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《中国航空学报》2021,34(6):1-17
Corundum abrasives with good chemical stability can be fabricated into various free abrasives and bonded abrasive tools that are widely used in the precision machining of various parts. However, these abrasives cannot satisfy the machining requirements of difficult-to-machine materials with high hardness, high strength, and strong wearing resistance. Although superhard abrasives can machine the above-mentioned materials, their dressing and manufacturing costs are high. By contrast, ceramic corundum abrasives fabricated by sol–gel method is a cost-effective product between conventional and superhard abrasives. Ceramic corundum abrasives exhibit self-sharpening and high toughness. In this review, the optimization methods of ceramic corundum abrasive properties are introduced from three aspects: precursor synthesis, particle shaping, and sintering. Firstly, the functional mechanism of seeds and additives on the microstructural and mechanical properties of abrasives is analyzed. Specifically, seeds can reduce the phase transition temperature and improve fracture toughness. The grain size and uniformly dense structure can be controlled by applying an appropriate amount of multicomponent additives. Then, the urgent need of engineering application and machinability of special shape ceramic corundum abrasives is reviewed, and three methods of abrasive shaping are summarized. The micromold replication technique is highly advanced and can be used to prepare functional abrasives. Additionally, the influence of a new sintering method, namely, two-step sintering technique, on the microstructural and mechanical performance of ceramic corundum abrasives is summarized. Finally, the challenge and developmental trend of the optimization of ceramic corundum abrasives are prospected. 相似文献
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高校校园文化建设刍议 总被引:2,自引:0,他引:2
更新观念,正确认识校园文化在学校可持续发展中的地位;与时俱进,充分挖掘在校园文化建设中所彰显的体现学校特色内外在形象;通过内隐与外在的学校形象表现,从公关的意识和策划的高度引发和阐述出实施校园文化建设的原则与加强校园文化建设的落脚点,以及校园文化建设对学校的整体效益和持续发展裨益所在。 相似文献
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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
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根据高速数传发射机的要求,提出基于联合映射的高速卫星发射机设计及基于查找表的FPGA(F ieldProgramm ab le Gate Array,现场可编程门阵列)硬件实现方案。该方法将发射机中数字部分的TCM编码和成形滤波一起设计,将多个卷积相乘项相加后再量化,减少了量化次数,提高了量化信噪比。并根据FPGA芯片内部结构设计硬件实现方案,符合SOC(System of Ch ip)的趋势。用片内的BLOCKRAM精心设计查找表,在X ILINX公司25万门芯片VIRTEX2-250中就能实现此方案。MODELSIM的时序仿真结果表明可支持高达200Mb it/s的数据。文章结尾针对未来更高速率的高速数传发射机给出了一种通用硬件实现方法。 相似文献
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深空测控的下行链路包括测控和数传2种典型的传输信道,其中数传信道一般具有发射功率大和数据传输速率高的特点,其带外辐射容易对测控信道产生干扰。以典型月球探测器为例,分析比较了数传信道采用常规BPSK(二进制相移键控)调制和基带滤波BPSK调制时,对测控信道的带外辐射影响,并对基带滤波BPSK调制的误码率性能进行了仿真分析,相应结论对未来深空探测任务测控系统总体设计具有十分重要的参考意义。 相似文献
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根据高速8PSK卫星调制器的要求,针对数字化基带成形滤波的信号处理特点,提出一种基于部分卷积和并行查表的高速卫星成形滤波器设计方法及基于现场可编程门阵列(FPGA)芯片结构的FPGA算法。用片内的BLOCKRAM精心设计查找表,通过改变查找表内容可适用于各种信道限带性能要求的传输系统。在X ILINX公司V irtex2-1000芯片上完成该方案,MODELSIM的时序仿真结果表明可支持高达400Mb it/s的输入数据,满足卫星通信高速成形的要求。 相似文献