全文获取类型
收费全文 | 811篇 |
免费 | 46篇 |
国内免费 | 30篇 |
专业分类
航空 | 354篇 |
航天技术 | 389篇 |
综合类 | 32篇 |
航天 | 112篇 |
出版年
2024年 | 1篇 |
2023年 | 28篇 |
2022年 | 3篇 |
2021年 | 11篇 |
2020年 | 20篇 |
2019年 | 18篇 |
2018年 | 20篇 |
2017年 | 8篇 |
2016年 | 9篇 |
2015年 | 5篇 |
2014年 | 57篇 |
2013年 | 27篇 |
2012年 | 26篇 |
2011年 | 35篇 |
2010年 | 27篇 |
2009年 | 43篇 |
2008年 | 70篇 |
2007年 | 69篇 |
2006年 | 48篇 |
2005年 | 35篇 |
2004年 | 15篇 |
2003年 | 22篇 |
2002年 | 13篇 |
2001年 | 46篇 |
2000年 | 17篇 |
1999年 | 19篇 |
1998年 | 27篇 |
1997年 | 4篇 |
1996年 | 20篇 |
1995年 | 17篇 |
1994年 | 88篇 |
1993年 | 20篇 |
1992年 | 4篇 |
1991年 | 4篇 |
1990年 | 4篇 |
1989年 | 2篇 |
1984年 | 5篇 |
排序方式: 共有887条查询结果,搜索用时 93 毫秒
231.
Ion-induced nucleation has been suggested to be a potentially important mechanism for atmospheric aerosol formation. Ions
are formed in the background atmosphere by galactic cosmic rays. A possible connection between galactic cosmic rays and cloudiness
has been However, the predictions of current atmospheric nucleation models are highly uncertain because the models are usually
based on the liquid drop model that estimates cluster thermodynamics based on bulk properties (e.g., liquid drop density and
surface tension). Sulfuric acid (H2SO4) and water are assumed to be the most important nucleating agents in the free troposphere. Measurements of the molecular
thermodynamics for the growth and evaporation of cluster ions containing H2SO4 and H2O were performed using a temperature-controlled laminar flow reactor coupled to a linear quadrupole mass spectrometer as well
as a temperature-controlled ion trap mass spectrometer. The measurements were complemented by quantum chemical calculations
of the cluster ion structures. The analysis yielded a complete set of H2SO4 and H2O binding thermodynamics extending from molecular cluster ions to the bulk, based on experimental thermodynamics for the small
clusters. The data were incorporated into a kinetic aerosol model to yield quantitative predictions of the rate of ion-induced
nucleation for atmospheric conditions. The model predicts that the negative ion-H2SO4-H2O nucleation mechanism is an efficient source of new particles in the middle and upper troposphere. 相似文献
232.
233.
A. Grimberg D. S. Burnett P. Bochsler H. Baur R. Wieler 《Space Science Reviews》2007,130(1-4):293-300
We discuss data of light noble gases from the solar wind implanted into a metallic glass target flown on the Genesis mission.
Helium and neon isotopic compositions of the bulk solar wind trapped in this target during 887 days of exposure to the solar
wind do not deviate significantly from the values in foils of the Apollo Solar Wind Composition experiments, which have been
exposed for hours to days. In general, the depth profile of the Ne isotopic composition is similar to those often found in
lunar soils, and essentially very well reproduced by ion-implantation modelling, adopting the measured velocity distribution
of solar particles during the Genesis exposure and assuming a uniform isotopic composition of solar wind neon. The results
confirm that contributions from high-energy particles to the solar wind fluence are negligible, which is consistent with in-situ
observations. This makes the enigmatic “SEP-Ne” component, apparently present in lunar grains at relatively large depth, obsolete.
20Ne/ 22Ne ratios in gas trapped very near the metallic glass surface are up to 10% higher than predicted by ion implantation simulations.
We attribute this superficially trapped gas to very low-speed, current-sheet-related solar wind, which has been fractionated
in the corona due to inefficient Coulomb drag. 相似文献
234.
杨俊清 《西安航空技术高等专科学校学报》2006,24(1):29-31
在细分曲面造型中,对Doo-Sabin曲面为代表的细分曲面的研究,已成为近几年来图形学领域最重要的研究课题,但已有文献在细分算法的实现方面缺乏具体操作过程,不便于工程应用。本文分析了Doo-Sabin细分算法的数据结构特点,研究了细分算法的具体实现过程,对连接规律进行了总结,实现了Doo-Sabin细分算法的二次曲面细分,为各种相关文献缺乏具体操作过程作了补充。 相似文献
235.
黄杰 《中国民航学院学报》1996,(6):65-67
利用递归函数显式化的一种新方法,给出了Akermann函数显式表示法,从而确定Akermann函数算法的时间复杂度为2幂函数级. 相似文献
236.
G. M. Mason 《Space Science Reviews》2007,130(1-4):231-242
3He-rich solar energetic particle (SEP) events show huge enrichments of 3He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution
instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these
events: the particle energy spectra are found to be either power-law or curved in shape, with the 3He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely
present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near
∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been
identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection
sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the
new insights found in the last few years. 相似文献
237.
We present the observational results on chromospheric spicules obtained at the Sayan observatory 50 cm coronograph. To investigate the evolution of chromospheric spicules, we analysed spicule spectra of strong chromospheric lines measured simultaneously at three altitudes above the solar limb during 5–60 min with a time resolution of 10 to 20 s. The spatial resolution was better than 1, and the spectral resolution was 0.03Å in 6563Å. The appearance of a spicule at a given altitude is preceded by an sharp increase in line-of-sight velocity and/or in line half-width at a lower level. Generally, the evolution has a non-monotonous impulsive character. Changes of line-of-sight velocities and other parameters of the line profile can be represented as the superposition of slow, evolutionary changes and fluctuations with periods of about 80 to 120 s. The amplitude of line-of-sight velocity fluctuations is 2–3 km/sec and tends to increase with height. By studying the phase delays of the fluctuations at different heights, we found that the propagation velocity exceeds 300 km s–1, and that the disturbances do not necessarily propagate upwards. 相似文献
238.
G. Trottet 《Space Science Reviews》1994,68(1-4):149-158
Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario. 相似文献
239.
W. M. Glencross 《Space Science Reviews》1994,68(1-4):87-92
Studies of sporadic outbursts, ranging from flares to nano-flares, invariably endow the solar corona with steady plasma conditions, prior to seeking a current-flow (or the associated magnetic structure) which induces instability. Such an approach does not incorporate a crucial feature of the natural configuration, namely, that the material is of chromospheric origin, and only resides at coronal altitudes for as long as it can acquire adequate energy. There is clearly a feedback loop involved, which allows plasma to moderate the transfer of energy from the field while making use of this heat to permeate coronal altitudes. An examination of the whole procedure is necessary if the location and threshold-conditions for the energy-conversion mechanism are to be identified.A critical step in the feedback procedure mentioned involves the supply line which links the corona to the chromosphere. Because the solar atmosphere has such large vertical dimensions, even a modest change in average temperature and/or density can place heavy demands on this artery: the problem is that a conventional conduction-dominated transition layer cannot readily accommodate a rapid increase in current-density or plasma-flow. (Restructuring of the temperature gradient, to provide the carriers with extra heat, is a very slow process.) A transition layer of this type is unable to endure for long at the base of a sporadically-heated atmosphere in any case, since it becomes the target for plasma falling in the gravitational field during each intermediate cooling phase. As a result, the gap between the chromosphere and corona is more abrupt than is usually considered, endowing the region with thermo-electric characteristics which allow energy to be extracted when modest current-densities arise. Energy-conversion at this region fulfills two rôles: it supplies at least part of the heat required by the overlying corona, and maintains contact between the chromosphere and corona via non-thermal transport processes. 相似文献
240.
车敦仁 《北京航空航天大学学报》1994,20(2):179-187
IDB(智能数据库)思想的提出,预示着人类的信息处理即将步入一个崭新的时代.IDB将计算机科学中近年来日趋发展成熟的五大主要技术,ΟΟ(面向对象)技术、DB(数据库)技术、AI(人工智能)、Hypertext/Hypermedia(超文本/超媒体)和正文数据库与联机信息检索技术,集成为一体.其中ΟΟ、AI和DB是IDB中的三大支柱技术.本文论述MIDS/BUAA数据模型(Datamodeling)的哲学,并介绍MIDS/BUAA系统的设计思想、动机、核心数据模型,系统的功能构成和它的Client/Server体系结构. 相似文献