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111.
以汽油/空气两相混气为可爆混合物,采用汽油机点火和半导体高能点火系统,实验研究了不同点火频率对脉冲爆震室中不同位置脉冲爆震波压力的影响,结果发现,充满度大,产生的紊流强度大,有利于爆震波的形成;在大多数情况下,用低能量(50mJ)的点火系统点火时,点火频率大于实际产生的爆震频率;用高能(IJ)点火系统时,可缩短烯向爆震转变(DDT)的距离,易产生爆震,所得爆震波的峰值压力明显增大,所得结果可为脉冲爆震发动机的设计、爆震点火系统选型提供重要参考。 相似文献
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WALLINTERFERENCECORRECTIONSFORHIGH-LIFTEXPERIMENTZhangWenhua(Faculty603ofNanjingUniversityofAeronauticsandAstronautics,Nanjin... 相似文献
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C. Fröhlich 《Space Science Reviews》2006,125(1-4):53-65
Since November 1978 a set of total solar irradiance (TSI) measurements from space is available, yielding a time series of
more than 25 years. Presently, there are three TSI composites available, called PMOD, ACRIM and IRMB, which are all constructed
from the same original data, but use different procedures to correct for sensitivity changes. The PMOD composite is the only
one which also corrects the early HF data for degradation. The results from the detailed analysis of the VIRGO radiometry
allow a good understanding of the effects influencing the long-term behaviour of classical radiometers in space. Thus, a re-analysis
of the behaviour of HF/NIMBUS-7 and ACRIM-I/SMM was indicated. For the former the situation is complicated by the fact that
there are no in-flight means to determine changes due to exposure to solar radiation by comparison with a less exposed radiometer
on the same spacecraft. The geometry and optical property of the cavity of HF is, however, very similar to the PMO6-type radiometers,
so the behaviour of the PMO6V radiometers on VIRGO can be used as a model. ACRIM-I had to be revised mainly due to a henceforth
undetected early increase and a more detailed analysis of its degradation. The results are not only important for solar radiometry
from space, but they also provide a more reliable TSI during cycle 21. The differences between the revised PMOD composite
and the ACRIM and IRMB are discussed by comparison with a TSI reconstruction from Kitt-Peak magnetograms. As the PMOD composite
is the only one which has reliable data for cycle 21, the behaviour of the three solar cycles can now be compared and the
similarities and differences discussed. 相似文献
116.
王新坤%万红%熊德赣%汪定江%陈名华 《宇航材料工艺》2004,34(4):35-38
以高模高强碳纤维M40J(6K)增强铝基复合管为研究对象,研究了真空反压液相浸渗工艺中,纤维束丝分散技术、预制件压缩强度提高技术及碳纤维涂层对管件成型及性能的影响。结果表明:SiCp可以起分散作用,有利于浸渍;加入10%的偏磷酸盐的预制件经680℃真空去胶后的压缩性能满足浸渗要求,纤维保持了较好的平直度且分布均匀。C-Al2O3涂层对复合材料的性能有较大影响,经涂层处理后的预制件所制备出的复合材料的强度比未经涂层处理的提高了13%左右。所制备的复合材料的比强度、比模量较高,密度小于2.5g/cm^3。 相似文献
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M. Lockwood 《Space Science Reviews》2006,125(1-4):95-109
In paleoclimate studies, cosmogenic isotopes are frequently used as proxy indicators of past variations in solar irradiance on centennial and millennial timescales. These isotopes are spallation products of galactic cosmic rays (GCRs) impacting Earth's atmosphere, which are deposited and stored in terrestrial reservoirs such as ice sheets, ocean sediments and tree trunks. On timescales shorter than the variations in the geomagnetic field, they are modulated by the heliosphere and thus they are, strictly speaking, an index of heliospheric variability rather than one of solar variability. Strong evidence of climate variations associated with the production (as opposed to the deposition) of these isotopes is emerging. This raises a vital question: do cosmic rays have a direct influence on climate or are they a good proxy indicator for another factor that does (such as the total or spectral solar irradiance)? The former possibility raises further questions about the possible growth of air ions generated by cosmic rays into cloud condensation nuclei and/or the modulation of the global thunderstorm electric circuit. The latter possibility requires new understanding about the required relationship between the heliospheric magnetic fields that scatter cosmic rays and the photospheric magnetic fields which modulate solar irradiance. 相似文献
119.
介绍了在某三级风扇上进行的固定式插板畸变试验,并详细分析了进气压力畸变对进、出口稳态压力和温度的影响。同时,采用频域和幅值域分析方法对脉动压力进行了分析,给出了脉动压力功率谱密度、幅值概率密度和自相关、互相关分析。 相似文献
120.
宋敏 《西安航空技术高等专科学校学报》2004,22(1):3-6
用正交法对斜齿圆柱齿轮传动进行参数优化设计 ,用方差分析法找出对质量影响最显著的因素 ,最后 ,由信噪比作为指标选出最佳参数组合 ,这是一种快速创新开发产品的设计方法。 相似文献