全文获取类型
收费全文 | 17209篇 |
免费 | 9206篇 |
国内免费 | 1496篇 |
专业分类
航空 | 21092篇 |
航天技术 | 3696篇 |
综合类 | 229篇 |
航天 | 2894篇 |
出版年
2024年 | 96篇 |
2023年 | 187篇 |
2022年 | 281篇 |
2021年 | 366篇 |
2020年 | 429篇 |
2019年 | 1182篇 |
2018年 | 1463篇 |
2017年 | 1326篇 |
2016年 | 1364篇 |
2015年 | 1226篇 |
2014年 | 1195篇 |
2013年 | 1227篇 |
2012年 | 1165篇 |
2011年 | 1202篇 |
2010年 | 1118篇 |
2009年 | 1292篇 |
2008年 | 1178篇 |
2007年 | 884篇 |
2006年 | 681篇 |
2005年 | 532篇 |
2004年 | 532篇 |
2003年 | 540篇 |
2002年 | 524篇 |
2001年 | 546篇 |
2000年 | 389篇 |
1999年 | 478篇 |
1998年 | 474篇 |
1997年 | 381篇 |
1996年 | 386篇 |
1995年 | 411篇 |
1994年 | 370篇 |
1993年 | 323篇 |
1992年 | 318篇 |
1991年 | 399篇 |
1990年 | 354篇 |
1989年 | 468篇 |
1988年 | 289篇 |
1987年 | 168篇 |
1986年 | 115篇 |
1985年 | 262篇 |
1984年 | 219篇 |
1983年 | 176篇 |
1982年 | 202篇 |
1981年 | 265篇 |
1980年 | 102篇 |
1979年 | 67篇 |
1978年 | 80篇 |
1975年 | 72篇 |
1974年 | 67篇 |
1972年 | 69篇 |
排序方式: 共有10000条查询结果,搜索用时 941 毫秒
411.
叶片摩擦阻尼器的优化设计方法研究 总被引:3,自引:1,他引:3
为减小叶片振动应力 ,防止叶片出现大应力的疲劳破坏 ,在叶片上设计干摩擦阻尼结构是最常用的方法之一。本文对叶片缘板摩擦阻尼器的工程优化设计方法进行了研究。研究了摩擦阻尼器参数对叶片响应的影响规律并提出了设计时应采取的措施。在阻尼器的材料和摩擦面结构已确定的情况下 ,优化设计的最主要的一个参数就是接触面的法向正压力 ,基于实际发动机中叶片激振力和粘性阻尼不易精确确定的实际 ,研究了激振力和粘性阻尼对法向正压力优化的影响 ,并提出了一种法向正压力的优化方法。由于这一优化方法对激振力和粘性阻尼值并不敏感 ,因此为工程上进行法向正压力的优化提供了理论方法 相似文献
412.
An ultrawideband (UWB) random-noise radar operating in the 1-2 GHz frequency band has been developed and held-tested at a 200 m range at the University of Nebraska. A unique heterodyne correlation technique based on a delayed transmitted waveform using a photonic delay line has been used to inject coherence within this system. The performance of this radar, assuming a point target, has been investigated from a statistical point of view by developing the theoretical basis for the system's receiver operating characteristics (ROC). Explicit analytical expressions for the joint probability density function (pdf) of the in-phase (I) and quadrature (Q) components of the receiver output have been derived under the assumption that the input signals are partially correlated Gaussian processes. The pdf and the complementary cumulative distribution function (cdf) for the envelope of the receiver output are also derived. These expressions are used to relate the probability of detection (Pd) to the probability of false alarm (Pf ) for different numbers of integrated samples, and the results are analyzed 相似文献
413.
Semenov Vladimir S. Kubyshkin Igor V. Kiendl Michael T. Biernat Helfried K. Rijnbeek Richard P. Besser Bruno P. 《Space Science Reviews》1997,82(3-4):451-461
In this article we address several criticisms of Petschek-type reconnection models which have recently been raised by Heikkila. We discuss features of the time-dependent Petschek-type models in the context of the solar wind-magnetosphere interaction, and point out that such models can incorporate and reproduce observed features at the magnetopause, such as plasma jets and erosion of the current sheet. We argue that some of Heikkila's criticisms can be attributed to weaknesses in the analysis due to incomplete experimental information, rather than to flaws in the concept of reconnection per se; in this category we include the question of which instability leads to the localised breakup of the magnetopause current sheet. Other criticisms are based on an adherence to steady-state models, and cannot be sustained within the extended time-dependent theory. We discuss, for example, how the time-dependent model can provide a consistent picture of how energy from the incoming solar wind is transferred and converted as it enters the magnetosphere. 相似文献
414.
A relative navigation system for formation flight 总被引:1,自引:0,他引:1
A relative navigation system based on both the Inertial Navigation System (INS) and the Global Positioning System (GPS) is developed to support situational awareness during formation flight. The architecture of the system requires an INS/GPS integration across two aircraft via a data link. A fault-tolerant federated filter is used to estimate the relative INS errors based on relative GPS measurements and a range measurement obtained from the data link. The filter is constructed based on a reduced-order model of the relative INS error process. A method for analyzing the filter performance is presented. A case involving two helicopters in formation flight is studied under three different night trajectories to account for the effect of vehicle motion on the INS state transition matrix. The results of the covariance analysis are compared with actual night results over an instrumented test range. 相似文献
415.
416.
J. Scudder F. Hunsacker G. Miller J. Lobell T. Zawistowski K. Ogilvie J. Keller D. Chornay F. Herrero R. Fitzenreiter D. Fairfield J. Needell D. Bodet J. Googins C. Kletzing R. Torbert J. Vandiver R. Bentley W. Fillius C. McIlwain E. Whipple A. Korth 《Space Science Reviews》1995,71(1-4):459-495
HYDRA is an experimental hot plasma investigation for the POLAR spacecraft of the GGS program. A consortium of institutions has designed a suite of particle analyzers that sample the velocity space of electron and ions between 2 keV/q – 35 keV/q in three dimensions, with a routine time resolution of 0.5 s. Routine coverage of velocity space will be accomplished with an angular homogeneity assumption of 16°, appropriate for subsonic plasmas, but with special 1.5° resolution for electrons with energies between 100 eV and 10 keV along and opposed to the local magnetic field. This instrument produces 4.9 kilobits s–1 to the telemetry, consumes on average 14 W and requires 18.7 kg for deployment including its internal shielding. The scientific objectives for the polar magnetosphere fall into four broad categories: (1) those to define the ambient kinetic regimes of ions and electrons; (2) those to elucidate the magnetohydrodynamic responses in these regimes; (3) those to assess the particle populations with high time resolution; and (4) those to determine the global topology of the magnetic field. In thefirst group are issues of identifying the origins of particles at high magnetic latitudes, their energization, the altitude dependence of the forces, including parallel electric fields they have traversed. In thesecond group are the physics of the fluid flows, regimes of current, and plasma depletion zones during quiescent and disturbed magnetic conditions. In thethird group is the exploration of the processes that accompany the rapid time variations known to occur in the auroral zone, cusp and entry layers as they affect the flow of mass, momentum and energy in the auroral region. In thefourth class of objectives are studies in conjunction with the SWE measurements of the Strahl in the solar wind that exploit the small gyroradius of thermal electrons to detect those magnetic field lines that penetrate the auroral region that are directly open to interplanetary space where, for example, the Polar Rain is observed. 相似文献
417.
418.
During encounters with comet Halley, the experiment PICCA onboard GIOTTO measured the gas phase organic ion composition of the coma and the experiment PUMA onboard VEGA-1 measured the dust composition. Joining both results, we obtain a consistent picture of the parent organic matter from which dust and gas is produced. One recognizes a complex unsaturated polycondensate, which splits during coma-formation into the more refractory C=C,C-N-containing dust part, and the more volatile C=C,C-O-containing gas part. The responsible exothermal chemical reactions, which are triggered by the sunlight, may play a major role in the dynamics of coma formation.This paper is a shortened and upgraded version of Krueger, F.R., Korth, A., and Kissel, J.: 1989, in S. Chang (ed.) Proc. of the ROSETTA Conf., Milpitas CA, January 1989, submitted. 相似文献
419.
<正> 用钻孔法测量残余应力时,使用的释放系数将对构件的残余应力测量精变产生影响。计算释放系数的理论方法有多种。其中普遍应用的公式,是由弹性力学通孔公式推导的应变片中心点处计算式。 相似文献
420.