排序方式: 共有158条查询结果,搜索用时 46 毫秒
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小行星形貌特征的分析与描述 总被引:1,自引:0,他引:1
小行星形貌特征的分析对深空探测器的导航、着陆点的选取具有重要意义。现有的深空星体形貌特征的分析与描述主要集中在火星、月球等类地天体上,而作为宇宙中为数众多、信息量丰富的小行星却鲜有文献对其形貌特征作详细深入的介绍。文章以Vesta、Eros、Mimas等人类已探测的小行星为例,分析了几种典型的小行星表面形貌特征,完善了凹坑、岩石等形貌特征的描述参数,并用仿真实验生成了Mimas小行星表面的Herschel凹坑模型。实验结果显示,所提出的特征描述方法具有较好的仿真度和实用性。 相似文献
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介绍了在粗糙集理论和群体智能理论的基础上提出的一种优化的用于文本挖掘的蚁群聚类算法。实验证明,该算法有效地降低了文本特征向量的维数,提高了运行效率和准确性。 相似文献
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Web结构的数据挖掘是对Web页面之间的结构进行挖掘。该文引入传统的数学方法:线性方程组表示Web页结构之间的关系及通过求解齐次线性方程组解来计算Web页的PageRank的键值,进而发现的Web结构中重要的Web页的知识可以被用来改进搜索引擎的性能。 相似文献
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E. Venechuk M.A. Franzen L.A. Roe D.W.G. Sears 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Sample return from small solar system objects is playing an increasingly important part in solar system exploration. Critical to such missions is a robust, simple, and economic sample collector. We have developed a collector such as this for near-Earth asteroid sample return missions that we have termed the Touch-and-Go Impregnable Pad (TGIP). The collector utilizes a silicone substrate that is pushed into the dust and gravel surface layer of the asteroid. As part of a systematic evaluation of the TGIP, we have investigated the resilience of this substrate to ionizing radiations. Several miniature versions of the collector, containing typically ∼3 g of the collection substrate, were exposed to 0.564 MeV beta particles from a 90Sr source and a 6 MeV electron beam in a linear accelerator to simulate the wide range of energies of solar and galactic ionizing radiation. Various radiation levels up to eight times greater than expected on a six-year asteroid mission (in the case of beta radiation) and 50 times greater than expected (in the case of the 6 MeV electron radiation) were administered to the substrate. After irradiation, the efficiency of the substrate in collecting samples of mock regolith was compared with that of collectors that had not been irradiated. No difference beyond experimental uncertainty was observed and we suggest that the operational TGIP will not be affected adversely by radiation doses expected during a typical six-year inner solar system mission. 相似文献
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J. L. Burch R. Goldstein T. E. Cravens W. C. Gibson R. N. Lundin C. J. Pollock J. D. Winningham D. T. Young 《Space Science Reviews》2007,128(1-4):697-712
The ion and electron sensor (IES) is part of the Rosetta Plasma Consortium (RPC). The IES consists of two electrostatic plasma
analyzers, one each for ions and electrons, which share a common entrance aperture. Each analyzer covers an energy/charge
range from 1 eV/e to 22 keV/e with a resolution of 4%. Electrostatic deflection is used at the entrance aperture to achieve
a field of view of 90°× 360° (2.8π sr). Angular resolution is 5°× 22.5° for electrons and 5°× 45° for ions with the sector
containing the solar wind being further segmented to 5°× 5°. The three-dimensional plasma distributions obtained by IES will
be used to investigate the interaction of the solar wind with asteroids Steins and Lutetia and the coma and nucleus of comet
67P/Churyumov–Gerasimenko (CG). In addition, photoelectron spectra obtained at these bodies will help determine their composition. 相似文献
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