지고 있다. 바이오매스는 광합성에 매우 중요한 요소인 클로로필(엽록소)의 총 함유량으로 추정할 수 있는데, 클로로필을 추정하기 위해서 다양한 식생지수들이 개발되었다. 식생지수들은 개발에 사용된 식생의 종류와 원격탐사 데이터에 따라 조금씩 차이를 가지고 있다. 하이퍼스펙트럴 영상은 다중분광 영상에 비하여 세분화된 각 파장대마다 물질에 따른 반사 및 흡수 특성이 다르기 때문에, 기존의 식생지수를 그대로 사용하기에 무리가 따른다. 본 연구는 항공기 탑재 하이퍼스펙트럴 영상을 이용하여 산림에 대한 바이오매스 추정을 위한 매개변수로 활용되는 적합한 식생지수는 무엇인지 평가하는 것을 목적으로 한다. 이를 위해 하이퍼스펙트럴 영상의 밴드 특성을 고려하여 다수의 식생지수 산출식 중 9개를 선정하고, SMA(spectral mixture analysis)를 통하여 대상지역의 산림을 대표하는 3개의 endmember를 추출하였다. 9개의 식생지수와 추출된 endmembers의 상관관계를 분석하였다. 상관분석 결과는 산림이 분포된 지역에서 Pearson 상관계수는 MTVI1과 TVI가 0.877의 상관계수를 가졌으며, 식생이 적고 토양의 분포가 확연한 지역에서는 MCARI가 0.9061로 매우 높은 상관계수를 보였다. 전반적으로 MTVI1과 TVI이 0.757의 동일한 상관계수를 가지며 식생에 대한 3개의 endmember를 가장 잘 설명하는 것으로 나타났다.

• 천문학회보
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• 제36권1호
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• pp.33.2-33.2
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• 2011

The anisotropic nature of the magnetic turbulence associated with magnetic dipolarizations in the Earth's plasma sheet is examined. Specifically we determine the power spectral indices for the perpendicular and parallel components of the fluctuating magnetic field with respect to the background magnetic field and compare them to determine possible anisotropic features. For this study, we identify a total of 47 dipolarization events from February 2008 using the magnetic field observations by the THEMIS A, D and E satellites when they are situated closely near the neutral sheet in the near-Earth tail. For the identified events, we estimate the spectral indices for the frequency range from 1.3 mHz to 42 mHz. The results show that for many events the spectral indices are larger for fluctuations in the ${\Psi}$ direction than for those in the other two directions, where the ${\Psi}$ direction is perpendicular to the background magnetic field line and to the azimuthal direction. This implies that the dipolarization-associated turbulence of the magnetic field is often anisotropic. We discuss how this result differs from what is expected from the theory of homogeneous, anisotropic, MHD turbulence.

• 천문학논총
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• 제8권1호
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• pp.243-263
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• 1993

One hundred forty two digital spectra of 110 standard stars with 1 A resolution in ${\lambda}{\lambda}\;3000\;A\;{\sim}4150\;A$ region were analyzed to determine the spectral indices sensitive to the atmospheric parameters. The standard stars cover the temperature in the range of $T_eff$ from ${\sim}4000^{\circ}$ to ${\sim}7000^{\circ}\;K$ and the surface gravity in the range of log g from 0 to 5 and the metal abundance [Fe/H] from -2.7 to 0.4. We have derived physical parameters, theta(=T/5040), log g, and [Fe/H] for the standard stars using indices, P(38/93), Fe I(A), Fe I(B), SrII, and $H{\delta}$, with overall accuracies of 0.067, 0.617, and 0.466, respectively. However for some region of spectral type and metallicity, those can be obtained with better accuracies. Those indices are found to be useful especially for stellar gravity determination.