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101.
Ch. Jacobi C. Arras D. Kürschner W. Singer P. Hoffmann D. Keuer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
During 2004 and 2005 measurements of mesospheric/lower thermospheric (80–100 km) winds have been carried out in Germany using three different ground-based systems, namely a meteor radar (36.2 MHz) at the Collm Observatory (51.3°N, 13°E), a MF radar (3.18 MHz) at Juliusruh (54.6°N, 13.4°E) and the LF D1 measurements using a transmitter (177 kHz) at Zehlendorf near Berlin and receivers at Collm with the reflection point at 52.1°N, 13.2°E. This provides the possibility of comparing the results of different radar systems in nearly the same measuring volume. Meteor radar winds are generally stronger than the winds observed by MF and especially by LF radars. This difference is small near 80 km but increases with height. The difference between meteor radar and medium frequency radar winds is larger during winter than during summer, which might indicate an indirect influence of gravity waves on spaced antenna measurements. 相似文献
102.
免维护铅酸蓄电池用滤气片的组成,烧结工艺及疏水处理工艺对孔隙率、透气率、疏水性及耐酸性有很大影响。以Al2O3和SiO2为主要成份的滤气片在1100~1600℃烧结后,经聚四氟乙烯疏水处理后用于免维护电池,能有效地阻止水份的损耗。 相似文献
103.
通常希望一个天线的波瓣图和阻抗能在一个较工的频率范围内保持不变。我们将这一类称为非频变天线。平面等角螺旋天线是一这一类天线的典型例子。本文主要叙述了平面等角螺旋天线的宽频带特性和工作原理,并简要介绍了它的设计方法。 相似文献
104.
天线雷达散射截面的分析与实验 总被引:2,自引:0,他引:2
本文利用天线散射的基本原理,以波导激励振子抛物面天线为例,计算并分析了天线的结构项散射雷达截面RCSs和模式项散射雷达截面RCSe,给出了此天线雷达截面的预估值。实验结果表明,理论预估值与实测值吻合较好,并且证明天线的模项RCSe大于结构项RCSs,天线总的雷达截面主要受天线模式散射的影响,减小模式项RCSe将有效地降低天线的雷达截面。本文结果为探索以克服天线模式散射为主的天线RCS减缩技术提供了理论依据 相似文献
105.
刘松波 《沈阳航空工业学院学报》2008,25(3)
机动目标运动状态的多步预测是为了更好的为机动目标的跟踪提供数据支持,因此要保证多步预测数据的可用性,需要知道预测的精度,由此要对预测数据做误差分析。本文在对机动目标运动轨迹实施多步预测的基础上分析了多步预测过程中随机误差的传递,以及传递的随机误差对多步预测的影响。仿真结果显示,预测中传递误差方差占预测误差方差的绝大部分,是影响预测精度的最重要因素之一。 相似文献
106.
就如何保证新一代导弹重要零件翼轴花键齿首齿位置精度达到±10’的机加工技术作了详细的阐述,着重就花键齿插齿过程中的工装定位、首齿位置精度的提高和测量方法进行了较为认真的研究。实践证明,该种插齿工艺方法能保证翼轴零件首齿位置精度的互换性,在具有类似的首齿位置精度要求的齿轮加工行业中有一定的先进性,并具有借鉴和推广价值。 相似文献
107.
Radar Imaging of Mercury 总被引:1,自引:0,他引:1
John K. Harmon 《Space Science Reviews》2007,132(2-4):307-349
Earth-based radar has been one of the few, and one of the most important, sources of new information about Mercury during
the three decades since the Mariner 10 encounters. The emphasis during the past 15 years has been on full-disk, dual-polarization
imaging of the planet, an effort that has been facilitated by the development of novel radar techniques and by improvements
in radar systems. Probably the most important result of the imaging work has been the discovery and mapping of radar-bright
features at the poles. The radar scattering properties of these features, and their confinement to permanently shaded crater
floors, is consistent with volume backscatter from a low-loss volatile such as clean water ice. Questions remain, however,
regarding the source and long-term stability of the putative ice, which underscores the need for independent confirmation
by other observational methods. Radar images of the non-polar regions have also revealed a plethora of bright features, most
of which are associated with fresh craters and their ejecta. Several very large impact features, with rays and other bright
ejecta spreading over distances of 1,000 km or more, have been traced to source craters with diameters of 80–125 km. Among
these large rayed features are some whose relative faintness suggests that they are being observed in an intermediate stage
of degradation. Less extended ray/ejecta features have been found for some of the freshest medium-size craters such as Kuiper
and Degas. Much more common are smaller (<40 km diameter) fresh craters showing bright rim-rings but little or no ray structure.
These smaller radar-bright craters are particularly common over the H-7 quadrangle. Diffuse areas of enhanced depolarized
brightness have been found in the smooth plains, including the circum-Caloris planitiae and Tolstoj Basin. This is an interesting
finding, as it is the reverse of the albedo contrast seen between the radar-dark maria and the radar-bright cratered highlands
on the Moon. 相似文献
108.
李云 《长沙航空职业技术学院学报》2004,4(1):34-36
本文介绍了Java 2D API的图象处理思想.通过以LookupOp查找表过滤器为例,分析了图象的即时模式模型,即对内存的缓冲区图象进行处理,再绘制到屏幕上的处理技术.同时介绍了利用Java 2D中提供的过滤器对图象数据的过滤操作. 相似文献
109.
空间微波交会雷达总体构想 总被引:1,自引:0,他引:1
结合我国载人航天工程未来发展的需要,分析了国外微波交会雷达技术的发展方向,提出了我国微波交会雷达的总体实施方案构想。 相似文献
110.
Yuan Xiao Yan Su Shun Dai Jianqing Feng Shuguo Xing Chunyu Ding Chunlai Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(10):3404-3419
The Lunar Regolith Penetrating Radar (LRPR) is an Ultra-Wideband (UWB) array-based Ground penetrating radar (GPR) onboard the lander of Chang’e-5 (CE-5) mission. The primary scientific objectives of the LRPR are to probe the thickness and structure of lunar regolith of the landing site, and support the drilling and sampling process. In order to evaluate the performance of the LRPR, a series of ground experiments are performed using the LRPR prototype mounted on a CE-5 lander model. The performance of the LRPR is evaluated by comparing the experimental data with the simulated data. Data processing and imaging method are verified, and the interferences from the lander and other aspects are analyzed. The results of the ground experiments and simulation demonstrate that the LRPR is able to meet the design requirement of 2-m detection depth. They also indicate that the upper and lower interfaces of the stratified structure in the lunar regolith can be well distinguished by the LRPR when the dielectric constant difference is greater than 0.3, and the imaging effect of the location under the dense antennas is better than that of other positions. However, the identification capability of the LRPR to the independent blocky objects is relatively poor mainly due to the clutters caused by the lander, the sparsity of the antenna elements compared to the size of the basalt block, the limited aperture of the antenna array, and the tail of the transmitted waveform. 相似文献