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首页> 外文期刊>Journal of geophysical research. Planets >Retrieval of Mars surface physical properties from OMEGA yperspectral images using regularized sliced inverse regression
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Retrieval of Mars surface physical properties from OMEGA yperspectral images using regularized sliced inverse regression

机译:检索火星表面物理性质ωyperspectral使用正则化图像切片逆回归

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摘要

In this paper, a method based on modeling and statistics is proposed to evaluate the physical properties of surface icy materials on Mars from hyperspectral images collected by the OMEGA instrument aboard the Mars Express spacecraft. The approach is based on the estimation of the functional relationship F between observed spectra and relevant physical parameters such as compound abundances and granularity. To this end, a database of synthetic spectra is generated by a radiative transfer model simulating the reflection of solar light by a granular mixture of H_2O ice, CO_2 ice, and dust. The database constitutes a training set used to estimate F. The high dimension of spectra is reduced by Gaussian regularized sliced inverse regression (GRSIR) to overcome the "curse of dimensionality" and, consequently, the sensitivity of the inversion to noise (ill-conditioned problems). Compared with other approaches, such as the k-NN, the partial least squares, and the support vector machines (SVM), GRSIR has the advantag e of being very fast, interpretable, and accurate. For instance, on simulated test data, the same level of accuracy is obtained by GRSIR and SVM for the estimation of the proportion of dust with a normalized root-mean-square error of 13%, but GRSIR performs 100 times faster. On real data, parameter maps generated by GRSIR from a sequence of three OMEGA observations of the bright permanent polar cap (ВРРС) are much smoother, detailed, and coherent than with other competing methods. They indicate that coarse-grained dry ice completely dominates (≈99.55-99.95 wt%) the material forming the top few centimeters of the ВРРС with dust and water only present as traces (from 300 to 1000 ppm). The maps show clear regional variations of water and dust contamination as well as CO_2 ice state of densification (mean free path around 5 cm on the average, with variations of ±50%) that must be related to meteorological and microphysical phenomena.
机译:本文基于建模和方法统计评估提出了物理在火星表面结冰的材料的性质高光谱图像采集的ω火星快车号宇宙飞船上。这种方法是基于估计的函数F观察之间的关系光谱和相关物理参数等复合丰度和粒度。合成光谱是由一个数据库辐射传输模型模拟反射太阳能灯的颗粒混合物H_2O的冰,冰二氧化碳和尘埃。构成训练集用于估计F。光谱的高维度是减少了高斯正规化切片逆回归(GRSIR)来克服“维度”的诅咒因此,的敏感性反演噪声(坏脾气的问题)。与其他方法相比,这样的事例,偏最小二乘回归和支持向量机(SVM), GRSIR advantag e非常快,可判断的,准确的。实例,模拟测试数据,相同的水平的准确性得到GRSIR和SVM估计的尘埃的比例归一化均方根误差为13%,但是GRSIR执行快100倍。生成的参数映射GRSIR序列3ω的观察明亮永久的极冠(ВРРС)更为顺畅,详细,连贯与其他竞争比方法。冰完全主导(≈99.55 - -99.95 wt %)材料形成的顶部几厘米ВРРС灰尘和水存在的痕迹(从300年到1000 ppm)。地区差异的水和灰尘污染以及二氧化碳冰的状态致密化(平均自由程约5厘米平均变化的±50%),必须相关的气象和微观物理学的现象。

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