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针对传统Canny边缘检测算法存在的不足,结合激光主动成像末制导的实际特点,提出了一种改进的Canny边缘检测算法.该算法在Canny边缘检测算法的基础上,采用同态滤波和提升小波变换级联的方法代替传统的高斯滤波器;采用3×3邻域的权值梯度计算方法代替原有的2×2邻域差分运算;采用Otsu自适应阈值计算方法,使算法可根据图像自身特点选择最合适的阈值.实验证明:该算法提升了传统Canny算子的抗干扰能力和鲁棒性,能够较好地保存边缘信息,准确检测出激光主动成像图像的边缘,具有较强的自适应性. 相似文献
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Matthew Wilkinson Graham Appleby 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The navigation and geodetic satellites that orbit the Earth at altitudes of approximately 20,000 km are tracked routinely by many of the Satellite Laser Ranging (SLR) stations of the International Laser Ranging Service (ILRS). In order to meet increasing demands on SLR stations for daytime and nighttime observations, any new mission needs to ensure a strong return signal so that the target is easily acquirable. The ILRS has therefore set a minimum effective cross-section of 100 million square metres for the on-board laser retro-reflector arrays (LRAs) and further recommends the use of ‘uncoated’ cubes in the arrays. Given the large number of GNSS satellites that are currently supported by SLR, it is informative to make an assessment of the relative efficiencies of the various LRAs employed. This paper uses the laser ranging observations themselves to deduce and then compare the efficiencies of the LRAs on the COMPASS-M1 navigation satellite, two satellites from the GPS and three from the GLONASS constellations, the two GIOVE test satellites from the upcoming Galileo constellation, the two Etalon geodetic spheres and the geosynchronous communications test satellite, ETS-8. All the LRAs on this set of satellites employ back-coated retro-reflector cubes, except those on the COMPASS-M1 and ETS-8 vehicles which are uncoated. A measure of return signal strength, and thus of LRA-efficiency, is calculated using the laser-range full-rate data archive from 2007 to 2010, scaled to remove the effects of variations in satellite range, atmospheric attenuation and retro-reflector target total surface area. Observations from five SLR stations are used in this study; they are Herstmonceux (UK), Yarragadee (Australia), Monument Peak and McDonald (USA) and Wettzell (Germany). Careful consideration is given to the treatment of the observations from each station in order to take account of local working practices and system upgrades. The results show that the uncoated retro-reflector cubes offer significant improvements in efficiency. 相似文献
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运用化学气相沉积(Chemical Vapor Deposition,CVD)技术制备了W体积分数分别10%,13%和18%的Ta/W两层层状复合材料,采用金相显微镜(OM)、扫描电镜(SEM)和室温拉伸实验对复合材料的性能进行分析。结果表明:运用CVD技术可以制备W体积分数不同,且密度优于理论密度99.4%的层状复合材料;复合材料中Ta,W层的晶粒均为柱状晶粒,离界面越近,晶粒越细;沉积态复合材料的力学性能优于纯CVD Ta和CVD W;1600℃×2 h的热处理后,复合材料的界面扩散层宽度显著增大,力学性能高于沉积态的力学性能,最高抗拉强度可达660 MPa。 相似文献
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P. Lejba S. Schillak 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The positions and velocities of the four Satellite Laser Ranging (SLR) stations: Yarragadee (7090), Greenbelt (7105), Graz (7839) and Herstmonceux (7840) from 5-year (2001–2005) SLR data of low orbiting satellites (LEO): Ajisai, Starlette and Stella were determined. The orbits of these satellites were computed from the data provided by 20 SLR stations. All orbital computations were performed by means of NASA Goddard’s GEODYN-II program. The geocentric coordinates were transformed to the topocentric North–South, East–West and Vertical components in reference to ITRF2005. The influence of the number of normal points per orbital arc and the empirical acceleration coefficients on the quality of station coordinates was studied. To get standard deviation of the coordinates determination lower than 1 cm, the number of the normal points per site had to be greater than 50. The computed positions and velocities were compared to those derived from LAGEOS-1/LAGEOS-2 data. Three parameters were used for this comparison: station coordinates stability, differences from ITRF2005 positions and velocities. The stability of coordinates of LEO satellites is significantly worse (17.8 mm) than those of LAGEOS (7.6 mm), the better results are for Ajisai (15.4 mm) than for Starlette/Stella (20.4 mm). The difference in positions between the computed values and ITRF2005 were little bit worse for Starlette/Stella (6.6 mm) than for LAGEOS (4.6 mm), the results for Ajisai were five times worse (29.7 mm) probably due to center of mass correction of this satellite. The station velocities with some exceptions were on the same level (≈1 mm/year) for all satellites. The results presented in this work show that results from Starlette/Stella are better than those from Ajisai for station coordinates determination. We can applied the data from LEO satellites, especially Starlette and Stella for determination of the SLR station coordinates but with two times lower accuracy than when using LAGEOS data. 相似文献
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一种新型燃烧室供油系统热防护方案 总被引:1,自引:0,他引:1
武禹张净玉李季骆东 《南京航空航天大学学报》2016,48(3):366-371
随着航空发动机燃烧室进口空气温度的不断升高,燃油在供油管路内受热氧化结焦从而引发诸多隐患的情况日益突出。本文针对某型中心分级、多点喷射供油系统,开展了以空气隔热屏结合“油冷”的热防护方案设计研究,并通过数值
模拟分析了热防护效果。研究表明,在典型高温进气工况下,空气隔热屏结构可将燃油管路湿壁温度降低至燃油氧化结焦临界温度以下;在慢车主油路停止供油的情况下,单一的空气隔热措施难以满足热防护设计要求,结合“油冷”方案可达到设计要求。 相似文献
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