Energization of charged particle in a time-dependent chaotic magnetic field with an implication of the production of seed particles in solar energetic particle events

We investigate the acceleration of charged particles in a time-dependent chaotic magnetic field in this work. In earlier works, it has been demonstrated that in an asymmetric wire-loop current systems (WLCSs), the magnetic field is of chaotic in nature. Furthermore, observations also showed that there exist time-varying current loops and current filaments in solar corona. It is therefore natural to conceive that the magnetic field on the solar surface is chaotic and time-dependent. Here, we develop a numerical model to study the acceleration process of charged particles in a time-varying chaotic magnetic field that is generated by an ensemble of 8 WLCSs. We found that the motion of energetic particles in the system is of diffusive in nature and a power law spectrum can quickly develop. The mechanism examined here may serve as an efficient pre-acceleration mechanism that generates the so-called seed particles for diffusive shock acceleration at a coronal mass ejection (CME) driven shock in large solar energetic particle (SEP) events.     

陀螺接线柱加工工艺方法研究

以陀螺接线柱的加工为研究对象,通过分析现有加工中的难点、问题和加工工艺流程,重点研究了车加工问题机理和表面处理后出现空腔问题的机理,分析出接线柱组件合格率偏低的主要原因。并在此基础上,提出优化的加工工艺方法,以此降低陀螺接线柱的缺陷率。     

应变片电测法在外场金属支架应力测试中的应用

外场金属支架在工作过程中需要进行应力监测，一般采用应变电测法，由于金属支架表面为曲面，可能会给测量带来影响。本文从计算分析和实验验证两个方面，探讨曲面对应变电测法测量结果的影响。最终得出由于金属支架曲率半径较大，应变片尺寸相对较小，曲面对测量产生的误差很小，可忽略，证明使用应变片法对金属支架进行应力监测是可行的。     

基于BP神经网络的某型无人机电气系统故障诊断研究

针对某型无人机对电气系统的故障诊断准确无误的要求。本文对基于较为成熟的BP神经网络无人机电气系统故障诊断方面的应用进行了研究。实例表明,BP神经网络在无人机电气系统故障诊断方面是一个很有效的方法。     

飞行模拟器电动操纵负荷系统多余力抑制研究

飞行模拟器操纵负荷系统是一种被动式力伺服系统,其多余力的抑制是提高操纵负荷系统力跟踪精度的关键。以研制的飞行模拟器电动操纵负荷系统原理样机为平台,对系统的工作原理和结构进行介绍,通过系统建模,在MATLAB/SIMULINK中仿真,对经典的前馈补偿和PID复合控制方法的多余力抑制效果进行仿真分析,并在原理样机上进行试验测试。试验结果验证了复合控制策略有效地抑制了多余力,提高了系统的跟踪精度。     

复杂电磁环境下RS422接口保护电路的实现

在复杂电磁环境下如果对422通信接口进行带电热插拔操作会引发高电压冲击,当热插拔瞬间放电电流大于串口芯片所能承受的最大电流时,串口通信接口电路会被烧毁,为了有效保护通信接口电路,介绍了一种的串口热插拔保护电路,它的原理是使用对地二极管将瞬态的高电压抑制下来,在不改动设备的前提下可以对422通信接口电路提供有效的保护。经实践证明对RS422接口电路有明显的保护作用,也可以应用于其他串行通信电路。     

碘工质电推进系统的储供设计及实验研究

碘工质以其低成本、低压且高密度贮存等特点越来越受到重视,承担固气相变和流量供给功能的储供系统是碘工质电推进系统的关键组件。为了提高直接影响阴极和推力器性能的流量供给准确性和稳定性,设计了可采用多种加热方式的碘工质储供系统,结合用于真空舱内的高精度质量传感器,实现了流量的动态监测及mg/s级别的碘蒸气流量控制。针对储罐外部加热、内部辐射加热以及二者复合加热三种加热方式开展实验测量,探究其对流量大小和稳定性的影响规律。结果表明,三种加热方式在满足实验所需条件下均可长期供给稳定流量,辐射加热式的响应时间最快,仅需要10min左右,而外部加热则超过1h;复合加热的方式热控调节虽更为复杂,但可以进一步降低功耗。     

粉末溅射平面薄膜型SnO2/CeO2酒敏元件性能测试

给出了SnO2/10?O2(0.4mm×0.6mm×0.4mm)元件的温耗特性曲线,研究了老化的温度和时间,研究了气敏电流Ig与气体浓度C的关系,并给出了一个普遍适用的规律.     

ELID超精密镜面磨削钝化膜状态变化的研究

建立了ELID磨削系统的电解反应回路等效模型,提出用极间电流表征金属结合剂砂轮表面的钝化膜状态,分析了钝化膜在ELID超精密镜面磨削电解预修锐阶段、在线电解修整动态磨削阶段和光磨阶段的状态变化。     

Locating Current Sheets in the Solar Corona

Current sheets are essential for energy dissipation in the solar corona, in particular by enabling magnetic reconnection. Unfortunately, sufficiently thin current sheets cannot be resolved observationally and the theory of their formation is an unresolved issue as well. We consider two predictors of coronal current concentrations, both based on geometrical or even topological properties of a force-free coronal magnetic field. First, there are separatrices related to magnetic nulls. Through separatrices the magnetic connectivity changes discontinuously. Coronal magnetic nulls are, however, very rare. Second, inspired by the concept of generalized magnetic reconnection without nulls, quasi-separatrix layers (QSL) were suggested. Through QSL the magnetic connectivity changes continuously, though strongly. The strength of the connectivity change can be quantified by measuring the squashing of the flux tubes which connect the magnetically conjugated photospheres. We verify the QSL and separatrix concepts by comparing the sites of magnetic nulls and enhanced squashing with the location of current concentrations in the corona. Due to the known difficulties of their direct observation, we simulated coronal current sheets by numerically calculating the response of the corona to energy input from the photosphere, heating a simultaneously observed Extreme Ultraviolet Bright Point. We did not find coronal current sheets at separatrices but at several QSL locations. The reason is that, although the geometrical properties of force-free extrapolated magnetic fields can indeed hint at possible current concentrations, a necessary condition for current sheet formation is the local energy input into the corona.