全文获取类型
收费全文 | 3254篇 |
免费 | 23篇 |
国内免费 | 13篇 |
专业分类
航空 | 1575篇 |
航天技术 | 1146篇 |
综合类 | 4篇 |
航天 | 565篇 |
出版年
2021年 | 26篇 |
2019年 | 23篇 |
2018年 | 54篇 |
2017年 | 51篇 |
2016年 | 45篇 |
2015年 | 26篇 |
2014年 | 71篇 |
2013年 | 91篇 |
2012年 | 82篇 |
2011年 | 119篇 |
2010年 | 79篇 |
2009年 | 137篇 |
2008年 | 153篇 |
2007年 | 99篇 |
2006年 | 71篇 |
2005年 | 92篇 |
2004年 | 90篇 |
2003年 | 99篇 |
2002年 | 72篇 |
2001年 | 115篇 |
2000年 | 65篇 |
1999年 | 68篇 |
1998年 | 87篇 |
1997年 | 58篇 |
1996年 | 93篇 |
1995年 | 112篇 |
1994年 | 111篇 |
1993年 | 48篇 |
1992年 | 71篇 |
1991年 | 34篇 |
1990年 | 32篇 |
1989年 | 78篇 |
1988年 | 28篇 |
1987年 | 24篇 |
1986年 | 33篇 |
1985年 | 90篇 |
1984年 | 90篇 |
1983年 | 65篇 |
1982年 | 66篇 |
1981年 | 99篇 |
1980年 | 19篇 |
1979年 | 25篇 |
1978年 | 29篇 |
1977年 | 27篇 |
1975年 | 29篇 |
1974年 | 23篇 |
1973年 | 21篇 |
1972年 | 20篇 |
1969年 | 20篇 |
1968年 | 18篇 |
排序方式: 共有3290条查询结果,搜索用时 31 毫秒
931.
Sudip Bhattacharyya M. Coleman Miller Tod E. Strohmayer Frederick K. Lamb Craig B. Markwardt 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2765-2767
We discuss millisecond period brightness oscillations and surface atomic spectral lines observed during type I X-ray bursts from a neutron star in a low mass X-ray binary system. We show that modeling of these phenomena can constrain models of the dense cold matter at the cores of neutron stars. We demonstrate that, even for a broad and asymmetric spectral line, the stellar radius-to-mass ratio can be inferred to better than 5%. We also fit our theoretical models to the burst oscillation data of the low mass X-ray binary XTE J1814-338, and find that the 90% confidence lower limit of the neutron star’s dimensionless radius-to-mass ratio is 4.2. 相似文献
932.
A. Fedorov E. Budnik J. -A. Sauvaud 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,30(12):2771-2779
The antiparallel merging model places the location of the reconnection region for a dominant interplanetary magnetic field (IMF) BY at high latitudes at the dayside magnetopause and predicts that the low-latitude boundary layer (LLBL) is located on open field lines of the magnetospheric flanks. Interball-1 data obtained in the wide local time range near the low-latitude magnetopause makes it possible to analyze the LLBL plasma population and to find a link between possible reconnection at high latitudes and LLBL occurrence. We found that no boundary layer was observed in the regions which have no topological connection with the merging site. All cases of LLBL observations are located downstream from a specific boundary. This boundary coincides with the first magnetospheric field line touching the reconnection region and can be located in a wide local time region depending on the instant IMF direction. Even the LLBL on closed field lines shows the tendency to be concentrated in the vicinity of this boundary. Thus we show that all types of observed LLBLs are linked to reconnection sites predicted by the antiparallel merging model. 相似文献
933.
G.C. Ho E.C. Roelof G.M. Mason D. Lario J.E. Mazur 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,32(12):2679-2684
Impulsive solar energetic particle (SEP) events are associated with impulsive X-ray flares, energetic electrons,and enhanced heavy ion abundances. Using instruments on ACE, we have examined the composition and origin of twelve impulsive SEP events from November 1997 to June 2000. All selected impulsive SEP events have enhanced 3He/4He ratios compared with the solar wind values. The range of 3He/4He ratios varies from 0.01 to 7.8. By assuming scatter-free propagation at zero degree pitch-angle, we fitted the minimum particle path lengths (from 1.2 to 1.4 AU, as expected), and estimated the ion event release time back at the Sun to within better than 30 minutes in most cases. We found only four events in which the release times agree for both 38–50 keV electrons and <1 MeV/nucleon ions. Five of our events have significant differences (>40 minutes) between the electron and ion onset times, all with ions injected later. Three impulsive ion events have no association with any impulsive electron event. Seven events have associated solar electromagnetic signatures (Type III radio bursts and/or X-ray flares). 相似文献
934.
E.E. Antonova I.L. Ovchinnikov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,19(12):1919-1922
A current sheet model with developed medium scale turbulence has been constructed. It is suggested that regular plasma flow in the current sheet is compensated by diffusive flux and plasma mixing, leading to temperature equalization. The analyzed turbulence has the form of electrostatic vortices in which electrons and ions move with the same velocities and hence does not lead to anomalous resistivity and current dissipation. It is possible to determine the plasma pressure dependence on magnetic vector potential and to find the Grad—Shafranov equation solutions. The theory is used to explain the Earth's magnetosphere plasma sheet characteristics. It is taken into account that experimentally observed plasma velocity fluctuations in the Earth's plasma sheet and quiescent prominences are much higher than regular plasma flow velocities. The analysis of turbulent current sheet dynamics after the regular motion weakening allows to construct the prominence formation theory. The decreasing of plasma pressure in the sheet due to diffusion leads to field-aligned plasma flow and plasma tube filling by cold chromospheric plasma by the action of siphon mechanism. 相似文献
935.
H.S. Sawant N. Srivastava H.E. Trigoso J.H.A. Sobral F.C.R. Fernandes J.R. Cecatto K.R. Subramanian 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,20(12):2359-2363
Radio observations of the eclipse on November 3, 1994, were carried out at Chapecó, Brazil by using a decimetric spectrograph having high spectral and time resolution. The light curve shows that: (1) Time variation of the radio flux before the totality was more compared to that after. (2) During the totality radio emission at 1.5 GHz was observed. Advantage of high spatial resolution ( 3.2 arc sec) possible during solar eclipse enabled us to determine the height of radio emission at 1.5 GHz. (3) Microwave bursts were observed associated with metric Type III-RS bursts. The source size of one of the microwave bursts was 7 arc sec and its physical parameters have been estimated. (4) The time difference between radio and optical contacts suggested for the first time asymmetrical limb brightening at 1.5 GHz. 相似文献
936.
937.
H.G. Mayr I. Harris R.E. Hartle K.H. Schatten H.A. Taylor K.L. Chan D.R. Stevens-Rayburn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(9):63-68
Superrotation on Venus is discussed in the context of comparative planetary atmospheres. In our planetary system, the rigid shell component (global average) of superrotation is ubiquitous (Jupiter, Saturn, Earth, Venus, Mars, Titan). The largest equatorial values of the component are between 25 and 150 m/sec. We present a simplified, heuristic analysis, utilizing mixing length theory to describe the small scale non-linear advections of energy and angular momentum, thereby providing a closure of the dynamic system. This leads to the conjecture that the zonal velocity may be crudely estimated by , approximating the observed planetary trends; with c the speed of sound, the parameter a being 1 or 2 for geostrophic or cyclostrophic conditions respectively, Pα an effective Prandtl number which becomes less than one when radiative cooling is important, So the average stability, Γ the adiabatic lapse rate and γ the ratio of specific heats. 相似文献
938.
M.R. Leese J.A.M. McDonnell S.F. Green E. Busoletti B.C. Clark L. Colangeli J.F. Crifo P. Eberhardt F. Giovane E. Grün B. Gustafson D.W. Hughes D. Jackson P. Lamy Y. Langevin I. Mann S. McKenna-Lawlor W.G. Tanner P.R. Weissman J.C. Zarnecki 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1996,17(12):137-140
939.
E. C. Stone R. E. Vogt F. B. McDonald B. J. Teegarden J. H. Trainor J. R. Jokipii W. R. Webber 《Space Science Reviews》1977,21(3):355-376
A cosmic-ray detector system (CRS) has been developed for the Voyager mission which will measure the energy spectrum of electrons from 3–110 MeV and the energy spectra and elemental composition of all cosmic-ray nuclei from hydrogen through iron over an energy range from 1–500 MeV/nuc. Isotopes of hydrogen through sulfur will be resolved from 2–75 MeV/nuc. Studies with CRS data will provide information on the energy content, origin and acceleration process, life history, and dynamics of cosmic rays in the galaxy, and contribute to an understanding of the nucleosynthesis of elements in the cosmic-ray sources. Particular emphasis will be placed on low-energy phenomena that are expected to exist in interstellar space and are known to be present in the outer Solar System. This investigation will also add to our understanding of the transport of cosmic rays, Jovian electrons, and low-energy interplanetary particles over an extended region of interplanetary space. A major contribution to these areas of study will be the measurement of three-dimensional streaming patterns of nuclei from H through Fe and electrons over an extended energy range, with a precision that will allow determination of anisotropies down to 1%. The required combination of charge resolution, reliability and redundance has been achieved with systems consisting entirely of solid-state charged-particle detectors.Principal Investigator of the Voyager Cosmic Ray Experiment. 相似文献
940.
Many radar systems now employ wideband waveforms and noncoherent averaging techniques to reduce the scintillation of the backscatter from ground clutter. The purpose of this paper is to quantify the effects of the wideband spectral shape on the clutter standard deviation after noncoherent averaging of the received signal. Relationships are developed which quantify the clutter standard deviation for any spectral shape and any ratio of transmitted band-width to processed bandwidth. 相似文献