首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   3390篇
  免费   47篇
  国内免费   11篇
航空   1283篇
航天技术   1089篇
综合类   37篇
航天   1039篇
  2022年   19篇
  2021年   52篇
  2019年   23篇
  2018年   135篇
  2017年   112篇
  2016年   123篇
  2015年   50篇
  2014年   119篇
  2013年   140篇
  2012年   124篇
  2011年   177篇
  2010年   136篇
  2009年   198篇
  2008年   197篇
  2007年   123篇
  2006年   80篇
  2005年   106篇
  2004年   103篇
  2003年   124篇
  2002年   98篇
  2001年   120篇
  2000年   42篇
  1999年   63篇
  1998年   62篇
  1997年   42篇
  1996年   44篇
  1995年   81篇
  1994年   63篇
  1993年   35篇
  1992年   47篇
  1991年   10篇
  1990年   19篇
  1989年   42篇
  1988年   11篇
  1987年   17篇
  1986年   16篇
  1985年   72篇
  1984年   57篇
  1983年   51篇
  1982年   45篇
  1981年   86篇
  1980年   25篇
  1979年   16篇
  1978年   14篇
  1977年   17篇
  1976年   14篇
  1975年   13篇
  1974年   12篇
  1972年   13篇
  1971年   11篇
排序方式: 共有3448条查询结果,搜索用时 0 毫秒
901.
Aerosol size distributions were retrieved by computing aerosol extinction parameters using extensive measurements of direct solar radiation made in the 0.4 and 0.6 μm wavelengths at Pune with Volz type sunphotometer during winter (November–February), pre-monsoon (March–May), monsoon (June–August) and post-monsoon (September–October) of 1980–1981. The computer aerosol size distributions are compared with the direct measurements made using Anderson eight-stage cascade impactor. There is agreement between the retrieved and measured size distributions. The retrieval method is simple and useful for intensive aerosol measurement programmes.  相似文献   
902.
This paper deals with the principal methods of achieving high-time resolution measurements for the study of fine structure of shocks and other discontinuities in space plasmas. In the measurements of ion energy spectra, we have obtained the time resolution about 1s.In the Soviet-Czechoslovak INTERSHOCK project we will obtain temporal resolution better than 0.1s in the measurement of the main plasma parameters. This will be obtained with the multichannel energy spectrometer and the on-board data acquisition and processing system triggered by the shock signature. This system controls the data sampling rate from some scientific instruments and switches on a high-sampling rate near the shock. The method implies detecting a shock by means of on-board processing of magnetic field and plasma parameters. The algorithm for this detection uses both parameters separately as well as in combinations.  相似文献   
903.
突发通信信号的降维检测方法及带宽参数分析   总被引:1,自引:0,他引:1  
胡亚  吴嗣亮 《宇航学报》2012,33(9):1295-1300
在突发通信信号检测中,在频率、带宽进行二维搜索的检测方法计算量大,提出了可减少计算量的降维检测方法,该方法在单一检测带宽下进行频率搜索检测突发通信信号。对其带宽参数选择进行了分析。理论计算和仿真表明,降维检测器用于单一速率信号检测时,当检测带宽与信号带宽一致时具有与二维检测器相同的检测性能,当检测带宽与信号带宽相差一倍时,信噪比损失2dB左右;用于混合速率突发信号检测时,最佳带宽与速率的概率分布、信噪比等多种因素有关;对发送功率不变的各速率均匀分布的混合速率突发信号,检测带宽匹配于最大信号带宽可在较高信噪比时获得最高的平均检测概率。这些分析为降维检测器的带宽参数选择提供了依据。  相似文献   
904.
Results of the analysis of 327 sessions of radio occultation on satellite-to-satellite paths are presented. The data are taken in the nighttime polar ionosphere in the regions with latitudes of 67°–88°, and in the period of high solar activity from October 26, 2003 to November 9, 2003. Typical ionospheric changes in the amplitude and phase of decimeter radio waves on paths GPS satellites-CHAMP satellite are presented. It is demonstrated that these data make it possible to determine characteristics of the sporadic E s structures in the lower ionosphere at heights of 75–120 km. Histograms of distribution of the lower and upper boundaries, thickness, and intensity of the E s structures are presented. Dispersion and spectra of amplitude fluctuations of decimeter radio waves caused by small-scale irregularity of the ionospheric plasma are analyzed. The relation of the polar E s structures and intensity of small-scale plasma irregularity to various manifestations of solar activity is discussed. The efficiency of monitoring the ionospheric disturbances caused by shock waves of the solar wind by the radio occultation method on satellite-to-satellite paths is demonstrated.  相似文献   
905.
In order to reveal the biological significance of gravity, microgravity effects have been studied at the cellular, organism and population levels. The following questions arise. Do any gravity-dependent processes exist in a cell? Is cell adaptation to weightlessness possible; if so, what role may cytoskeleton, the genetic apparatus play in it? What are the consequences of the lack of convection in weightlessness for the performance of morphogenesis? Do the integral characteristics of living beings change in weightlessness? Is there any change in "biological capacity" of space, its resistance to expansion of life? What are the direction and intensity of microgravity action as a factor of natural selection, the driving force of evolution? These problems are discussed from a theoretical point of view, and in the light of results obtained in experiments from aboard biosatellites "Cosmos".  相似文献   
906.
The Soyuz 22 space cabin atmosphere was studied for volatile organic trace contaminants. By gas chromatography the following constituents were identified: methane, ethane, heptane, methanol, ethanol, n-propanol, acetaldehyde, acetone, ethyl benzene. Except for acetone, concentrations of the above compounds were close to the values determined in the mock-up experiments.  相似文献   
907.
    
The hypersonic hyperalfvèn plasma flow around electroconductive bodies is considered and electromagnetic inductive plasma-body interaction is analyzed. The possible applications of results obtained in this analysis to body motion in ionosphere and interplanetary plasma are discussed.  相似文献   
908.
    
Since 1988 high sensitivity dosimeter-radiometer “Liulin” has been installed on board the MIR space station. Device measured absorbed dose rate and flux of penetrating particles. Results of measurements showed that after powerful solar proton events (SPE) September–October, 1989 and March, 1991 additional quasistable radiation belts were formed in the near earth space within the interval L=1.8−3.0. These “new” belts were observed as an additional maximums in flux (and sometimes dose) channels when crossing the SAA region. “New” belts were quasi stable and existed at least several months, decaying slightly after SPE. Dose to flux ratio analysis showed that major components of these belts were energetic electrons and protons arising in connection with preceding SPEs.  相似文献   
909.
This paper studies the dynamic loads of bevel gears with circular and straight teeth with the overlap factors less than two (εα < 2) and more than two (εα > 2). The advantages of the gears with straight teeth with εα > 2 are shown.  相似文献   
910.
A joint team of researchers under the auspices of the Center for Space Debris Information Collection, Processing and Analysis of the Russian Academy of Sciences collaborates with 15 observatories around the world to perform observations of space debris. For this purpose, 14 telescopes were equipped with charge-coupled device (CCD) cameras, Global Positioning System (GPS) receivers, CCD frame processing and ephemeris computation software, with the support of the European and Russian grants. Many of the observation campaigns were carried out in collaboration with the Astronomical Institute of the University of Bern (AIUB) team operating at the Zimmerwald observatory and conducting research for the European Space Agency (ESA), using the Tenerife/Teide telescope for searching and tracking of unknown objects in the geostationary region (GEO). More than 130,000 measurements of space objects along a GEO arc of 340.9°, collected and processed at Space Debris Data Base in the Ballistic Center of the Keldysh Institute of Applied Mathematics (KIAM) in 2005–2006, allowed us to find 288 GEO objects that are absent in the public orbital databases and to determine their orbital elements. Methods of discovering and tracking small space debris fragments at high orbits were developed and tested. About 40 of 150 detected unknown objects of magnitudes 15–20.5 were tracked during many months. A series of dedicated 22-cm telescopes with large field of view for GEO survey tasks is in process of construction. 7 60-cm telescopes will be modernized in 2007.  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号