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471.
在航空替代燃料缺乏足够飞行数据,几乎不可能通过有限发动机和飞行实验来评价其安全特性状况下,研究开发了一种简便却可保证适航安全性的方法来研究航空替代燃料的安全性能.“即用性”航空替代燃料被认为是发动机更换最频繁的部件,从而采用相似类比、使用经验方法来验证“即用性”燃料的适航符合性.以航空煤油实际使用经验为基准,提炼燃料性能、燃料系统、燃烧性能、发动机性能、飞机性能5个层次上参数化描述的安全边界,与通过航空替代燃料在5个层次上得到的工作边界进行相似类比,从而预测发动机使用替代燃料的安全性.该方法提炼了替代燃料在发动机安全性上的判定准则,还降低了认证流程的燃料成本和时间成本. 相似文献
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航空发动机进气系统结冰适航性条款研究 总被引:3,自引:0,他引:3
发动机进气系统结冰通常给发动机工作带来不利影响,甚至引起飞行事故,因此CCAR 33.68"进气系统的结冰"对每型发动机在结冰条件下的运行提出了适航性要求。对航空发动机防冰系统的适航性要求进行了解读,归纳了防冰方式对防冰系统的数值计算/关键点分析、试验验证进行了研究,介绍了典型符合性验证案例。本研究了可为国内开展航空发动机防冰适航性工作提供技术支持。 相似文献
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为了准确评估民用涡扇发动机空中起动试验性能与适航标准体系的符合性,在分析、解读中国民用航空局运输类飞机适航标准和美国联邦航空管理局咨询通告的基础上,制定了民用涡扇发动机空中起动飞行试验方案,以ARJ21-700型支线飞机配装的CF34-10A涡扇发动机合格审定试飞为平台,国内首次进行了相关试飞技术研究及飞行试验。试验结果表明:该空中起动飞行试验方案合理可行,能够完整、全面地验证民用涡扇发动机对适航标准体系的符合性。发动机最高起动边界为22500ft,起动高度指标设计合理,起动功能正常、可靠,满足适航标准要求。飞机待机状态双发失效后至起动成功高度损失为1457 ft,远小于适航标准规定的5000 ft指标。项目形成的试飞方案及积累的试飞经验为后续C919,C929等民用客机及其配装发动机的适航审定提供直接技术支持。 相似文献
475.
对我厂的频率标准XSR型铷原子频标发生的故障及具体检修情况作了较详细的分析和介绍。可供修复同类或其他类铷原子频标参考。 相似文献
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R. de Jesus Y. Sahai F.L. Guarnieri P.R. Fagundes A.J. de Abreu V.G. Pillat W.L.C. Lima 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The ionospheric sounding observations using the Canadian Advanced Digital Ionosondes (CADIs) operational at Palmas (PAL; 10.2°S, 48.2°W; dip latitude 6.6°S; a near-equatorial station), and São José dos Campos (SJC, 23.2°S, 45.9°W; dip latitude 17.6°S; a low-latitude station located under the southern crest of the equatorial ionospheric anomaly), Brazil, are analyzed during the different seasons viz., winter (June and July 2003), spring (September and October 2003), summer (December 2003 and January 2004), and fall (March and April 2004). The period used has medium solar activity (sunspot number between 77.4 and 39.3). The seasonal mean variations (using only geomagnetically quiet days) of the ionospheric parameters foF2 (critical frequency of the F-region), hpF2 (virtual height at 0.834 foF2; considered to be close to hmF2 (peak height of the F-region)), and h’F (minimum virtual height of the F-region) are calculated and compared between PAL and SJC. The prominent differences between PAL and SJC are as follows: h’F variations show strong post-sunset enhancement at PAL during the seasons of spring, summer, and fall; hpF2 variations show pre-sunrise uplifting of the F-layer at both stations during all the seasons and the hpF2 values during the daytime are lower at SJC compared with PAL during all the seasons; the foF2 variations show mid-day bite-out at PAL during all the seasons and SJC shows strong equatorial ionospheric anomaly during summer and fall seasons. Also, the seasonal variations of the ionospheric parameters foF2 and hpF2 (with ±1 standard deviation) observed at PAL and SJC are compared with the IRI-2007 model results of foF2 and hmF2. In addition, variations of the foF2 and hpF2 observed at SJC are compared with the IRI-2001 model results of foF2 and hmF2. It should be pointed out that the ionospheric parameter hpF2 is much easier to obtain using computer program developed at UNIVAP compared with hmF2 (using POLAN program). During the daytime due to underlying ionization hpF2 estimated is higher (approximately 50 km) than the true peak height hmF2. During the nighttime hpF2 is fairly close to hmF2. The comparison between the foF2 variations observed at PAL and SJC with the IRI-2007 model results shows a fairly good agreement during all the seasons. However, the comparison between the hpF2 variations observed at PAL and SJC with the hmF2 variations with the IRI-2007 model results shows: (1) a fairly good agreement during the nighttime in all the seasons; (2) the model results do not show the pre-sunrise uplifting of the F-layer at PAL and SJC in any season; (3) the model results do not show the post-sunset uplifting of the F-layer at PAL; (4) considering that, in general, hpF2 is higher than hmF2 during the daytime by about 50 km, the model results are in good agreement at PAL and SJC during all the seasons except summer at SJC, when large discrepancies in the observed hpF2 and modeled hmF2 are observed. Also, it has been observed that, in general, hmF2 values for SJC calculated using IRI-2001 are higher than IRI-2007 during the daytime in winter, summer, and fall. However, hmF2 values for SJC calculated using IRI-2001, are lower than IRI-2007 during the nighttime in spring. 相似文献
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