全文获取类型
收费全文 | 191篇 |
免费 | 32篇 |
国内免费 | 21篇 |
专业分类
航空 | 92篇 |
航天技术 | 76篇 |
综合类 | 14篇 |
航天 | 62篇 |
出版年
2023年 | 4篇 |
2022年 | 6篇 |
2021年 | 12篇 |
2020年 | 11篇 |
2019年 | 13篇 |
2018年 | 8篇 |
2017年 | 7篇 |
2016年 | 16篇 |
2015年 | 4篇 |
2014年 | 19篇 |
2013年 | 9篇 |
2012年 | 15篇 |
2011年 | 11篇 |
2010年 | 9篇 |
2009年 | 7篇 |
2008年 | 8篇 |
2007年 | 7篇 |
2006年 | 2篇 |
2005年 | 6篇 |
2004年 | 6篇 |
2003年 | 5篇 |
2002年 | 6篇 |
2001年 | 6篇 |
2000年 | 8篇 |
1999年 | 7篇 |
1998年 | 3篇 |
1997年 | 6篇 |
1996年 | 5篇 |
1995年 | 2篇 |
1994年 | 5篇 |
1993年 | 1篇 |
1992年 | 3篇 |
1991年 | 2篇 |
1990年 | 2篇 |
1989年 | 2篇 |
1988年 | 1篇 |
排序方式: 共有244条查询结果,搜索用时 312 毫秒
31.
Rebecca La Norcia Dario Spiller Fabio Curti Christian Circi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(11):3409-3425
A study on reconfiguration manoevres applied to a tetrahedral formation in highly elliptical orbits is proposed, by using a propellantless solution. The manoeuvring strategy consists in exploiting certain environmental forces, specifically those provided by solar radiation pressure and atmospheric drag, by actively controlling the satellites’ attitudes. Through inverse dynamics particle swarm optimization the optimal attitudes required for the manoeuvres are evaluated, whereas the configuration’s evolution is simulated by a high-fidelity orbital simulator. The goal of the reconfiguration problem is to find an optimal control in order for the four spacecraft to reach a desired configuration in a specified portion of orbit, where the desired configuration is evaluated by a shape and size geometric parameter. By increasing the manoeuvring time and the satellites’ area to mass ratio, all the case studies considered are successfully verified. 相似文献
32.
在深空探测任务中,光学自主导航的精度受导航敏感器件安装精度的影响较大。提出了一种基于期望最大化-扩展卡尔曼滤波(EM-EKF)的光学自主导航系统光轴偏差补偿算法。算法基于条件概率的思想,预先设定状态变量和观测量的统计特性参数,通过不断地最大化条件期望,得到出现概率最大的状态变量估值和光轴偏差参数估值。该算法可分为4步:EKF、固定区间平滑、求解条件期望和期望最大化,不断迭代即可得到光轴偏差估计值。以火星探测近火段为例进行仿真验证,经光轴偏差补偿后,导航精度由100 km提升至20 km以内。 相似文献
33.
Galileo operational orbits are slightly affected by the 3 to 5 tesseral resonance, an effect that can be much more important in the case of disposal orbits. Proceeding by canonical perturbation theory we show that the part of the long-term Hamiltonian corresponding to the non-centralities of the Earth's gravitational potential can be replaced by an intermediary that shows the pendulum dynamics of the 3 to 5 tesseral resonance problem. Inclusion of lunisolar perturbations requires a semi-analytical integration, which is compared with the corresponding results from the well-established Draper Semi-analytical Satellite Theory. 相似文献
34.
35.
典型卫星轨道的位移损伤剂量计算与分析 总被引:3,自引:3,他引:0
位移损伤剂量是评估电子元器件在轨发生位移损伤导致性能退化的重要参数。文章首先给出了位移损伤剂量的等效原理和计算方法,即用位移损伤等效注量来表征卫星轨道带电粒子导致的位移损伤剂量;之后分别采用3种不同的太阳质子注量模型,计算了典型大椭圆轨道的位移损伤等效注量,并结合计算结果对不同模型的特点和适用性进行了分析;其后针对4种典型卫星轨道,计算了不同飞行寿命期内的位移损伤等效注量,发现不同轨道的位移损伤剂量有较大差异,并结合空间带电粒子辐射环境分布特点及卫星轨道参数等分析了差异的产生原因;最后,分析不同的太阳质子注量预估方法对位移损伤剂量计算结果的影响,总结了不同轨道、不同飞行寿命情况下卫星经受的带电粒子辐射环境的严酷程度。研究结果可为卫星内部元器件位移损伤效应防护工作提供参考。 相似文献
36.
37.
Earth and Mars observation using periodic orbits 总被引:1,自引:0,他引:1
E. Ortore C. Circi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012,49(1):185-195
This paper reports the results of a general study carried out on the Periodic Multi-SunSynchronous Orbits (PMSSOs), which the classical Periodic SunSynchronous Orbits (PSSOs) represent a specific solution of. Such orbits allow to obtain cycles of observation of the same region in which the solar illumination regularly varies according to the value of the orbit elements and comes back to the initial condition after a time interval which is multiple of the revisit time. Therefore this kind of orbits meets all the remote sensing applications that need observations of the same area at different local times (for example the reconstruction of the day-nighttime trend of the surface temperature of the planet) and it is particularly suitable to the study of several terrestrial and martian phenomena (diurnal cycle of the hazes and clouds, dynamics of the thermal tides, density variations, meteorology phenomena, etc.). The design of PMSSO is based on the variation of the Right Ascension of the Ascending Node due to the Earth oblateness (referred as basic solution). However, with respect to the basic solution, the analysis of the perturbative effects has demonstrated the need, especially in the case of Mars, to take into account all the superior harmonics of the gravitational field. To this end a corrective factor, to add to the basic equations, has been proposed, allowing a significant saving of propellant (of the order of 2 km/s per year). Besides, single and multi-plane satellite constellations have been taken into account in order to improve the repetition of observation and the ground spatial resolution. 相似文献
38.
限制性三体问题下共线平动点附近的拟周期轨道在深空探测中具有重要的实际应用价值,得到了各航天大国的广泛重视。通过将动力学中心流形结构引入轨道控制方法的设计之中,得到了基于投影到中心流形的共线平动点拟周期轨道稳定保持策略。首先推导了会合坐标到中心流形坐标的正则变换方法,在此基础上设法通过引入轨道机动,将偏差状态点投影到中心流形上,从而达到消除不稳定分量的目的。该方法充分整合了平动点的动力学特性,并且也适用于周期轨道的稳定保持。通过对Lissajous轨道和晕轨道的数值仿真表明,该方法较以往方法具有更强的稳定性,能在显著降低轨控燃料消耗的基础上达到较好的稳定保持效果。 相似文献
39.
Elisa Maria Alessi Gerard Gómez Josep J. Masdemont 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The purpose of this work is to compute transfer trajectories from a given Low Earth Orbit (LEO) to a nominal Lissajous quasi-periodic orbit either around the point L1 or the point L2 in the Earth–Moon system. This is achieved by adopting the Circular Restricted Three-Body Problem (CR3BP) as force model and applying the tools of Dynamical Systems Theory. 相似文献
40.