全文获取类型
收费全文 | 3991篇 |
免费 | 3篇 |
国内免费 | 9篇 |
专业分类
航空 | 1733篇 |
航天技术 | 1439篇 |
综合类 | 10篇 |
航天 | 821篇 |
出版年
2021年 | 28篇 |
2018年 | 56篇 |
2017年 | 51篇 |
2016年 | 47篇 |
2014年 | 65篇 |
2013年 | 104篇 |
2012年 | 88篇 |
2011年 | 156篇 |
2010年 | 110篇 |
2009年 | 152篇 |
2008年 | 201篇 |
2007年 | 113篇 |
2006年 | 93篇 |
2005年 | 122篇 |
2004年 | 140篇 |
2003年 | 135篇 |
2002年 | 92篇 |
2001年 | 125篇 |
2000年 | 63篇 |
1999年 | 99篇 |
1998年 | 107篇 |
1997年 | 77篇 |
1996年 | 70篇 |
1995年 | 109篇 |
1994年 | 125篇 |
1993年 | 64篇 |
1992年 | 79篇 |
1991年 | 38篇 |
1990年 | 48篇 |
1989年 | 71篇 |
1988年 | 37篇 |
1987年 | 38篇 |
1986年 | 56篇 |
1985年 | 135篇 |
1984年 | 113篇 |
1983年 | 92篇 |
1982年 | 79篇 |
1981年 | 159篇 |
1980年 | 32篇 |
1979年 | 35篇 |
1978年 | 38篇 |
1977年 | 35篇 |
1976年 | 30篇 |
1975年 | 36篇 |
1974年 | 31篇 |
1973年 | 31篇 |
1972年 | 41篇 |
1971年 | 22篇 |
1970年 | 22篇 |
1969年 | 21篇 |
排序方式: 共有4003条查询结果,搜索用时 328 毫秒
921.
An optimization method for composite lattice shell structures under axially compressive loads is proposed aiming at the preliminary design. The method implements and improves some previous results of the fully analytical approach which is currently adopted at the state-of-the-art. The fully analytical approach provides the minimum mass solution under buckling and strength constraints, irrespective of other possible design limitations, such as, shell stiffness constraints. As a consequence, the minimum mass solution turns out to be satisfactory whereas other requirements are absent or automatically achieved but, on the contrary, it can drive the final preliminary configuration far from the real optimum.The proposed method implements numerical minimization allowing the designer to easily handle suboptimal configurations which are located in the vicinity of the minimum mass solution. When stiffness requirement is present (as in most cases) the benefit of this approach – in terms of weight saving with respect to the analytical design – is finally shown with a practical example. 相似文献
922.
In September 2011, the European Space Agency (ESA) and the German Space Agency (DLR) organized the first European SpaceTweetup during the German Aerospace day. One of the authors was one of 60 participants at this SpaceTweetup in Cologne and experienced the concept of a Tweetup and the engagement of the participants from the inside view. 相似文献
923.
V.P. Chuprova S.K. GerasimovaV.G. Grigoryev P.A. KrivoshapkinG.F. Krymsky V.P. MamrukovaV.M. Migunov A.N. PrikhodkoG.V. Shafer G.V. Skripin Ye.Ye. SorokinS.A. Starodubtsev V.E. Timofeev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Some unknown historical facts of cosmic ray studies in the north-east of the former Soviet Union related to the Yakutsk scientific group are reported for the benefit of the international scientific community. It focuses on the founders of Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of Russian Academy of Sciences. A chronology of measurements of cosmic ray intensity variations since 1949 in Yakutia (Sakha Republic; NE Siberia) is given. In particular, for the first time the data of the first solar cosmic ray event registered at Yakutsk (GLE04), with a small ionization chamber S-2 (volume: 20 L) are presented. Moreover, the data of the large ionization chamber ASK-1 (volume: 950 L) for the 1953–2003 period useful for specialists in the field of cosmic ray variations are also shown. 相似文献
924.
Based on the archive OMNI data for the period 1976–2000 an analysis has been made of 798 geomagnetic storms with D
st
< −50 nT and their interplanetary sources-large-scale types of the solar wind: CIR (145 magnetic storms), Sheath (96), magnetic
clouds MC (62), and Ejecta (161). The remaining 334 magnetic storms have no well-defined sources. For the analysis, we applied
the double method of superposed epoch analysis in which the instants of the magnetic storm beginning and minimum of D
st
index are taken as reference times. The well-known fact that, independent of the interplanetary source type, the magnetic
storm begins in 1–2 h after a southward turn of the IMF (B
z
< 0) and both the end of the main phase of a storm and the beginning of its recovery phase are observed in 1–2 h after disappearance
of the southward component of the IMF is confirmed. Also confirmed is the result obtained previously that the most efficient
generation of magnetic storms is observed for Sheath before MC. On the average parameters B
z
and E
y
slightly vary between the beginning and end of the main phase of storms (minimum of D
st
and D
st
* indices), while D
st
and D
st
* indices decrease monotonically proportionally to integral of B
z
and E
y
over time. Such a behavior of the indices indicates that the used double method of superposed epoch analysis can be successfully
applied in order to study dynamics of the parameters on the main phase of magnetic storms having different duration. 相似文献
925.
926.
The paper is devoted to studying the motion of meteor bodies with mass outflow in a planet’s atmosphere, taking into account the non-isothermal character of the latter. Analytical solutions are obtained at the constant parameter of mass outflow in the model of a nonfragmenting meteoroid. A theoretical analysis of the derived regularities of the ballistics of such bodies is presented. 相似文献
927.
本文描述用电子束辉光法测量高超声速流中平均密度、速度以及密度变化特征的物理原理和过程。对此法用于平板上激波层稳定性问题的适用范围和限制条件作了分析。内容通过风洞实验结果加以说明。 相似文献
928.
Dempsey T. Sahin G. Morton Y.T. Hopper C.M. 《Aerospace and Electronic Systems Magazine, IEEE》2009,24(8):23-30
Wireless ad hoc networks have fundamentally altered today's battlefield, with applications ranging from unmanned air vehicles to randomly deployed sensor networks. Security and vulnerabilities in wireless ad hoc networks have been considered at different layers, and many attack strategies have been proposed, including denial of service (DoS) through the intelligent jamming of the most critical packet types of flows in a network. This investigates the effectiveness of intelligent jamming in wireless ad hoc networks using the Dynamic Source Routing (DSR) and TCP protocols and introduces an intelligent classifier to facilitate the jamming of such networks. Assuming encrypted packet headers and contents, our classifier is based solely on the observable characteristics of size, inter-arrival timing, and direction and classifies packets with up to "9.4% accuracy in our experiments. 相似文献
929.
R. Werner D. Valev At. Atanassov I. Kostadinov B. Petkov G. Giovanelli K. Stebel A. Petritoli E. Palazzi M. Gausa T. Markova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Areas with dimensions of 1000–3000 km in which the total ozone content (TOC) decreases fast are called ozone mini-holes. They are generated mainly dynamically in two ways, either by poor-ozone air mass transport from the tropics to higher latitudes by planetary wave activity or, they are connected with strong adiabatic uplifting of the tropopause height. An ozone mini-hole, generated by the second mechanism, was observed over the Balkan Peninsula on 19/21 March 2005. In the middle of March, the polar vortex was strongly disturbed by Rossby waves, reaching up to the lower stratosphere. Warming episodes over a geographical area, covering the Barents Sea and the Polar Sea north from Central Siberia, displaced a polar vortex fragment extremely southwards. However, the vorticity was weak and the stratospheric temperatures did not reach low values, providing conditions for ozone chemical destruction via heterogenic reactions. At the same time, a Rossby wave ridge was located below the European polar fragment. In the period from 13 to 19 March, the thermal tropopause over Sofia was uplifted almost by 3 km. Ozone distributions observed by the SCIAMACHY instrument on 18–21 March show a fast TOC decrease westwards from Ireland, which was moving eastwards during the next days, increasing the area in which the ozone content decreased. On 20/21 March low ozone content was observed above the Stara Zagora (42°N, 25°E) ground-based station by means of the GASCOD instrument, using DOAS technique. The TOMS Earth probe instrument detected 237 DU over Sofia. This is a record low March value from the beginning of the TOMS instrument measurements in 1978. In March/April the ozone distribution was characterized by its mean annual maximum of 360 DU at 42°N. 相似文献
930.
Costas array generation and search methodology 总被引:1,自引:0,他引:1
Beard J.K. Russo J.C. Erickson K.G. Monteleone M.C. Wright M.T. 《IEEE transactions on aerospace and electronic systems》2007,43(2):522-538
Costas arrays are permutation matrices that provide sequencing schemes for frequency hop in FSK waveforms. Such frequency-shift keying (FSK) waveforms can be designed to have nearly ideal ambiguity function properties in both the time and frequency directions: the Costas property permits at most one coincident tone in autocorrelations in both time and frequency. Costas arrays are found by number-theoretic generators and their extensions, and by exhaustive search methods. Two new extensions of number-theoretic methods are introduced here that find two new Costas arrays. All Costas arrays for orders 24, 25, and 26 are disclosed here, including previously unknown examples. 相似文献