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李瑞祥%王治易%肖杰%欧阳求保%王文龙 《宇航材料工艺》2001,31(5):32-35
介绍了SiCp/Al复合材料的机械性能、热力学性能、加工性能,以及在太阳电池阵展开机构中的应用情况。分析认为采用SiCp/Al复合材料,充分发挥了其高比模量、高比强度和良好的耐磨性能,其管材、型材已达到了应用阶段。 相似文献
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液体火箭发动机故障诊断中的特征提取 总被引:1,自引:0,他引:1
对液体火箭发动机故障的原始特征进行特征提取和选择,以使所建立的故障标准模式由少数几个新特征给予有效的表达。比较了不同原始特征分布矩阵对特征提取结果有效性的影响,并对采用新特征来代表各种故障的效果进行了检验,结果同采用原始特征的效果很接近。 相似文献
938.
Thomas H. Zurbuchen 《Space Science Reviews》2007,130(1-4):515-526
The extraordinary life and scientific achievements of Johannes Geiss span an almost impossible breadth of scientific topics,
from the study of rocks to tenuous plasmas, from volcanoes to meteorites. But, his impact also extends way beyond the field
of science. Professor Geiss is a well-known teacher and a highly successful science leader whose impact has been felt at the
University of Bern, in Switzerland, and around the globe. We present here a brief summary of this highly successful career
via a pictorial overview and a movie compiled by a former student who had the good luck to work with Professor Geiss during
his years at the University of Bern.
Electronic Supplementary Material The online version of this article () contains supplementary material, which is available to authorized users. 相似文献
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Madeeha Talha Ghulam Murtaza Jean L. Rasson Nabeel Ahmed Mahrukh Peerzada 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):66-74
In this study, Sq(H) field results for Sonmiani geomagnetic observatory (SON), Pakistan are presented first time for solar cycle i.e., Solar Cycle 24. Sonmiani observatory was established in 2008 and was included in the list of INTERMAGNET Magnetic Observatory (IMO) in 2012. The analysis of Sq(H) field is performed to examine diurnal, annual and seasonal behaviour of Sq(H) field at Sonmiani along with Honolulu which is used as reference observatory. Both the observatories lie at the Equatorial Ionisation Anomaly (EIA) crest. In general strong dependency of Sq(H) field on solar cycle has been observed. First peak of SC24 was visible in Sq(H) field at both observatories. However, at HON maximum Sq(H) was observed in 2015 instead of 2014, a year later than the year of solar maximum. Prominent longitudinal difference has been noted between both observatories. At HON, maximum Sq(H) was observed during equinox while at SON it was noted during equinox and summer as a consequence of shift in latitude of Sq focus. Phase shift of Sq(H) at SON followed a general trend, that is maximum Sq(H) shifted to later hours in solar maximum as compared to solar minimum. Whereas, an opposite trend was noted at HON which might be due to coastal effect. In case of seasonal phase shift, at both observatories maximum Sq(H) occurred at later hours in summer than in winter which is opposite to the results obtained by many workers. These points need further investigation and geomagnetic as well as wind, and electric field data of other observatories situated at the EIA crest region is required to interpret the Sq(H) phase shift extensively. 相似文献