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71.
72.
针对现有的基于虚拟信道紧迫度的动态调度算法的不足,提出了一种新的高级在轨系统虚拟信道动态调度算法。该算法首先估算虚拟信道的紧迫度和数据帧的紧迫度,然后用加权系数将二者结合起来构造成一个全新的虚拟信道传送紧迫度函数,再根据该函数的值进行判决调度。对于高级在轨系统中不同速率、不同性质、不同类型的星上数据源,该算法均可通过选择合适的加权系数灵活地分配传输时隙,保证各用户合理、动态地占用物理信道,满足对数据的传输时延要求,因此具有广泛的适用性。理论分析和仿真结果表明,本文提出的算法比基于虚拟信道紧迫度的动态调度算法具有更好的性能 相似文献
73.
Hui Lei ZhiGang Li XuHai Yang WenJun Wu Xuan Cheng Ying Yang ChuGang Feng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
A new strategy of precise orbit determination (POD) for GEO (Geostationary Earth Orbit) satellite using SATRE (SAtellite Time and Ranging Equipment) is presented. Two observation modes are proposed and different channels of the same instruments are used to construct different observation modes, one mode receiving time signals from their own station and the other mode receiving time signals from each other for two stations called pairs of combined observations. Using data from such a tracking network in China, the results for both modes are compared. The precise orbit determination for the Sino-1 satellite using the data from 6 June 2005 to 13 June 2005 has been carried out in this work. The RMS (Root-Mean-Square) of observing residuals for 3-day solutions with the former mode is better than 9.1 cm. The RMS of observing residuals for 3-day solutions with the latter mode is better than 4.8 cm, much better than the former mode. Orbital overlapping (3-day orbit solution with 1-day orbit overlap) tests show that the RMS of the orbit difference for the former mode is 0.16 m in the radial direction, 0.53 m in the along-track direction, 0.97 m in the cross-track direction and 1.12 m in the 3-dimension position and the RMS of the orbit difference for the latter mode is 0.36 m in the radial direction, 0.89 m in the along-track direction, 1.18 m in the cross-track direction and 1.52 m in the 3-dimension position, almost the same as the former mode. All the experiments indicate that a meter-level accuracy of orbit determination for geostationary satellite is achievable. 相似文献
74.
阐述了高准确度捷联惯性测量装置全温测试系统的校准测试方法。通过对软硬件进行校准测试,验证了该系统可以完成不同种类的惯性测量装置误差建模和综合测试。 相似文献
75.
76.
多随机变量的桁架结构系统的可靠性分析及优化设计 总被引:2,自引:0,他引:2
针对桁架结构系统,采用随机有限元法(SFEM)计算结构系统的响应量,考虑内力重新分配,建立失效模式的安全余量方程,用验算点法计算失效模式安全余量的可靠性指标,用改进的分枝限界法,寻找主要失效模式,通过对主要失效模式方程线性化研究,计算失效模式安全余量之间的相关系数,寻找主要失效模式,通过对主要失效模式方程线性化研究,计算失效模式安全余量之间的相关系数,最后用PNET法计算出结构系统的失效概率,同时给出多随机变量的结构系统可靠度的敏度表达式,采用最佳矢量法,求解了大型桁架结构系统基于可靠性指标约束下的最小重量的优化设计问题,最后,给出了实际算例,计算结果表明;采用随机有限元法能更好地考虑结构系统的多个随机变量对系统可靠性产生的影响;所采用的可靠性分析方法和优化方法是有效的。 相似文献
77.
民用飞机主制造商建立设计保证系统,旨在民机研制过程中充分发挥自主适航的能力,通过组织机构、职责、程序和资源落实设计、适航以及独立监督三大职能,以保证航空产品的设计或者设计更改满足适航当局的要求。其中,设计保证系统适航职能的适航独立核查功能正是这一保证的关键。基于对设计保证系统适航独立核查功能的具体分析基础上,从设计保证系统的规划与设计层面提出了实现适航独立核查功能的机制,给出了机制中需明确的责任主体、职责与资质要求、工作流程与支撑工具以及管理程序等方面的建议,并从大数据知识的技术支撑和阶梯式递进的人才培训保障两方面以不断优化改进的方法工具与人力配置来深化适航独立核查的功能与效果,进而增强设计保证系统对飞机型号研制的保证作用。 相似文献
78.
高精度电磁标定力源是微推力测量系统的重要组成要素之一。为了获得性能优良的电磁标定力,本文综合采用数值模拟及实验测量两种方法分析研究了线圈和永磁铁相对位置变化时,磁铁几何尺寸对电磁力输出特性的影响:对于直径较大、厚度较小的永磁铁而言,其电磁力随相对位置的变化会存在极值,且极值点附近的电磁力具有较好的稳定性和一致性。根据电磁力变化趋势特性,提出了线圈和永磁铁相对基准中心(极值点)位置的高精度设置方案,且基准中心位置附近的电磁力变异系数可达0.00252,为高性能电磁力的获得提供了基础。最后,确定了大直径永磁铁+线圈组合型电磁力产生装置,并基于拟合方法建立了一定包络区间内的高精度电磁力控制关系式,其拟合曲线的估计标准误差约为0.0137,为微推力测量台架的标定提供了理论指导和技术支持。 相似文献
79.
P.A. Chaizy T.G. DimbylowP.M. Allan M.A. Hapgood 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this paper, Science Operations Planning Expertise (SOPE) is defined as the expertise that is held by people who have the two following qualities. First they have both theoretical and practical experience in operations planning, in general, and in space science operations planning in particular. Second, they can be used, on request and at least, to provide with advice the teams that design and implement science operations systems in order to optimise the performance and productivity of the mission. However, the relevance and use of such SOPE early on during the Mission Design Phase (MDP) is not sufficiently recognised. As a result, science operations planning is often neglected or poorly assessed during the mission definition phases. This can result in mission architectures that are not optimum in terms of cost and scientific returns, particularly for missions that require a significant amount of science operations planning. Consequently, science operations planning difficulties and cost underestimations are often realised only when it is too late to design and implement the most appropriate solutions. In addition, higher costs can potentially reduce both the number of new missions and the chances of existing ones to be extended. Moreover, the quality, and subsequently efficiency, of SOPE can vary greatly. This is why we also believe that the best possible type of SOPE requires a structure similar to the ones of existing bodies of expertise dedicated to the data processing such as the International Planetary Data Alliance (IPDA), the Space Physics Archive Search and Extract (SPASE) or the Planetary Data System (PDS). Indeed, this is the only way of efficiently identifying science operations planning issues and their solutions as well as of keeping track of them in order to apply them to new missions. Therefore, this paper advocates for the need to allocate resources in order to both optimise the use of SOPE early on during the MDP and to perform, at least, a feasibility study of such a more structured SOPE. 相似文献
80.