全文获取类型
收费全文 | 325篇 |
免费 | 1篇 |
国内免费 | 5篇 |
专业分类
航空 | 198篇 |
航天技术 | 76篇 |
综合类 | 1篇 |
航天 | 56篇 |
出版年
2022年 | 2篇 |
2021年 | 5篇 |
2019年 | 3篇 |
2018年 | 34篇 |
2017年 | 20篇 |
2016年 | 1篇 |
2015年 | 9篇 |
2014年 | 5篇 |
2013年 | 14篇 |
2012年 | 8篇 |
2011年 | 12篇 |
2010年 | 16篇 |
2009年 | 17篇 |
2008年 | 14篇 |
2007年 | 15篇 |
2006年 | 14篇 |
2005年 | 12篇 |
2004年 | 9篇 |
2003年 | 5篇 |
2002年 | 4篇 |
2001年 | 8篇 |
2000年 | 6篇 |
1999年 | 10篇 |
1998年 | 5篇 |
1997年 | 9篇 |
1996年 | 2篇 |
1995年 | 8篇 |
1994年 | 7篇 |
1993年 | 3篇 |
1992年 | 3篇 |
1990年 | 1篇 |
1988年 | 1篇 |
1986年 | 2篇 |
1985年 | 9篇 |
1984年 | 13篇 |
1983年 | 3篇 |
1982年 | 5篇 |
1981年 | 10篇 |
1980年 | 1篇 |
1978年 | 1篇 |
1972年 | 1篇 |
1970年 | 2篇 |
1967年 | 1篇 |
1963年 | 1篇 |
排序方式: 共有331条查询结果,搜索用时 265 毫秒
141.
Navigational aids impair spatial memory for experienced environments, but the cognitive mechanisms underlying impairment remain an open question. Recent evidence implicates divided attention, but to date no study has directly manipulated divided attention in navigational aid contexts. The present study addresses this need. Participants navigated virtual towns with aid presence and divided attention factorially crossed in a within-participants design. They then completed spatial memory assessments. Divided attention alone impaired spatial memory. Navigational aid presence impaired spatial memory when attention was undivided, replicating previous findings, but did not to a greater extent when attention was divided. These findings suggest that navigational aids divide attention sufficiently to impair spatial memory. 相似文献
142.
Energisation of O+ and O+
2 Ions at Mars: An Analysis of a 3-D Quasi-Neutral Hybrid Model Simulation
E. Kallio A. Fedorov S. Barabash P. Janhunen H. Koskinen W. Schmidt R. Lundin H. Gunell M. Holmström Y. Futaana M. Yamauchi A. Grigoriev J. D. Winningham R. Frahm J. R. Sharber 《Space Science Reviews》2006,126(1-4):39-62
We have studied the loss of O+ and O+
2 ions at Mars with a numerical model. In our quasi-neutral hybrid model ions (H+, He++, O+, O+
2) are treated as particles while electrons form a massless charge-neutralising fluid. The employed model version does not
include the Martian magnetic field resulting from the crustal magnetic anomalies. In this study we focus the Martian nightside
where the ASPERA instrument on the Phobos-2 spacecraft and recently the ASPERA-3 instruments on the Mars Express spacecraft
have measured the proprieties of escaping atomic and molecular ions, in particular O+ and O+
2 ions. We study the ion velocity distribution and how the escaping planetary ions are distributed in the tail. We also create
similar types of energy-spectrograms from the simulation as were obtained from ASPERA-3 ion measurements. We found that the
properties of the simulated escaping planetary ions have many qualitative and quantitative similarities with the observations
made by ASPERA instruments. The general agreement with the observations suggest that acceleration of the planetary ions by
the convective electric field associated with the flowing plasma is the key acceleration mechanism for the escaping ions observed
at Mars. 相似文献
143.
Émilie Hardy Agnès Levy Gilles Métris Manuel Rodrigues Pierre Touboul 《Space Science Reviews》2013,180(1-4):177-191
The MICROSCOPE space mission aims at testing the Equivalence Principle (EP) with an accuracy of 10?15. The test is based on the precise measurement delivered by a differential electrostatic accelerometer on-board a drag-free microsatellite which includes two cylindrical test masses submitted to the same gravitational field and made of different materials. The experiment consists in testing the equality of the electrostatic acceleration applied to the masses to maintain them relatively motionless at a well-known frequency. This high precision experiment is compatible with only very little perturbations. However, aliasing arises from the finite time span of the measurement, and is amplified by measurement losses. These effects perturb the measurement analysis. Numerical simulations have been run to estimate the contribution of a perturbation at any frequency on the EP violation frequency and to test its compatibility with the mission specifications. Moreover, different data analysis procedures have been considered to select the one minimizing these effects taking into account the uncertainty about the frequencies of the implicated signals. 相似文献
144.
We present an overview of the properties of magnetohydrodynamic turbulence within corotating interaction regions (CIRs) and
its effects on energetic particles. We stress the importance of both the population of fluctuations in the inner heliosphere
and the changing local environment in determining their properties at larger heliospheric distances. We present observations
from two typical CIRs, one at 0.3 AU before compression regions have formed and the other well developed at 5.1 AU, and discuss
the properties of fluctuations within them and show that it is possible to distinguish different regions of the CIR on the
basis of the turbulence itself. The strength of the turbulence varies strongly within and close to the CIRs, explaining changes
in the mean free path of energetic particles of several orders of magnitude with implications for the modulation of cosmic
rays and for diffusive acceleration of particles. The mechanisms by which turbulent fluctuations within interaction regions
scatter energetic particles are briefly discussed on a theoretical basis.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
145.
E Chassefière J-L Bertaux J-J Berthelier M Cabane V Ciarletti G Durry F Forget M Hamelin F Leblanc M Menvielle M Gerasimov O Korablev S Linkin G Managadze A Jambon G Manhès Ph Lognonné P Agrinier P Cartigny D Giardini T Pike W Kofman A Herique P Coll A Person F Costard Ph Sarda Ph Paillou M Chaussidon B Marty F Robert S Maurice M Blanc C d'Uston J-Ch Sabroux J-F Pineau P Rochette 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(8):1702-1709
In view to prepare Mars human exploration, it is necessary to promote and lead, at the international level, a highly interdisciplinary program, involving specialists of geochemistry, geophysics, atmospheric science, space weather, and biology. The goal of this program will be to elaborate concepts of individual instruments, then of integrated instrumental packages, able to collect exhaustive data sets of environmental parameters from future landers and rovers of Mars, and to favour the conditions of their implementation. Such a program is one of the most urgent need for preparing human exploration, in order to develop mitigation strategies aimed at ensuring the safety of human explorers, and minimizing risk for surface operations. A few main areas of investigation may be listed: particle and radiation environment, chemical composition of atmosphere, meteorology, chemical composition of dust, surface and subsurface material, water in the subsurface, physical properties of the soil, search for an hypothesized microbial activity, characterization of radio-electric properties of the Martian ionosphere. Scientists at the origin of the present paper, already involved at a high degree of responsibility in several Mars missions, and actively preparing in situ instrumentation for future landed platforms (Netlander--now cancelled, MSL-09), express their readiness to participate in both ESA/AURORA and NASA programs of Mars human exploration. They think that the formation of a Mars Environment working group at ESA, in the course of the AURORA definition phase, could act positively in favour of the program, by increasing its scientific cross-section and making it still more focused on human exploration. 相似文献
146.
Andrew S. Rivkin Jian-Yang Li Ralph E. Milliken Lucy F. Lim Amy J. Lovell Britney E. Schmidt Lucy A. McFadden Barbara A. Cohen 《Space Science Reviews》2011,163(1-4):95-116
Our understanding of the composition of Ceres is driven by remote sensing of its surface. We review spectral observations of Ceres over wavelengths from the ultraviolet to the radio, as well as non-spectral data such as thermal inertia, photometric properties, radar experiments, and surface variability. We also discuss the closest likely meteorite analogs to Ceres and consider the likelihood that material from Ceres could be delivered to Earth. 相似文献
147.
Aaron L. Gardony Tad T. Brunyé Caroline R. Mahoney Holly A. Taylor 《Spatial Cognition & Computation》2013,13(4):319-350
Abstract Research has demonstrated navigational aids impair spatial memory, but has not considered important spatial cognitive concepts. For example, impairment may stem from spatial perspective switches between route-based aids and survey-based memory assessments. Further, the verbal format of aid instructions may selectively interfere with verbal working memory (VWM). To address these potential explanations, participants navigated desktop virtual environments in a goal-directed manner. In each within-participants condition, participants either navigated with a verbal or tonal aid that presented mixed spatial perspective instructions or without aid. Both aids yielded slight navigational advantages and steep spatial memory costs despite their mixed perspective instructions. The equivalent impairment between information formats suggests navigational aids impair spatial memory by dividing attention rather than selective interference of VWM. 相似文献
148.
149.
150.
V. Dehant H. Lammer Y. N. Kulikov J.-M. Grießmeier D. Breuer O. Verhoeven Ö. Karatekin T. Van Hoolst O. Korablev P. Lognonné 《Space Science Reviews》2007,129(1-3):279-300
In light of assessing the habitability of Mars, we examine the impact of the magnetic field on the atmosphere. When there
is a magnetic field, the atmosphere is protected from erosion by solar wind. The magnetic field ensures the maintenance of
a dense atmosphere, necessary for liquid water to exist on the surface of Mars. We also examine the impact of the rotation
of Mars on the magnetic field. When the magnetic field of Mars ceased to exist (about 4 Gyr ago), atmospheric escape induced
by solar wind began. We consider scenarios which could ultimately lead to a decrease of atmospheric pressure to the presently
observed value of 7 mbar: a much weaker early martian magnetic field, a late onset of the dynamo, and high erosion rates of
a denser early atmosphere. 相似文献