全文获取类型
收费全文 | 988篇 |
免费 | 129篇 |
国内免费 | 259篇 |
专业分类
航空 | 519篇 |
航天技术 | 424篇 |
综合类 | 62篇 |
航天 | 371篇 |
出版年
2024年 | 4篇 |
2023年 | 16篇 |
2022年 | 22篇 |
2021年 | 48篇 |
2020年 | 51篇 |
2019年 | 34篇 |
2018年 | 42篇 |
2017年 | 40篇 |
2016年 | 52篇 |
2015年 | 54篇 |
2014年 | 87篇 |
2013年 | 73篇 |
2012年 | 79篇 |
2011年 | 65篇 |
2010年 | 77篇 |
2009年 | 77篇 |
2008年 | 59篇 |
2007年 | 57篇 |
2006年 | 92篇 |
2005年 | 48篇 |
2004年 | 22篇 |
2003年 | 35篇 |
2002年 | 34篇 |
2001年 | 19篇 |
2000年 | 20篇 |
1999年 | 30篇 |
1998年 | 23篇 |
1997年 | 9篇 |
1996年 | 21篇 |
1995年 | 24篇 |
1994年 | 21篇 |
1993年 | 10篇 |
1992年 | 12篇 |
1991年 | 2篇 |
1990年 | 1篇 |
1989年 | 6篇 |
1988年 | 1篇 |
1987年 | 2篇 |
1984年 | 7篇 |
排序方式: 共有1376条查询结果,搜索用时 31 毫秒
91.
92.
S. W. Kahler 《Space Science Reviews》2007,129(4):359-390
Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several
acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks
driven by coronal mass ejections (CMEs) with speeds ≳1000 km s−1. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with
CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the
sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known
several decades ago, but recent observations have presented a more complex picture. We review early and recent observational
results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus
flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from
flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic
proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events;
electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks
are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares.
Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions
for future work are given. 相似文献
93.
R. C. Wiens D. S. Burnett C. M. Hohenberg A. Meshik V. Heber A. Grimberg R. Wieler D. B. Reisenfeld 《Space Science Reviews》2007,130(1-4):161-171
The Genesis mission returned samples of solar wind to Earth in September 2004 for ground-based analyses of solar-wind composition,
particularly for isotope ratios. Substrates, consisting mostly of high-purity semiconductor materials, were exposed to the
solar wind at L1 from December 2001 to April 2004. In addition to a bulk sample of the solar wind, separate samples of coronal
hole (CH), interstream (IS), and coronal mass ejection material were obtained. Although many substrates were broken upon landing
due to the failure to deploy the parachute, a number of results have been obtained, and most of the primary science objectives
will likely be met. These objectives include He, Ne, Ar, Kr, and Xe isotope ratios in the bulk solar wind and in different
solar-wind regimes, and 15N/14N and 18O/17O/16O to high precision. The greatest successes to date have been with the noble gases. Light noble gases from bulk solar wind
and separate solar-wind regime samples have now been analyzed. Helium results show clear evidence of isotopic fractionation
between CH and IS samples, consistent with simplistic Coulomb drag theory predictions of fractionation between the photosphere
and different solar-wind regimes, though fractionation by wave heating is also a possible explanation. Neon results from closed
system stepped etching of bulk metallic glass have revealed the nature of isotopic fractionation as a function of depth, which
in lunar samples have for years deceptively suggested the presence of an additional, energetic component in solar wind trapped
in lunar grains and meteorites. Isotope ratios of the heavy noble gases, nitrogen, and oxygen are in the process of being
measured. 相似文献
94.
95.
基于轴对称排气系统设计了一套S弯二元喷管的实验模型,在实验工况下测量了喷管实验件的部分流场参数和远场红外辐射特性,对S弯二元喷管的红外辐射特性进行了分析和研究,并与基准轴对称喷管的红外辐射实验结果进行了对比。结果表明:上方探测平面是S弯二元喷管的主要辐射方向,其最大辐射角度为15°,在该方向角上固体壁面辐射的贡献最大。下方和侧向探测平面各方向角的红外辐射强度明显小于上方探测平面,主要是由于S弯二元喷管遮挡了大部分的内部高温壁面。与基准轴对称喷管对比,S弯二元喷管有着明显的红外抑制作用,在尾部方向S弯二元喷管的积分辐射强度相比轴对称喷管降低了81%,最大辐射强度相比轴对称喷管降低了47%,燃气辐射降低50%。 相似文献
96.
97.
为解决太阳能无人机(UAV)总体设计中任务需求表达模糊、技术指标重要度排序决策困难的问题,提出了基于模糊质量功能展开(FQFD)的太阳能无人机总体设计指标排序方法。该方法在传统质量功能展开(QFD)质量屋的基础上,引入三角模糊数,表征任务需求的不确定性和模糊性;在模糊隶属度函数未知的情况下,采用α加权修正水平截集去模糊化方法计算技术指标重要度,获得技术指标重要度排序,为总体设计优化决策提供依据。最后以长航时太阳能无人机的总体设计为例,对任务需求—工程特性—技术指标的两级质量屋模型进行计算分析,得到续航能力、巡航高度、动力系统效率、巡航速度和气动效率是太阳能无人机最重要的5个技术指标的结果。此方法客观性较强,可处理复杂的系统不确定性,为太阳能无人机总体方案设计及决策应用提供参考依据。 相似文献
98.
以降低涡扇发动机排气系统红外辐射为目的,针对某型涡扇排气系统构建1/3缩比模型,采用实验的方法比较了中心锥有/无冷却的排气系统喷流温度场和红外辐射场,验证了中心锥冷却结构能够大幅度降低涡扇发动机排气系统尾向红外辐射强度.研究结果表明:中心锥表面在外涵气体冷却下温度降低,同时尾焰核心温度也降低.当涵道比为0.3时,在0°~10°范围内,气膜冷却中心锥体排气系统红外辐射降低24%~32%;在20°~90°范围内,红外辐射强度降低0.8%~2.1%.当涵道比增加到0.8时,0°方向的红外辐射强度降低60%;20°~90°范围内的红外辐射强度降低了33%~51%. 相似文献
99.
Almost all theoretical and numerical models for the modulation of cosmic ray in the heliosphere are based on Parker's transport equation which contains all the important basic physical processes. The relative importance of the various mechanisms is however not established and may vary significantly over 22 years. The simultaneous measurements of solar wind parameters, heliospheric magnetic field properties and cosmic rays over a wide range of energies and positions in the heliosphere have brought the realization that modulation is much more complicated than what the original drift models predicted. In the process the sophistication of models based on solving Parker's equation has increased by orders of magnitude. A short review of the global modulation of cosmic rays is given from a theoretical and modelling point of view. 相似文献
100.
针对氢氧火箭发动机羽烟紫外辐射特性参数分析,提出一种基于紫外CCD(change coupled device)相机采集的单幅辐射图像,同时反演羽烟内紫外辐射源项和吸收系数的方法.该方法将羽烟简化为发射-吸收轴对称介质,通过对辐射图像数据进行Able变换得到三维介质内辐射强度分布,利用最小二乘法将反演问题转化为使计算得到的与Abel变换得到的辐射强度误差最小的最优化问题,然后利用共轭梯度法求解该最优化问题.通过在求解正问题得到的准确值的基础上添加随机噪声,模拟辐射图像数据,分析了测量误差对算法反演精度的影响.结果表明:该算法对测量误差不敏感,能够准确的重建羽烟内的辐射源项和吸收系数分布. 相似文献