首页> 外文会议>International workshop on the analysis of multi-temporal remote sensing images >TACKLING WITH THE LIMITATIONS OF THE RASTER DATA MODEL: VECTOR-BASED PREPROCESSING OF MODIS REFLECTIVE BANDS
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TACKLING WITH THE LIMITATIONS OF THE RASTER DATA MODEL: VECTOR-BASED PREPROCESSING OF MODIS REFLECTIVE BANDS

机译:解决光栅数据模型的局限性:基于向量的MODIS反射频段预处理

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The Moderate Resolution Imaging Spectroradiometer (MODIS) instruments onboard NASA's Terra and Aqua satellites provide continuous observations and have been increasingly used in different disciplines since 1999. A whole suite of derived products is also produced in a systematic manner. However, these data have some intrinsic characteristics that make their processing a delicate issue when used on pixel- or subpixel-scale studies. Due to the wide field of view, the actual ground pixel size changes continuously off-nadir both in along-track and along-scan directions. All kinds of resampling carried out due to the fixed cell size implemented in the raster data model inevitably result in artifacts in the data. The MODIS gridding process also has a large influence. The average overlap between grid cells and "real" observations is less than 30%. Our results based on synthetic MODIS images show that in our case, an artificial variance of 28% is introduced by the only procedure of raster-based nearest neighbor resampling. Therefore, the accuracy of current MODIS data at its original resolution is not sufficient for carrying out pixel- or subpixel-level studies such as spectral unmixing or pixel-level change detection. Spatial or temporal aggregation is widely used to cope with these issues, but may lead to a considerable loss of information. In this work, we propose and demonstrate an alternative solution based on the vector data model. By using MODIS swath products and geolocation datasets, a polygon layer is created, in which each polygon represents the real pixel footprint sensed during image acquisition. To test the increase of accuracy yielded by the new method, correlation with same-day high resolution (HR) SPOT images is used as an indicator. The results are encouraging: the original 250-m MODIS product in the near infrared domain shows an r2 value of 0.61 with the reference SPOT data, whereas the new method yielded almost 0.8 with the same conditions.
机译:中央钢板砧座的适度分辨率成像光谱仪(MODIS)仪器(MODIS)仪器在NASA的TERRA和AQUA卫星上提供了连续的观察,并且自1999年以来越来越多地用于不同的学科。一系列衍生产品的套件也以系统的方式生产。然而,这些数据具有一些内在的特征,当在像素或亚像素级研究中使用时,它们处理了一个微妙的问题。由于视场宽,实际地面像素尺寸沿轨道和扫描方向连续地偏离Nadir。由于栅格数据模型中实现的固定单元尺寸而执行的各种重采样不可避免地导致数据中的伪像。 MODIS Gridding过程也有很大的影响力。网格细胞和“真实”观察之间的平均重叠小于30%。我们基于合成MODIS图像的结果显示,在我们的情况下,通过光栅的最近邻重采样的唯一程序引入了28%的人工方差。因此,其原始分辨率的当前MODIS数据的准确性不足以进行像素或子像素级研究,例如光谱解密或像素电平变化检测。空间或时间聚合广泛用于应对这些问题,但可能导致相当大的信息损失。在这项工作中,我们提出并展示了一种基于矢量数据模型的替代解决方案。通过使用MODIS SWATH产品和地理位置数据集,创建多边形层,其中每个多边形表示在图像采集期间感测的真实像素占用。为了测试新方法产生的精度的提高,与当天高分辨率(HR)点图像的相关性用作指示器。结果令人鼓舞:近红外域中的原始250-M Modis产品显示R2值为0.61,其中参考点数据,而新方法几乎达到0.8,条件相同。

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