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This article examines the long-term ‘Star Wars’ R&D programme initiated by President Reagan - the Strategic Defense Initiative (SDI). The nature of this initiative and the research programme that has been approved are described. There is still considerable uncertainty over where the SDI research will eventually lead - whether it be a limited BMD system designed to protect military targets or a comprehensive shield to protect the USA and its allies. The feasibility and potential implications of the SDI are examined with this caveat in mind. 相似文献
175.
Sylvaine Turck-Chièze Suzanne Talon 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):855-860
The picture of the solar radiative zone is evolving quickly. This review is separated in two parts. We first recall how the two powerful probes of the solar interior, namely the neutrinos and helioseismology have scrutinized the microscopic properties of the solar radiative plasma. Recent observations stimulate today complementary activities beyond the standard stellar model through theoretical modeling of angular momentum transport by rotation, internal waves or (and) by magnetic fields to get access to the dynamical motions of this important region of the Sun. So in the second part, we summarize the first impact of such processes on the radiative zone. 相似文献
176.
New methods of local helioseismology and uninterrupted time series of solar oscillation data from the Solar and Heliospheric
Observatory (SOHO) have led to a major advance in our understanding of the structure and dynamics of active regions in the
subsurface layers. The initial results show that large active regions are formed by repeated magnetic flux emergence from
the deep interior, and that their roots are at least 50 Mm deep. The active regions change the temperature structure and flow
dynamics of the upper convection zone, forming large circulation cells of converging flows. The helioseismic observations
also indicate that the processes of magnetic energy release, flares and coronal mass ejections, might be associated with strong
(1–2 km/s) shearing flows, 4–6 Mm below the surface. 相似文献
177.
Junwei Zhao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):838-845
Time–distance helioseismology is one of the local helioseismology techniques that are used to derive the interior properties of the Sun. It has been used to study the structures and flow fields beneath sunspots on local scales, as well as used to derive interior rotational rates and meridional flow velocities on global scales. In addition to the efforts in improving time–distance measurements and inversions, theoretical modeling is also carried out to enhance the accuracy of sensitivity kernels. Recently, by use of realistic numerical simulation on solar convection, we have also started to investigate the validity of time–distance studies. 相似文献
178.
提出了一种适用于内置式永磁同步电机(IPMSM)直接转矩控制驱动系统的效率优化方法。基于考虑铁心损耗的IPMSM模型,对电机损耗与运行转速、电磁转矩以及定子磁链三者之间的关系进行了研究分析。根据典型的IPMSM直接转矩控制不使用零电压矢量的特点,对电机功率损耗计算式进行了简化,推导得出在一定运行工况条件下IPMSM的效率最优定子磁链幅值。仿真结果验证了该方法不仅可以保持直接转矩控制动态响应的快速性,而且有效地提高了电机在稳态运行时的效率。 相似文献
179.
为获得复合材料作为风扇包容机匣时遭受叶片冲击载荷时的动态响应、损伤与失效模式,在空气炮装置上使用叶片形弹体对Kevlar织物层合板开展了弹道冲击试验,结果发现:复合材料靶板厚度提高25%,复合材料靶板吸收的能量提高约92%;随着叶片弹体速度的增加,复合材料靶板的损伤破坏逐渐严重,从轻微的压痕,转变为横向和纵向裂纹与分层损伤,再转变为矩形穿孔,同时靶板背面出现纤维断裂、纤维拔出与分层失效等现象;在叶片弹体撞击下,靶板上在与弹体接触的局部区域形成鼓胀变形,并在弹体击穿或反弹后发生变形回复;叶片弹体的横滚角将导致叶片的作用范围增大,使得靶板抗冲击性能有所提高。 相似文献
180.
针对内置式永磁同步电机(IPMSM)无位置传感器的转子位置和速度估计的难点,提出了一种基于改进定子磁链观测器的转子位置、速度的估计方法。该方法结构简单,涉及电机参数少。通过引入有效磁链概念对IPMSM的电压方程进行等效变换,对两相静止坐标系下的反电动势进行积分。为了抑制反电动势的积分环节带来的积分饱和和直流漂移问题,设计了截止频率可以自动调节的低通滤波器来代替积分器。对于在低速时低通滤波器所带来的磁链幅值衰减和相位超前问题,利用饱和反馈对观测误差进行补偿。最后通过锁相环进行位置的估计。搭建了MATLAB/Simulink仿真平台。仿真表明:该方法能够实现对IPMSM全速度范围内的转子位置的高精度估计。 相似文献