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181.
S.A. Kiehas V.S. Semenov I.V. Kubyshkin M.V. Kubyshkina T. Penz H.K. Biernat R. Nakamura 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(8):1292-1297
Magnetic reconnection is one of the most fundamental processes in the magnetosphere. We present here a simple method to determine the essential parameters of reconnection such as reconnected flux and location of the reconnection site out of single spacecraft data via remote sensing. On the basis of a time-dependent reconnection model, the dependence of the reconnected flux on the magnetic field z-component Bz is shown. The integral of Bz over time is proportional to the reconnected flux and depends on the distance between the reconnection site and the actual position where Bz is measured. This distance can be estimated from analysis of magnetic field Bz data. We apply our method to Cluster measurements in the Earth’s magnetotail. 相似文献
182.
C.P. Escoubet J. Berchem J.M. Bosqued K.J. Trattner M.G.G.T. Taylor F. Pitout C. Vallat H. Laakso A. Masson M. Dunlop H. Reme I. Dandouras A. Fazakerley 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1528-1536
Double cusps have been observed on a few occasions by polar orbiting spacecraft and ground-based observatories. The four Cluster spacecraft observed two distinct regions, showing characteristics of a double cusp, during a mid-altitude cusp pass on 7 August 2004. The Wind spacecraft detected a southward turning of the Interplanetary Magnetic Field (IMF) at the beginning of the cusp crossings and IMF–Bz stayed negative throughout. Cluster 4 observed a high energy step in the ion precipitation around 1 keV on the equatorward side of the cusp and a dense ion population in the cusp centre. Cluster 1, entering the cusp around 1 min later, observed only a partial ion dispersion with a low energy cutoff reaching 100 eV, together with the dense ion population in the cusp centre. About 9 min later, Cluster 3 entered the cusp and observed full ion dispersion from a few keV down to around 50 eV, together with the dense ion population in the centre of the cusp. The ion flow was directed poleward and eastward in the step/dispersion, whereas in the centre of the cusp the flow was directed poleward and westward. In addition the altitude of the source region of ion injection in the step/dispersion was found 50% larger than in the cusp centre. This event could be explained by the onset of dayside reconnection when the IMF turned southward. The step would be the first signature of component reconnection near the subsolar point, and the injection in the centre of the cusp a result of anti-parallel reconnection in the northern dusk side of the cusp. A three-dimensional magnetohydrodynamic (MHD) simulation is used to display the topology of the magnetic field and locate the sources of the ions during the event. 相似文献
183.
30CrMnSiA钢管外圆磁力研磨工艺的研究 总被引:1,自引:0,他引:1
采用化学粘结Fe+SiC磁性料对30CrMnSiA钢管外圆进行磁力研磨试验,研究了磨料成分、粒度以及研磨时间与研磨后表面粗糙度的关系,试验所得到的研磨表面粗糙度达到了Ra0.05μm。 相似文献
184.
V. Dehant H. Lammer Y. N. Kulikov J.-M. Grießmeier D. Breuer O. Verhoeven Ö. Karatekin T. Van Hoolst O. Korablev P. Lognonné 《Space Science Reviews》2007,129(1-3):279-300
In light of assessing the habitability of Mars, we examine the impact of the magnetic field on the atmosphere. When there
is a magnetic field, the atmosphere is protected from erosion by solar wind. The magnetic field ensures the maintenance of
a dense atmosphere, necessary for liquid water to exist on the surface of Mars. We also examine the impact of the rotation
of Mars on the magnetic field. When the magnetic field of Mars ceased to exist (about 4 Gyr ago), atmospheric escape induced
by solar wind began. We consider scenarios which could ultimately lead to a decrease of atmospheric pressure to the presently
observed value of 7 mbar: a much weaker early martian magnetic field, a late onset of the dynamo, and high erosion rates of
a denser early atmosphere. 相似文献
185.
186.
A direct drive actuator (DDA) with direct drive valves (DDVs) as the control device is an ideal solution for a flight actuation system. This paper presents a novel triple-redundant voice coil motor (TRVCM) used for redundant DDVs. The TRVCM features electrical/mechanical hybrid triple-redundancy by securing three stators along with three moving coils in the same frame. A permanent magnet (PM) Halbach array is employed in each redundant VCM to simplify the system structure. A back-to-back design between neighborly redundancies is adopted to decouple the magnetic flux linkage. The particle swarm optimization (PSO) method is implemented to optimize design parameters based on the analytical magnetic circuit model. The optimization objective function is defined as the acceleration capacity of the motor to achieve high dynamic performance. The optimal geometric parameters are verified with 3D magnetic field finite element analysis (FEA). A research prototype has been developed for experimental purpose. The experimental results of magnetic field density and force output show that the proposed TRVCM has great potential of applications in DDA systems. 相似文献
187.
Lutz Rastätter Maria M. Kuznetsova David G. Sibeck David H. Berrios 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
In this paper we present recent additions to the visualization toolset offered by the Community Coordinated Modeling Center (CCMC). Two suites of visualization tools are available that can address different needs during the analysis of model simulations of the magnetosphere that are provided by the CCMC. The online, server-side visualization allows the user to quickly browse through simulation runs and now can create maps of magnetic field line topology in the magnetosphere. The second tool, SWX, can be used on the client computer after data have been downloaded. With this second tool the user can interact directly with the three-dimensional objects that are being rendered. We present results from a simulation of a Flux Transfer Event that was performed at the CCMC using a magnetohydrodynamic model of the Earth’s magnetosphere with a high resolution grid focused on the dayside magnetosheath and dayside magnetopause. The simulation shows that the FTE that results from localized magnetic reconnection is a complicated three-dimensional structure that requires modern visualization techniques. Visualization techniques that are presented here allow the researcher to fully appreciate the complexity contained in magnetospheric simulation results. 相似文献
188.
189.
V.A. Kotov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(10):3385-3389
Time variations of the magnetic field of the Sun, seen as a star (the data 1968–2018, with more than 27 thousand daily measurements of the solar mean magnetic field), allowed to specify the rotation period of the gravitating solar mass: 27.027(6)?days, synodic. This indicates a presumably unknown physical connection between motions of the Sun and the Earth: in the course of a year our star accomplishes nearly 27 half-revolutions, while the planet itself performs an identical number of its spinnings during one complete axial revolution of the Sun. True origin of this strange Sun–Earth resonance is unknown, but it is supposed the phenomenon might be caused by slight coherent perturbations of gravity within the solar system. 相似文献
190.
本文介绍了磁通门磁强计校准装置的系统组成,包括大开口大均匀区的三轴磁场线圈、磁场线圈非均匀性的补偿方法、三轴磁场线圈非正交性补偿方法、串并联组合磁场线圈分流电路等,分析了校准装置的测量不确定度主要来源,给出了验证结果。该装置可开展磁通门磁强计(含传感器)示值误差、线性度、正交度等参数的校准,其成果已应用于十多家单位的磁场测试系统和数十家单位的磁通门磁强计校准。 相似文献