全文获取类型
收费全文 | 4717篇 |
免费 | 3篇 |
国内免费 | 9篇 |
专业分类
航空 | 2289篇 |
航天技术 | 1404篇 |
综合类 | 10篇 |
航天 | 1026篇 |
出版年
2021年 | 28篇 |
2018年 | 199篇 |
2017年 | 164篇 |
2016年 | 78篇 |
2015年 | 41篇 |
2014年 | 66篇 |
2013年 | 108篇 |
2012年 | 123篇 |
2011年 | 257篇 |
2010年 | 213篇 |
2009年 | 257篇 |
2008年 | 269篇 |
2007年 | 223篇 |
2006年 | 81篇 |
2005年 | 150篇 |
2004年 | 136篇 |
2003年 | 123篇 |
2002年 | 81篇 |
2001年 | 122篇 |
2000年 | 60篇 |
1999年 | 86篇 |
1998年 | 107篇 |
1997年 | 77篇 |
1996年 | 70篇 |
1995年 | 109篇 |
1994年 | 125篇 |
1993年 | 69篇 |
1992年 | 76篇 |
1991年 | 32篇 |
1990年 | 42篇 |
1989年 | 68篇 |
1988年 | 30篇 |
1987年 | 26篇 |
1986年 | 38篇 |
1985年 | 125篇 |
1984年 | 111篇 |
1983年 | 91篇 |
1982年 | 77篇 |
1981年 | 155篇 |
1980年 | 31篇 |
1979年 | 34篇 |
1978年 | 37篇 |
1977年 | 34篇 |
1976年 | 29篇 |
1975年 | 34篇 |
1974年 | 29篇 |
1973年 | 31篇 |
1972年 | 41篇 |
1971年 | 22篇 |
1970年 | 22篇 |
排序方式: 共有4729条查询结果,搜索用时 489 毫秒
991.
Mino K. Gong G. Kolar J.W. 《IEEE transactions on aerospace and electronic systems》2005,41(3):1008-1018
Novel hybrid 12-pulse line interphase transformer (LIT) rectifier systems with integrated single-switch or two-switch boost-type output stage that ensure a constant output voltage independent of mains and load conditions are proposed for supplying actuators of future more electric aircraft. The principle of operation, the dimensioning, and the system control are discussed. The theoretical considerations are experimentally confirmed for a 10 kW laboratory prototype. Finally, the single-and the two-switch system are comparatively evaluated concerning the level of input current ripple, power factor, and overall efficiency. 相似文献
992.
W. Hermsen J.B.G.M. Bloemen L. Blitz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The radial distribution of the high-energy (70 MeV-5 GeV) gamma-ray emissivity in the outer Milky Way is derived. The kinematics of HI are used to construct column-density maps in three galacto-centric distance ranges in the outer Galaxy. These maps are used in combination with COS-B gamma-ray data to determine gamma-ray emissivities in these distance ranges. A steep negative gradient of the emissivity for the 70 MeV-150 MeV energy range is found in the outer Galaxy. The emissivity for the 300 MeV-5 GeV range is found to be approximately constant (within 20%) and equal to the local value out to large (20 kpc) galacto-centric distances. These results imply a hardening of the gamma-ray spectrum with increrasing distance and for R > 16 kpc the spectrum is shown to be consistent with a π°-decay spectrum with the intensity expected from the local measurement of the cosmic-ray nuclei spectrum. The energy-dependent decrease is interpreted as a steep gradient in the cosmic-ray electron density and a near constancy of the nuclear component. The galactic origin of electrons with energies up to several hundreds of MeV is confirmed, while for cosmic-ray nuclei with energies of a few GeV either confinement in a large galactic halo or an extragalactic origin is suggested by the data. 相似文献
993.
G A Soffen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1986,6(11):57-60
The emergence of the first life on the earth is now established as an early event, and closely related to the evolving earth. Laboratory experiments examining possible chemical events have revealed a multitude of plausible pathways. Lack of knowledge of the primitive terrestrial conditions contemporary with the evolving prebolic organic chemistry limits reconstruction techniques. The primitive earth's aqueous history is essential to unraveling this problem. Based on our current knowledge of other planets of the solar system, we do not expect close analogues to the early earth. We still do not know if there was a second origin or if only earth has life. This may depend upon the question of the survival of information bearing chemical systems in a dynamic or chaotic environment and the chemical protection afforded within such a system. Water is the central molecule of controversy: the blessing and the curse of the chemist. New and novel chemical mechanisms and systems abound. 相似文献
994.
K. Papadopoulos J. G. Lyon C. C. Goodrich P. J. Cargill A. S. Sharma R. Kulkarni CL. L. Chang A. Mankofsky 《Space Science Reviews》1995,71(1-4):671-690
The objective of the University of Maryland ISTP theory project is the development of the analytical and computational tools, which, combined with the data collected by the space and ground-based ISTP sensors, will lead to the construction of the first causal and predictive global geospace model. To attain this objective a research project composed of four complementary parts is conducted. First the global interaction of the solar wind-magnetosphe re system is studied using three-dimensional MHD simulations. Appropriate results of these simulations are made available to other ISTP investigators through the Central Data Handling Facility (CDHF) in a format suitable for comparison with the observations from the ISTP spacecrafts and ground instruments. Second, simulations of local processes are performed using a variety of non-MHD codes (hybrid, particle and multifluid) to study critical magnetospheric boundary layers, such as the magnetopause and the magnetotail. Third, a strong analytic effort using recently developed methods of nonlinear dynamics is conducted, to provide a complementary semi-empirical understanding of the nonlinear response of the magnetosphere and its parts to the solar wind input. The fourth part will be conducted during and following the data retrieval and its objective is to utilize the data base in conjunction with the above models to produce the next generation of global and local magnetospheric models. Special emphasis is paid to the development of advanced visualization packages that allow for interactive real time comparison of the experimental and computational data. Examples of the computational tools and of the ongoing investigations are presented. 相似文献
995.
H Schmidt-B?cking U Ramm G Kraft J Ullrich H Berg C Kelbch R E Olson R DuBois S Hagmann F Jiazhen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(2-3):7-15
Biological damages such as mutations, chromosomal aberrations etc. are a consequence of biochemical changes mostly in the DNA. With ionizing radiation, these chemical changes are due to primary ionization events and secondary ionization effects caused by the primarily produced electrons. Differences in the biological response of densely ionizing radiation, like heavy charged particles, in comparison to sparsely ionizing radiation, such as X- or gamma-rays, are mainly due to the differences in the production of the so called delta-electrons. Therefore, the emission process of electrons i.e. the cross section for the primary ionization event as well as the energy and angular distribution of the emitted electrons should be understood in detail. The delta-electron emission processes occuring in fast heavy ion atom collisions are explained qualitatively. The different spectral structures of electron emission arising from either the target or the projectile are explained in terms of simple models of the kinetics of momentum transfer induced by the COULOMB forces. In collisions of very heavy ions with matter, high nuclear COULOMB forces are created. These forces lead to a strong polarization of the electronic states of the participated electrons. The effects of this polarization are discussed. 相似文献
996.
G W Barendsen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(2-3):385-392
Evidence is reviewed concerning the variation of RBE values of high-LET radiations for non-stochastic effects, generally impairment of tissue integrity and function. The RBE values are dependent on the type of radiation, the type of tissue effect and the dose rate or fractionation schedule. RBE values depend strongly on the effect considered, with high values for late effects in lung, kidney and central nervous system. RBE values generally increase with decreasing dose rate or dose per fraction. Maximum values can be derived by extrapolation on the basis of a radiobiological model. These values are denoted RBEm to distinguish them from RBEM derived for stochastic effects, e.g. carcinogenesis. Values of RBEm are generally in the range of 2 to 10 and are considerably smaller by a factor of 2 to 5 than values of RBEM for various types of stochastic effects. RBE values for effects from actual exposures to mixtures of high-LET and low-LET radiations can be derived by considering the doses received and the tissue at risk. Applications of RBEm values will yield estimates of maximum values of equivalent doses and these should only be applied for planning medical interventions if the contribution from high-LET radiation is small. The selection of Q values for radiation protection is mostly based on RBE--values and the application of Q values in cases where non-stochastic effects are important might therefore result in an overestimate of the risks of exposure. 相似文献
997.
998.
999.
G A Ubbels W Berendsen S Kerkvliet J Narraway 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(1):181-194
Egg rotation and centrifugation experiments strongly suggest a role for gravity in the determination of the spatial structure of amphibian embryos. Decisive experiments can only be made in Space. Eggs of Xenopus laevis, the South African clawed toad, were the first vertebrate eggs which were successfully fertilized on Sounding Rockets in Space. Unfixed, newly fertilized eggs survived reentry, and a reasonable number showed a seemingly normal gastrulation but died between gastrulation and neurulation. Only a few reached the larval stage, but these developed abnormally. In the future, we intend to test whether this abnormal morphogenesis is due to reentry perturbations, or due to a real microgravity effect, through perturbation of the reinitiation of meiosis and other processes, or started by later sperm penetration. 相似文献
1000.
EXOSAT has been used to carry out a series of observations of the dwarf nova SS Cygni covering both quiescent and outburst states which provide a detailed picture of its behaviour at X-ray wavelengths. These results provide strong support for a new coronal model for the X-ray emission from non-magnetic white dwarf systems. 相似文献