全文获取类型
收费全文 | 987篇 |
免费 | 195篇 |
国内免费 | 259篇 |
专业分类
航空 | 988篇 |
航天技术 | 148篇 |
综合类 | 182篇 |
航天 | 123篇 |
出版年
2024年 | 1篇 |
2023年 | 18篇 |
2022年 | 32篇 |
2021年 | 42篇 |
2020年 | 52篇 |
2019年 | 55篇 |
2018年 | 47篇 |
2017年 | 37篇 |
2016年 | 65篇 |
2015年 | 62篇 |
2014年 | 73篇 |
2013年 | 55篇 |
2012年 | 64篇 |
2011年 | 80篇 |
2010年 | 55篇 |
2009年 | 75篇 |
2008年 | 65篇 |
2007年 | 57篇 |
2006年 | 44篇 |
2005年 | 32篇 |
2004年 | 36篇 |
2003年 | 35篇 |
2002年 | 39篇 |
2001年 | 18篇 |
2000年 | 26篇 |
1999年 | 27篇 |
1998年 | 30篇 |
1997年 | 24篇 |
1996年 | 26篇 |
1995年 | 19篇 |
1994年 | 28篇 |
1993年 | 23篇 |
1992年 | 29篇 |
1991年 | 23篇 |
1990年 | 12篇 |
1989年 | 14篇 |
1988年 | 20篇 |
1987年 | 1篇 |
排序方式: 共有1441条查询结果,搜索用时 31 毫秒
101.
102.
基于BP网络的机组工作量评估方法研究 总被引:2,自引:0,他引:2
为研究机组工作量的评估问题,搭建了模拟飞行实验平台,设定了7种不同负荷的飞行任务。模拟飞行中,对被试的生理指标进行测量,并采集其主观评价值。采用BP网络进行数学建模,将生理指标测量值作为输入、NASA-TLX表法的评价值作为输出,利用输入、输出模式对对网络进行训练,并对该方法进行验证。结果表明,基于BP网络的机组工作量评估方法,较传统方法更为稳定、精确,且大大降低了被试数量。提高训练模式对的数量、简化生理指标的测量过程,并保证测量精度是该方法成功的关键。 相似文献
103.
The past dozen years have produced a new paradigm with regard to the source regions of comets in the early solar system. It
is now widely recognized that the likely source of the Jupiter-family short-period comets (those with Tisserand parameters,
T > 2 and periods, P, generally < 20 years) is the Kuiper belt in the ecliptic plane beyond Neptune. In contrast, the source
of the Halley-type and long-period comets (those with T < 2 and P > 20 years) appears to be the Oort cloud. However, the comets
in the Oort cloud almost certainly originated elsewhere, since accretion is very inefficient at such large heliocentric distances.
New dynamical studies now suggest that the source of the Oort cloud comets is the entire giant planets region from Jupiter
to Neptune, rather than primarily the Uranus-Neptune region, as previously thought. Some fraction of the Oort cloud population
may even be asteroidal bodies formed inside the orbit of Jupiter. These comets and asteroids underwent a complex dynamical
random walk among the giant planets before they were ejected to distant orbits in the Oort cloud, with possible interesting
consequences for their thermal and collisional histories. Observational evidence for diversity in cometary compositions is
limited, at best.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
104.
本文从当前高校体育教学的周期短、学时少、教学方法单一的特点出发,充分的利用现代计算机网路多媒体技术,设计一套符合高校体育教育的多媒体教学平台系统,以满足学生课余时间的自主学习,增加教学的延伸性、娱乐性,为高校体育教育目标的实现提供保障。 相似文献
105.
106.
以提高大截面Z型材四轴滚弯成形精度为目的,通过综合考虑材料属性、几何特征和成形半径等因素对回弹的影响,建立了引入中性层偏移的大截面Z型材弯曲回弹解析模型,研究了7075-O和7475-O铝合金Z型材在不同滚弯成形半径下的回弹规律,并进行滚弯成形实验验证。结果表明,与忽略中性层偏移影响的型材回弹预测经验模型相比,基于中性层偏移的回弹预测模型能够准确预测大截面Z型材的回弹量,在相同的曲率半径下,预测回弹变形的最大相对误差从11.681%减小到3.347%。 相似文献
107.
K.G. Ratovsky A.V. OinatsA.V. Medvedev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The diurnal and seasonal variations of F2 layer characteristics (critical frequency, peak height and bottomside thickness) over Irkutsk, Russia (52.3 N and 104.3 E) are studied by the method of running medians. The comparison with the IRI-2001 model during the decrease in solar activity in 2003–2006 revealed cases of both close agreement and systematic differences between predictions and observations. The systematic difference is not the only reason for disagreement between IRI and observations; there are also intrayear variations which are not associated with seasonal behavior. The period of observation was too short to make conclusions about solar activity dependence of the noon bottomside thickness and the modification of its diurnal behavior with decreasing solar activity. 相似文献
108.
S.A. Pulinets 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The concept of the Global Electric Circuit (GEC) provides an explanation of the existence of a vertical atmospheric electric field and coupling between the ground and ionosphere. Presently, ionospheric physics pays more attention to electric fields and coupling processes in the polar and auroral regions, whereas in other areas the potential difference between the ground and ionosphere usually is not taken into account. Regional processes exist, however, that are able to significantly affect the GEC parameters and through modification of the ionospheric potential to create plasma density irregularities of different scales within the ionosphere. One such source of ionosphere modification is air ionization in the vicinity of active tectonic faults, which takes place due to increased radon emanation. This paper considers the process of local modification of the GEC and corresponding ionospheric variability due to tectonic activity. 相似文献
109.
The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field. 相似文献
110.