全文获取类型
收费全文 | 830篇 |
免费 | 157篇 |
国内免费 | 84篇 |
专业分类
航空 | 202篇 |
航天技术 | 436篇 |
综合类 | 19篇 |
航天 | 414篇 |
出版年
2024年 | 5篇 |
2023年 | 24篇 |
2022年 | 35篇 |
2021年 | 60篇 |
2020年 | 40篇 |
2019年 | 46篇 |
2018年 | 52篇 |
2017年 | 31篇 |
2016年 | 57篇 |
2015年 | 48篇 |
2014年 | 77篇 |
2013年 | 52篇 |
2012年 | 57篇 |
2011年 | 59篇 |
2010年 | 65篇 |
2009年 | 58篇 |
2008年 | 50篇 |
2007年 | 40篇 |
2006年 | 41篇 |
2005年 | 28篇 |
2004年 | 21篇 |
2003年 | 17篇 |
2002年 | 14篇 |
2001年 | 12篇 |
2000年 | 17篇 |
1999年 | 15篇 |
1998年 | 12篇 |
1997年 | 9篇 |
1996年 | 5篇 |
1995年 | 4篇 |
1994年 | 2篇 |
1993年 | 3篇 |
1992年 | 1篇 |
1991年 | 6篇 |
1990年 | 2篇 |
1989年 | 2篇 |
1988年 | 3篇 |
1987年 | 1篇 |
排序方式: 共有1071条查询结果,搜索用时 156 毫秒
71.
Recent studies on human missions to Mars suggest revisiting the parameters that have the most important impact on the complexity, the initial mass in low Earth orbit, the risks and the development costs for the first journey to the red planet. In the last NASA reference mission, a trade tree is proposed. 相似文献
72.
针对低低跟踪(SST-LL)重力测量卫星K频段测距(KBR)系统相位中心在轨标定问题,提出了一种应用预测卡尔曼滤波算法的KBR系统在轨标定算法。首先,以磁力矩器和姿态控制喷气发动机为执行部件,对一颗卫星施加一定的组合力矩,使其绕另一颗卫星进行周期性姿态机动;然后,将星敏感器数据代入预测卡尔曼滤波算法中估计出卫星姿态;最后,根据KBR系统观测值与卫星姿态角之间的关系,利用扩展卡尔曼滤波算法估计出KBR系统相位中心的位置。数值仿真结果表明:KBR系统相位中心可以被实时估计,当存在较大的卫星姿态动力学模型误差时,KBR系统相位中心的标定误差仍在0.3mrad以内,证明此算法估计精度较高且鲁棒性强。 相似文献
73.
太阳帆日心定点悬浮转移轨道设计 总被引:1,自引:0,他引:1
研究了太阳帆航天器日心定点悬浮轨道(HFDO)的转移轨道设计问题,以球坐标形式建立了太阳帆的动力学模型,基于该模型给出在日心悬浮轨道基础上实现定点悬浮的条件,提出了一种实现日心定点悬浮的转移轨道设计方法。首先,确定定点悬浮的位置;然后,设计经过该位置的绕日极轨轨道;最后,实施轨道减速实现定点悬浮,并给出了解析形式的轨道控制律。结合太阳极地观测任务,设计了定点悬浮在太阳北极1AU处的太阳帆转移轨道。仿真结果表明:该轨道转移方案总耗时3.5年,太阳帆定点到黄北极距日心1AU处,此后只要保持太阳光垂直照射帆面,即可维持稳定的悬浮状态。 相似文献
74.
Xu Huang Ye Yan Yang Zhou 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
To achieve hovering, a spacecraft thrusts continuously to induce an equilibrium state at a desired position. Due to the constraints on the quantity of propellant onboard, long-time hovering around low-Earth orbits (LEO) is hardly achievable using traditional chemical propulsion. The Lorentz force, acting on an electrostatically charged spacecraft as it moves through a planetary magnetic field, provides a new propellantless method for orbital maneuvers. This paper investigates the feasibility of using the induced Lorentz force as an auxiliary means of propulsion for spacecraft hovering. Assuming that the Earth’s magnetic field is a dipole that rotates with the Earth, a dynamical model that characterizes the relative motion of Lorentz spacecraft is derived to analyze the required open-loop control acceleration for hovering. Based on this dynamical model, we first present the hovering configurations that could achieve propellantless hovering and the corresponding required specific charge of a Lorentz spacecraft. For other configurations, optimal open-loop control laws that minimize the control energy consumption are designed. Likewise, the optimal trajectories of required specific charge and control acceleration are both presented. The effect of orbital inclination on the expenditure of control energy is also analyzed. Further, we also develop a closed-loop control approach for propellantless hovering. Numerical results prove the validity of proposed control methods for hovering and show that hovering around low-Earth orbits would be achievable if the required specific charge of a Lorentz spacecraft becomes feasible in the future. Typically, hovering radially several kilometers above a target in LEO requires specific charges on the order of 0.1 C/kg. 相似文献
75.
76.
77.
针对月球轨道交会对接地面高精度引导需求,对同波束干涉测量差分相延观测模型进行分析验证。根据甚长基线干涉测量几何时延观测量同一波前的定义,推导出同波束差分时延观测量的观测模型。并提出一种精确的同波束干涉测量差分相时延闭合算法,同时结合SELENE任务实测的数据计算差分相时延闭合值,用于对观测模型进行验证。实测数据计算结果表明,采用本文提出的精确算法显著地消除同一波前差分相时延闭合值中的趋势项,差分相时延闭合值的精度在0.5ps~1ps范围内,验证了观测模型的正确性。该研究对于后续的月球交会对接地面高精度测定轨任务分析设计将具有一定的参考价值。 相似文献
78.
轨姿控液体火箭发动机水击仿真模拟 总被引:4,自引:0,他引:4
以轨姿控液体火箭发动机为研究对象,根据模块化思想,利用AMESim建立了仿真平台,仿真计算了发动机系统工作中管路的水击压力。结果表明:轨控发动机的工作是引起大水击的主要因素。通过与理论计算和试验数据的对比表明,仿真模型较好地描述了管路水击的生成过程。介绍了减小系统水击量的措施。 相似文献
79.
80.
N. Zolotukhina N. Polekh V. Kurkin O. Pirog S. Samsonov A. Moiseyev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We present an observational study of magnetospheric and ionospheric disturbances during the December 2006 intense magnetic storm associated with the 4В/Х3.4 class solar flare. To perform the study we utilize the ground data from North–East Asian ionospheric and magnetic observatories (60–72°N, 88–152°E) and in situ measurements from LANL, GOES, Geotail and ACE satellites. The comparative analysis of ionospheric, magnetospheric and heliospheric disturbances shows that the interaction of the magnetosphere with heavily compressed solar wind and interplanetary magnetic field caused the initial phase of the magnetic storm. It was accompanied by the intense sporadic E and F2 layers and the total black-out in the nocturnal subauroral ionosphere. During the storm main phase, LANL-97A, LANL 1994_084, LANL 1989-046 and GOES_11 satellites registered a compression of the dayside magnetosphere up to their orbits. In the morning–noon sector the compression was accompanied by an absence of reflections from ionosphere over subauroral ionospheric station Zhigansk (66.8°N, 123.3°E), and a drastic decrease in the F2 layer critical frequency (foF2) up to 54% of the quite one over subauroral Yakutsk station (62°N, 129.7°E). At the end of the main phase, these stations registered a sharp foF2 increase in the afternoon sector. At Yakutsk the peak foF2 was 1.9 time higher than the undisturbed one. The mentioned ionospheric disturbances occurred simultaneously with changes in the temperature, density and temperature anisotropy of particles at geosynchronous orbit, registered by the LANL-97A satellite nearby the meridian of ionospheric and magnetic measurements. The whole complex of disturbances may be caused by radial displacement of the main magnetospheric domains (magnetopause, cusp/cleft, plasma sheet) with respect to the observation points, caused by changes in the solar wind dynamic pressure, the field of magnetospheric convection, and rotation of the Earth. 相似文献