首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   243篇
  免费   0篇
  国内免费   3篇
航空   149篇
航天技术   48篇
综合类   2篇
航天   47篇
  2022年   1篇
  2021年   6篇
  2019年   3篇
  2018年   33篇
  2017年   18篇
  2016年   1篇
  2015年   7篇
  2014年   3篇
  2013年   11篇
  2012年   7篇
  2011年   10篇
  2010年   10篇
  2009年   12篇
  2008年   8篇
  2007年   14篇
  2006年   4篇
  2005年   11篇
  2004年   8篇
  2003年   4篇
  2002年   2篇
  2001年   7篇
  2000年   4篇
  1999年   3篇
  1998年   3篇
  1997年   5篇
  1996年   1篇
  1995年   5篇
  1994年   5篇
  1993年   2篇
  1992年   2篇
  1986年   2篇
  1985年   9篇
  1984年   7篇
  1983年   3篇
  1982年   2篇
  1981年   9篇
  1978年   1篇
  1970年   1篇
  1967年   1篇
  1963年   1篇
排序方式: 共有246条查询结果,搜索用时 15 毫秒
241.
Impact analysis of the transponder time delay on radio-tracking observables   总被引:1,自引:0,他引:1  
Accurate tracking of probes is one of the key points of space exploration. Range and Doppler techniques are the most commonly used. In this paper we analyze the impact of the transponder delay, i.e. the processing time between reception and re-emission of a two-way tracking link at the satellite, on tracking observables and on spacecraft orbits. We show that this term, only partially accounted for in the standard formulation of computed space observables, can actually be relevant for future missions with high nominal tracking accuracies or for the re-processing of old missions. We present several applications of our formulation to Earth flybys, the NASA GRAIL and the ESA BepiColombo missions.  相似文献   
242.
243.
In order to get the maximum scientific return from available resources, the wave experimenters on Cluster established the Wave Experiment Consortium (WEC). The WEC's scientific objectives are described, together with its capability to achieve them in the course of the mission. The five experiments and the interfaces between them are shown in a general block diagram (Figure 1). WEC has organised technical coordination for experiment pre-delivery tests and spacecraft integration, and has also established associated working groups for data analysis and operations in orbit. All science operations aspects of WEC have been worked out in meetings with wide participation of investigators from the five WEC teams.  相似文献   
244.
Events in energetic solar protons with the energy > 4 MeV at the stage of their decay are considered for the period from 1974 to 2001. It is shown that in the events with the exponential shape of decay for west flares (relative to the observation point), the characteristic decay time τ and the power index γ of the energy spectrum decrease with an increase in the angular distance between the observer and the source of the particles on the Sun, while this effect is absent for east flares.  相似文献   
245.
    
This article discusses relevant physical properties of the regolith at the Mars InSight landing site as understood prior to landing of the spacecraft. InSight will land in the northern lowland plains of Mars, close to the equator, where the regolith is estimated to be (geq3mbox{--}5~mbox{m}) thick. These investigations of physical properties have relied on data collected from Mars orbital measurements, previously collected lander and rover data, results of studies of data and samples from Apollo lunar missions, laboratory measurements on regolith simulants, and theoretical studies. The investigations include changes in properties with depth and temperature. Mechanical properties investigated include density, grain-size distribution, cohesion, and angle of internal friction. Thermophysical properties include thermal inertia, surface emissivity and albedo, thermal conductivity and diffusivity, and specific heat. Regolith elastic properties not only include parameters that control seismic wave velocities in the immediate vicinity of the Insight lander but also coupling of the lander and other potential noise sources to the InSight broadband seismometer. The related properties include Poisson’s ratio, P- and S-wave velocities, Young’s modulus, and seismic attenuation. Finally, mass diffusivity was investigated to estimate gas movements in the regolith driven by atmospheric pressure changes. Physical properties presented here are all to some degree speculative. However, they form a basis for interpretation of the early data to be returned from the InSight mission.  相似文献   
246.
    
Brack A 《Astrobiology》2005,5(5):576-578
  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号