Hyperspectral Unmixing Overview: Geometrical, Statistical, and Sparse Regression-Based Approaches

Imaging spectrometers measure electromagnetic energy scattered in their instantaneous field view in hundreds or thousands of spectral channels with higher spectral resolution than multispectral cameras. Imaging spectrometers are therefore often referred to as hyperspectral cameras (HSCs). Higher spectral resolution enables material identification via spectroscopic analysis, which facilitates countless applications that require identifying materials in scenarios unsuitable for classical spectroscopic analysis. Due to low spatial resolution of HSCs, microscopic material mixing, and multiple scattering, spectra measured by HSCs are mixtures of spectra of materials in a scene. Thus, accurate estimation requires unmixing. Pixels are assumed to be mixtures of a few materials, called endmembers. Unmixing involves estimating all or some of: the number of endmembers, their spectral signatures, and their abundances at each pixel. Unmixing is a challenging, ill-posed inverse problem because of model inaccuracies, observation noise, environmental conditions, endmember variability, and data set size. Researchers have devised and investigated many models searching for robust, stable, tractable, and accurate unmixing algorithms. This paper presents an overview of unmixing methods from the time of Keshava and Mustard's unmixing tutorial [1] to the present. Mixing models are first discussed. Signal-subspace, geometrical, statistical, sparsity-based, and spatial-contextual unmixing algorithms are described. Mathematical problems and potential solutions are described. Algorithm characteristics are illustrated experimentally.Comment: This work has been accepted for publication in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensin

A Study on Change Detection in Hyperspectral Image

Change detection is the procedure of obtaining changes between two Hyperspectral pictures of same topographical zone taken at two unique times. It conveys the essential and important change data of a scene. Due to a breakthrough in Hyperspectral remote sensing Hyperspectral remote sensors can capable of producing narrow spectral resolution images. These high resolution spectral and spatial hyperspectral images can find small variations in images. This work describes an efficient algorithm for detecting changes in Hyperspectral images by using spectral signatures of Hyperspectral images. The objective is developing of a proficient algorithm that can show even small variations in Hyperspectral images. It reviews Hierarchical method for finding changes in Hyperspectral images by comparing spectral homogeneity between spectral change vectors. For any scenery locating and also exploration regarding adjust delivers treasured data regarding achievable changes. Hyperspectral satellite detectors get effectiveness throughout gathering data with large spectral rings. These types of detectors typically deal with spatially and also spectrally high definition graphics and this can be used by adjust discovery. This particular function is actually elaborated and also applied your adjust discovery procedure by simply controlling Hyperspectral graphics. The main aim with this thesis is actually studying and also constructing of Hyperspectral adjust discovery algorithms This kind of analysed approach is really applied to assess Hyperspectral picture image resolution files along with the approach analysed in this particular thesis is really change breakthrough making use of Hierarchical method of spectral change vectors and also making use of principal ingredient examination and also k-means clustering. This particular document offers applying and also verify of trends Hyperspectral image

A subpixel target detection algorithm for hyperspectral imagery

The goal of this research is to develop a new algorithm for the detection of subpixel scale target materials on the hyperspectral imagery. The signal decision theory is typically to decide the existence of a target signal embedded in the random noise. This implies that the detection problem can be mathematically formalized by signal decision theory based on the statistical hypothesis test. In particular, since any target signature provided by airborne/spaceborne sensors is embedded in a structured noise such as background or clutter signatures as well as broad band unstructured noise, the problem becomes more complicated, and particularly much more under the unknown noise structure. The approach is based on the statistical hypothesis method known as Generalized Likelihood Ratio Test (GLRT). The use of GLRT requires estimating the unknown parameters, and assumes the prior information of two subspaces describing target variation and background variation respectively. Therefore, this research consists of two parts, the implementation of GLRT and the characterization of two subspaces through new approaches. Results obtained from computer simulation, HYDICE image and AVI RIS image show that this approach is feasible

Hyperspectral sub-pixel target detection using hybrid algorithms and Physics Based Modeling

This thesis develops a new hybrid target detection algorithm called the Physics Based-Structured InFeasibility Target-detector (PB-SIFT) which incorporates Physics Based Modeling (PBM) along with a new Structured Infeasibility Projector (SIP) metric. Traditional matched filters are susceptible to leakage or false alarms due to bright or saturated pixels that appear target-like to hyperspectral detection algorithms but are not truly target. This detector mitigates against such false alarms. More often than not, detection algorithms are applied to atmospherically compensated hyperspectral imagery. Rather than compensate the imagery, we take the opposite approach by using a physics based model to generate permutations of what the target might look like as seen by the sensor in radiance space. The development and status of such a method is presented as applied to the generation of target spaces. The generated target spaces are designed to fully encompass image target pixels while using a limited number of input model parameters. Evaluation of such target spaces shows that they can reproduce a HYDICE image target pixel spectrum to less than 1% RMS error (equivalent reflectance) in the visible and less than 6% in the near IR. Background spaces are modeled using a linear subspace (structured) approach characterized by basis vectors found by using the maximum distance method (MaxD). The SIP is developed along with a Physics Based Orthogonal Projection Operator (PBosp) which produces a 2 dimensional decision space. Results from the HYDICE FR I data set show that the physics based approach, along with the PB-SIFT algorithm, can out perform the Spectral Angle Mapper (SAM) and Spectral Matched Filter (SMF) on both exposed and fully concealed man-made targets found in hyperspectral imagery. Furthermore, the PB-SIFT algorithm performs as good (if not better) than the Mixture Tuned Matched Filter (MTMF)

Mineral identification using data-mining in hyperspectral infrared imagery

Les applications de l’imagerie infrarouge dans le domaine de la géologie sont principalement des applications hyperspectrales. Elles permettent entre autre l’identification minérale, la cartographie, ainsi que l’estimation de la portée. Le plus souvent, ces acquisitions sont réalisées in-situ soit à l’aide de capteurs aéroportés, soit à l’aide de dispositifs portatifs. La découverte de minéraux indicateurs a permis d’améliorer grandement l’exploration minérale. Ceci est en partie dû à l’utilisation d’instruments portatifs. Dans ce contexte le développement de systèmes automatisés permettrait d’augmenter à la fois la qualité de l’exploration et la précision de la détection des indicateurs. C’est dans ce cadre que s’inscrit le travail mené dans ce doctorat. Le sujet consistait en l’utilisation de méthodes d’apprentissage automatique appliquées à l’analyse (au traitement) d’images hyperspectrales prises dans les longueurs d’onde infrarouge. L’objectif recherché étant l’identification de grains minéraux de petites tailles utilisés comme indicateurs minéral -ogiques. Une application potentielle de cette recherche serait le développement d’un outil logiciel d’assistance pour l’analyse des échantillons lors de l’exploration minérale. Les expériences ont été menées en laboratoire dans la gamme relative à l’infrarouge thermique (Long Wave InfraRed, LWIR) de 7.7m à 11.8 m. Ces essais ont permis de proposer une méthode pour calculer l’annulation du continuum. La méthode utilisée lors de ces essais utilise la factorisation matricielle non négative (NMF). En utlisant une factorisation du premier ordre on peut déduire le rayonnement de pénétration, lequel peut ensuite être comparé et analysé par rapport à d’autres méthodes plus communes. L’analyse des résultats spectraux en comparaison avec plusieurs bibliothèques existantes de données a permis de mettre en évidence la suppression du continuum. Les expérience ayant menés à ce résultat ont été conduites en utilisant une plaque Infragold ainsi qu’un objectif macro LWIR. L’identification automatique de grains de différents matériaux tels que la pyrope, l’olivine et le quartz a commencé. Lors d’une phase de comparaison entre des approches supervisées et non supervisées, cette dernière s’est montrée plus approprié en raison du comportement indépendant par rapport à l’étape d’entraînement. Afin de confirmer la qualité de ces résultats quatre expériences ont été menées. Lors d’une première expérience deux algorithmes ont été évalués pour application de regroupements en utilisant l’approche FCC (False Colour Composite). Cet essai a permis d’observer une vitesse de convergence, jusqu’a vingt fois plus rapide, ainsi qu’une efficacité significativement accrue concernant l’identification en comparaison des résultats de la littérature. Cependant des essais effectués sur des données LWIR ont montré un manque de prédiction de la surface du grain lorsque les grains étaient irréguliers avec présence d’agrégats minéraux. La seconde expérience a consisté, en une analyse quantitaive comparative entre deux bases de données de Ground Truth (GT), nommée rigid-GT et observed-GT (rigide-GT: étiquet manuel de la région, observée-GT:étiquetage manuel les pixels). La précision des résultats était 1.5 fois meilleur lorsque l’on a utlisé la base de données observed-GT que rigid-GT. Pour les deux dernières epxérience, des données venant d’un MEB (Microscope Électronique à Balayage) ainsi que d’un microscopie à fluorescence (XRF) ont été ajoutées. Ces données ont permis d’introduire des informations relatives tant aux agrégats minéraux qu’à la surface des grains. Les résultats ont été comparés par des techniques d’identification automatique des minéraux, utilisant ArcGIS. Cette dernière a montré une performance prometteuse quand à l’identification automatique et à aussi été utilisée pour la GT de validation. Dans l’ensemble, les quatre méthodes de cette thèse représentent des méthodologies bénéfiques pour l’identification des minéraux. Ces méthodes présentent l’avantage d’être non-destructives, relativement précises et d’avoir un faible coût en temps calcul ce qui pourrait les qualifier pour être utilisée dans des conditions de laboratoire ou sur le terrain.The geological applications of hyperspectral infrared imagery mainly consist in mineral identification, mapping, airborne or portable instruments, and core logging. Finding the mineral indicators offer considerable benefits in terms of mineralogy and mineral exploration which usually involves application of portable instrument and core logging. Moreover, faster and more mechanized systems development increases the precision of identifying mineral indicators and avoid any possible mis-classification. Therefore, the objective of this thesis was to create a tool to using hyperspectral infrared imagery and process the data through image analysis and machine learning methods to identify small size mineral grains used as mineral indicators. This system would be applied for different circumstances to provide an assistant for geological analysis and mineralogy exploration. The experiments were conducted in laboratory conditions in the long-wave infrared (7.7μm to 11.8μm - LWIR), with a LWIR-macro lens (to improve spatial resolution), an Infragold plate, and a heating source. The process began with a method to calculate the continuum removal. The approach is the application of Non-negative Matrix Factorization (NMF) to extract Rank-1 NMF and estimate the down-welling radiance and then compare it with other conventional methods. The results indicate successful suppression of the continuum from the spectra and enable the spectra to be compared with spectral libraries. Afterwards, to have an automated system, supervised and unsupervised approaches have been tested for identification of pyrope, olivine and quartz grains. The results indicated that the unsupervised approach was more suitable due to independent behavior against training stage. Once these results obtained, two algorithms were tested to create False Color Composites (FCC) applying a clustering approach. The results of this comparison indicate significant computational efficiency (more than 20 times faster) and promising performance for mineral identification. Finally, the reliability of the automated LWIR hyperspectral infrared mineral identification has been tested and the difficulty for identification of the irregular grain’s surface along with the mineral aggregates has been verified. The results were compared to two different Ground Truth(GT) (i.e. rigid-GT and observed-GT) for quantitative calculation. Observed-GT increased the accuracy up to 1.5 times than rigid-GT. The samples were also examined by Micro X-ray Fluorescence (XRF) and Scanning Electron Microscope (SEM) in order to retrieve information for the mineral aggregates and the grain’s surface (biotite, epidote, goethite, diopside, smithsonite, tourmaline, kyanite, scheelite, pyrope, olivine, and quartz). The results of XRF imagery compared with automatic mineral identification techniques, using ArcGIS, and represented a promising performance for automatic identification and have been used for GT validation. In overall, the four methods (i.e. 1.Continuum removal methods; 2. Classification or clustering methods for mineral identification; 3. Two algorithms for clustering of mineral spectra; 4. Reliability verification) in this thesis represent beneficial methodologies to identify minerals. These methods have the advantages to be a non-destructive, relatively accurate and have low computational complexity that might be used to identify and assess mineral grains in the laboratory conditions or in the field

Nonlinear hyperspectral unmixing: strategies for nonlinear mixture detection, endmember estimation and band-selection

Tese (doutorado) - Universidade Federal de Santa Catarina, Centro Tecnológico, Programa de Pós-Graduação em Engenharia Elétrica, Florianópolis, 2016.Abstract : Mixing phenomena in hyperspectral images depend on a variety of factors such as the resolution of observation devices, the properties of materials, and how these materials interact with incident light in the scene. Different parametric and nonparametric models have been considered to address hyperspectral unmixing problems. The simplest one is the linear mixing model. Nevertheless, it has been recognized that mixing phenomena can also be nonlinear. Kernel-based nonlinear mixing models have been applied to unmix spectral information of hyperspectral images when the type of mixing occurring in the scene is too complex or unknown. However, the corresponding nonlinear analysis techniques are necessarily more challenging and complex than those employed for linear unmixing. Within this context, it makes sense to search for different strategies to produce simpler and/or more accurate results. In this thesis, we tackle three distinct parts of the complete spectral unmixing (SU) problem. First, we propose a technique for detecting nonlinearly mixed pixels. The detection approach is based on the comparison of the reconstruction errors using both a Gaussian process regression model and a linear regression model. The two errors are combined into a detection test statistics for which a probability density function can be reasonably approximated. Second, we propose an iterative endmember extraction algorithm to be employed in combination with the detection algorithm. The proposed detect-then-unmix strategy, which consists of extracting endmembers, detecting nonlinearly mixed pixels and unmixing, is tested with synthetic and real images. Finally, we propose two methods for band selection (BS) in the reproducing kernel Hilbert space (RKHS), which lead to a significant reduction of the processing time required by nonlinear unmixing techniques. The first method employs the kernel k-means (KKM) algorithm to find clusters in the RKHS. Each cluster centroid is then associated to the closest mapped spectral vector. The second method is centralized, and it is based upon the coherence criterion, which sets the largest value allowed for correlations between the basis kernel functions characterizing the unmixing model. We show that the proposed BS approach is equivalent to solving a maximum clique problem (MCP), that is, to searching for the largest complete subgraph in a graph. Furthermore, we devise a strategy for selecting the coherence threshold and the Gaussian kernel bandwidth using coherence bounds for linearly independent bases. Simulation results illustrate the efficiency of the proposed method.Imagem hiperespectral (HI) é uma imagem em que cada pixel contém centenas (ou até milhares) de bandas estreitas e contíguas amostradas num amplo domínio do espectro eletromagnético. Sensores hiperespectrais normalmente trocam resolução espacial por resolução espectral devido principalmente a fatores como a distância entre o instrumento e a cena alvo, e limitada capacidade de processamento, transmissão e armazenamento históricas, mas que se tornam cada vez menos problemáticas. Este tipo de imagem encontra ampla utilização em uma gama de aplicações em astronomia, agricultura, imagens biomédicas, geociências, física, vigilância e sensoriamento remoto. A usual baixa resolução espacial de sensores espectrais implica que o que se observa em cada pixel é normalmente uma mistura das assinaturas espectrais dos materiais presentes na cena correspondente (normalmente denominados de endmembers). Assim um pixel em uma imagem hiperespectral não pode mais ser determinado por um tom ou cor mas sim por uma assinatura espectral do material, ou materiais, que se encontram na região analisada. O modelo mais simples e amplamente utilizado em aplicações com imagens hiperespectrais é o modelo linear, no qual o pixel observado é modelado como uma combinação linear dos endmembers. No entanto, fortes evidências de múltiplas reflexões da radiação solar e/ou materiais intimamente misturados, i.e., misturados em nível microscópico, resultam em diversos modelos não-lineares dos quais destacam-se os modelos bilineares, modelos de pós não-linearidade, modelos de mistura íntima e modelos não-paramétricos. Define-se então o problema de desmistura espectral (ou em inglês spectral unmixing - SU), que consiste em determinar as assinaturas espectrais dos endmembers puros presentes em uma cena e suas proporções (denominadas de abundâncias) para cada pixel da imagem. SU é um problema inverso e por natureza cego uma vez que raramente estão disponíveis informações confiáveis sobre o número de endmembers, suas assinaturas espectrais e suas distribuições em uma dada cena. Este problema possui forte conexão com o problema de separação cega de fontes mas difere no fato de que no problema de SU a independência de fontes não pode ser considerada já que as abundâncias são de fato proporções e por isso dependentes (abundâncias são positivas e devem somar 1). A determinação dos endmembers é conhecida como extração de endmembers e a literatura apresenta uma gama de algoritmos com esse propósito. Esses algoritmos normalmente exploram a geometria convexa resultante do modelo linear e da restrições sobre as abundâncias. Quando os endmembers são considerados conhecidos, ou estimados em um passo anterior, o problema de SU torna-se um problema supervisionado, com pares de entrada (endmembers) e saída (pixels), reduzindo-se a uma etapa de inversão, ou regressão, para determinar as proporções dos endmembers em cada pixel. Quando modelos não-lineares são considerados, a literatura apresenta diversas técnicas que podem ser empregadas dependendo da disponibilidade de informações sobre os endmembers e sobre os modelos que regem a interação entre a luz e os materiais numa dada cena. No entanto, informações sobre o tipo de mistura presente em cenas reais são raramente disponíveis. Nesse contexto, métodos kernelizados, que assumem modelos não-paramétricos, têm sido especialmente bem sucedidos quando aplicados ao problema de SU. Dentre esses métodos destaca-se o SK-Hype, que emprega a teoria de mínimos quadrados-máquinas de vetores de suporte (LS-SVM), numa abordagem que considera um modelo linear com uma flutuação não-linear representada por uma função pertencente a um espaço de Hilbert de kernel reprodutivos (RKHS). Nesta tese de doutoramento diferentes problemas foram abordados dentro do processo de SU de imagens hiperespectrais não-lineares como um todo. Contribuições foram dadas para a detecção de misturas não-lineares, estimação de endmembers quando uma parte considerável da imagem possui misturas não-lineares, e seleção de bandas no espaço de Hilbert de kernels reprodutivos (RKHS). Todos os métodos foram testados através de simulações com dados sintéticos e reais, e considerando unmixing supervisionado e não-supervisionado. No Capítulo 4, um método semi-paramétrico de detecção de misturas não-lineares é apresentado para imagens hiperespectrais. Esse detector compara a performance de dois modelos: um linear paramétrico, usando mínimos-quadrados (LS), e um não-linear não-paramétrico usando processos Gaussianos. A idéia da utilização de modelos não-paramétricos se conecta com o fato de que na prática pouco se sabe sobre a real natureza da não-linearidade presente na cena. Os erros de ajuste desses modelos são então comparados em uma estatística de teste para a qual é possível aproximar a distribuição na hipótese de misturas lineares e, assim, estimar um limiar de detecção para uma dada probabilidade de falso-alarme. A performance do detector proposto foi estudada considerando problemas supervisionados e não-supervisionados, sendo mostrado que a melhoria obtida no desempenho SU utilizando o detector proposto é estatisticamente consistente. Além disso, um grau de não-linearidade baseado nas energias relativas das contribuições lineares e não-lineares do processo de mistura foi definido para quantificar a importância das parcelas linear e não-linear dos modelos. Tal definição é importante para uma correta avaliação dos desempenhos relativos de diferentes estratégias de detecção de misturas não-lineares. No Capítulo 5 um algoritmo iterativo foi proposto para a estimação de endmembers como uma etapa de pré-processamento para problemas SU não supervisionados. Esse algoritmo intercala etapas de detecção de misturas não-lineares e estimação de endmembers de forma iterativa, na qual uma etapa de estimação de endmembers é seguida por uma etapa de detecção, na qual uma parcela dos pixels mais não-lineares é descartada. Esse processo é repetido por um número máximo de execuções ou até um critério de parada ser atingido. Demonstra-se que o uso combinado do detector proposto com um algoritmo de estimação de endmembers leva a melhores resultados de SU quando comparado com soluções do estado da arte. Simulações utilizando diferentes cenários corroboram as conclusões. No Capítulo 6 dois métodos para SU não-linear de imagens hiperespectrais, que empregam seleção de bandas (BS) diretamente no espaço de Hilbert de kernels reprodutivos (RKHS), são apresentados. O primeiro método utiliza o algoritmo Kernel K-Means (KKM) para encontrar clusters diretamente no RKHS onde cada centroide é então associada ao vetor espectral mais próximo. O segundo método é centralizado e baseado no critério de coerência, que incorpora uma medida da qualidade do dicionário no RKHS para a SU não-linear. Essa abordagem centralizada é equivalente a resolver um problema de máximo clique (MCP). Contrariamente a outros métodos concorrentes que não incluem uma escolha eficiente dos parâmetros do modelo, o método proposto requer apenas uma estimativa inicial do número de bandas selecionadas. Os resultados das simulações empregando dados, tanto sintéticos como reais, ilustram a qualidade dos resultados de unmixing obtidos com os métodos de BS propostos. Ao utilizar o SK-Hype, para um número reduzido de bandas, são obtidas estimativas de abundância tão precisas quanto aquelas obtidas utilizando o método SK-Hype com todo o espectro disponível, mas com uma pequena fração do custo computacional

An Image fusion algorithm for spatially enhancing spectral mixture maps

An image fusion algorithm, based upon spectral mixture analysis, is presented. The algorithm combines low spatial resolution multi/hyperspectral data with high spatial resolution sharpening image(s) to create high resolution material maps. Spectral (un)mixing estimates the percentage of each material (called endmembers) within each low resolution pixel. The outputs of unmixing are endmember fraction images (material maps) at the spatial resolution of the multispectral system. This research includes developing an improved unmixing algorithm based upon stepwise regression. In the second stage of the process, the unmixing solution is sharpened with data from another sensor to generate high resolution material maps. Sharpening is implemented as a nonlinear optimization using the same type of model as unmixing. Quantifiable results are obtained through the use of synthetically generated imagery. Without synthetic images, a large amount of ground truth would be required in order to measure the accuracy of the material maps. Multiple band sharpening is easily accommodated by the algorithm, and the results are demonstrated at multiple scales. The analysis includes an examination of the effects of constraints and texture variation on the material maps. The results show stepwise unmixing is an improvement over traditional unmixing algorithms. The results also indicate sharpening improves the material maps. The motivation for this research is to take advantage of the next generation of multi/hyperspectral sensors. Although the hyperspectral images will be of modest to low resolution, fusing them with high resolution sharpening images will produce a higher spatial resolution land cover or material map