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Xilinx SRAM型FPGA抗辐射设计技术研究 总被引:10,自引:2,他引:10
针对Xilinx SRAM型FPGA在空间应用中的可行性,分析了Xilinx SRAM型FPGA的结构,以及空间辐射效应对这种结构FPGA的影响,指出SRAM型的FPGA随着工艺水平的提高、器件规模的增大和核电压的降低,抗总剂量效应不断提高,抵抗单粒子效应,尤其是单粒子翻转和单粒子瞬态脉冲的能力降低。分析了FPGA综合后常见的Half-latch在辐射环境中的影响并结合实际工程实践给出了解决上述问题的一些有用办法和注意事项,如,冗余设计、同步设计、算术逻辑运算结果校验、白检等。最后还提出一种基于COTS器件的“由顶到底”的星载信号处理平台结构,分析了这种结构在抵抗辐射效应时的优势。有关FPGA抗辐射的可靠性设计方法已经在某卫星通信载道中成功应用,并通过了各种卫星环境试验,该技术可以为有关航天电子设备设计提供参考。 相似文献
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Balázs Zábori Attila Hirn Pál Bencze 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The main point of the paper is to use the simultaneous measurements of the energetic particle flux by TriTel and those of electron density by a Langmuir probe to study the question of to what extent solar electromagnetic and corpuscular radiation (galactic cosmic rays, particle precipitation from the radiation belts) are responsible for the ionization of the atmosphere. The electron density measured by the Langmuir probe is the sum of the ionization produced by the solar electromagnetic radiation and that due to the corpuscular radiation. The ionization produced by the solar electromagnetic radiation may be computed. The flux of energetic particles in an energy range may be determined by taking the difference between the threshold energy of the TriTel telescopes and the energy corresponding to the local cut-off rigidity. As the ESEO satellite will have a quasi-polar and circular orbit, the cut-off rigidity will change from low to high latitudes, thus enabling the assignment of different energy bands for the telescopes. Thus, it will be possible to determine which energy bands of particle produce ionization at different latitudes. 相似文献
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Leakage due to wear is one of the main failure modes of aero-hydraulic spool valves. This paper established a practical coupling wear model for aero-hydraulic spool valves based on dynamic system modelling theory. Firstly, the experiment for wear mechanism verification proved that adhesive wear and abrasive wear did coexist during the working process of spool valves. Sec-ondly coupling behavior of each wear mechanism was characterized by analyzing actual time-variation of model parameters during wear evolution process. Meanwhile, Archard model and three-body abrasive wear model were utilized for adhesive wear and abrasive wear, respectively. Furthermore, their coupling wear model was established by calculating the actual wear volume. Finally, from the result of formal test, all the required parameters for our model were obtained. The relative error between model prediction and data of pre-test was also presented to verify the accuracy of model, which demonstrated that our model was useful for providing accurate prediction of spool valve’s wear life. 相似文献
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将nc-Si:H薄膜进行等离子和高温氧化处理,测量了样品的氢,氧含量,Raman谱,红外吸收谱,光致发光(PL),结果表明两种氧化方式都将氧掺入薄膜中,但不同处理方式氧在薄膜中的键合形式不同Raman谱表明氧化处理对薄膜中晶粒大小及晶态比没有影响,用晶粒-表面模型对氧化引起的光致发光(PL)蓝移进行了解释。 相似文献
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We study kinetic excitation mechanisms for high-frequency dispersive Alfvén waves in the solar corona, solar wind, and Earth's
magnetosphere. The ion-cyclotron and Cherenkov kinetic effects are important for these waves which we call the ion-cyclotron
kinetic Alfvén waves (ICKAWs). Ion beams, anisotropic particles distributions and currents provide free energy for the excitation
of ICKAWs in space plasmas. As particular examples we consider ICKAW instabilities in the coronal magnetic reconnection events,
in the fast solar wind, and in the Earth's magnetopause. Energy conversion and transport initiated by ICKAW instabilities
is significant for the whole dynamics of Sun-Earth connection chain, and observations of ICKAW activity could provide a diagnostic/predictive
tool in the space environment research.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
39.
S.A. Demin Y.A. Nefedyev A.O. Andreev N.Y. Demina S.F. Timashev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):639-644
The analysis of turbulent processes in sunspots and pores which are self-organizing long-lived magnetic structures is a complicated and not yet solved problem. The present work focuses on studying such magneto-hydrodynamic (MHD) formations on the basis of flicker-noise spectroscopy using a new method of multi-parametric analysis. The non-stationarity and cross-correlation effects taking place in solar activity dynamics are considered. The calculated maximum values of non-stationarity factor may become precursors of significant restructuring in solar magnetic activity. The introduced cross-correlation functions enable us to judge synchronization effects between the signals of various solar activity indicators registered simultaneously. 相似文献
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