全文获取类型
收费全文 | 817篇 |
免费 | 36篇 |
国内免费 | 35篇 |
专业分类
航空 | 309篇 |
航天技术 | 455篇 |
综合类 | 34篇 |
航天 | 90篇 |
出版年
2024年 | 1篇 |
2023年 | 31篇 |
2022年 | 1篇 |
2021年 | 10篇 |
2020年 | 25篇 |
2019年 | 23篇 |
2018年 | 14篇 |
2017年 | 5篇 |
2016年 | 4篇 |
2015年 | 7篇 |
2014年 | 66篇 |
2013年 | 34篇 |
2012年 | 34篇 |
2011年 | 31篇 |
2010年 | 35篇 |
2009年 | 45篇 |
2008年 | 73篇 |
2007年 | 63篇 |
2006年 | 56篇 |
2005年 | 47篇 |
2004年 | 21篇 |
2003年 | 23篇 |
2002年 | 11篇 |
2001年 | 44篇 |
2000年 | 14篇 |
1999年 | 8篇 |
1998年 | 23篇 |
1997年 | 7篇 |
1996年 | 15篇 |
1995年 | 18篇 |
1994年 | 63篇 |
1993年 | 22篇 |
1992年 | 4篇 |
1990年 | 3篇 |
1989年 | 2篇 |
1984年 | 5篇 |
排序方式: 共有888条查询结果,搜索用时 15 毫秒
91.
This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized
flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating
the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields
sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach. 相似文献
92.
T. Van Doorsselaere I. Arregui J. Andries M. Goossens S. Poedts 《Space Science Reviews》2005,121(1-4):79-89
We will discuss the observed, heavily damped transversal oscillations of coronal loops. These oscillations are often modeled
as transversal kink oscillations in a cylinder. Several features are added to the classical cylindrical model. In our models
we include loop curvature, longitudinal density stratification, and highly inhomogeneous radial density profiles.
In this paper, we will first give an overview of recently obtained results, both analytically and numerically. After that,
we shed a light on the computational aspects of the modeling process. In particular, we will focus on the parallellization
of the numerical codes. 相似文献
93.
王飞 《中国民航学院学报》1996,(6):51-58
介绍了用于对微机测控系统输入接口板、输出接口板测试硬件系统的构成,设计了接口卡电路.针对两块电路板,提出了对数字电路板的测试和故障诊断分四个层次,即整板级、功能模块级、单片级和功能输出点级的思想,采取了对功能输出点进行编码的方法建立数字电路板测试的标准知识库,提出了使用功能标志矩阵的方法对各个层次的测试结果进行存储的方法,并根据各个层次测试的关系及相应功能标志矩阵的关系建立了智能化故障诊断程序. 相似文献
94.
本文用SCL-90症状自评量表方法,对我校三个年级的部分班级进行了测查。分析表明:我院大学生的心理健康状况不容乐观。本文还对学生管理现状提出了进一步改进建议。 相似文献
95.
本文通过具体例题,阐述了双向弯曲变形构件中危险截面的判定方法,论证了合成弯矩大的截面不一定是危险截面的结论。 相似文献
96.
基于Lagrange方法的航天员舱外活动计算机仿真 总被引:2,自引:0,他引:2
在比较各种地面微重力模拟设备的优缺点的基础上,阐述了计算机动态仿真航天员舱外活动(EVA,Extra Vehicular Activity)的必要性。简要的概述了应用计算多刚体系统动力学对EVA进行仿真的步骤。描述了拉格朗日方程在仿真过程中的应用,建立了用于仿真的动力学方程。选取典型的EVA,得出了描述该EVA系统运动的拉格朗日动力学方程。利用反向运动学和反向动力学对该EVA进行了仿真计算,并对结果进行了分析。 相似文献
97.
基于事件的EMR遥操作自适应规划与控制方法 总被引:1,自引:0,他引:1
提出了基于事件的舱外自由移动机器人 (ExtravehicularMobileRobot,简称EMR)系统在任务空间内的自适应规划与控制方法 ,使系统具有处理突发事件和不确定事件的能力 ,同时提高了系统的自主性和适应能力 ,增强了遥操作的安全性 ,仿真证明了该方法的正确性和有效性。 相似文献
98.
99.
O.S. Oyekola 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
We use hourly monthly median values of propagation factor M(3000)F2 data observed at Ouagadougou Ionospheric Observatory (geographic12.4°N, 1.5°W; 5.9o dip), Burkina Faso (West Africa) during the years Januar1987–December1988 (average F10.7 < 130 × 10−22 W/m2/Hz, representative of low solar flux conditions) and for January 1989–December1990 (average F10.7 ? 130 × 10−22 W/m2/Hz, representative of high solar epoch) for magnetically quiet conditions to describe local time, seasonal and solar cycle variations of equatorial ionospheric propagation factor M(3000)F2 in the African region. We show that that seasonal trend between solar maximum and solar minimum curves display simple patterns for all seasons and exhibits reasonable disparity with root mean square error (RMSE) of about 0.31, 0.29 and 0.26 for December solstice, June solstice and equinox, respectively. Variability Σ defined by the percentage ratio of the absolute standard deviation to the mean indicates significant dissimilarity for the two solar flux levels. Solar maximum day (10–14 LT) and night (22–02 LT) values show considerable variations than the solar minimum day and night values. We compare our observations with those of the IRI 2007 to validate the prediction capacity of the empirical model. We find that the IRI model tends to underestimate and overestimate the observed values of M(3000)F2, in particular, during June solstice season. There are large discrepancies, mainly during high solar flux equinox and December solstice between dawn and local midnight. On the other hand, IRI provides a slightly better predictions for M(3000)F2 between 0900 and 1500 LT during equinox low and high solar activity and equinox high sunspot number. Our data are of great importance in the area of short-wave telecommunication and ionospheric modeling. 相似文献
100.
R. D’Amicis R. BrunoB. Bavassano 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Within the framework of the solar wind—magnetosphere coupled system, intense perturbations in the solar wind, causing geomagnetic storms and substorms, have been widely studied by means of the so-called coupling parameters. However, remarkable variations in the geomagnetic field occur even in absence of such perturbations. In those conditions, solar wind MHD turbulence might have a role. Recent results have shown that solar wind turbulence can be described not only as a mixture of inward and outward stochastic Alfvénic fluctuations, but includes also advected structures, dominated by an excess of magnetic energy. 相似文献