全文获取类型
收费全文 | 5089篇 |
免费 | 13篇 |
国内免费 | 8篇 |
专业分类
航空 | 2328篇 |
航天技术 | 1824篇 |
综合类 | 18篇 |
航天 | 940篇 |
出版年
2021年 | 55篇 |
2019年 | 29篇 |
2018年 | 123篇 |
2017年 | 82篇 |
2016年 | 81篇 |
2015年 | 43篇 |
2014年 | 147篇 |
2013年 | 159篇 |
2012年 | 168篇 |
2011年 | 220篇 |
2010年 | 149篇 |
2009年 | 255篇 |
2008年 | 324篇 |
2007年 | 142篇 |
2006年 | 119篇 |
2005年 | 156篇 |
2004年 | 129篇 |
2003年 | 170篇 |
2002年 | 104篇 |
2001年 | 175篇 |
2000年 | 86篇 |
1999年 | 108篇 |
1998年 | 139篇 |
1997年 | 92篇 |
1996年 | 106篇 |
1995年 | 137篇 |
1994年 | 142篇 |
1993年 | 74篇 |
1992年 | 109篇 |
1991年 | 55篇 |
1990年 | 37篇 |
1989年 | 98篇 |
1988年 | 46篇 |
1987年 | 50篇 |
1986年 | 39篇 |
1985年 | 119篇 |
1984年 | 100篇 |
1983年 | 82篇 |
1982年 | 94篇 |
1981年 | 129篇 |
1980年 | 44篇 |
1979年 | 40篇 |
1978年 | 35篇 |
1977年 | 26篇 |
1976年 | 32篇 |
1975年 | 28篇 |
1974年 | 30篇 |
1973年 | 25篇 |
1972年 | 30篇 |
1971年 | 23篇 |
排序方式: 共有5110条查询结果,搜索用时 62 毫秒
471.
Robert O. Pepin 《Space Science Reviews》2000,92(1-2):371-395
Xenon plays a crucial role in models of atmospheric evolution in which noble gases are fractionated from their initial compositions
to isotopically heavier distributions by early hydrodynamic escape of primordial planetary atmospheres. With the assumption
that nonradiogenic Xe isotope ratios in present-day atmospheres were generated in this way, backward modeling from these ratios
through the fractionating process can in principle identify likely parental Xe compositions and thus the probable sources
of noble gases in pre-escape atmospheres. Applied to Earth, this approach simultaneously establishes the presence of an atmospheric
Xe component due principally to fission of extinct 244Pu and identifies a composition called U-Xe as primordial Xe. Pu-Xe comprises 4.65±0.30% of atmospheric 136Xe, and 6.8±0.5% of the present abundance of 129Xe derives from decay of extinct 129I. U-Xe is identical to the measured composition of solar-wind Xe except for deficits of the two heaviest isotopes – an unexpected
difference since the modeling otherwise points to solar wind compositions for the lighter noble gases in the primordial terrestrial
atmosphere. Evidence for the presence of U-Xe is not restricted to the early Earth; modeling based on a purely meteoritic
data set defines a parental component in chondrites and achondrites with the same isotopic distribution. Results of experimental
efforts to measure this composition directly in meteorites are promising but not yet conclusive. U-Xe also appears as a possible
base component in interstellar silicon carbide, here with superimposed excesses of 134Xe and 136Xe six-fold larger than those in the solar wind. These compositional differences imply mixing of U-Xe with a nucleogenetic
heavy-isotope component whose relative abundance in the solar accretion disk and in pre-solar environments varied both spatially
and temporally.
In contrast to Earth, the U-Xe signature on Mars was apparently overwhelmed by local accretion of materials rich in either
chondritic Xe or solar-wind Xe. Data currently in hand from SNC meteorites on the composition of the present atmosphere are
insufficiently precise to constrain a modeling choice between these two candidates for primordial martian Xe. They likewise
do not permit definitive resolution of a 244Pu component in the atmosphere although its presence is allowed within current measurement uncertainties.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
472.
The basic principles of selecting some design parameters of a lightweight airplane for the contemporary Russian market are presented. Recommendations for selecting these parameters with the service requirements specified are given based on the study performed. 相似文献
473.
Flutter and time errors are critical factors in all instrumentation recording. This paper presents analytically the relationship between flutter, time base error, and time base error difference (sometimes called jitter), and the effects of these factors on direct and FM recording. Methods of measuring these quantities are discussed and experimental examples are given. Finally, a measurement method for the interchannel time error is presented, and some trends of correlation among all channels are discussed. 相似文献
474.
到过法国的旅游者,一般都知道巴黎有两个著名的歌舞表演厅,—个是位于市中心香榭丽舍大道的丽都,一个是位于城北蒙马特高地脚下白色广场附近的红磨坊。屋顶上装着长长的、闪烁着红光的大叶轮的红磨坊则是较为地道的法国式歌舞厅。MCG公司以法国红磨坊红磨坊为设计理念,把次情景带进了香港兰桂坊酒店Bisous酒吧。然而Bisous的设计并非照搬红色的浪漫风情,而是将未来趋势的一种极简概念设计结合了新的元素,将红磨坊的主题得以抽象化和现代化。以现今最时新的手法,完整地呈现了"红磨坊"的内心世界,概念可能不算创新,但精彩程度符合了当下时尚的思想! 相似文献
475.
476.
477.
Peebles Peyton Z. Berkowitz R. S. 《IEEE transactions on aerospace and electronic systems》1968,(6):845-854
The problem of determining target parameters of a known number of radar targets falling in the same range-Doppler-angle-angle resolution cell is examined for the noise-free case. The required minimum number of radar beams is determined, based upon approximating the beam patterns by a Taylor series expansion, both for the general problem and for factorable beams. Signal processors for target position estimation are developed for the two-target case and equations are presented for the general case. 相似文献
478.
J.S. Kaastra R. Lieu T. Tamura F.B.S. Paerels J.W. den Herder 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2504-2508
We discuss the detection of soft excess X-ray emission in a sample of 19 clusters of galaxies observed by XMM-Newton. In 6/19 clusters evidence for a soft X-ray excess is found. Four of these clusters show soft X-ray and O VII line emission from gas with a temperature of 0.2 keV. The centroid of this oxygen line is consistent with the redshift of the cluster. The intensity and spatial extend of the soft excess agrees with previous PSPC measurements. These observations are interpreted as emission from warm-hot intergalactic medium filaments, with density enhancements near the cluster centers, consistent with theoretical predictions. In the other two soft excess clusters a non-thermal origin is consistent with the data. 相似文献
479.
Application of SVM on satellite images to detect hotspots in Jharia coal field region of India 总被引:1,自引:0,他引:1
R.S. Gautam D. Singh A. Mittal P. Sajin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(11):1784-1792
The present paper deals with the application of Support Vector Machine (SVM) and image analysis techniques on NOAA/AVHRR satellite image to detect hotspots on the Jharia coal field region of India. One of the major advantages of using these satellite data is that the data are free with very good temporal resolution; while, one drawback is that these have low spatial resolution (i.e., approximately 1.1 km at nadir). Therefore, it is important to do research by applying some efficient optimization techniques along with the image analysis techniques to rectify these drawbacks and use satellite images for efficient hotspot detection and monitoring. For this purpose, SVM and multi-threshold techniques are explored for hotspot detection. The multi-threshold algorithm is developed to remove the cloud coverage from the land coverage. This algorithm also highlights the hotspots or fire spots in the suspected regions. SVM has the advantage over multi-thresholding technique that it can learn patterns from the examples and therefore is used to optimize the performance by removing the false points which are highlighted in the threshold technique. Both approaches can be used separately or in combination depending on the size of the image. The RBF (Radial Basis Function) kernel is used in training of three sets of inputs: brightness temperature of channel 3, Normalized Difference Vegetation Index (NDVI) and Global Environment Monitoring Index (GEMI), respectively. This makes a classified image in the output that highlights the hotspot and non-hotspot pixels. The performance of the SVM is also compared with the performance obtained from the neural networks and SVM appears to detect hotspots more accurately (greater than 91% classification accuracy) with lesser false alarm rate. The results obtained are found to be in good agreement with the ground based observations of the hotspots. This type of work will be quite helpful in the near future to develop a hotspots monitoring system using these operational satellites data. 相似文献
480.
We review the implications of modern higher-dimensional theories of gravity for astrophysics and cosmology. In particular, we discuss the latest developments of STM theory in connection with dark matter, particle dynamics and the cosmological constant, as well as related aspects of quantum theory. There are also more immediate tests of extra dimensions, notably involving perturbations of the cosmic 3K microwave background and the precession of a supercooled gyroscope in Earth orbit. We also outline some general features of embeddings, and include pictures of the big bang as viewed from a higher dimension. 相似文献