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111.
C. Scotto 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
An algorithm is proposed for evaluation of the probability of occurrence of an F1 layer or L condition, based on tables. Observations independent of the tables database are used for comparison between the estimated probability of occurrence, the formulation used at present in IRI, and the occurrence actually observed. The importance of the inclusion of L condition in the electron density profile model is shown. 相似文献
112.
Patrick A. Nsumei Bodo W. Reinisch Xueqin Huang Dieter Bilitza 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The ionospheric characteristics of the F2 layer peak have been measured with ionosondes from the ground or with satellites from space. The most common characteristics are the F2-peak density NmF2 and peak height hmF2. In addition to these two parameters this paper studies the F2-peak scale height. Comparing the median values of hmF2 and NmF2 obtained from topside and bottomside sounding shows good agreement in general. The Chapman scale height values for the F2 layer peak derived from topside profiles, Hm,top, are generally several times larger than Hm,bot derived from bottomside profiles. 相似文献
113.
提出了一种基于Windows环境下的活塞裙部外圆复杂型面在位检测的新方法,并设计了在位检测的软、硬件系统.同时,根据活塞裙部型面的特点,在现有常用误差处理算法的基础上进行了改进,新的误差处理方法具有更强的适用性. 相似文献
114.
回流焊温度曲线热容研究 总被引:4,自引:0,他引:4
本文全面的分析了回流焊温度曲线在回流焊工艺中的作用,回流焊工艺的工艺特点、影响回流焊温度曲线的各种因素。如何从热容的思想建立回流焊温度曲线的方法?如何调整温度曲线通过控制温度曲线改善工艺过程,减少回流焊工艺的缺陷? 相似文献
115.
Physiologic and metabolic responses of wheat seedlings to elevated and super-elevated carbon dioxide
Lanfang H. Levine Hirokazu Kasahara Joachim Kopka Alexander Erban Ines Fehrl Fatma Kaplan Wei Zhao Ramon C. Littell Charles Guy Raymond Wheeler John Sager Aaron Mills Howard G. Levine 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The metabolic consequence of suboptimal (400 μmol mol−1 or ppm), near-optimal (1500 ppm) and supra-optimal (10,000 ppm) atmospheric carbon dioxide concentrations [CO2] was investigated in an attempt to reveal plausible underlying mechanisms for the differential physiological and developmental responses to increasing [CO2]. Both non-targeted and targeted metabolite profiling by GC–MS and LC–MS were employed to examine primary and secondary metabolites in wheat (Triticum aestivum, cv Yocoro rojo) continuously exposed to these [CO2] levels for 14, 21 and 28 days. Metabolite profile was altered by both [CO2] and physiological age. In general, plants grown under high [CO2] exhibited a metabolite profile characteristic of older plants under ambient CO2. Elevated [CO2] resulted in higher levels of phosphorylated sugar intermediates, though no clear trend in the content of reducing sugars was observed. Transient starch content was enhanced by increasing [CO2] to a much greater extent at 10,000 ppm CO2 than at 1500 ppm CO2. The percentage increase of starch content resulting from CO2 enrichment declined as plants develope. In contrast, elevated [CO2] promoted the accumulation of secondary metabolites (flavonoids) progressively to a greater extent as plants became mature. Elevated [CO2] to 1500 ppm induced a higher initial growth rate, while super-elevated [CO2] appeared to negate such initial growth promotion. However, after 4 weeks, there was no difference in vegetative growth between 1500 and 10,000 ppm CO2-grown plants, both elevated CO2 levels resulted in an overall 25% increase in biomass over the control plants. More interestingly, elevated atmospheric [CO2] reduced evapotranspiration rate (ET), but further increase to the supra-optimal level resulted in increased ET (a reversed trend), i.e. ET at 1500 ppm < ET at 10,000 ppm < ET at 400 ppm. The differential effect of elevated and super-elevated CO2 on plants was further reflected in the nitrogen dynamics. These results provide the potential metabolic basis for the differential productivity and stomatal function of plants grown under elevated and super-elevated CO2 levels. 相似文献
116.
为了阐明测点布局对航空发动机进气总压畸变测试结果的影响,利用旋转总压测量耙对5种畸变流场的稳态和动态总
压畸变成分进行了测试,计算了旋转总压测量耙位于不同位置时畸变流场的稳态周向总压畸变指数和动态总压畸变指数,分析了
不同测点布局下总压畸变指数计算结果的偏差。结果表明:测量耙/测点与畸变流场的相对周向位置对总压畸变指数计算结果的
准确性至关重要,对于所分析的5种畸变流场,增加测量耙/测点周向数目并不能使总压畸变指数计算结果的偏差单调减小,但可
降低其对测量耙/测点周向位置的敏感度。基于畸变区域周向分布设计稳态总压畸变测量耙的周向位置,组合使用不同相对半径
处测点对动态总压畸变进行监测,可提高总压畸变指数计算结果的准确性。 相似文献
117.
118.
分散度检验法和横截面收益绝对差检验法是检验证券市场中羊群行为的两种方法。运用这两种方法对中国证券市场进行实证分析,结果表明:在中国的证券市场中确实存在着明显的羊群行为。 相似文献
119.
最大标准差和最大变异系数方法 总被引:2,自引:0,他引:2
本文提出的最大标准差方法和最大变异系数方法,能充分利用以往数据和经验提供的信息,大大减少了试件个数。与国际上常用的单侧容限系数法相比,可节省大量试件;而在试件个数相同的情况下,则可得到更接近母体百分位值的置信下限(如安全寿命或安全疲劳极限等)。 相似文献
120.
K. Andreov L. Pech 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1871-1880
This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper. 相似文献