Oscillation of Quasi-Steady Earth＇s Magnetosphere

A three-dimensional magnetohydrodynamics （MHD） code is designed specially for global simulations of the solar wind-magnetosphere-ionosphere system. The code possesses a high resolution in capturing MHD shocks and discontinuities and a low numerical dissipation in examining possible instabilities inherent in the system. The ionosphere is approximated by a spherical shell with uniform height-integrated conductance. The solar wind is steady, and the interplanetary magnetic field is either due northward or due southward. The code is then run to find solutions of the whole system. It is found that the system has never reached a steady state, but keeps oscillating with a period of about one hour in terms of density variation at the geosynchronous orbit. However, if a certain artificial resistivity is added either in the whole numerical box or in the reconnection sites only, the reconnections change from intermittent to steady regime and the oscillation disappears accordingly. We conclude that the Earth＇s magnetosphere tends to be in a ceaseless oscillation status because of the low dissipation property inherent in the magnetospheric plasma, and the oscillation may be driven by intermittent magnetic reconnections that occur somewhere in the magnetopause and/or the magnetotail.     

基于亏量方程的多重网格解法

基于亏量方程提出了一种生成多重网格插值公式的新方法,新插值公式充分利用了粗网格的信息,因而具有更高的精度.对Poisson方程,各向异性方程,双调和方程,甚至三维问题的数值试验表明,新插值公式改进了多重网格法的渐近收敛速度,节省了存储空间及计算时间.     

Effect of change in large and fast solar wind dynamic pressure on geosynchronous magnetic field

We present a comparison of changes in large and sharp solar wind dynamic pressure, observed by several spacecraft, with fast disturbances in the magnetospheric magnetic field, measured by the geosynchronous satellites. More than 260 changes in solar wind pressure during the period 1996--2003 are selected for this study. Large statistics show that an increase (a decrease) in dynamic pressure always results in an increase (a decrease) in the magnitude of geosynchronous magnetic field. The amplitude of response to the geomagnetic field strongly depends on the location of observer relative to the noon meridian, the value of pressure before disturbance, and the change in amplitude of pressure.     

π介子在大变形核上散射的高级形变效应

本文研究了π介子在大变形核上散射的高级形变效应.结果表明,对微分截面的贡献是小的.     

用煤系高岭土制备轻质隔热材料的研究

以煤系高岭土、紫木节粘土为主要原料,以木屑和聚苯乙烯球为造孔剂,制备了体积密度为0.74 g/cm3、抗压强度为2.84 MPa,导热系数0.15 W/m.K的莫来石质轻质隔热耐高温材料。优化的工艺条件为:配料中煤系高岭土用量达到了90 wt%,添加木屑和聚苯乙烯球总加入量为12 wt%作为复合造孔剂,最终烧成温度为1300℃。通过XRD、SEM等分析的得到:轻质隔热材料的物相组成为莫来石、刚玉和少量方石英。材料内部的孔结构特征为1~2 mm的相对孤立的较大孔和微米级的小孔。     

π介子在大变形核上的散射

在程函理论的框架下, 利用π核一级光学势, 我们讨论了π^±介子在大变形核上的弹性与非弹性散射. 在封闭近似下, 我们考虑了到达低激发态的虚激发对弹性散射的影响. 对于180MeV的π^±在¹⁵²Sm核上的散射, 理论结果与实验数据作了比较.     

反应温度和锆英石添加量对石英碳热还原氮化产物的影响

本研究中选用石英和焦炭为原料、天然锆英石为添加剂,采用XRD、SEM和EDS等分析方法,研究了反应温度和锆英石添加量对石英碳热还原氮化产物影响.研究结果表明:在0.13 MPa的流动氮气气氛中,反应温度在1450～1550℃时,石英的碳热还原氮化产物中含有Si2N2O、β-SiC和β-Si3N4物相;当反应温度为1600℃时,石英的碳热等在1600℃条件下,石英碳热还原氮化产物主要含有柱状β-Si3N4和少量纤维状β-SiC物相;当添加10wt;的天然锆英石时,产物的主要成分为β-Si3N4 、ZrN以及少量βSiC物相;当锆英石添加量为20wt;到50wt;时,产物中不仅含有β-Si3N4和ZrN物相,还存在c-ZrO2,m-ZrO2,Si2N2O及β-SiC等物相.     

高阶ICCG误差阵模与条件数的估计

文[1]针对模型问题,应用高阶近似LU分解法给出了阶为0,1,2时ICCG法的预处理阵表达式,进而估计了误差阵的无穷模及条件数。针对更复杂的高阶问题给出了三阶和四阶ICCG法误差阵无穷模的估计以及相应的条件数上限。在不同节点数的条件下,对实际计算的条件数与文中所给出的上限作了比较。     

多重网格插值算子的改进算法

本文在多重网格法Gauss-Seidel型插值算子的基础上，再用Jacobi松弛予以修正得到高精度算法，多重网格法的两层收敛性也获得了证明，数值例子进一步证实了新算法的效率．     

溶胶-凝胶法制备Y_(3-x)Ce_xAl_5O_(12)纳米粉体的研究

以Y(NO3)3.6H2O、Ce(NO3)3.6H2O、Al(NO3)3.9H2O、柠檬酸为主要原料,以聚乙二醇作为分散剂,采用溶胶-凝胶法合成了纳米级YAG∶Ce3+粉体。研究了煅烧温度、溶液中金属离子浓度、溶液pH值及Ce3+掺杂量等因素对制备纳米YAG∶Ce3+粉体的颗粒尺寸、颗粒形貌、物相的影响。结果表明:当溶液pH为=4.0、金属离子浓度为0.50 mol/L、煅烧温度为1000℃时,可以制备出具有良好的分散性,平均粒径在30 nm的粉体。