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71.
为提高压气机叶型优化设计水平,基于中弧线曲率控制方法编写了压气机叶片造型程序,将中弧线曲率控制参数作为优化变量,结合粒子群寻优算法对传统可控扩散叶型(CDA)进行了优化研究。结果表明:基于中弧线曲率控制的叶片造型程序能够对CDA叶型进行较好的拟合,拟合叶型的气动性能与设计要求较符。优化叶型在设计点的总压损失降低了约6.34%,优化叶型总压损失随攻角变化较为平缓。在一定攻角范围内,叶型中弧线曲率峰值的前移能够将吸力面马赫数峰值前移,提高叶型吸力面的扩压能力,降低总压损失。在大攻角工况下,改进的中弧线曲率分布能够显著降低叶型总压损失。将中弧线曲率控制参数作为优化变量进行CDA叶型的优化是可行的。 相似文献
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获取舰载直升机实用风限图,仅依靠实装飞行试验或建模仿真都是非常困难的。通过起降飞行模拟试验获取理论风限图,结合少量的海上实装飞行验证试验是一种综合较优的方法。起降飞行模拟试验需要真实飞行员和高等级飞行模拟器参与,飞行模拟器中的母舰气流场数据、母舰运动可由建模仿真或试验测试得到,且必须考虑母舰气流场的非定场特性;只有当飞行员视景或视觉反馈受限时(如能见度降低时),飞行模拟器基座的六自由度运动才是必需的;用DIPES或Bedford方法量化飞行员主观操纵负担,结合记录的客观操纵数据,评判起降难度;典型的飞行模拟试验程序包含了不同风况下的进近和甲板着舰,通常每隔15°和5kn一个风况。通过起降飞行模拟试验得到的理论风限图,可以更加有效和安全地指导海上实装飞行验证试验,最终获得实用风限图。 相似文献
74.
为了给载人航天器乘员营造一个良好的生活工作环境,需要将众多空气环境参数控制在指标范围内。文章结合载人航天器专业知识,基于Modelica统一建模语言建立了一种载人航天器环热控系统仿真分析模型;利用该模型仿真分析了温湿度控制风机取不同转速时,载人航天器空气环境参数随乘员代谢水平的变化趋势。结果表明:在其他参数不变的情况下,温湿度控制风机转速越大,空气温度越低,相对湿度越高;乘员代谢水平变化对空气环境参数有显著影响,通过调节系统运行参数可将各空气参数有效控制在指标范围内。舱体温度与氧分压、二氧化碳分压、舱体相对湿度有密切关系且相互影响,不可单独分析。 相似文献
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Shlomi Ziskin Nir J. Shaviv 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The 20th century temperature anomaly record is reproduced using an energy balance model, with a diffusive deep ocean. The model takes into account all the standard radiative forcings, and in addition the possibility of a non-thermal solar component. The model is parameterized and then optimized to produce the most likely values for the climate parameters and radiative forcings which reproduce the 20th century global warming. We find that the best fit is obtained with a negligible net feedback. We also show that a non-thermal solar component is necessarily present, indicating that the total solar contribution to the 20th century global warming, of ΔTsolar = 0.27 ± 0.07 °C, is much larger than can be expected from variation in the total solar irradiance alone. However, we also find that the largest contribution to the 20th century warming comes from anthropogenic sources, with ΔTman = 0.42 ± 0.11 °C. 相似文献
78.
Michiel Otten Claudia Flohrer Tim Springer John Dow 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
This paper gives an overview of the DORIS related activities at the Navigation Support Office of the European Space Operations Centre. The DORIS activities were started in 2002 because of the launch of the Envisat satellite where ESOC is responsible for the validation of the Envisat Precise Orbits and a brief overview of the key Envisat activities at ESOC is given. Typical orbit comparison RMS values between the CNES POE (GDR-C) and the ESOC POD solution is 6.5, 18.8 and 23.1 mm in radial-, along- and cross-track direction. In the framework of the generation of the ITRF2008 ESOC participated in the reprocessing of all three space geodetic techniques; DORIS, SLR, and GPS. Here the main results of our DORIS reprocessing, in the framework of the International DORIS Service (IDS), are given. The WRMS of the weekly ESOC solution (esawd03) for the 2004–2009 period compared to the IDS-1 combined solution is of the order of 12 mm. Based on the long time series of homogeneously processed data a closer look is taken at the estimated solar radiation pressure parameters of the different satellites used in this DORIS analysis. The main aim being the stabilization of the Z-component of the geocentre estimates. We conclude that the ESOC participation to the IDS ITRF2008 contribution has been beneficial for both ESOC and the IDS. ESOC has profited significantly from the very open and direct communications and comparisons that took place within the IDS during the reprocessing campaign. 相似文献
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Kh. Karami S. Ghader A. Raeen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by and are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively. 相似文献