全文获取类型
收费全文 | 7589篇 |
免费 | 29篇 |
国内免费 | 23篇 |
专业分类
航空 | 3890篇 |
航天技术 | 2649篇 |
综合类 | 33篇 |
航天 | 1069篇 |
出版年
2021年 | 53篇 |
2019年 | 53篇 |
2018年 | 99篇 |
2017年 | 64篇 |
2016年 | 59篇 |
2014年 | 138篇 |
2013年 | 180篇 |
2012年 | 164篇 |
2011年 | 228篇 |
2010年 | 166篇 |
2009年 | 259篇 |
2008年 | 343篇 |
2007年 | 188篇 |
2006年 | 184篇 |
2005年 | 187篇 |
2004年 | 171篇 |
2003年 | 248篇 |
2002年 | 147篇 |
2001年 | 255篇 |
2000年 | 152篇 |
1999年 | 189篇 |
1998年 | 233篇 |
1997年 | 160篇 |
1996年 | 209篇 |
1995年 | 273篇 |
1994年 | 251篇 |
1993年 | 151篇 |
1992年 | 183篇 |
1991年 | 99篇 |
1990年 | 92篇 |
1989年 | 198篇 |
1988年 | 88篇 |
1987年 | 88篇 |
1986年 | 88篇 |
1985年 | 253篇 |
1984年 | 206篇 |
1983年 | 180篇 |
1982年 | 192篇 |
1981年 | 231篇 |
1980年 | 81篇 |
1979年 | 61篇 |
1978年 | 68篇 |
1977年 | 69篇 |
1976年 | 49篇 |
1975年 | 87篇 |
1974年 | 53篇 |
1973年 | 53篇 |
1972年 | 75篇 |
1971年 | 56篇 |
1970年 | 54篇 |
排序方式: 共有7641条查询结果,搜索用时 234 毫秒
641.
Kerwin JP 《Acta Astronautica》1975,2(1-2):85-87
The facts presented represent, for convenience, a composite clinical picture of the three crewmen aboard Skylab II as observed by me. 相似文献
642.
Koivo A.J. Kahne S.J. Koivo H.N. 《IEEE transactions on aerospace and electronic systems》1970,(3):306-312
The effect of bounded deterministic disturbances (external and/or internal) on a chosen performance index (PI) is investigated. Upper and lower bounds of the PI about a nominal value are determined by the application of the optimum control theory. A computational procedure is also proposed to determine an approximately optimal feedback controller for time-lag systems. Such a controller is designed here on the basis of min-max criteria. Numerical examples illustrate the proposed approach. 相似文献
643.
Musal H.M. Thomas P.D. Vinokur M. 《IEEE transactions on aerospace and electronic systems》1970,(2):252-254
The evaluation of the double convolution integrat involved in the expression of the radar response to scattering from a turbulent ionized wake is simplified by the approximation technique presented here, so that the Doppler spectrum parameters can be explicitly expressed in terms of the wake characteristics. 相似文献
644.
J. C. Kosik 《Space Science Reviews》1978,22(4):481-497
Two different utilisations of magnetospheric models are described in this paper. In the first one very crude analytical expressions are used to describe the motion of energetic particles and the evolution of fluxes along a given orbit. In the second one, the exact internal and external fields are used for field line tracing and the determination of conjugate points. Applications to the calculation of synchronous fluxes and the Geos conjugate points are given. 相似文献
645.
The influence of sudden increases of electron content on the accurate determination of the position of a satellite is investigated based on a spherically stratified ionospheric model. Using the total electron content information from Faraday rotation measurements, a procedure is presented whereby the corrections of satellite position due to the unpredicted electron increase can be accounted for without the need to know the spatial distribution of the additional electrons. 相似文献
646.
All tracking systems suffer, to some extent, from signal level fluctuations. The signal fluctuations are modeled by a Gaussian process and the noise performance of both linear and nonlinear first-order tracking systems is considered. In the nonlinear case, the Ito versus Stratonovich calculus difficulty arises, but it is resolved to make sense physically. Several analytical results are obtained which are useful in analyses of tracking systems. 相似文献
647.
Smith G.H. Cunningham D.R. Ziemer R.E. 《IEEE transactions on aerospace and electronic systems》1973,(4):548-555
Plots of performance degradation are used to compare the effects of fading and intersymbol interference in a two- component specular multipath digital communications channel. Similar plots are then used to compare two practical receivers designed to combat the interference. Degradation plots are shown to allow easy identification of each receiver's range of usefulness, as well as identification of variance bounds demanded of channel parameter estimates which the receivers require. 相似文献
648.
Cullers DK 《Acta Astronautica》1986,13(1):31-37
Highly monochromatic signals, such as TV carriers, can be detected sensitively by using a narrow filter (b < or = 1 Hz) and performing power accumulation on its output. If instead a low-duty-cycle pulsed signal of the same total energy is present, the sensitivity of a square law device, followed by a thresholding operation (to eliminate most samples containing only noise), followed by the algorithm to be described, is greater by about 7 dB in typical cases. This is particularly interesting to SETI because such a pulsed signal is exactly what is sent by a rotating beacon with a directional antenna. Such a pulsed signal is, therefore, a good candidate for an extraterrestrial beacon. Software for detecting this signal type is now ready for field testing with the NASA Multichannel Spectrum Analyzer (MCSA). 相似文献
649.
The detection of X-rays from Nova Muscae 1983 (discovered on January 18, 1983) constitutes the first detection of X-rays from a classical nova during outburst. X-ray observations were carried out on 1984 April 20 and July 14 when Nova Mus had entered the nebular stage. During both observations no significant flux was observed with the medium energy detectors (2–50 keV). The source was detected with the low energy detector (.04–2 keV) using 3000 Å Lexan and Parlene- N-Aluminium filters; counting rates of (3.4 ± 1.2) × 103 and (3.7 ± 1.2 × 10-3 counts/sec were measured with the respective filters. The source was detected again on July 14 with about the same intensity. Either a shocked shell of circumstellar gas emitting 107 thermal bremsstrahlung at 1035 erg/sec intensity or a white dwarf remnant emitting 3.5 × 105 blackbody radiation at 1037 erg/sec luminosity are compatible with the measurements.Spectra taken in the visual spectral range show strong forbidden coronal emission lines of [FeVII] 6085, [FeX] 6374, and as never observed before in such a strength, [FeXIV] 5303 requiring excitation temperatures of 2 × 106 °K. 相似文献
650.
J. R. Barcus 《Space Science Reviews》1972,13(2):295-312
Analysis of recent observations (from balloons, spacecraft, and surface observatories) demonstrate regional, shell, and nearpoint conjugacy at L ~ 7 during precipitative events which were characterized by local acceleration as well as release of gradient-drifted electrons injected during substorms. A number of new features of magnetospheric dynamics relating to substorm development and sudden-commencement effects, have been brought to light which, though poorly understood at present, may prove of considerable importance and are worthy of further investigation.
- During the initial period of instability in substorm evolution, preceding the slower magnetotail convective injection, precipitation of waves of electrons in rapid polewards motion exhibit L-shell conjugacy near midnight.
- Transient, large scale expansions of the magnetospheric electron population accompanied by temporally imbedded substorms display large scale regional conjugacy and are simultaneously observed as similarly transient intensity dropouts at balloon altitudes.
- Precipitation from gradient-drifting electrons in the dayside magnetosphere exhibits near point-conjugacy, at least down to the order of 50 km and quite probably less.
- Analysis of the approach to and attainment of spectral equilibrium in the precipitation observed from drifting electrons may provide information about either, or both, the source spectrum at injection and the process of local release.
- The specific precipitation effect sometimes observed at the time of an SC remains a rather puzzling feature, although it seems clear now that the acceleration and/or release process responsible is of a highly local nature and works selectively at small pitch angles well within the magnetospheric boundary. Coupling of the interplanetary shock with the magnetosphere must be an important aspect, but the details are not clear as yet.
- On at least one occasion, a large part (perhaps all) of the magnetospheric electron population varied in a nearly synchronous manner in response to solar wind induced distortions during the variable compressive phase of a sudden commencement geomagnetic storm.