全文获取类型
收费全文 | 1353篇 |
免费 | 387篇 |
国内免费 | 226篇 |
专业分类
航空 | 1054篇 |
航天技术 | 293篇 |
综合类 | 191篇 |
航天 | 428篇 |
出版年
2024年 | 6篇 |
2023年 | 24篇 |
2022年 | 67篇 |
2021年 | 74篇 |
2020年 | 81篇 |
2019年 | 61篇 |
2018年 | 59篇 |
2017年 | 56篇 |
2016年 | 73篇 |
2015年 | 99篇 |
2014年 | 94篇 |
2013年 | 89篇 |
2012年 | 115篇 |
2011年 | 112篇 |
2010年 | 117篇 |
2009年 | 113篇 |
2008年 | 102篇 |
2007年 | 76篇 |
2006年 | 88篇 |
2005年 | 58篇 |
2004年 | 47篇 |
2003年 | 24篇 |
2002年 | 36篇 |
2001年 | 28篇 |
2000年 | 36篇 |
1999年 | 37篇 |
1998年 | 29篇 |
1997年 | 31篇 |
1996年 | 20篇 |
1995年 | 13篇 |
1994年 | 8篇 |
1993年 | 16篇 |
1992年 | 14篇 |
1991年 | 10篇 |
1990年 | 14篇 |
1989年 | 13篇 |
1988年 | 11篇 |
1987年 | 9篇 |
1986年 | 2篇 |
1985年 | 1篇 |
1984年 | 1篇 |
1982年 | 2篇 |
排序方式: 共有1966条查询结果,搜索用时 46 毫秒
412.
Wenjie Lou Ming Zhu Xiao Guo Haoquan Liang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1111-1121
This paper presents two sliding mode controllers to address the trajectory tracking problem of unmanned airships in the presence of unknown wind disturbance. The sliding mode controller proposed first is designed by a fast power rate reaching law(FPRRL). The disturbance is compensated by a radial basis function neural network (RBFNN). To avoid the aggressive adaptation, the controller is augmented by a command filter. The controller provides good robustness and tracking performance with no chattering under the hypothesis of ideal wind field. However, serious chattering occurs when simulation is performed under discontinuous wind field. To simulate the wind in practice, the wind field employed in the simulation is generated by the combination of a constant field and white noise. The controller is improved subsequently with an extended model to suppress the chattering induced by the white noise. The enhanced controller manipulates the derivation of system input, thus attenuating the chattering. Stability analysis shows that both controllers drive the tracking error into a controllable small region near zero. Simulations are provided to validate the performance of the proposed controllers under different wind hypothesis. 相似文献
413.
414.
415.
416.
Linfeng He Liang Lang Qingxia Li Wenchao Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
A hybrid method, combining the radiative transfer theory and the method of moments (MoM), is proposed to study the potential effect of the lunar surface roughness on the microwave brightness temperature. The total upward emission reaching the lunar surface from below media is calculated by the radiative transfer theory, and then the brightness temperature is obtained by weighting the bidirectional transmission coefficients which is computed using the MoM. The method is validated by both flat and rough surface models with analytic solutions. With the hybrid method, brightness temperatures from simulated lunar model are calculated and compared to those from a flat layered model. The comparisons show that the effect of rough surface on brightness temperature cannot be ignored and also depends on many other factors, such as observation angle and polarizations. For vertical polarization, an optimal observation angle may exist to reduce the effect of surface roughness. These results indicate that the knowledge of lunar surface roughness is important in microwave remote sensing to the Moon and may probably provide a guide to lunar projects in future. 相似文献
417.
Liang Li Zhiqiang Chen Ronglan Xu Ya Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The plasma density distribution of plasmasphere in the geomagnetic equatorial plane can help us study the magnetosphere like plasmasphere, ionosphere and their kinetics. In this paper, we introduce a new inversion method, GE-ART, to calculate the plasma density distribution in the geomagnetic equatorial plane from the Extreme Ultraviolet (EUV) data of IMAGE satellite under the assumption that the plasma density is constant along each geomagnetic field line. The new GE-ART algorithm was derived from the traditional Algebraic Reconstruction Techniques (ART) in Computed Tomography (CT) which was different from the several existing methods. In this new method, each value of the EUV image data was back-projected evenly to the geomagnetic field lines intersected by this EUV sight. A 3-D inversion matrix was produced by the contributions of all the voxels contained in the plasmasphere covered by the EUV sensor. That is, we considered that each value of the EUV image data was relative to the plasma densities of all the voxels passed through by the corresponding EUV radiation, which is the biggest difference to all the existing inversion methods. Finally, the GE-ART algorithm was evaluated by the real EUV data from the IMAGE satellite. 相似文献
418.
419.
测量并分析计算了角分辨紫外光电子谱仪的电子能量分析器的聚焦特性 ,分析计算了紫外光斜入射时光电信号的校正因子。结果表明 :偏离分析器聚焦中心 β角的光电子被分析器接收的几率为高斯函数exp( - β2 /β0 2 ) ,且 β0 =3.5° ;斜入射光电信号的校正因子是光入射角α的函数且大于cosα 相似文献
420.