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31.
利用远程系统浏览技术,研究并实现了一种基于Reliance的高可靠航电文件系统的远程浏览系统。系统采用客户端/服务器架构,通过在综合化航电系统内核中建立一个嵌入式文件服务器,可使得用户通过集成在E—clipseIDE中的远程文件浏览器客户端,对此文件系统进行访问、浏览和管理。系统能够有效地提高远程文件操作的可视性和透明性,功能丰富,操作简便,可移植性好,易于扩展。 相似文献
32.
酚醛树脂固化度的X射线衍射分析 总被引:1,自引:0,他引:1
发展使用X射线衍技术对酚醛树脂固化度进行研究,确定了酚醛树脂固化度与X射线散射最大值的 关系,得出了利用2θ角来标定树脂固化度的公式。该方法具有快速、无损、灵敏度主同的优点,并可适用于各种不同的酚醛树脂。 相似文献
33.
Sergio Fabiani Enrico CostaRonaldo Bellazzini Alessandro BrezSergio Di Cosimo Francesco LazzarottoFabio Muleri Alda RubiniPaolo Soffitta Gloria Spandre 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012,49(1):143-149
The Sun is the nearest astrophysical source with a very intense emission in the X-ray band. The study of energetic events, such as solar flares, can help us to understand the behaviour of the magnetic field of our star. There are in the literature numerous studies published about polarization predictions, for a wide range of solar flares models involving the emission from thermal and/or non-thermal processes, but observations in the X-ray band have never been exhaustive.The gas pixel detector (GPD) was designed to achieve X-ray polarimetric measurements as well as X-ray images for far astrophysical sources. Here we present the possibility to employ this instrument for the observation of our Sun in the X-ray band. 相似文献
34.
J.S. Kaastra R. Lieu T. Tamura F.B.S. Paerels J.W. den Herder 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2504-2508
We discuss the detection of soft excess X-ray emission in a sample of 19 clusters of galaxies observed by XMM-Newton. In 6/19 clusters evidence for a soft X-ray excess is found. Four of these clusters show soft X-ray and O VII line emission from gas with a temperature of 0.2 keV. The centroid of this oxygen line is consistent with the redshift of the cluster. The intensity and spatial extend of the soft excess agrees with previous PSPC measurements. These observations are interpreted as emission from warm-hot intergalactic medium filaments, with density enhancements near the cluster centers, consistent with theoretical predictions. In the other two soft excess clusters a non-thermal origin is consistent with the data. 相似文献
35.
S.G. Anokhin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
We present here new XMM-Newton observations of 3 relatively cool clusters at z ≈ 0.4, complemented by archival observations of 3 other clusters at similar redshift. We derived the M–T and R–T relations from the hydrostatic equation using an isothermal temperature distribution. 相似文献
36.
F. Bocchino R. Bandiera Y. Gallant 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(3):407-410
The investigation of the general properties of non-thermal (NT) X-ray shell supernova remnants (SNRs), of which SN 1006 is the prototype, is important to understand how electrons are accelerated in SNR shocks and what is the origin of cosmic rays. Using the XMM-Newton satellite, we are carrying on a survey of putative non-thermal SNR candidates previously unknown or little studied in the X-ray band, in order to investigate the different manifestations of NT emission in SNR shells. The SNRs we have selected are likely to expand in a low density medium, and therefore to have a low thermal X-ray emission, that usually outshines the non-thermal one. We report here preliminary results obtained on the SNR shell DA 530. 相似文献
37.
A.A. Hady 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The space science research has been started in Egypt since 1910 by measuring the solar constant as indication of solar radiation at Helwan Observatory. The solar sunspot studies and its influence on the Nile flooding was erected and operated at Helwan as a first solar station in Egypt during 1957. Zeiss-Coude’ refractor was installed in 1964. Astronomy and space science educations started in Egypt at the university level since 1936 at Department of Astronomy and Meteorology of Cairo University. Undergraduate and graduate education in Egypt will be discussed in this work. 相似文献
38.
39.
用高分辨的三晶体x—射线衍射仪测量了Zr、Cu金属交替的多层膜的x—射线小角反射谱。用扩展了的Born—wolf光学模型对Zr、Cu多层膜的x—射线小角反射数据进行了定量分析。结果表明,该金属多层膜在其生长方向具有超晶格结构。在两层金属膜之间的界面上,由于内扩散,形成了界面交混层,它使x—射线小角反射所产生的高阶Bragg峰的强度减弱。由于两种金属膜的晶格不匹配,使高阶Bragg峰加宽。界面的粗糙度可用来模拟x—射线小角反射曲线的阻尼振荡效应。 相似文献
40.
受快速傅里叶变换(fast Fourier transform,FFT)的影响,基于FFT和压缩感知(compressive sensing, CS)的脉冲星周期快速估计算法的计算量大。为进一步减小计算量并提高计算精度,利用离散余弦变换(discrete cosine transform,DCT)取代FFT,提出了一种基于DCT-CS的脉冲星周期超快速估计算法。在该方法中,利用DCT提取脉冲星信号的低频部分构建低频DCT矩阵;构建畸变轮廓字典并获取累积轮廓;提出了利用最大值超分辨率稀疏恢复估计脉冲星周期的方法。仿真结果表明,DCT-CS的脉冲星周期估计精度达到了3.82×10-12 s,计算时间达到了9.31 ms。与FFT-CS相比,周期估计精度提高了约16%,计算时间缩短了约37.5%,实现了实时高精度的脉冲星周期估计。 相似文献