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991.
Feng Chen Lina Tang Cuiping Wang Quanyi Qiu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The failure of scan-line corrector (SLC-off) has resulted in the limited use of Landsat 7 ETM+ images. Considering its characteristics, many attempts have been conducted to recover the SLC-off ETM+ image. While much attention has been paid to recovering the optically multispectral bands, few researches have been done to reconstruct the thermal band. Main purposes of our study were to evaluate the possibility that using China Brazil Earth Resources Satellite (CBERS) as auxiliary data to recover the thermal band of SLC-off ETM+, and discuss the usage of the recovered one. The adaptive window linear histogram match (AWLHM) method was selected primarily, followed by the modified one. Results illustrated the feasibility of using the modified AWLHM method with the linear combination of CBERS-01 band3 and band4 to reconstruct the SLC-off thermal band. It encourages that further researches should be done to enable more scientific application of SLC-off ETM+, particularly its’ thermal band. 相似文献
992.
纳米二氧化钛吸入对小鼠肺部和血清生化指标的影响 总被引:1,自引:0,他引:1
将成年健康的小鼠(每组8只)暴露在含有1 500 mg/m3纳米二氧化钛气溶胶密闭装置内,以暴露在空气中的小鼠作为对照,研究了纳米二氧化钛对小鼠肺部组织和血清生化指标的影响.经过不同时间的暴露后将小鼠处死,收集血样并取肺部组织进行生化指标分析和组织病理学检验.血清生化指标检测结果显示,在所有的试验组中,乳酸脱氢酶的活性均提高,丙氨酸氨基转移酶的活性和尿素氮在暴露28天组中增加,肌酐在暴露14天组和28天组中均增加,其他血清学指标未见明显异常.组织病理学检测结果显示,暴露28天的肺泡间隙有纳米粒子存在,并且肺部炎症逐渐增强. 相似文献
993.
数控加工效率低下已经成为一个普遍问题,不仅严重制约了我国航空工业的发展,而且造成了巨大的经济损失和资源浪费。本文从航空结构件的特点出发,提出了基于航空结构件典型特征的数控加工方法优化,在此基础之上达到结构件加工的整体优化,以提高加工效率及质量。 相似文献
994.
995.
996.
Long-term photometric signature study of two GEO satellites 总被引:1,自引:0,他引:1
Xiao-Fen Zhao Yong Yu Yin-Dun Mao Zheng-Hong Tang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(8):2241-2251
Geostationary earth orbit satellites have been extensively used for unique high-orbit stationary characteristics. Long-term precise investigation is an important issue in the observation of GEO satellites, since it can provide valuable information on the satellites’ operation state, discrimination and early warning analysis. Ground-based optical-electronic devices play a significant role in the observation. 4-month photometric signature variation of two satellites is presented based on the successive observations using the 1.56-meter telescope of Shanghai Astronomical Observatory (SHAO). It can be concluded that the long-term brightness change mainly results from the sun declination angle and regular orbit maneuver. Moreover, the solar panel offsets of the two satellites are analyzed and found to be approximately 4 degrees. Estimation of photometric accuracy reaches 0.15 mag for the application of CCD drift-scan optical-electronic technique. 相似文献
997.
空间碎片环境工程模式参数分析 总被引:3,自引:0,他引:3
为了评估空间碎片对航天器造成的危害 ,必须建立空间碎片环境工程模式。文章介绍了空间碎片环境的特点及其工程模式表征方法 ,并比较、分析了几种主要空间碎片环境工程模式的参数 ;从数学建模及风险评估应用的需求出发 ,提出了空间碎片环境工程模式参数的建议方案 相似文献
998.
有限推力轨迹优化问题的直接打靶法研究 总被引:3,自引:0,他引:3
研究了求解有限推力轨迹优化问题的直接打靶方法。说明了利用直接打靶法将最优轨迹问题转化为参数优化问题的基本转换方法 ;给出了状态和控制变量的等式 (或不等式 )约束的转化方法 ;从插值和数值积分两个方面对转换过程中产生的误差进行了深入分析。最后 ,以最优交会问题为例 ,说明了不同节点数目和积分步数对计算结果的影响 相似文献
999.
1000.
Tarter JC Backus PR Mancinelli RL Aurnou JM Backman DE Basri GS Boss AP Clarke A Deming D Doyle LR Feigelson ED Freund F Grinspoon DH Haberle RM Hauck SA Heath MJ Henry TJ Hollingsworth JL Joshi MM Kilston S Liu MC Meikle E Reid IN Rothschild LJ Scalo J Segura A Tang CM Tiedje JM Turnbull MC Walkowicz LM Weber AL Young RE 《Astrobiology》2007,7(1):30-65
Stable, hydrogen-burning, M dwarf stars make up about 75% of all stars in the Galaxy. They are extremely long-lived, and because they are much smaller in mass than the Sun (between 0.5 and 0.08 M(Sun)), their temperature and stellar luminosity are low and peaked in the red. We have re-examined what is known at present about the potential for a terrestrial planet forming within, or migrating into, the classic liquid-surface-water habitable zone close to an M dwarf star. Observations of protoplanetary disks suggest that planet-building materials are common around M dwarfs, but N-body simulations differ in their estimations of the likelihood of potentially habitable, wet planets that reside within their habitable zones, which are only about one-fifth to 1/50th of the width of that for a G star. Particularly in light of the claimed detection of the planets with masses as small as 5.5 and 7.5 M(Earth) orbiting M stars, there seems no reason to exclude the possibility of terrestrial planets. Tidally locked synchronous rotation within the narrow habitable zone does not necessarily lead to atmospheric collapse, and active stellar flaring may not be as much of an evolutionarily disadvantageous factor as has previously been supposed. We conclude that M dwarf stars may indeed be viable hosts for planets on which the origin and evolution of life can occur. A number of planetary processes such as cessation of geothermal activity or thermal and nonthermal atmospheric loss processes may limit the duration of planetary habitability to periods far shorter than the extreme lifetime of the M dwarf star. Nevertheless, it makes sense to include M dwarf stars in programs that seek to find habitable worlds and evidence of life. This paper presents the summary conclusions of an interdisciplinary workshop (http://mstars.seti.org) sponsored by the NASA Astrobiology Institute and convened at the SETI Institute. 相似文献