全文获取类型
收费全文 | 4724篇 |
免费 | 9篇 |
国内免费 | 13篇 |
专业分类
航空 | 2241篇 |
航天技术 | 1894篇 |
综合类 | 19篇 |
航天 | 592篇 |
出版年
2021年 | 34篇 |
2019年 | 40篇 |
2018年 | 84篇 |
2017年 | 50篇 |
2016年 | 52篇 |
2015年 | 22篇 |
2014年 | 98篇 |
2013年 | 124篇 |
2012年 | 106篇 |
2011年 | 157篇 |
2010年 | 111篇 |
2009年 | 196篇 |
2008年 | 275篇 |
2007年 | 128篇 |
2006年 | 100篇 |
2005年 | 117篇 |
2004年 | 121篇 |
2003年 | 161篇 |
2002年 | 98篇 |
2001年 | 158篇 |
2000年 | 92篇 |
1999年 | 130篇 |
1998年 | 142篇 |
1997年 | 101篇 |
1996年 | 110篇 |
1995年 | 151篇 |
1994年 | 165篇 |
1993年 | 82篇 |
1992年 | 115篇 |
1991年 | 55篇 |
1990年 | 55篇 |
1989年 | 116篇 |
1988年 | 40篇 |
1987年 | 61篇 |
1986年 | 45篇 |
1985年 | 160篇 |
1984年 | 105篇 |
1983年 | 105篇 |
1982年 | 122篇 |
1981年 | 145篇 |
1980年 | 50篇 |
1979年 | 58篇 |
1978年 | 42篇 |
1977年 | 33篇 |
1976年 | 27篇 |
1975年 | 29篇 |
1974年 | 26篇 |
1973年 | 22篇 |
1972年 | 31篇 |
1969年 | 21篇 |
排序方式: 共有4746条查询结果,搜索用时 62 毫秒
31.
Alice K. Harding 《Space Science Reviews》1996,75(1-2):257-268
Young pulsars surrounded by supernova remnants can power synchrotron nebulae through the injection of relativistic particles. Inverse Compton scattering by the high-energy electrons and positrons can produce TeV gamma-ray emission strong enough to be detectable by ground-based telescopes. The Crab nebula is the archetypical example of a gamma-ray plerion and was the first detected TeV source. The observed spectrum is consistent with predictions of synchrotron-self Compton models. This paper will review such models for the Crab and other plerions. Inverse-Compton scattering on other soft photon sources, particularly the 2.7K microwave background, may also be detectable in older remnants. 相似文献
32.
Moisseev S. Soshin K. Nakaoka M. 《IEEE transactions on aerospace and electronic systems》2005,41(1):174-180
A novel high-frequency transformer linked full-bridge type soft-switching phase-shift pulsewidth modulated (PWM) controlled dc-dc power converter is presented, which can be used as a power conditioner for small-scale photovoltaic and fuel cell power generation systems as well as isolated boost dc-dc power converter for automotive ac power supply. In these applications with low-voltage large-current sources, the full-bridge circuit is the most attractive topology due to the possibility of using low-voltage high-performance metal-oxide-semiconductor field-effect transistor (MOSFET) and achieving high efficiency of the dc-dc power converter. A tapped-inductor filter including the freewheeling diode is newly implemented in the output stage of the full-bridge phase-shift PWM dc-dc converter to achieve soft-switching operation for the wide load variation range. Moreover, in the proposed converter circuit, the circulating current is effectively minimized without using additional resonant circuit and auxiliary power switching devices. The practical effectiveness of the proposed soft-switching dc-dc power converter was verified in laboratory level experiment with 1 kW 100 kHz breadboard setup using power MOSFETs. Actual efficiency of 94-97% was obtained for the wide duty cycle and load variation ranges. 相似文献
33.
34.
35.
L.B. Tsirulnik T.V. Kuznetsova V.N. Oraevsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,20(12):2369-2372
A new method of nonlinear spectral analysis (called the method of global minimum: MGM), based on the best presentation (in sense of minimal squares) of a given time data set as a sum of sinusoids whose frequencies, amplitudes and phases are to be determined, has been used to find periodicities in annual Wolf sunspot numbers (W) during the period 1700–1995. The possible future behaviour of the 11-year solar cycle (based on an extrapolation of the calculated model) is also presented. The main characteristics of the 23rd solar cycle are as follows: the W maximum occurs about 2004, with a peak of nearly 220. An unusually large value of W will occur during the 23rd cycle, which should be characterised by the longest maximum, specifically, W will be greater than 100 during the 11-year period from 1997 to 2007. The first sharp rise will occur during the period 1996–1998, the second sharp during 2002–2004. The main features of the 24 year cycle are as follows: the next minimum in W, associated with the 24th solar cycle, should occur in the year 2008 and the maximum in 2014. W is expected to peak at about 180. The minimum value for the 25th year cycle is expected to occur in the year 2019. It is shown that the accuracy of these predictions depends, first of all, on the extrapolation of the hyperlong harmonic of the calculated polyharmonic model fit of observed annual sunspot numbers during the period 1700–1995. The error bars in the definition of the maximum and minimum epochs can be as large as two years. 相似文献
36.
T. J. Ponman A. M. Read 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):361-364
Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band. 相似文献
37.
Senrad: an advanced wideband air-surveillance radar 总被引:1,自引:0,他引:1
Skolnik M. Linde G. Meads K. 《IEEE transactions on aerospace and electronic systems》2001,37(4):1163-1175
The generic characteristics and performance of an experimental long-range air-surveillance radar, known at the Naval Research Laboratory as Senrad, is described. Its distinguishing feature is that it can operate with simultaneous transmissions over a very wide bandwidth-from 850 to 1400 MHz. The technology and type of experimental radar equipment employed are discussed and examples are given of its performance capabilities obtained by means of very wideband operation. The unusually wide bandwidth of this radar allows 1) improved detection and tracking performance because of the absence of the nulls that are common in the antenna elevation radiation-pattern of a single-frequency radar; 2) moving target indication (MTI) without loss of targets due to blind speeds and without the need for multiple PRFs (pulse repetition frequencies); 3) accurate height finding with a fan-beam radar by taking advantage of the multipath time difference as a function of target height; 4) a form of limited target recognition based on high range-resolution; and 5) a reduction of the effectiveness of electronic countermeasures that can seriously degrade more narrowband radars 相似文献
38.
A representative switched-capacitor DC-DC converter topology is presented, circuit operation is explained, and control strategies are identified. State-space averaging is used to analyze steady-state performance and to develop control criteria and design equations. The analytical results are verified by SPICE simulation 相似文献
39.
The Freja ultraviolet imager 总被引:2,自引:0,他引:2
J. S. Murphree R A. King T. Payne K. Smith D. Reid J. Adema B. Gordon R. Wlochowicz 《Space Science Reviews》1994,70(3-4):421-446
Auroral images acquired by satellite instrumentation have proven to be a crucial component of the scientific equiry into the physical processes of the Earth's magnetosphere. TheFreja mission provided an opportunity to extend these measurements into the temporal and spatial regime commonly associated with ground-based optical imagers. Employing the basic procedure used successfully in theViking program allowed image repetition rates of 6 s to be achieved with simultaneous exposure of all pixels within the field-of-view. Typical exposure times of 0.3 s required development of an improved image intensifier system and operational requirements resulted in image formats covering approximately one-third of a spin. Simultaneously exposing two broad-band UV cameras, the instrument generates in its normal operational mode 264.6 kbytes per image pair. Results from initial operations confirm the design approach and suggest such imagers can be routinely included on challenging low cost missions such asFreja. 相似文献
40.