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A. Das A. DasGupta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Occurrence of Spread F is more or less a daily phenomenon in the equatorial and low latitudinal stations during high to moderate sunspot number years. In this paper efforts have been made to identify possible precursors of Equatorial Spread F (ESF) using the Total Electron Content (TEC) data of seven GAGAN (GPS Aided Geo Augmented Navigation) stations in India during the two equinoxes of moderate sunspot number year 2004. Large Scale Periodic Structures found prior to TEC bite out can be taken as possible precursors to ESF. A threshold value of the peak to peak amplitude of this wave structure is chosen 2.6 TEC unit above which there is a possibility of ESF or TEC bite out with S4 > 0.26. 相似文献
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利用先驱体聚合物浸渍-裂解(PIP)技术制备SiBN纤维增强氮化物陶瓷基复合材料,对SiBN纤维、聚硅硼氮烷有机先驱体裂解以及SiBN纤维增强氮化物陶瓷基复合材料性能进行了分析。研究表明:聚硅硼氮烷先驱体在氨气气氛下裂解得到的陶瓷产物碳含量较低,其裂解产物介电常数在3.0左右,介电损耗小于0.01;SiBN纤维中C和O元素含量均较高,碳的存在对材料介电性能影响明显;制备的氮化物陶瓷基复合材料弯曲强度为88.52 MPa,弹性模量为20.03 GPa。 相似文献
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H.-L. Lam 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A study of the relationship between solar wind low-energy energetic particles using data from the Electron, Proton, and Alpha Monitor (EPAM) onboard the Advanced Compositional Explorer spacecraft (ACE) and geomagnetic activity using data from Canadian magnetic observatories in Canada’s polar cap, auroral zone, and subauroral zone was carried out for a period spanning 1997–2005. Full halo coronal mass ejections (CMEs) were used to gauge the initial particle enhancements and the subsequent geomagnetic activity. It was found that maximum geomagnetic activity is related to maximum particle enhancements in a non-linear fashion. Quadratic fit of the data results in expressions that can be easily used in an operational space weather setting to forecast geomagnetic disturbance quantitatively. A superposed epoch analysis shows increase in particle flux level starts hours before geomagnetic activity attains its peak, affirming the precursory nature of EPAM particles for the impending geomagnetic impact of CME. This can supplement the decision process in formulating geomagnetic warning after the launch of CME from the Sun but before the arrival of shock at Earth. The empirical relationships between solar wind low-energy energetic particles and geomagnetic activity revealed in this statistical study can be easily codified, and thus utilized in operational space weather forecast to appraise the geoeffectiveness of the CME and to provide a quantitative forecast for maximum geomagnetic activity in Canada’s polar cap, auroral zone, and subauroral zone after the occurrence of a CME. 相似文献
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余煜玺%李效东%曹峰%邢欣%冯春祥 《宇航材料工艺》2002,32(6):10-13
先驱体交联处理是SiC陶瓷纤维制备过程中的主要步骤。为了更好地促进交联技术的发展,本文详细综述了先驱体法制备了SiC陶瓷纤维过程中聚碳硅烷纤维的交联方式,比较了各种交联方式的优缺点,指出了各种交联方式的适用范围,为交联方式的选择提供一些参考。 相似文献
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王建方%陈朝辉%刘希丛%肖加余%郑文伟 《宇航材料工艺》2001,31(4):40-43
应用物理学的逾渗理论对PIP法制备Cf/SiC复合材料浸渍和裂解过程进行了模拟解释和分析,并在此基础上对工艺进行了优化,使Cf/SiC复合材料的密度由原来的1.75g/cm^3提高到2.03g/cm^3,强度由原来的300MPa提高到500MPa。 相似文献
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以不同质量比Si C/Zr C有机前驱体混合溶液为浸渍剂,采用前驱体浸渍裂解法(PIP)制得C/CSi C-Zr C复合材料。对C/C-Si C-Zr C复合材料的组成、微观结构及烧蚀性能进行了分析和测试,探讨了Si C/Zr C前驱体配比对复合材料烧蚀性能的影响。结果表明,随着Zr C含量的增加,复合材料的质量烧蚀率和线烧蚀率呈现出先减小后增大的趋势。采用质量比为1∶3的Si C/Zr C前驱体混合溶液制备的C/C-Si C-Zr C复合材料具有相对较好的烧蚀性能,试样在氧乙炔焰下3 000℃烧蚀20 s,其质量烧蚀率和线烧蚀率分别为-0.65 mg/s和21μm/s。Si C-Zr C复相陶瓷中Zr C含量过低或过高均不利于提高其氧化稳定性,而Zr C含量适中的Si C-Zr C复相陶瓷具有较好的氧化稳定性。 相似文献
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周长江%魏红%陈朝辉 《宇航材料工艺》2001,31(1):15-18
以聚碳硅烷为先驱体,Ti粉为活性填料,研究了Ti粉对聚碳硅烷裂解反应及先驱体转化法制备的块体复相陶瓷的性能的影响,并表征了其晶相组成,结果表明,Ti粉可促进PCS的裂解反 ,增加先驱体的陶瓷产率,能降低先驱体在裂解过程中的线性收缩率和气孔率,提高陶瓷材料性能。 相似文献