Numerical study of magnetic reconnection possibly occurring near heliospheric current sheet

The third-order accurate upwind compact difference scheme has been applied for the numerical study of the magnetic reconnection driven by a plasma blob impacting the heliospheric current sheet, under the framework of the two-dimensional compressible magnetohydrodynamics. The results show that the driven reconnection near the current sheet could occur in about 10–30 min for the interplanetary high magnetic Reynolds number, R_M = 2000–10,000, a stable magnetic reconnection structure can be formed in hour order of magnitude, and there appear some basic properties such as the multiple X-line reconnections, vortex structures, filament current systems, splitting and collapse of the high-density plasma blob. These results are helpful in understanding and identifying the magnetic reconnection phenomena possibly occurring near the heliospheric current sheets.     

用经验模式参数研究电离层发电机效应

本文利用MSIS-86和IRI-86模式的基本参数,求得热层风系和电导率的三维分布;继而从发电机理论得到了电离层电位及层电流密度在北半球的分布和变化。本研究将大量数据统计平均的大气模式参数与热层、电离层理论研究联系了起来。     

Storm-time formation of a relativistic electron belt and some relevant phenomena in other magnetospheric plasma domains

An empirical formula relating the strength of a storm given by its |Dst|_max with the L-coordinate of the peak of storm-injected relativistic electrons is one of a few well-confirmed quantitative relations found in the magneto-spheric physics. We successively extended a dataset of the formula’s basic storms with several events of high Dst-amplitude up to the highest observed |Dst|_max = 600 nT. Possible applying of the formula to the predicting of the ring-current plasma-pressure distribution and the lowest westward electrojet position for a storm are discussed. We have also analyzed the 2000–2001 years’ data on relativistic electrons from our instruments installed on EXPRESS-A (geosynchronous orbit; E_e = 0.8–6 MeV), Molniya-3 (h = 500 × 40 000 km, i = 63°; E_e = 0.8–5.5 MeV) and GLONASS (h = 20 000 km, i = 64°; E_e  l MeV) along with other correlated measurements: GOES series (E_e > 2 MeV), geomagnetic indices (Dst, AE, AL) and interplanetary parameters (solar wind, IMF). The goal is to investigate which outer conditions are most responsible for the high/low output of the storm-injected relativistic electrons. For the geosynchronous orbit, two factors are found as the necessary condition of the highest electron output: high and long-lasting substorm activity on a storm recovery phase and high velocity of solar wind. On the contrary, extremely low substorm activity surely observed during whole the storm recovery phase constitutes a sufficient condition of the non-increased after-storm electron intensity. For the first time found cases of the increased after-storm electron intensity observed at the inner L-shells with no simultaneously seen increase in the geosynchronous distances are presented.     

垂直射流混合的三维湍流数值模拟

采用三维ＳＩＭＰＬＥ程序和ｋ－ε双方程湍流模型对三维受限垂直射流进行数值模拟,研究了不同的几何变量和流动参数对射流穿透和混合的影响。模拟结果表明,三维垂直射流最显著的流动特征是形成了流向旋涡。射流与来流的混合程度取决于旋涡的位置、作用范围和强弱。单股射流随动量比、旋涡强度和尺度的增加,混合增强。对于单排多股射流,喷孔间距直接影响旋涡涡心位置。密排射流,旋涡过于靠近下壁面,旋涡无法影响上面来流;但喷孔排列也不能过于稀疏,否则涡对靠的太近,旋涡对侧面影响不大。Ｓ／Ｈ和动量比不变,改变孔径Ｄ对射流穿透几乎无影响。这一重要结论说明Ｓ／Ｈ和Ｊ是决定多股受限射流穿透深度的最重要的量。     

无陀螺飞行器姿态和角速度确定

通过预测滤波方法研究了利用矢量观测确定无陀螺飞行姿态和角速度的方法。给出的观测滤波法在一定的二次型优化准则下，对飞行器姿态和名义姿态运动模型的等效角速度误差可同时进行实时估计，能够准确跟踪敏感器的测量，有效减小模型误差的影响，数值仿真结果验证了算法的优越性。     

关于大电流测试问题的研究

采用电流比较仪,AD交直流标准电阻,高准确度数字多用表组成校验系统,解决大电流测试问题.     

高校青年教师思想道德建设刍议

通过对当前高校青年教师思想道德现状的分析,在肯定青年教师积极、健康、向上主流的同时,指出了存在的三个方面的问题,进而从社会大环境、学校小环境和青年教师自身三个方面深入研究了青年教师思想道德“衰微”的成因。在此基础上,探讨了加强和改进高校青年教师思想道德建设的思路和对策。     

Distribution of electric current in solar plasma loops

The distributing profile of electric current in solar plasma loop is a key factor for the MHD instabilities of the loops. However, it is very difficult to measure such profile in single loop. In this paper, we assume that, in spite of the complexity of the structure in most of the sunspots, the distribution of the electric current in some small simple sunspots may reflect the main feature of the distribution in solar plasma loops. We utilize the high-cadence, high-resolution vector magnetograms observed by Big Bear Solar Observatory (BBSO) to derive the longitudinal electric current and analyze the distribution of the longitudinal electric current in the region of sunspots, and simulate the distributing features of the solar plasma loops. From these analysis, we find that the electric current in some small simple sunspots, or to say in plasma loops, are concentrated to their center. Such distribution feature is consistent with the theory of pinch effect in current-carrying plasma loops.     

增减材复合制造内部缺陷的涡流检测

涡流检测（ECT）技术具有非接触、无需耦合剂、检测灵敏等特点，适用于加工环境较为特殊的增减材复合制造（ASHM）中。本文建立了无缺陷半无限大试样内部涡流分布的解析模型，开展了预制人工缺陷的钛合金增材试样检测实验，研究了ECT深度与激励频率、提离量之间的关系。理论分析与实验结果均表明，内部缺陷较深时，低激励频率条件下缺陷产生的电抗增量信号较大，不同提离量下的电抗增量信号相差不大，因此检测位置较深的内部缺陷时可采用较低的激励频率并适当提高提离量。在本文实验条件下，ECT最佳激励频率为90 kHz；提离量增加到0.97 mm时，有效检测深度略有减小。这一结论可为ECT技术与ASHM的集成提供理论依据。     

Effect of Electromagnetic Stirring on the Quality of K417 Superalloy Ingots

The effect of electromagnetic stirring on the inner quality of K417 superalloy ingots is studied with EPMA and optical microscope.The results show that while an electromagnetic stirring with 50Hz frequency and 80A current is imposed,the equiax crystals of K417 superalloy ingots can be effectively refined and increased,and the central shrinkage porosity and the dendritic segregation of K417 superalloy ingots are greatly reduced,so the inner quality of K417 superalloy ingots is obviously improved.