全文获取类型
收费全文 | 3804篇 |
免费 | 655篇 |
国内免费 | 675篇 |
专业分类
航空 | 2903篇 |
航天技术 | 870篇 |
综合类 | 933篇 |
航天 | 428篇 |
出版年
2024年 | 20篇 |
2023年 | 62篇 |
2022年 | 102篇 |
2021年 | 161篇 |
2020年 | 192篇 |
2019年 | 203篇 |
2018年 | 194篇 |
2017年 | 192篇 |
2016年 | 218篇 |
2015年 | 189篇 |
2014年 | 245篇 |
2013年 | 235篇 |
2012年 | 287篇 |
2011年 | 306篇 |
2010年 | 217篇 |
2009年 | 250篇 |
2008年 | 212篇 |
2007年 | 200篇 |
2006年 | 173篇 |
2005年 | 174篇 |
2004年 | 133篇 |
2003年 | 111篇 |
2002年 | 115篇 |
2001年 | 87篇 |
2000年 | 75篇 |
1999年 | 94篇 |
1998年 | 54篇 |
1997年 | 76篇 |
1996年 | 76篇 |
1995年 | 74篇 |
1994年 | 91篇 |
1993年 | 73篇 |
1992年 | 69篇 |
1991年 | 51篇 |
1990年 | 48篇 |
1989年 | 41篇 |
1988年 | 20篇 |
1987年 | 9篇 |
1986年 | 4篇 |
1984年 | 1篇 |
排序方式: 共有5134条查询结果,搜索用时 218 毫秒
971.
972.
亚、跨、超声速下空腔流场特性实验研究 总被引:1,自引:0,他引:1
在FL-21跨、超声速风洞中对空腔流场特性进行了较为深入的实验研究.空腔的长深比L/D为7、8、9、12、15,试验马赫数M范围为0.6、0.9、1.2、1.5、1.8,试验雷诺数Re为1.23~2.26×107.研究表明:空腔流场特性主要由空腔长深比L/D和来流马赫数所决定,这两个参数的变化均能引起空腔的流场类型发生变化.另外,边界层厚度涠钥涨坏撞康难沽Ψ植家灿凶畔灾挠跋?随着边界层厚度与空腔深度之比?D的减小,空腔的流场类型有向闭式穴流动转变的趋势. 相似文献
973.
Ballistic Missile Trajectory Prediction(BMTP) is critical to air defense systems. Most Trajectory Prediction(TP) methods focus on the coast and reentry phases, in which the Ballistic Missile(BM) trajectories are modeled as ellipses or the state components are propagated by the dynamic integral equations on time scales. In contrast, the boost-phase TP is more challenging because there are many unknown forces acting on the BM in this phase. To tackle this difficult problem, a novel BMTP method by ... 相似文献
974.
多元线性回归的预测建模方法 总被引:25,自引:1,他引:24
根据历史的样本数据,建立多元线性回归的预测模型;从而在不需要未来样本数据的情况下,预测未来时刻多元线性回归模型中的回归参数,以及主要的模型精度评估指标.对多元线性回归模型参数的预测,转化为对其变量集合的增广矩阵的叉积阵的预测.对叉积阵进行谱分解,利用高维群点主轴旋转的预测建模方法,通过Givens变换得到特征向量矩阵的转角值,对自由取值的转角以及特征值建立预测模型.仿真实验例示了该方法的主要计算步骤;计算结果显示,利用本模型得到的拟合值精度较高,预测值真实可信.最终计算结果和实验结果吻合较好,表明这种方法可以用于分析和预测众多领域中因变量对自变量的回归关系问题. 相似文献
975.
The five main types of antisunward propagating energetic fluxes (particles and emission) may be thought of as well established to date, the effects of which lead to a particilar character of disturbance in the near-terrestrial environment (the Earth's magnetosphere, ionosphere and atmosphere). The strongest global restructuring of the magnetosphere and ionosphere is caused by fluxes of relatively dense n of 1-70 cm-3 at the Earth's orbit) Solar Wind (SW) quasi-neutral, low-energy (E < 10 keV) plasma which cause magnetospheric and ionospheric storms lasting 24 hours or longer. For that reason, main attention is given to their study at the initial stage of research. The physical essence of the method of predicting disturbances in the near-terrestrial space environment, the amplitude of which can be expressed in, for example, the Kp index units, involves:(1) identifying all the most geo-effective SW streams of type, (2) determing their sources on the solar disk,and (3) quantifying the correlations between the characteristics of their solar sources with a maximum value of the Kp-index that is caused by the concerned type of SW stream. Semi-phenomenological relations have been obtained, which relate parameters of type SW stream sources to characteristics of geomagnetic storms:storm commencement, the time at which the storm intensity reaches its maximum values, the storm duration,as well as to the storm amplitude expressed in terms of geomagnetic indeces. 相似文献
976.
The high flux of energetic electron on geostationary orbit can induce many kinds of malfunction of the satellite there, within which the bulk-charging is the most significant that several broadcast satellite failures were confirmed to be due to this effect. The electron flux on geostationary orbit varies in a large range even up to three orders accompanied the passage of interplanetary magnetic cloud and the following geomagnetic disturbances. Upon the investigation of electron flux enhancement events, two types of events were partitioned as recurrent events and random ones. Both of the two kinds of events relate to the interplanetary conditions such as solar wind parameters, IMF etc and their evolution characters as well. As for the recurrent events, we found that, (1) all of the events exhibits periodic recurrence about 27 days, (2) significant increase of electron flux relates to interplanetary index and characters of their distribution, (3) the electron flux also has relation to solar activity index. An artificial neural network was constructed to estimate the flux I day ahead. The random electron flux enhancement events are rare and present different distribution figures to the recurrent ones. The figure of the random events and the conditions of their occurrence is also discussed in this paper. 相似文献
977.
用SGP4模型和卡尔曼滤波实现空间碎片轨道预报 总被引:1,自引:0,他引:1
文章将扩展卡尔曼滤波算法成功应用于求空间碎片的双行元初值及其轨道预报问题。首先推导出扩展的卡尔曼滤波求双行元的计算公式;然后针对地面观测站对空间碎片的监测进行了应用研究,编制了相应的计算程序并进行了数学仿真。结果表明该算法可以较准确地得到监测目标的双行元初值,从而可实现中长期轨道预报。 相似文献
978.
979.
复杂陶瓷件烧结过程温度场数值模拟及仿真 总被引:3,自引:0,他引:3
随着陶瓷应用领域的不断扩展,对其品质要求也越来越高.而传统的设计工艺与制造过程是相分离的,到最终生产工艺的定型需要大量的反复修改.为解决传统陶瓷设计工艺只能依靠经验的现状,节约成本,缩短生产周期,故开发了复杂陶瓷零构件烧结过程计算机仿真软件.首先借助传热学原理来建立温度场模型,其次借助有限差分法处理温度场模型,编写出此仿真模拟软件的核心计算代码,从而实现了复杂陶瓷零件和组合构件烧结过程中温度场的模拟仿真. 相似文献
980.