全文获取类型
收费全文 | 803篇 |
免费 | 156篇 |
国内免费 | 82篇 |
专业分类
航空 | 187篇 |
航天技术 | 430篇 |
综合类 | 13篇 |
航天 | 411篇 |
出版年
2024年 | 7篇 |
2023年 | 24篇 |
2022年 | 34篇 |
2021年 | 59篇 |
2020年 | 40篇 |
2019年 | 45篇 |
2018年 | 50篇 |
2017年 | 29篇 |
2016年 | 56篇 |
2015年 | 46篇 |
2014年 | 75篇 |
2013年 | 51篇 |
2012年 | 54篇 |
2011年 | 58篇 |
2010年 | 64篇 |
2009年 | 57篇 |
2008年 | 49篇 |
2007年 | 39篇 |
2006年 | 39篇 |
2005年 | 26篇 |
2004年 | 18篇 |
2003年 | 17篇 |
2002年 | 12篇 |
2001年 | 12篇 |
2000年 | 16篇 |
1999年 | 15篇 |
1998年 | 11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1041条查询结果,搜索用时 7 毫秒
791.
792.
Aleix Pinardell Pons Ron Noomen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):1992-2002
GTO objects can potentially collide with operative satellites in LEO and GEO protected regions. Internationally accepted debris mitigation guidelines require that these objects exit these protected regions within 25?years, e.g. by re-entering and burning up in Earth’s atmosphere. In this paper, an inventory of the GTO debris generated from Ariane 5 launches in the period 2012–2017 is provided, and it is expected that none of these objects will re-enter within 25?years. For future launches, natural perturbations can be exploited to increase compliance with mitigation guidelines without the use of extra propellant or complex de-orbiting systems, which is attractive from an economic point of view. The lifetime of GTO objects is very sensitive to initial conditions and some environmental and body-related parameters, mainly due to the effect of solar gravity on the perigee altitude. As a consequence, the lifetime of a specific GTO object cannot be predicted accurately, but its probability of re-entering in less than 25?years can be estimated with proper accuracy by following a statistical approach. By propagating the orbits of over 800,000 simulated Ariane 5 GTO objects, it was found that the launch time leading to the highest probability of compliance with debris mitigation guidelines for GEO launches from Kourou corresponds to about 2 PM local time, regardless of the date of launch, which leads to compliance rates ranging from 60 to 100%. Current practice is to launch at around 5–9?PM, so a change in procedures would be required in order to reach a higher degree of compliance with debris mitigation guidelines, which was predicted to be on average below 20% for the objects generated in the period 2012–2017. 相似文献
793.
通过对地球同步轨道(GEO)卫星运动特点的分析,阐明其对多普勒分辨率的影响。传统的双基合成孔径雷达(SAR)多普勒分辨率表达式由于不考虑雷达平台加速度矢量带来的影响,并不适用于GEO星弹双基SAR系统。根据收发平台的双曲线轨迹对目标的回波多普勒特性影响,首先利用梯度方法推导了GEO星弹双基SAR系统的多普勒分辨率表达式;随后详细地分析了GEO卫星与导弹的空间几何关系及多普勒参数,特别是加速度矢量对多普勒分辨率的影响。仿真结果验证了所推导多普勒分辨率表达式的有效性,其有助于双基SAR理论系统完整性的提高,为后续系统设计及应用实践提供理论支撑。 相似文献
794.
Minghu Tan Colin McInnes Matteo Ceriotti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(8):2099-2115
Since the Sun-Earth libration points L1 and L2 are regarded as ideal locations for space science missions and candidate gateways for future crewed interplanetary missions, capturing near-Earth asteroids (NEAs) around the Sun-Earth L1/L2 points has generated significant interest. Therefore, this paper proposes the concept of coupling together a flyby of the Earth and then capturing small NEAs onto Sun–Earth L1/L2 periodic orbits. In this capture strategy, the Sun-Earth circular restricted three-body problem (CRTBP) is used to calculate target Lypaunov orbits and their invariant manifolds. A periapsis map is then employed to determine the required perigee of the Earth flyby. Moreover, depending on the perigee distance of the flyby, Earth flybys with and without aerobraking are investigated to design a transfer trajectory capturing a small NEA from its initial orbit to the stable manifolds associated with Sun-Earth L1/L2 periodic orbits. Finally, a global optimization is carried out, based on a detailed design procedure for NEA capture using an Earth flyby. Results show that the NEA capture strategies using an Earth flyby with and without aerobraking both have the potential to be of lower cost in terms of energy requirements than a direct NEA capture strategy without the Earth flyby. Moreover, NEA capture with an Earth flyby also has the potential for a shorter flight time compared to the NEA capture strategy without the Earth flyby. 相似文献
795.
James B. Pezent Rohan Sood Andrew Heaton 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(9):2981-2994
Regions outside the reach of traditional propulsion systems or the ones that require significant propellant, may be reached by harnessing the solar radiation pressure and leveraging coupled dynamics to maneuver a sail-based spacecraft. Earth-trailing orbits have recently been investigated for getting a unique perspective of the Sun while maintaining the spacecraft in close proximity to Earth. Vertical orbits trailing the Earth exhibit the additional capability to view the Sun from above and below the ecliptic plane. In this work, families of sail-based orbits are explored for varying Earth-trailing angles and Z amplitudes in the Sun-Earth circular restricted three-body problem. Optimization is carried out to ensure that the non-traditional vertical orbits exhibit a constant pitch angle control history, as well as symmetry across the X-Y plane. The stability of the resulting orbit families is assessed using an extension of Flouquet theory to Differential Algebraic Equations. Results indicate that sail-based Earth-trailing vertical orbits can be more stable than traditional sub-L1 sail-based vertical orbits. 相似文献
796.
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
797.
Xuefeng Tao Zhi Li Can Xu Yurong Huo Yasheng Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(8):2304-2318
This paper focuses on the track-to-object association problem based on the two-line elements (TLE) set. The TLE’s short-term propagation error characteristics are analyzed to capture its uncertainty. Further, a four-step track-to-object association algorithm is designed for the optical observation data. First, for too-short arc tracklets, a circular orbit determination algorithm is proposed to calculate the inclination and the right ascension of the ascending node. Second, the TLEs are filtered based on these results. Nearly 96% of the TLEs can be filtered, which significantly improves the association efficiency. The last two steps consist of two association processes. A first-order association process is implemented first to get candidate objects, with the angles root mean square error as the metric. Then a precise association process checks the candidate objects and gives the final association result. The proposed approach is tested with simulated and observed data, respectively. With simulated data, the true positive rate is 98.7%. With the observed data, the association results were validated using the precise orbit ephemerides. 相似文献
798.
卫星电源系统配置方案的优化设计 总被引:1,自引:0,他引:1
对卫星电源系统配置方案进行优化设计是减轻电源系统质量的一条重要途径。以太阳则步轨道卫星为背景,对四种典型的直接能量传输方式的电源系统配置建立了能量传递图,推出了能量平衡方程。在此基础上,建立了以电源系统的质量功率比最小为目标函数的优化模型;以降交点地方时,高峰功耗与长期功耗比和光照区与星蚀区负载长期功率比为设计变量,通过算例对这四种DET方式进行了优化分析比较,归纳出电源系统配置方案的优化设计结论 相似文献
799.
针对嫦娥5T服务舱(CE5T)拓展试验中的绕地大椭圆轨道,分析了轨道动力学演化趋势,通过测轨数据类型组合策略分析了统一S频段测量(USB)和甚长基线干涉测量(VLBI)在定轨中的贡献,得到了百米级的精密定轨精度;针对地月第二平动点(L2)绕飞轨道,分析了地心和月心积分的轨道动力学差异,制定了精密定轨的参数求解策略,得到了百米级的精密定轨精度;针对月球交会对接轨道的特点,选取三种不同的重力场模型定轨,比较了三者在轨道预报和数据拟合的差异,并与嫦娥3号(CE3)环月轨道的定轨精度进行比对,验证了不同重力场的适用范围,从计算精度和效率两方面制定了优化的定轨策略。 相似文献
800.