全文获取类型
收费全文 | 617篇 |
免费 | 87篇 |
国内免费 | 127篇 |
专业分类
航空 | 401篇 |
航天技术 | 273篇 |
综合类 | 61篇 |
航天 | 96篇 |
出版年
2024年 | 1篇 |
2023年 | 9篇 |
2022年 | 19篇 |
2021年 | 32篇 |
2020年 | 31篇 |
2019年 | 27篇 |
2018年 | 33篇 |
2017年 | 24篇 |
2016年 | 37篇 |
2015年 | 24篇 |
2014年 | 44篇 |
2013年 | 56篇 |
2012年 | 51篇 |
2011年 | 52篇 |
2010年 | 57篇 |
2009年 | 47篇 |
2008年 | 50篇 |
2007年 | 37篇 |
2006年 | 45篇 |
2005年 | 25篇 |
2004年 | 20篇 |
2003年 | 16篇 |
2002年 | 11篇 |
2001年 | 8篇 |
2000年 | 4篇 |
1999年 | 9篇 |
1998年 | 6篇 |
1997年 | 4篇 |
1996年 | 5篇 |
1995年 | 14篇 |
1994年 | 3篇 |
1993年 | 10篇 |
1992年 | 3篇 |
1991年 | 3篇 |
1990年 | 6篇 |
1989年 | 2篇 |
1988年 | 4篇 |
1984年 | 2篇 |
排序方式: 共有831条查询结果,搜索用时 31 毫秒
161.
162.
火星大气层的主要成分为二氧化碳,如果能够利用低温等离子体方法高效分解二氧化碳,使其转化为氧气和一氧化碳加以利用,可以大幅降低航天员生命保障相关载荷长途运输的成本,进一步提高生命保障能力.低温等离子体放电过程中会产生大量活性组分,可以在数百度温度下实现二氧化碳的高效解离,是具有很大潜力的二氧化碳解离与转化方式.设计了一种... 相似文献
163.
直流电弧等离子体炬内部物理过程复杂且具动态性,较难对其进行准确描述与深入研究,且其工作温度较高,其状态参数难以使用常规方式测量。针对直流电弧等离子体炬,建立流动、传热和电磁相互耦合的数值模型,基于Fluent软件对直流电弧等离子体炬进行三维数值模拟和特性分析,设计并搭建了一套热焓探针实验系统,完成对直流电弧等离子体炬射流参数的测量分析。结果表明:建立的数值模型模拟结果与实验测量结果吻合较好,误差在10%以内;炬内温度与速度最大值与工作气流量呈正相关,均出现在靠近阴极区域,且沿轴线逐渐降低;等离子体炬内高温区与高电流密度区重合。 相似文献
164.
165.
L.N. Sidorova S.V. Filippov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(6):1412-1424
In this paper we consider an idea of the troposphere tide influence on the character of the longitudinal variations in the distribution of the equatorial plasma bubbles (EPBs) observed in the topside ionosphere. For this purpose, the obtained EPB longitudinal patterns were compared with the thermosphere and ionosphere characteristics having the prominent “wave-like” longitudinal structures with wave number 4, which are uniquely associated with the influence of the troposphere DE3 tides. The characteristics of the equatorial mass density anomaly (EMA), equatorial ionization anomaly (EIA), zonal wind and pre-reversal E?×?B drift enhancement (PRE) were used for comparison. The equinox seasons during high solar activity were under consideration. It was obtained that the longitudinal patterns of the EMA and zonal wind show the surprising similarity with the EPB distributions (R???0.8, R???0.72). On the other hand, the resemblance with the ionosphere characteristics (EIA, PRE) is rather faint (R???0.37, R???0.12). It was shown that the thermosphere zonal winds are the most possible transfer mediator of the troposphere DE3 tide influence. The most successful moment for the transfer of the troposphere DE3 tide energy takes place in the beginning of the EPB production, namely, during the seed perturbation development. 相似文献
166.
为了探寻入口边界层厚度变化对高马赫数进气道自起动性能的影响,对简化的二元高马赫数进气道的加速自起动过程进行数值仿真研究,分析了边界层厚度对自起动过程中流场波系结构变化和自起动性能的影响机制,获得了不同边界层厚度下的进气道自起动性能及主分离包高度的变化规律。结果表明:随着边界层相对厚度从0.05增加至0.3,进气道的自起动马赫数一开始保持不变,然后快速增大;相同主流条件下,不起动流场跨越主分离包无量纲压升和主分离包高度随边界层相对厚度的增大均变小;边界层动量损失厚度和跨越主分离包无量纲压升对进气道起动性能影响重大。 相似文献
167.
Ebenezer Agyei-Yeboah Paulo Roberto Fagundes Alexandre Tardelli Valdir Gil Pillat Alessio Pignalberi Venkatesh Kavutarapu Michael Pezzopane Francisco Vieira 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(8):2416-2438
This investigation uses simultaneous observations from all-sky imager system and an ionosonde collocated at Araguatins (5.65° S, 48.07° W and dip-latitude of 4.17° S), a near-equatorial region in Brazil. These simultaneous observations were used to investigate the occurrence of plasma bubbles and blobs in the field of the imaging system and their association with atypical range Spread-F signature in ionograms. Also, in-situ observation of plasma density from Swarm satellites were used to support the ground-based observations. Using a few cases, a methodology will be established to identify in the plasma blobs (atypical ESF) in the ionograms when there is the simultaneous observation of plasma bubbles and blobs in the field of view of the ionosonde. For this purpose, simultaneous sequence of OI 630.0 nm nightglow images and ionograms are presented for different case studies; 1. when there is the absence of a plasma bubble or blob, 2. when there is only the occurrence of plasma bubbles and 3. when there is the occurrence of plasma bubbles and blobs, in order to compare traces in the ionogram in all these case studies. With these we can cover all kinds of signatures in the ionograms corresponding to no irregularities, plasma bubbles only and plasma bubbles-blobs. These OI 630.0 nm nightglow and ionograms recorded simultaneously make it possible to establish a novel methodology to recognize in ionograms cases when there is the occurrence of Spread-F signature associated with bubble-blob in the FOV of the ionosonde. 相似文献
168.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(6):1607-1614
In this paper, we extend the stability analysis of cold sharp shear flows to warm astrophysical cases with, inevitable, gradual velocity gradient in the interface region in the presence of viscosity effect. Using linear perturbation theory as well as the local approximation method, the instability growth rate of the excited electromagnetic modes has been investigated for the relativistic and non-relativistic cases of solar wind interacting with interstellar plasma medium. Results show that astrophysical shear systems with a small velocity gradient in the transition region are more stable rather than larger ones. Moreover, dependent on the viscosity coefficient value, the viscosity effects could have a positive role on the instability growth rate of the system in some range of initial bulk velocity, while it plays a destructive role in other velocity ranges. 相似文献
169.
Alam E. Kherani Matheus Mascarenhas Eurico R. De Paula Jose H. A. Sobral Fernando Bertoni 《Space Science Reviews》2005,121(1-4):253-269
We present a three-dimensional simulation of collisional-interchange-instability in the equatorial-low-latitude F region of
ionosphere. The instability is responsible for the generation of large plasma density depletion or bubble. General 3D potential
and continuity equations are derived to simulate the phenomena. To understand the linear aspect of the instability, the general
3D linear growth rate is derived using 3D potential equation. The linear growth characteristics are compared with earlier
field-aligned-integrated growth analyses. The numerical simulation of bubble in the 3D spherical polar geometry is finally
presented. Distinct evolution characteristics of bubble in 3D and 2D simulation are further discussed. 相似文献
170.
彩色氦气泡流动显示是一极好的新技术。在风洞中应用彩色氦气泡进行流动显示已于1984年3月在哈尔滨空气动力研究所实现了,获得了丰富多采的彩色迹线,摄制了清晰的彩色录象和彩色照片。不久之后,进行了轿车、面包车、高楼、船舵、鱼鳞波表面、细长体、圆柱体、降落伞和各种飞机模型的试验。 本文描述了彩色氦气泡流动显示技术,介绍了在风洞中进行流动显示的一般装置、基本原理和应用。 相似文献