排序方式: 共有76条查询结果,搜索用时 31 毫秒
21.
S.V. Vadawale M. Shanmugam Y.B. Acharya A.R. Patel S.K. Goyal B. Shah A.K. Hait A. Patinge D. Subrahmanyam 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The remote X-ray fluorescence spectroscopy is a powerful technique to investigate the elemental abundances in the atmosphere-less planetary bodies. The experiment involves measuring spectra of fluorescent X-rays from lunar surface using a low energy X-ray detector onboard an orbiting satellite. Since the flux of fluorescent X-ray lines critically depend on the flux and spectrum of the incident solar X-rays, it is essential to have simultaneous and accurate measurement of X-ray from both Moon and Sun. In the context of Moon, this technique has been employed since early days of space exploration to determine elemental composition of lunar surface. However, so far it has not been possible to exploit it to its full potential due to various reasons. Therefore it is planned to continue the remote X-ray fluorescence spectroscopy experiment on-board Chandrayaan-2 which includes both lunar X-ray observations and solar X-ray observations as two separate payloads. The lunar X-ray observations will be carried out by Chandra Large Area Soft x-ray Spectrometer (CLASS) experiment; whereas the solar X-ray observations will be carried out by a separate payload, Solar X-ray Monitor (XSM). Here we present the overall design of the XSM instrument, the present development status as well as preliminary results of the laboratory model testing. XSM instrument will have two packages namely – XSM sensor package and XSM electronics package. XSM will accurately measure spectrum of Solar X-rays in the energy range of 1–15 keV with energy resolution ∼200 eV @ 5.9 keV. This will be achieved by using state-of-the-art Silicon Drift Detector (SDD), which has a unique capability of maintaining high energy resolution at very high incident count rate expected from Solar X-rays. XSM onboard Chandrayaan-2 will be the first experiment to use such detector for Solar X-ray monitoring. 相似文献
22.
23.
聚碳硅烷PC—P是制备力学性能优异的低电阻率碳化硅纤维的先驱体。利用IR、TG、凝胶含量分析等手段研究了聚碳硅烷PC—P不熔化纤维的热解过程。研究表明,聚碳硅烷PC—P不熔化纤维高温热解过程与PCS不熔化纤维类似,但在300℃左右存在明显的自交联现象,使PC—P不熔化纤维的凝胶含量迅速增加,这是PC—P纤维在不熔化程度较低情况下能够通过高温烧成的原因。 相似文献
24.
郭伟凯%李家俊%赵乃勤%周福刚 《宇航材料工艺》2003,33(6):12-15,46
对目前吸波材料中用的纤维吸收剂——碳纤维、碳化硅纤维、金属纤维等的吸波特性、改性方法作了回顾,得出不同纤维的混杂和采用异型纤维是得到宽、轻、薄、强的结构吸波材料的有效方法。 相似文献
25.
郑春满%李效东%王亦菲%王应德%冯春祥 《宇航材料工艺》2005,35(3):7-10
为制备耐高温性能良好的SiC纤维,必须降低纤维中的氧含量,本文详细综述了国内外先驱体转化法制备Sic纤维中降低氧含量的方法,分析了各种方法的优缺点,比较可行有效的方法有电子束/γ射线辐射交联法、高温脱氧法和低度预氧化 热交联法,为制备高性能SiC纤维提供了一些参考。 相似文献
26.
掺混型碳化硅纤维微波吸收剂的制备 总被引:5,自引:0,他引:5
运用功率超声将平均粒径30nm的超细金属铁粉均匀分散到聚碳硅烷中,通过熔融纺丝,不熔化处理,烧结,制备出具有良好力学性能,电阻率连续可调的掺混弄烨奔走陶瓷纤维。 相似文献
27.
钠盐对铝硅合金的变质 总被引:2,自引:0,他引:2
采用高纯铝和硅(> 99.99% w t)配制Al-10% Si二元合金,经三元钠盐变质,研究合金中共晶硅相。结果表明:铝硅合金共晶凝固时,硅相滞后于铝相结晶。进行钠盐变质处理后,共晶凝固时硅相滞后更加明显,并使之由片状转变为纤维状。钠盐变质后的共晶硅中有较多的孪晶,孪晶轴为(111)Si;孪晶方向为(211)Si,共晶两相的位向关系符合〔100〕Al∥〔110〕Si。钠盐变质后的共晶硅以孪晶沟槽(TPRE)长大机制进行分枝、细化和弯曲,从而证明孪晶沟槽长大机制是产生变质结构的重要途径。 相似文献
28.
29.
碳化硅纤维增韧碳化硅陶瓷基复合材料的发展现状及其在航空发动机上的应用 总被引:2,自引:0,他引:2
碳化硅纤维增韧碳化硅陶瓷基复合材料(SiC/SiC CMC)具有低密度、高强高模、耐高温抗氧化、抗蠕变、抗热冲击、耐腐蚀、材料热膨胀系数小等性能优点,在航空发动机上具有巨大的应用潜力。从碳化硅纤维、制备工艺、界面相和涂层等方面综述了国内外SiC/SiC CMC的发展现状,并基于SiC/SiC CMC的性能特点对其在航空发动机燃烧室火焰筒、混合器、涡轮罩环/静子叶片/转子叶片、喷管调节片等热端部件上的应用情况进行了介绍。 相似文献
30.