全文获取类型
收费全文 | 6472篇 |
免费 | 28篇 |
国内免费 | 12篇 |
专业分类
航空 | 2987篇 |
航天技术 | 2008篇 |
综合类 | 29篇 |
航天 | 1488篇 |
出版年
2021年 | 59篇 |
2019年 | 39篇 |
2018年 | 216篇 |
2017年 | 170篇 |
2016年 | 143篇 |
2015年 | 64篇 |
2014年 | 153篇 |
2013年 | 188篇 |
2012年 | 192篇 |
2011年 | 297篇 |
2010年 | 254篇 |
2009年 | 343篇 |
2008年 | 364篇 |
2007年 | 244篇 |
2006年 | 135篇 |
2005年 | 194篇 |
2004年 | 164篇 |
2003年 | 199篇 |
2002年 | 139篇 |
2001年 | 219篇 |
2000年 | 103篇 |
1999年 | 120篇 |
1998年 | 152篇 |
1997年 | 105篇 |
1996年 | 131篇 |
1995年 | 195篇 |
1994年 | 155篇 |
1993年 | 88篇 |
1992年 | 123篇 |
1991年 | 42篇 |
1990年 | 57篇 |
1989年 | 121篇 |
1988年 | 50篇 |
1987年 | 48篇 |
1986年 | 48篇 |
1985年 | 159篇 |
1984年 | 141篇 |
1983年 | 123篇 |
1982年 | 116篇 |
1981年 | 158篇 |
1980年 | 47篇 |
1979年 | 43篇 |
1978年 | 41篇 |
1977年 | 40篇 |
1976年 | 30篇 |
1975年 | 47篇 |
1974年 | 33篇 |
1973年 | 23篇 |
1972年 | 43篇 |
1971年 | 28篇 |
排序方式: 共有6512条查询结果,搜索用时 78 毫秒
801.
D. Horns for the H.E.S.S. collaboration 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):2024-2028
Observations of the Galactic center region with the H.E.S.S. telescopes have established the existence of a steady, extended source of gamma-ray emission coinciding with the position of the super massive black hole Sgr A*. This is a remarkable finding given the expected presence of dense self-annihilating Dark Matter in the Galactic center region. The self-annihilation process is giving rise to gamma-ray production through hadronization including the production of neutral pions which decay into gamma-rays but also through (loop-suppressed) annihilation into final states of almost mono-energetic photons. We study the observed gamma-ray signal (spectrum and shape) from the Galactic center in the context of Dark Matter annihilation and indicate the prospects for further indirect Dark Matter searches with H.E.S.S. 相似文献
802.
J W Wilson R K Tripathi G D Qualls F A Cucinotta R E Prael J W Norbury J H Heinbockel J Tweed 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(6):1319-1327
Improved spacecraft shield design requires early entry of radiation constraints into the design process to maximize performance and minimize costs. As a result, we have been investigating high-speed computational procedures to allow shield analysis from the preliminary design concepts to the final design. In particular, we will discuss the progress towards a full three-dimensional and computationally efficient deterministic code for which the current HZETRN evaluates the lowest-order asymptotic term. HZETRN is the first deterministic solution to the Boltzmann equation allowing field mapping within the International Space Station (ISS) in tens of minutes using standard finite element method (FEM) geometry common to engineering design practice enabling development of integrated multidisciplinary design optimization methods. A single ray trace in ISS FEM geometry requires 14 ms and severely limits application of Monte Carlo methods to such engineering models. A potential means of improving the Monte Carlo efficiency in coupling to spacecraft geometry is given in terms of re-configurable computing and could be utilized in the final design as verification of the deterministic method optimized design. 相似文献
803.
The study of the electrical environment of the Earth's atmosphere has rapidly advanced during the past century. Great strides have been made towards the understanding of lightning and thunderstorms and in relating them to the global electric circuit. The electromagnetic fields and currents connect different parts of the Earth's environment, and any type of perturbation in one region affects another region. Starting from the traditional views in which the electrodynamics of one region has been studied in isolation from the neighboring regions, the modern theory of the global electrical circuit has been discussed briefly. Interconnection and electrodynamic coupling of various regions of the Earth's environment can be easily studied by using the global electric circuit model. Deficiencies in the model and the possibility of improvement in it have been suggested. Application of the global electric circuit model to the understanding of the Earth's changes of climate has been indicated. 相似文献
804.
G. V. Kasatkin 《Cosmic Research》2007,45(2):110-125
Attractive forces inside a thin nonuniform meteor ring are found and their features are revealed. 相似文献
805.
B. I. Rabinovich 《Cosmic Research》2007,45(5):393-407
This paper continues the series of papers [1–5] and generalizes the previous results to a proto-ring of magnetized plasma whose density decreases in the radial direction. The problem of quantization of the sector and orbital velocities, and of the radii and periods of revolution of elite plasma rings is considered. A new concept of super-elite rings is introduced. Their isomorphism with the orbits of the planets and planetary satellites in the Solar System is proved. This isomorphism also extends to the orbits of electrons in the Bohr’s model of the hydrogen atom. 相似文献
806.
E.B. Romanova O.M. Pirog N.M. Polekh A.V. Tashchilin G.A. Zherebtsov J.K. Shi X. Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(4):569-578
The results of modeling of ionospheric disturbances observed in the East Asian region during moderate storms are presented. The numerical model for ionosphere–plasmasphere coupling developed at the ISTP SB RAS is used to interpret the data of observations at ionospheric stations located in the longitudinal sector of 90–130°E at latitudes from auroral zone to equator. There is obtained a reasonable agreement between measurements and modeling results for winter and equinox. In the summer ionosphere, at the background of high ionization by the solar EUV radiation in the quiet geomagnetic period the meridional thermospheric wind strongly impacts the electron concentration in the middle and auroral ionosphere. The consistent calculations of the thermospheric wind permit to obtain the model results which are closer to summer observations. The actual information about the space-time variations of thermosphere and magnetosphere parameters should be taken into account during storms. 相似文献
807.
West W.C. Whitacre J.F. Brandon E.J. Ratnakumar B.V. 《Aerospace and Electronic Systems Magazine, IEEE》2001,16(8):31-33
Recent successes in the effort to miniaturize spacecraft components using MEMS technology, integrated passive components, and low power electronics have driven the need for very low power, low profile, low mass micro-power sources for micro/nanospacecraft applications. Recent work at JPL has focused upon developing thin film/micro-batteries compatible with temperature sensitive substrates. A process to prepare crystalline LiCoO2 films with RF sputtering and moderate (<700°C) annealing temperature has been developed. Thin film batteries with cathode films prepared with this process have specific capacities approaching the practical limit for LiCoO2, with acceptable rate capabilities and discharge voltage profiles. Solid-state micro-scale batteries have also been fabricated with feature sizes on the order of 50 microns 相似文献
808.
We report new calculations of transition radiation spectra which are correct for arbitrary energy of a particle at all frequencies down to plasma frequency. The importance of the emission mechanism for solar flares are discussed. 相似文献
809.
Over 8,000 altitude deviations are reported to NASA's Aviation Safety Reporting System each year. This is almost one an hour. The narratives of pilot incidents relate how errors made in the automation-assisted altitude change task are caused by the difficulty pilots are having interacting with automatic systems. This paper discusses the impact of increased automation in glass-cockpit airliners on the altitude deviations reported by pilots. By observing the way information is processed by the cockpit system, the author suggests that the philosophies of design and training need to change in order to facilitate, not debilitate, the aircrew 相似文献
810.
C. S. Zerefos D. S. Balis P. Zanis C. Meleti A. F. Bais K. Tourpali D. Melas I. Ziomas E. Galani K. Kourtidis A. Papayannis Z. Gogosheva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2001,27(12):1955-1963
Intensive measurements of UV solar irradiance, total ozone and surface ozone were carried out during the solar eclipse of 11 August 1999 at Thessaloniki, Greece and Stara Zagora, Bulgaria, located very close to the footprint of the moon's shadow during the solar eclipse with the maximum coverage of the solar disk reaching about 90% and 96% respectively. It is shown that during the eclipse the diffuse component is reduced less compared to the decline of the direct solar irradiance at the shorter wavelengths. A 20-minute oscillation of erythemal UV-B solar irradiance was observed before and after the time of the eclipse maximum under clear skies, indicating a possible 20-minute fluctuation in total ozone presumably caused by the eclipse induced gravity waves. The surface ozone measurements at Thessaloniki display a decrease of around 10–15 ppbv during the solar eclipse. Similarly, ozone profile measurements with a lidar system indicate a decrease of ozone up to 2 km during the solar eclipse. The eclipse offered the opportunity to test our understanding of tropospheric ozone chemistry. The use of a chemical box model suggested that photochemistry can account for a significant portion of the observed surface ozone decrease. 相似文献