全文获取类型
收费全文 | 4398篇 |
免费 | 5篇 |
国内免费 | 21篇 |
专业分类
航空 | 2237篇 |
航天技术 | 1665篇 |
综合类 | 21篇 |
航天 | 501篇 |
出版年
2018年 | 45篇 |
2017年 | 32篇 |
2014年 | 63篇 |
2013年 | 93篇 |
2012年 | 73篇 |
2011年 | 121篇 |
2010年 | 89篇 |
2009年 | 147篇 |
2008年 | 236篇 |
2007年 | 83篇 |
2006年 | 91篇 |
2005年 | 104篇 |
2004年 | 129篇 |
2003年 | 146篇 |
2002年 | 81篇 |
2001年 | 110篇 |
2000年 | 86篇 |
1999年 | 86篇 |
1998年 | 137篇 |
1997年 | 88篇 |
1996年 | 113篇 |
1995年 | 129篇 |
1994年 | 149篇 |
1993年 | 86篇 |
1992年 | 121篇 |
1991年 | 53篇 |
1990年 | 55篇 |
1989年 | 130篇 |
1988年 | 47篇 |
1987年 | 55篇 |
1986年 | 73篇 |
1985年 | 171篇 |
1984年 | 109篇 |
1983年 | 103篇 |
1982年 | 106篇 |
1981年 | 151篇 |
1980年 | 65篇 |
1979年 | 47篇 |
1978年 | 44篇 |
1977年 | 41篇 |
1975年 | 51篇 |
1974年 | 39篇 |
1973年 | 46篇 |
1972年 | 40篇 |
1971年 | 43篇 |
1970年 | 37篇 |
1969年 | 44篇 |
1968年 | 30篇 |
1967年 | 29篇 |
1966年 | 30篇 |
排序方式: 共有4424条查询结果,搜索用时 703 毫秒
231.
Clark R.N. Masreliez C.J. Burrows J.W. 《IEEE transactions on aerospace and electronic systems》1976,(4):459-463
A scheme to provide redundant sensor data in an automatic control system using the principle of functional redundancy is described. Normally there are three redundant radar altimeters used in the terminal phase of automatic landing of jet transport airplanes. This scheme replaces one of these altimeters with a data processing scheme based on a Kalman filter. The filter is driven by altitude rate and acceleration signals from the air data computer and vertical accelerometer. A special initialization technique employs the two altimeter signals. The feasibility of this scheme is indicated by tests in which data obtained from these several sensors during flight tests are used to drive the functionally redundant altimeter. 相似文献
232.
H. Kunow N. U. Crooker J. A. Linker R. Schwenn R. von Steiger 《Space Science Reviews》2006,123(1-3):1-2
233.
A. G. Yahnin I. V. Despirak A. A. Lubchich B. V. Kozelov N. P. Dmitrieva M. A. Shukhtina H. K Biernat 《Space Science Reviews》2006,122(1-4):97-106
Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation
of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the
data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The
poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated
with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are
generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that
the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison
of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase
shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm
development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic
plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for
monitoring of substorm intensity in terms of the magnetic flux and energy dissipation. 相似文献
234.
Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity,
magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs
as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their
emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article
we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing
observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the
inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour
high-latitude activity. 相似文献
235.
Energetic particle observations in the interplanetary medium provide fundamental information about the origin, development
and structure of coronal mass ejections. This paper reviews the status of our understanding of the ways in which particles
are energised at the Sun in association with CMEs. This understanding will remain incomplete until the relationship between
CMEs and flares is determined and we know the topology of the associated magnetic fields. The paper also discusses the characteristics
of interplanetary CMEs that may be probed using particle observations. 相似文献
236.
R. Schwenn J. C. Raymond D. Alexander A. Ciaravella N. Gopalswamy R. Howard H. Hudson P. Kaufmann A. Klassen D. Maia G. Munoz-Martinez M. Pick M. Reiner N. Srivastava D. Tripathi A. Vourlidas Y.-M. Wang J. Zhang 《Space Science Reviews》2006,123(1-3):127-176
CMEs have been observed for over 30 years with a wide variety of instruments. It is now possible to derive detailed and quantitative information on CME morphology, velocity, acceleration and mass. Flares associated with CMEs are observed in X-rays, and several different radio signatures are also seen. Optical and UV spectra of CMEs both on the disk and at the limb provide velocities along the line of sight and diagnostics for temperature, density and composition. From the vast quantity of data we attempt to synthesize the current state of knowledge of the properties of CMEs, along with some specific observed characteristics that illuminate the physical processes occurring during CME eruption. These include the common three-part structures of CMEs, which is generally attributed to compressed material at the leading edge, a low-density magnetic bubble and dense prominence gas. Signatures of shock waves are seen, but the location of these shocks relative to the other structures and the occurrence rate at the heights where Solar Energetic Particles are produced remains controversial. The relationships among CMEs, Moreton waves, EIT waves, and EUV dimming are also cloudy. The close connection between CMEs and flares suggests that magnetic reconnection plays an important role in CME eruption and evolution. We discuss the evidence for reconnection in current sheets from white-light, X-ray, radio and UV observations. Finally, we summarize the requirements for future instrumentation that might answer the outstanding questions and the opportunities that new space-based and ground-based observatories will provide in the future. 相似文献
237.
A. Galli P. Wurz H. Lammer H. I. M. Lichtenegger R. Lundin S. Barabash A. Grigoriev M. Holmström H. Gunell 《Space Science Reviews》2006,126(1-4):447-467
We have evaluated the Lyman-α limb emission from the exospheric hydrogen of Mars measured by the neutral particle detector of the ASPERA-3 instrument on Mars Express in 2004 at low solar activity (solar activity index = 42, F10.7=100). We derive estimates for the hydrogen exobase density, n H = 1010 m?3, and for the apparent temperature, T > 600 K. We conclude that the limb emission measurement is dominated by a hydrogen component that is considerably hotter than the bulk temperature at the exobase. The derived values for the exosphere density and temperature are compared with similar measurements done by the Mariner space probes in the 1969. The values found with Mars Express and Mariner data are brought in a broader context of exosphere models including the possibility of having two hydrogen components in the Martian exosphere. The present observation of the Martian hydrogen exosphere is the first one at high altitudes during low solar activity, and shows that for low solar activity exospheric densities are not higher than for high solar activity. 相似文献
238.
239.
240.
为达到IHPTET计划第三阶段目标,普惠公司进行了XTC67/1核心机试验。该公司在实施XTC67/1计划中取得了一些成果,但也存在一些问题 相似文献