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The solar illumination conditions on the lunar surface represent a key resource with respect to returning to the Moon. As a supplement to mapping the solar illumination by exploring data, lighting simulations using high-resolution topography could produce quantitative illumination maps. In this study, a theoretical model is proposed for estimating the solar illumination conditions. It depends only on the solar altitude and topographical factors. Besides the selenographic longitude and latitude, the former is determined by the selenographic longitude and latitude at the subsolar site, the geocentric ecliptical latitude, and the dimensionless distance of the Sun–Moon relative to 1 AU, which are function of time. The latter is determined by comparing the elevations in solar irradiance direction within 210 km in which the topography might shadow the behind sites to the critical elevations determining whether the behind sites are shadowed or not. Compared to Zuber's model, the model proposed in this study is simpler and easier for computing. It is parameterized with selenographic coordinates, elevations, and time. With high-resolution topography data, the solar illumination conditions at any selenographic coordination could be estimated by this model at any date and time. The lunar surface is illuminated when the solar altitude is non-zero and all the elevations within 210 km in solar irradiance direction are lower than the critical elevations. Otherwise it would be shadowed. 相似文献
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《地学前缘(英文版)》2023,14(4):101562
The remote mapping of minerals and discrimination of ore and waste on surfaces are important tasks for geological applications such as those in mining. Such tasks have become possible using ground-based, close-range hyperspectral sensors which can remotely measure the reflectance properties of the environment with high spatial and spectral resolution. However, autonomous mapping of mineral spectra measured on an open-cut mine face remains a challenging problem due to the subtleness of differences in spectral absorption features between mineral and rock classes as well as variability in the illumination of the scene. An additional layer of difficulty arises when there is no annotated data available to train a supervised learning algorithm. A pipeline for unsupervised mapping of spectra on a mine face is proposed which draws from several recent advances in the hyperspectral machine learning literature. The proposed pipeline brings together unsupervised and self-supervised algorithms in a unified system to map minerals on a mine face without the need for human-annotated training data. The pipeline is evaluated with a hyperspectral image dataset of an open-cut mine face comprising mineral ore martite and non-mineralised shale. The combined system is shown to produce a superior map to its constituent algorithms, and the consistency of its mapping capability is demonstrated using data acquired at two different times of day. 相似文献
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受地下复杂构造和地震数据采集系统的影响,使地震波对地下目标的照明出现不均匀性,地震采集系统难以有效地获取地下某些目标的反射信息,进而使数据偏移成像在这些目标体上出现成像阴影. 根据波场和Green函数的窗口Fourier框架展开,利用角度域波动方程偏移成像和波动方程照明分析,并结合波动方程反演理论,提出一种角度域波动方程偏移成像阴影照明补偿方法. 这种补偿方法能同时考虑地震数据采集系统和波场传播路径对偏移成像的影响,消除复杂构造区的偏移成像阴影,改进波动方程叠前深度偏移成像在复杂构造区的成像效果. 相似文献
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试图运用波场动力学途径,旨在增强观测系统分析评估,本文提出基于单程波方程的角度域照明分析方法.本文方法不仅可用于观测系统设计,对叠前成像资料的考量、叠前振幅补偿和AVA（Amplitude Versus Angle,振幅随角度变化）反演也必具重要的意义.文中通过目的层邻域单个绕射点的正、反传波场分析,给出地下目标的水平和倾斜界面随角度变化的成像照明强度.单程波方法可用于模拟地震波在复杂速度构造下的传播,并得到较准确的幅值和多次到达的波场,用以对绕射点正、反传分析时可在照明分析中简明地利用幅值信息和多次到达的波场.本文方法可显现复杂盖层下目标的照明情况.本文中也对照明能量随传播距离的几何扩散进行补偿,突显了角度域的照明均匀度和范围,从而使得所分析的结果可直接应用于AVA的分析及补偿.针对照明分析的特点,文中建议可用一种快速的单程波波场延拓策略——频率速度相关变步长波场深度延拓.数值实验结果表明了本文方法是可行且有效的. 相似文献
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基于"嫦娥一号"激光测高数据的月球极区光照条件研究 总被引：1，自引：0，他引：1
月球极区光照模型为研究月球车着陆点选择和水冰存在的探测提供了依据.利用"嫦娥一号"探月卫星获取的激光测高数据,得到了全月面高精度的数字高程模型(DEM),特别是在月球两极地区,地形细节清晰可见,为极区光照模型的建立提供了精确的数据基础.本文通过由测高数据建立的DEM和月球轨道参数相结合,采用地形最大高度角法,对月球极区的光照条件及其应用进行了研究和分析.光照率的计算周期为19年,考虑了黄道和白道交点进动的影响(18.6年).计算结果表明:(1)未发现有持续光照区;(2)有长久阴影区存在;(3)在南极或北极的夏季,撞击坑边沿高地处可以享受到连续的光照;(4)Shackleton撞击坑可以作为月球车着陆的首选目标之一. 相似文献
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三维地形模型光照和动态显示的新方法 总被引：5，自引：0，他引：5
介绍了一种具有真实感的三维地形模型光照显示的新方法,给出了相应的构建多精度数字高程模型ＤＥＭ的步骤,并讨论了适应三维地形模型光照显示的消隐,可见性测试,光照模型,浓淡处理等处理算法的方法,此外还讨论了适合身机动态显示三维地形模型的方法。 相似文献
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3‐D shallow‐water seismic survey evaluation and design using the focal‐beam method: a case study offshore Abu Dhabi 
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下载免费PDF全文 For 3‐D shallow‐water seismic surveys offshore Abu Dhabi, imaging the target reflectors requires high resolution. Characterization and monitoring of hydrocarbon reservoirs by seismic amplitude‐versus‐offset techniques demands high pre‐stack amplitude fidelity. In this region, however, it still was not clear how the survey parameters should be chosen to satisfy the required data quality. To answer this question, we applied the focal‐beam method to survey evaluation and design. This subsurface‐ and target‐oriented approach enables quantitative analysis of attributes such as the best achievable resolution and pre‐stack amplitude fidelity at a fixed grid point in the subsurface for a given acquisition geometry at the surface. This method offers an efficient way to optimize the acquisition geometry for maximum resolution and minimum amplitude‐versus‐offset imprint. We applied it to several acquisition geometries in order to understand the effects of survey parameters such as the four spatial sampling intervals and apertures of the template geometry. The results led to a good understanding of the relationship between the survey parameters and the resulting data quality and identification of the survey parameters for reflection imaging and amplitude‐versus‐offset applications. 相似文献
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全方位观测系统是目前海上一种可以实现连续环状采集的地震观测系统,它有效扩大目标层上面元的采集方位范围,能够更全面地反映地下构造信息,具有极高的生产效率.本文在波前构建法三维射线追踪技术的基础上,通过获得模拟偏移振幅强度作为照明量,来衡量目标层对不同观测系统的照明响应,为评价和优化不同观测系统提供指导依据.测试结果表明:与平行观测系统相比,全方位观测系统在目标层上的照明能量的连续性和均匀性最好,能够有效地改善平行观测系统下照明阴影区的照明效果,是一种理想的观测系统,可以广泛适用于海上复杂地质环境下的地震采集工作. 相似文献
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Unequal illumination of the subsurface highly impacts the quality of seismic imaging. Different image points receive different folds of reflection‐angle illumination, which can be caused by irregular acquisition or by wave propagation in complex media. Illumination problems can deteriorate amplitudes in migrated images. To address this problem, we present a method of stacking angle‐domain common‐image gathers, in which we use local similarity with soft thresholding to determine the folds of local illumination. Normalization by local similarity regularizes local illumination of reflection angles for each image point of the subsurface model. This approach compensates for irregular illumination by selective stacking in the image space, regardless of the cause of acquisition or propagation irregularities. Additional migration is not required because the methodology is implemented in the reflection angle domain after migration. We use two synthetic examples to demonstrate that our method can normalize migration amplitudes and effectively suppress migration artefacts. 相似文献