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排序方式: 共有6765条查询结果,搜索用时 31 毫秒
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Kugusheva A. D. Kalegaev V. V. Vlasova N. A. Petrov K. A. Bazilevskaya G. A. Makhmutov V. S. 《Cosmic Research》2021,59(6):446-455
Cosmic Research - The results of an analysis of the space–time characteristics and dynamics of precipitations of magnetospheric electrons with energies in the range from 0.1 to 0.7 MeV are... 相似文献
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在机器人自动制孔过程中,制孔点位信息通常从待制孔工件工艺数模上获取,而待制孔工件安装过程中会出现位置偏移和变形,由工艺数模得到的点位信息无法直接满足孔位精度要求。为了保证自动制孔的孔位精度,提出了一种基于遗传算法的插值Coons曲面孔位修正方法。利用制孔区域边角基准孔建立双线性Coons误差曲面模型,通过模型计算出待制孔的误差补偿向量,并补偿至理论制孔位置。针对误差曲面切矢模长无法确定的情况,利用制孔区域内的基准孔构建遗传算法模型,计算出切矢模长最优值,使拟合的误差曲面更符合实际制孔区域曲面。通过试验对算法的有效性和精度进行验证,结果表明:采用基于遗传算法的插值Coons曲面孔位修正方法,可以使孔位误差得到有效的补偿。补偿后的平均孔位误差仅为0.195 6 mm,与传统的插值曲面方法相比,孔位误差降低了5%~10%。 相似文献
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E. R. Muslimov E. Hugot M. Ferrari T. Behaghel N. K. Pavlycheva 《Russian Aeronautics (Iz VUZ)》2018,61(1):1-7
The possibility of constructing an optical scheme of a telescope for a small satellite based on mirrors with freeform surfaces and a curved photodetector is considered. It is shown that the use of a new element base allows the effective area of the main mirror to be maximized and the field of view up to 9.4 times to be increased in comparison with the classical scheme of the Ritchey–Chretien scheme in ensuring the high image quality. 相似文献
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针对光学遥感卫星飞轮微振动引起的成像质量下降问题,设计了一种组合隔振装置,并采用仿真分析与实验测试相结合的方法对隔振方案设计的合理性进行验证。首先,将测量的飞轮扰振数据引入光学卫星的有限元模型中,计算出飞轮扰振对光学相机的像素偏移影响;其次,设计了组合隔振方案并基于有限元方法对其隔振效果进行验证;最后,搭建了光学成像微振动实验测试平台,对不同转速下飞轮微振动造成的像素偏移影响进行精确测量。实验结果表明,组合隔振装置对300 Hz以上高频段飞轮扰振有较大衰减作用,最大像素偏移降到0.01个像素以下,隔振效率达到80%以上;通过对比可知,实验测试与仿真计算得到的像素偏移结果在低频段一次谐波响应及模态响应表现出较好一致性,但在高频段二者存在一定偏差。 相似文献
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Snyder S. Schipper B. Vallot L. Parker N. Spitzer C. 《Aerospace and Electronic Systems Magazine, IEEE》1992,7(5):3-11
In November 1990, a differential GPS/inertial flight test was conducted to acquire a system performance database and demonstrate automatic landing using an integrated differential GPS/INS with barometric and radar altimeters. Flight test results obtained from postflight data analysis are presented. These results include characteristics of DGPS/inertial error, using a laser tracker as a reference. In addition, data are provided on the magnitude of the differential correlations and vertical channel performance with and without radar altimeter augmentation. Flight test results show one sigma DGPS/inertial horizontal errors of 9 ft and one sigma DGPS inertial vertical errors of 15 ft. Without selective availability effects, the differential corrections are less than 10 ft and are dominated by receiver unique errors over the time period of an approach. Therefore, the one sigma performance of the autonomous GPS (8-ft horizontal and 20-ft vertical) is very similar to the DGPS/inertial performance. Postprocessed results also demonstrate significant improvements in vertical channel performance when GPS/inertial is aided with radar altimeter along with a low-resolution terrain map 相似文献
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T Berger M Hajek L Summerer N Vana Y Akatov V Shurshakov V Arkhangelsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(6):1414-1419
The Atominstitute of the Austrian Universities has conducted various space research missions in the last 12 years in cooperation with the Institute for Biomedical Problems in Moscow. They dealt with the exact determination of the radiation hazards for cosmonauts and the development of precise measurement devices. Special emphasis will be laid on the last experiment on space station MIR the goal of which was the determination of the depth distribution of absorbed dose and dose equivalent in a water filled Phantom. The first results from dose measurements onboard the International Space Station (ISS) will also be discussed. The spherical Phantom with a diameter of 35 cm was developed at the Institute for Biomedical Problems and had 4 channels where dosimeters can be exposed in different depths. The exposure period covered the timeframe from May 1997 to February 1999. Thermoluminescent dosimeters (TLDs) were exposed inside the Phantom, either parallel or perpendicular to the hull of the spacecraft. For the evaluation of the linear energy transfer (LET), the high temperature ratio (HTR) method was applied. Based on this method a mean quality factor and, subsequently, the dose equivalent is calculated according to the Q(LET infinity) relationship proposed in ICRP 26. An increased contribution of neutrons could be detected inside the Phantom. However the total dose equivalent did not increase over the depth of the Phantom. As the first Austrian measurements on the ISS dosimeter packages were exposed for 248 days, starting in February 2001 at six different locations onboard the ISS. The Austrian dosimeter sets for this first exposure on the ISS contained five different kinds of passive thermoluminescent dosimeters. First results showed a position dependent absorbed dose rate at the ISS. 相似文献