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排序方式: 共有690条查询结果,搜索用时 31 毫秒
281.
基于太阳震荡的时间延迟是一种新型天文导航量测量,可以提供探测器相对反射天体的距离信息,与星光角距量测量结合,可以提高导航性能。然而,星光角距量测模型与时间延迟量测模型均含有火卫一相对火星的位置矢量,火卫一的星历误差将影响导航精度。针对这一问题,提出了一种基于在线估计的天文测角/时间延迟量测组合导航方法,建立了包含火卫一位置及速度的状态模型,利用星光角距及时间延迟量测量同时对火卫一的位置和速度进行在线估计,仿真结果表明,提出的方法可以有效抑制火卫一星历误差对组合导航精度的影响,为探测器提供高精度的自主导航信息。 相似文献
282.
巡视探测器悬架机构综述 总被引:1,自引:0,他引:1
悬架机构是巡视探测器移动系统的重要组成部分,其性能直接影响着巡视探测器的通过性能、越障能力和稳定性等。文章分析了目前应用于巡视探测器的各种悬架,分别为杠杆导向的扭力式独立悬架、摇臂转向架悬架、五轮五点接触悬吊式悬架、平行架一叉形架悬架、三体柔性悬架、ExoMars巡视探测器悬架系列(RCL-C、RCL-E、CRAB和Double Spring)、正反四边形悬架等。在分析的基础上总结了巡视探测器悬架机构的发展趋势,同时为我国月面巡视探测器移动部分悬架机构的选择提出了建议。 相似文献
283.
本文试图说明在喷气发动机上或燃气轮机的进气道内建立聚氧滞氮的流场,增加燃烧室氧的浓度,组织富氧燃烧.提高涡轮前的温度和整机热效率.加大喷气发动机的推力,降低航空煤油耗量,减少喷气尾气对大气的污染.对各种可能的聚氧滞氮的方案进行了初步探索. 相似文献
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The Geospace Double Star Project (DSP) consists of two small satellites operating in the near-earth equatorial and polar regions, respectively. The goals of DSP are: (1) to provide high-resolution field, particle, and wave measurements in some important near-earth active regions which have not been covered by current ISTP missions, such as the near-earth plasma sheet and its boundary layer, the ring current, the radiation belts, the dayside magnetopause boundary layer, and the polar region; (2) to investigate the trigger mechanisms of magnetic storms, magnetospheric substorms, and magnetospheric particle events,as well as the responses of geospace storms to solar activities and interplanetary disturbances; (3) to set up the models describing the spatial and temporal variations of the near-earth space environment.To realize the above goals, the equatorial satellite TC-1 and the polar satellite TC-2 will accommodate, respectively, eight instruments on board. TC-1was launched successfully in December 2003 while the polar satellite (TC-2)will be launched in July 2004. The orbit of the equatorial satellite TC-1 consists of a perigee at 550 km, an apogee at 60 000 km, and an inclination of about 28.5; while the orbit of the polar satellite will have a perigee of 700 km, an apogee of 40 000 km, and an inclination of about 90. The two satellites will take coordinated measurements with Cluster Ⅱ and will first form a "six-point exploration" in geospace.The operational status of TC-1 are introduced in this paper. 相似文献
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Burak Yaglioglu Ozan Tekinalp 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(11):3546-3558
The problem of obtaining long term relative orbit configurations for spacecraft clusters with realistic operational considerations such as safety, station keeping and inter-spacecraft distances is addressed. Two different approaches are developed for station keeping and safety objectives. In the first approach, relative orbit configurations, or relative TLEs, are found minimizing deviations from reference mean orbit which would maximize the station-keeping objective. In second one, relative configurations are found from a reference initial condition by minimizing probability of collision, hence maximizing the safety objective, between the spacecraft in the cluster which are propagated numerically through a high precision orbit propagator. For the design optimization, a derivative free algorithm is proposed. Effectiveness of the approaches is demonstrated through simulations. Using this design framework, several configurations can be found by exploring the limits of the clusters in terms of spacecraft number, distance bounds and probabilities of collision for long time intervals. 相似文献
290.
Michael Angelopoulos David Redman Wayne H. Pollard Timothy W. Haltigin Peter Dietrich 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Ground-penetrating radar (GPR) is the leading geophysical candidate technology for future lunar missions aimed at mapping shallow stratigraphy (<5 m). The instrument’s exploration depth and resolution capabilities in lunar materials, as well as its small size and lightweight components, make it a very attractive option from both a scientific and engineering perspective. However, the interaction between a GPR signal and the rover body is poorly understood and must be investigated prior to a space mission. In doing so, engineering and survey design strategies should be developed to enhance GPR performance in the context of the scientific question being asked. This paper explores the effects of a rover (simulated with a vertical metal plate) on GPR results for a range of heights above the surface and antenna configurations at two sites: (i) a standard GPR testing site with targets of known position, size, and material properties, and; (ii) a frozen lake for surface reflectivity experiments. Our results demonstrate that the GPR antenna configuration is a key variable dictating instrument design, with the XX polarization considered optimal for minimizing data artifact generation. These findings could thus be used to help guide design requirements for an eventual flight instrument. 相似文献