Computer-Aided Mapping of Hyper- and Multi-Spectral Data

超光谱和多光谱数据的计算机辅助绘图

• 批准号: 269661170
• 负责人: Professor Dr.-Ing. Gernot A. Fink
• 金额: --
• 依托单位: Arbeitsgebiet Bildsignalverarbeitung (BV)
• 依托单位国家: 德国
• 项目类别: Research Grants
• 财政年份: 2015
• 资助国家: 德国
• 起止时间: 2014-12-31 至 2019-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/269661170?language=en
• 关键词: Computer; Aided; Mapping; Hyper; Multi

Computer aided mapping of multi-spectral and hyper-spectral data is an important application in planetary science. The light reflected from a planetary surface is acquired in many channels across a broad range of wavelengths. This allows for analyzing physical and geological surface properties, e.g., in order to determine the occurrence of certain minerals or rocks or to explore planets for future space missions. For this purpose, large databases of multi-spectral and hyper-spectral images are commonly analyzed by experts mostly in a manual fashion. The objective of this project is to support such analyses with automated machine learning methods. A major challenge lies in the lack of annotated training material which is required in order to estimate classifiers from sample data. For this reason, it is proposed in the project to follow an active learning strategy. Image regions are clustered in an unsupervised manner before individual annotations are requested from the expert. The annotations correspond to prototypical regions and can be propagated to similar and so far unknown regions. Based on the increasing amount of annotated samples, deep neural networks are trained in order to automate the mapping process further. Modeling the uncertainty of the automated decisions is one of the most important aspects in the project. The capabilities of the machine learning methods become transparent and improve the interpretability of the results for the expert. Another very important aspect is the representation of image regions. Instead of an assignment to only a single class in the classification process, regions are represented in terms of attributes which characterize a region with respect to selected properties. Classes of regions are recognized by their attributes. This even allows for recognizing classes which are unseen in the training data set. The methods will be evaluated on multi-spectral and hyper-spectral images as well as semantic segmentation benchmarks considered in the computer vision community. A qualitative analysis is performed by a planetary geologist who evaluates the support provided by the methods in the exploration of a new data set.

多光谱和高光谱数据的计算机辅助制图是行星科学中的一个重要应用。从行星表面反射的光是通过许多通道在很宽的波长范围内获得的。这允许分析物理和地质表面性质，例如，为了确定某些矿物或岩石的出现，或为未来的空间任务探索行星。为此，专家通常以手工方式分析多光谱和高光谱图像的大型数据库。这个项目的目标是用自动化的机器学习方法来支持这种分析。一个主要的挑战在于缺乏带注释的训练材料，这是根据样本数据估计分类器所必需的。因此，在项目中建议采用主动学习策略。在专家要求单独的注释之前，以无监督的方式对图像区域进行聚类。注释对应于原型区域，并且可以传播到相似且迄今未知的区域。基于标注样本数量的增加，训练深度神经网络以进一步实现映射过程的自动化。对自动化决策的不确定性进行建模是项目中最重要的方面之一。机器学习方法的能力变得透明，并提高了专家对结果的可解释性。另一个非常重要的方面是图像区域的表示。在分类过程中，区域不是只分配给一个类，而是用属性来表示，这些属性根据所选的属性来表征一个区域。区域的类别是通过其属性来识别的。这甚至允许识别训练数据集中不可见的类。这些方法将在多光谱和超光谱图像以及计算机视觉界考虑的语义分割基准上进行评估。定性分析由行星地质学家执行，他在新数据集的探索中评估方法所提供的支持。