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   2387篇
  免费   531篇
  国内免费   405篇
航空   2204篇
航天技术   435篇
综合类   246篇
航天   438篇
  2023年   53篇
  2022年   78篇
  2021年   120篇
  2020年   91篇
  2019年   82篇
  2018年   72篇
  2017年   137篇
  2016年   157篇
  2015年   108篇
  2014年   151篇
  2013年   113篇
  2012年   182篇
  2011年   203篇
  2010年   135篇
  2009年   208篇
  2008年   191篇
  2007年   179篇
  2006年   190篇
  2005年   119篇
  2004年   101篇
  2003年   92篇
  2002年   64篇
  2001年   60篇
  2000年   64篇
  1999年   51篇
  1998年   62篇
  1997年   56篇
  1996年   29篇
  1995年   30篇
  1994年   26篇
  1993年   33篇
  1992年   14篇
  1991年   25篇
  1990年   19篇
  1989年   14篇
  1988年   7篇
  1987年   4篇
  1986年   1篇
  1984年   1篇
  1981年   1篇
排序方式: 共有3323条查询结果,搜索用时 15 毫秒
1.
In our study we analyze and compare the response and behavior of the ionospheric F2 and of the sporadic E-layer during three strong (i.e., Dst?<??100nT) individual geomagnetic storms from years 2012, 2013 and 2015, winter time period. The data was provided by the state-of the art digital ionosonde of the Széchenyi István Geophysical Observatory located at midlatitude, Nagycenk, Hungary (IAGA code: NCK, geomagnetic latitude: 46.17° geomagnetic longitude: 98.85°). The local time of the sudden commencement (SC) was used to characterize the type of the ionospheric storm (after Mendillo and Narvaez, 2010). This way two regular positive phase (RPP) ionospheric storms and one no-positive phase (NPP) storm have been analyzed. In all three cases a significant increase in electron density of the foF2 layer can be observed at dawn/early morning (around 6:00 UT, 07:00 LT). Also we can observe the fade-out of the ionospheric layers at night during the geomagnetically disturbed time periods. Our results suggest that the fade-out effect is not connected to the occurrence of the sporadic E-layers.  相似文献   
2.
    
在众多光阳极材料中,纳米结构材料α-Fe2O3由于其光吸收显著、化学稳定性好、储量丰富等优势,被认为是最有前途的材料之一。利用水热法制备了具有良好光解水性能的Co和P掺杂α-Fe2O3纳米材料。经过掺杂后α-Fe2O3纳米材料仍为纳米棒状形貌,纳米棒的粒径增加。实验发现,Co掺杂α-Fe2O3制成的电极在标准光照射下的最大光生电流密度为0.453 mA/cm2,是未掺杂样品的20.6倍,P掺杂α-Fe2O3制成的电极在标准光照射下的最大光生电流密度为0.276 mA/cm2,是未掺杂样品的12.5倍,具备了高效光解水性能。同时通过SEM、TEM、XRD、UV-Vis和Mott-Schottky测试等方法,结合形貌与结构表征,研究了α-Fe2O3的光电化学分解水性能影响机理。  相似文献   
3.
In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.  相似文献   
4.
以Gd2O3和正硅酸乙酯(TEOS)为原材料,采用并流化学共沉淀法合成Gd2SiO5粉体材料。研究Gd2SiO5前驱体的热响应特征、Gd2SiO5粉体的物相组成和微观形貌,并对Gd2SiO5粉体的合成机理进行初步探讨。结果表明:前驱体的低Gd/Si摩尔比和反应体系的高pH值会导致Gd2SiO5粉体生成Gd9.33(SiO4)6O2杂质相,相反则会导致生成Gd2O3杂质相。当Gd/Si摩尔比为20∶11、pH值为9~10、合成温度为1000~1300℃时,合成的粉体纯度较高,Gd2SiO5颗粒呈不规则形貌特征,平均粒度为100~200 nm。Gd2SiO5合成过程中,前驱体以一种—[Si—O—Gd]—网络结构存在,在煅烧过程中逐渐转化为Gd2SiO5晶体以及Gd9.33(SiO4)6O2和Gd2O3杂相。  相似文献   
5.
The comparison of the IRI model with the foF2 distribution in the equatorial anomaly region obtained by topside sounding onboard the Interkosmos-19 satellite has been carried out. The global distribution of foF2 in terms of LT-maps was constructed by averaging Intercosmos-19 data for summer, winter, and equinox. These maps, in fact, represent an empirical model of the equatorial anomaly for high solar activity F10.7 ~ 200. The comparison is carried out for the latitudinal foF2 profiles in the characteristic longitudinal sectors of 30, 90, 210, 270, and 330°, as well as for the longitudinal variations in foF2 over the equator. The largest difference between the models (up to 60%) for any season was found in the Pacific longitudinal sector of 210°, where there are a few ground-based sounding stations. Considerable discrepancies, however, are sometimes observed in the longitudinal sectors, where there are many ground-based stations, for example, in the European or Indian sector. The discrepancies reach their maximum at 00 LT, since a decay of the equatorial anomaly begins before midnight in the IRI model and after midnight according to the Interkosmos-19 data. The discrepancies are also large in the morning at 06 LT, since in the IRI model, the foF2 growth begins long before sunrise. In the longitudinal variations in foF2 over the equator at noon, according to the satellite data, four harmonics are distinguished in the June solstice and at the equinox, and three harmonics in the December solstice, while in the IRI model only two and one harmonics respectively are revealed. In diurnal variations in foF2 and, accordingly, in the equatorial anomaly intensity, the IRI model does not adequately reproduce even the main, evening extremum.  相似文献   
6.
沈高峰  王振军  刘丰华  张映锋  蔡长春  徐志锋  余欢 《航空学报》2021,42(12):424816-424816
针对新型的叠层穿刺碳纤维织物增强铝基复合材料(CF/Al复合材料),通过细观力学数值模拟与实验结合的方法研究了其在准静态拉伸载荷作用下的渐进损伤与断裂力学行为。复合材料经向拉伸弹性模量、极限强度与断裂应变的实验结果分别为129.61 GPa、630.14 MPa和0.75%,细观力学模型预测误差分别为-9.41%、7.57%和1.33%,均匀化计算的宏观应力-应变曲线与实验曲线总体上相符。经向拉伸变形初期首先出现经/纬纱交织处基体合金的局部损伤,随着拉伸应变量的增大依次发生纬纱和穿刺纱的横向开裂,拉伸变形后期基体合金与经纱失效引起宏观应力-应变曲线的急剧下降,复合材料拉伸断口表现为经纱轴向断裂及纬纱和穿刺纱横向开裂共存的形貌特征,纤维拔出和基体断裂导致的经纱轴向断裂是诱发复合材料最终失效的主要机制。  相似文献   
7.
王维彬  巩岩博 《推进技术》2021,42(7):1458-1465
系统性地回顾了长征五号运载火箭芯一级50t级氢氧火箭发动机YF-77的设计与研制历程。通过分析氢氧发动机的特点以及国内外氢氧发动机的发展现状,阐述了国内新一代运载火箭研发的技术路线和50t级氢氧火箭发动机的研制背景;对50t级氢氧火箭发动机的总体技术方案及其特点进行了分析与总结,并在此基础上对发动机主要组件的技术方案及其特点开展分析;对发动机热试车情况、可靠性验证情况和故障排除情况进行了分析;对50t级氢氧火箭发动机的研制情况、技术特点进行了总结,并对国内氢氧发动机和液氧/甲烷发动机的发展进行了展望。  相似文献   
8.
典型近α型钛合金Ti6242合金制备盘锻件的综合力学性能与其棒材原始微观组织特征密切相关。本研究选取具有明显微观组织特征差别的3种Ti6242钛合金棒材为研究对象,定量化评估不同Ti6242钛合金棒材锻造态、固溶态和固溶+时效态的微观组织差别和演变规律,并讨论棒材微观组织差别和演变对综合力学性能的影响。研究结果显示具有明显差别的不同棒材微观组织在经历相同的固溶和时效处理后,其初生α相体积分数差别趋于相近,而初生α相的尺寸分布和形状分布等微观组织特征仍保留差别;力学性能结果显示室温拉伸力学性能趋于近似,而低周疲劳和保载疲劳力学性能对微观组织特征较为敏感。对比不同特征组织和力学性能分析结果,具有细小非等轴状且没有明显取向集中分布初生α相的棒材原始组织有助于获得更好的疲劳性能。  相似文献   
9.
《中国航空学报》2021,34(3):105-117
Swirl-Loop Scavenging (SLS) improves the performance of 2-stroke aircraft diesel engine because the involved swirl may not only benefit the scavenging process, but also facilitate the fuel atomization and combustion. The arrangement of scavenge port angles greatly influences in-cylinder flow distribution and swirl intensity, as well as the performance of the SLS engine. However, the mechanism of the effect and visualization experiment are rarely mentioned in the literature. To further investigate the SLS, Particle Image Velocimetry (PIV) experiment and Computational Fluid Dynamics (CFD) simulation are adopted to obtain its swirl distribution characteristics, and the effect of port angles on scavenging performance is discussed based on engine fired cycle simulation. The results illustrate that Reynolds Stress Turbulence model is accurate enough for in-cylinder flow simulation. Tangential and axial velocity distribution of the flow, as well as the scavenging performance, are mainly determined by geometric scavenge port angles αgeom and βgeom. For reinforcement of scavenging on cross-sections and meridian planes, αgeom value of 27° and βgeom value of 60° are preferred, under which the scavenging efficiency reaches as high as 73.7%. Excessive swirl intensity has a negative effect on SLS performance, which should be controlled to a proper extent.  相似文献   
10.
唐亮  李平  张锋  胡洪波 《推进技术》2020,41(5):1082-1088
测量液体火箭发动机的热载荷是获取燃烧室内部信息的重要方法。为了获取N_2O/C_2H_4预混推进剂燃烧室内壁的热载荷,建立了液体火箭发动机的热流计算的反问题方法,该方法基于对燃烧室壁面温度场的直接求解,通过对轴向多个位置测量温度的反演计算得到燃烧室内壁热流和温度。研究表明:应用文中建立的传热反问题方法能够较为准确地获得热流随时间及空间的分布;热电偶的位置对计算准确性有明显的影响,与理论深度偏差在0.2mm以内的随机深度偏差可导致超过4%热流反演误差;N_2O/C_2H_4预混推进剂燃烧室热流及温度沿轴向逐渐降低,表明燃烧室内的反应释热过程主要在燃烧室头部附近发生。  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