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141.
讨论高斯白噪声背景下基于周期图法的残留载波BPSK(RC-BPSK)信号的检测问题。标准周期图法在正弦信号检测中的性能最优,但是在RC-BPSK信号检测中的性能却不佳;能量检测法只在信噪比很低的情况下性能较好;在信噪比较高时,虽然Bartlett法有较好的性能,但需要分段多次计算周期图,不利于与其他检测方法配合使用。文中在频谱匹配法的基础上发展了一种频谱相关检测方法,仿真结果表明该方法可以获得和Bartlett法相似的性能,同时只需要计算一次周期图。 相似文献
142.
文章基于航天器无源产品在二次电子倍增微放电过程中,多载波信号通过会在近载波产生互调产物这一机理,介绍了在多载波情况下,用检测近载波互调产物变化来检测微放电的新方法。依据无源互调的幂级数非线性分析方法,建立双载波线性模型加以分析,说明距离载波较近的三阶互调产物的功率变化比载波功率变化快,提供了这种检测方法的理论依据,最后用实验结果验证了此方法。 相似文献
143.
针对高轨目标编目与成像的应用需求,提出一种运行于亚同步轨道、兼具对同步带目标远距离探测编目和近距离成像侦察的高轨天基星座。根据同步带目标探测编目要求,推导和分析了星座的轨道部署和光学相机扫描方式对目标探测效能的影响,确定了顺行轨道的双星星座可行解更多,综合探测效能更高。设计了一种符合顺光观测约束的姿态导引律,结合可行解中选取一组解进行仿真,结果表明:在夏至和秋分两种工况下,采用顺行轨道的双星星座,可对轨道倾角不大于相机半视场的所有同步带目标进行无缝遍历,且每天的探测次数不小于4次,观测弧长不小于1分钟,与理论推导一致。 相似文献
144.
145.
非高斯杂波背景中的两个距离扩展目标检测器 总被引:2,自引:0,他引:2
针对采用球不变随机向量(SIRV)建模的非高斯杂波背景中检测具有稀疏散射点的距离扩展目标问题,先假设目标强散射点的位置信息已知,采用广义似然比检验(GLRT)理论,提出了基于散射点位置的GLRT (SL-GLRT) 检测器。然后,采用门限法估计散射点的位置信息,提出了双门限恒虚警率(DT-CFAR)检测器,推导了虚警概率与检测门限关系的解析表达式,并给出门限的确定方法。与现有方法相比,散射点位置信息已知时, SL-GLRT 具有最佳的检测性能,散射点位置信息未知时,DT-CFAR具有较好的鲁棒性。 相似文献
146.
基于检测前跟踪的超视距雷达微弱目标检测方法 总被引:1,自引:0,他引:1
天波超视距雷达(over-the-horizonradar,OTHR)通过快速傅立叶变换(FFr)实现相干积累,再利用常规的方法进行目标检测。但这种方法在弱目标、低信噪比的情况下效果并不好。本文提出了一种基于检测前跟踪(track-before-detect,TBD)的OTHR弱目标检测方法,利用数学形态学对每帧弱目标回波信号进行滤波,再通过动态规划方法进行检测。仿真结果表明,该方法能够有效地提高OTHR对弱目标的检测能力,运算效率高,实用性强。 相似文献
147.
James A. Blake Paul Chote Don Pollacco William Feline Grant Privett Andrew Ash Stuart Eves Arthur Greenwood Nick Harwood Thomas R. Marsh Dimitri Veras Christopher Watson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):360-370
Recent anomalies exhibited by satellites and rocket bodies have highlighted that a population of faint debris exists at geosynchronous (GEO) altitudes, where there are no natural removal mechanisms. Despite previous optical surveys probing to around 10–20 cm in size, regular monitoring of faint sources at GEO is challenging, thus our knowledge remains sparse. It is essential that we continue to explore the faint debris population using large telescopes to better understand the risk posed to active GEO satellites. To this end, we present photometric results from a survey of the GEO region carried out with the 2.54 m Isaac Newton Telescope in La Palma, Canary Islands. We probe to 21st visual magnitude (around 10 cm, assuming Lambertian spheres with an albedo of 0.1), uncovering 129 orbital tracks with GEO-like motion across the eight nights of dark-grey time comprising the survey. The faint end of our brightness distribution continues to rise until the sensitivity limit of the sensor is reached, suggesting that the modal brightness could be even fainter. We uncover a number of faint, uncatalogued objects that show photometric signatures of rapid tumbling, many of which straddle the limiting magnitude of our survey over the course of a single exposure, posing a complex issue when estimating object size. This work presents the first instalment of DebrisWatch, an ongoing collaboration between the University of Warwick and the Defence Science and Technology Laboratory (UK) investigating the faint population of GEO debris. 相似文献
148.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):364-378
This paper presents an algorithm to detect very faint object streaks on CCD images acquired with an optical system. The proposed detection method uses image filters simulating the geometrical form and orientation of possible streaks on the CCD image. The method searches for a matching between streak and filter evaluating the convolutions of the image with all possible filters. Based on the statistics of the image background a threshold is applied in order to accept, respectively reject, the possible streak candidates. The detection probabilities and the effect of different parameter settings are estimated with tests on simulated images, while subframes of real images are used to evaluate the applicability of the algorithm to real cases. The detection probability of this method depends on the length and on the signal-to-noise ratio of the streak. For long streaks, a detection for signal-to-noise values around 0.5 is achieved. The further characterization of the detected streak (e.g. centroid and length), which is not performed in the current algorithm, and the reduction of the computation time, which is relatively high for full acquired frames, as well as possible improvements are briefly addressed. 相似文献
149.
《中国航空学报》2021,34(11):154-168
In the classical form, the Poisson Multi-Bernoulli Mixture (PMBM) filter uses a PMBM density to describe target birth, surviving, and death, which does not model the appearance of spawned targets. Although such a model can handle target birth, surviving, and death well, its performance may degrade when target spawning arises. The reason for this is that the original PMBM filter treats the spawned targets as birth targets, ignoring the surviving targets’ information. In this paper, we propose a Kullback–Leibler Divergence (KLD) minimization based derivation for the PMBM prediction step, including target spawning, in which the spawned targets are modeled using a Poisson Point Process (PPP). Furthermore, to improve the computational efficiency, three approximations are used to implement the proposed algorithm, such as the Variational Multi-Bernoulli (VMB) filter, the Measurement-Oriented marginal MeMBer/Poisson (MOMB/P) filter, and the Track-Oriented marginal MeMBer/Poisson (TOMB/P) filter. Finally, simulation results demonstrate the validity of the proposed filter by using the spawning model in these three approximations. 相似文献
150.