排序方式: 共有123条查询结果,搜索用时 765 毫秒
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一种基于纯天文观测的火星车自主导航方法 总被引:2,自引:0,他引:2
提出了一种基于纯天文观测的火星车自主天文导航新方法.该方法仅需利用由星敏感器视场内测量得到的火星卫星(火卫一、火卫二)和某一恒星之间的星光角距,结合火星车的运动模型,通过Unscented粒子滤波方法,即可获得高精度的火星车实时位置信息.计算机仿真结果表明了该方法的有效性,同时对几个关键的精度影响因素进行了仿真分析. 相似文献
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波动是无碰撞等离子体中能量重新分配的重要途径。对波动的研究有助于更准确地认识太阳风与火星的相互作用,认识火星空间环境的特征。介绍了火星空间中常见的几种磁场低频波动,包括离子回旋波(Ion-CyclotronWave,ICW)、磁流体动力学(MagnetoHydro Dynamic,MHD)波、镜像模波、哨声波以及磁场锯齿状波动,总结了这几类波动的特征和可能的形成机制,说明不同种类的波动所反映的不同的物理过程。由于波粒相互作用在火星离子逃逸的过程中起到了重要作用,波动可影响火星环境的演化。 相似文献
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基于GA-SVM的GNSS-IR土壤湿度反演方法 总被引:1,自引:1,他引:1
针对提高大范围土壤湿度测量精度的问题,研究了土壤湿度的全球卫星导航系统干涉测量法(GNSS-IR),提出了一种基于支持向量机(SVM)的土壤湿度反演模型,利用遗传算法(GA)的自动寻优功能寻找SVM的最佳参数。结果表明,GA-SVM模型在测试集上得到的土壤湿度反演值与实测值的平均绝对百分比误差(MAPE)仅为0.69%,最大相对误差(MRE)为1.22%,线性回归方程决定系数达到了0.956 9。进一步与统计回归、粒子群优化的SVM模型(PSO-SVM)及反向传播(BP)神经网络方法进行对比,结果说明:在样本数目有限的情况下,GA-SVM方法更适用于土壤湿度的GNSS-IR技术反演,且反演精度较高,泛化性能良好。 相似文献
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对于同种土样形成的固化土,水泥掺量增加到一定程度后单位水泥量产生的固化土抗压强度增量会显著提高;物理性质相近的土样掺加等量的水泥后固化土抗压强度有显著的差异.为解释上述试验现象,测定了相应固化土孔隙液中主要离子的浓度,并进行热力学计算.结果表明:水泥掺量较少时,固化土孔隙液中Ca(OH)2不饱和,单位水泥量水化生成的胶凝性物质量较少,故产生的固化土抗压强度增量也较小;当土样中水泥掺量达到一定程度后,固化土孔隙液中Ca(OH)2饱和,固化土中胶凝性物质能充分生成,单位水泥量产生的固化土抗压强度增量较大.物理性质相近的土样掺加相同的水泥量,固化土孔隙液中Ca(OH)2离子浓度不同,故而固化土抗压强度也不同. 相似文献
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Yu.A. Berkovich S.O. SmolyaninaN.M. Krivobok A.N. ErokhinA.N. Agureev N.A. Shanturin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A Manned Mars Mission scenario had been developed in frame of the Project 1172 supported International Science & Technology Center in Moscow. The Mars transit vehicle (MTV) supposed to have a crew of 4–6 with Pilot Laboratory compartment volume of 185 m3 and with inner diameter of 4.1 m. A vegetable production facility with power consumption up to 10 kW is being considered as a component of the life support system to supply crew members by fresh vegetables during the mission. Proposed design of conveyor-type plant growth facility (PGF) comprised of 4-modules. Each module has a cylindrical planting surface and spiral cylindrical LED assembly to provide a high specific productivity relative to utilized onboard resources. Each module has a growth chamber that will be from 0.7 m to 1.5 m in length, and a crop illuminated area from 1.7 m2 to 4.0 m2. Leafy crops (cabbage, lettuce, spinach, chard, etc.) have been selected for module 1, primarily because of the highest specific productivity per consumed resources. Dietitians have recommended also carrot crop for module 2, pepper for module 3 and tomato for module 4. The maximal total PGF light energy estimated as 1.16 kW and total power consumption as about 7 kW. The module 1 characteristics have been calculated using own experimental data, information from the best on ground plant growth experiments with artificial light were used to predict crop productivity and biomass composition in the another modules. 4-module PGF could produce nearly 0.32 kg per crew member per day of fresh edible biomass, which would be about 50% of recommended daily vegetable supplement. An average crop harvest index is estimated as 0.75. The MTV food system could be entirely closed in terms of vitamins C and A with help of the PGF. In addition the system could provide 10–25% of essential minerals and vitamins of group B, and about 20% of food fibers. The present state of plant growth technology allows formulating of requirements specification for the flight-qualified modules. 相似文献
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国外海洋盐度与土壤湿度探测卫星的发展 总被引:5,自引:2,他引:3
文章调查研究了国外海洋盐度与土壤湿度探测卫星发展情况、探测机理;重点对SMOS、Aquarius、SMAP等三颗最具代表性的土壤湿度和海洋盐度探测卫星进行了研究分析,比对了三颗卫星的主要技术指标,并总结了其技术发展特点和关键技术;最后结合我国技术基础对发展我国盐度与湿度卫星提出了建议。 相似文献
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