激光陀螺磁特性研究

本文分析了激光陀螺磁敏感原理,研究了腔内激光束椭偏度的产生机理,设计了高消光比激光束椭偏度测量系统。实验结果表明,激光陀螺磁灵敏度大小与磁场方向有关,输出激光束的椭偏度越大,磁灵敏度越大。研究表明,通过减小输出激光束的椭偏度,可减小激光陀螺磁灵敏度,从而增强激光陀螺环境适应性,提高激光陀螺的成品率。     

Driving major solar flares and eruptions: A review

This review focuses on the processes that energize and trigger M- and X-class solar flares and associated flux-rope destabilizations. Numerical modeling of specific solar regions is hampered by uncertain coronal-field reconstructions and by poorly understood magnetic reconnection; these limitations result in uncertain estimates of field topology, energy, and helicity. The primary advances in understanding field destabilizations therefore come from the combination of generic numerical experiments with interpretation of sets of observations. These suggest a critical role for the emergence of twisted flux ropes into pre-existing strong field for many, if not all, of the active regions that produce M- or X-class flares. The flux and internal twist of the emerging ropes appear to play as important a role in determining whether an eruption will develop predominantly as flare, confined eruption, or CME, as do the properties of the embedding field. Based on reviewed literature, I outline a scenario for major flares and eruptions that combines flux-rope emergence, mass draining, near-surface reconnection, and the interaction with the surrounding field. Whether deterministic forecasting is in principle possible remains to be seen: to date no reliable such forecasts can be made. Large-sample studies based on long-duration, comprehensive observations of active regions from their emergence through their flaring phase are needed to help us better understand these complex phenomena.     

磁响应Fe3O4/HCS复合微球的制备及特性

由壳聚糖与环氧丙烷制备了羟丙基壳聚糖(HCS)。将其配制成水溶液,利用离子凝胶法,与多聚磷酸钠(TPP)反应,制备了粒径在0.6μm羟丙基壳聚糖微球。再用滴定水解法制备了四氧化三铁微粒,激光粒度分析显示滴定水解法制备的Fe3O4粒径分布较窄,粒径小。在此基础上采用交联聚合法制备了Fe3O4/HCS复合微球,微球为实心,四氧化三铁微粒被包裹于微球内部,形状规则,粒径约为0.8μm,经过磁响应分析表明Fe3O4/HCS复合微球具有磁响应性。     

温度对磁屏蔽霍尔推力器磁场构型的影响研究

霍尔推力器磁路设计主要通过常温静态磁场仿真得到，并实测推力器非工作状态常温磁场进行复核。大功率霍尔推力器将面临更为严峻的热问题，推力器工作时磁路系统受高温影响，因此在常温下仿真得到的磁场位形会因温度升高而产生偏移，不能反映推力器真实工作时的磁场情况。为研究霍尔推力器工作时热量对磁路系统的影响，通过热磁耦合仿真对10kW磁屏蔽霍尔推力器的热态磁场分布进行研究，并对热态、常温仿真结果进行了对比，发现在阳极附近的径向磁感应强度Br的差异比放电室出口更大。常温设计的磁屏蔽构型在热态时偏离磁屏蔽，磁场和壁面最大不符合度达到13%，通过陶瓷出口型面修正后重新获得磁屏蔽效果，使最大不符合度降低到4.8%以下。合理热设计有助于降低热载荷，热仿真得到磁路系统最高温度低于500℃，低于0.78倍的居里温度Tc磁性急剧转变点，不会出现磁性能急剧下降，但热量对磁屏蔽霍尔推力器磁场构型的影响是应该考虑的。     

车载中频高速同步发电机设计

对车载中频高速同步发电机设计思路和设计特点进行阐述。根据设计思路和设计特点制造了试验样机,在制造过程中着重对磁极线圈的绑扎与固定、三相旋转整流器的内部结构做了改进。进行了电机性能的试验分析,对采取的技术措施进行验证,验证了设计方法的有效性。这为同类电机设计提供了参考。     

复合舵机本体精密加工技术

复合舵机是控制系统中重要的执行部件，在航空航天等领域有着广泛的应用。针对行业内复合舵机本体工艺流程冗长、数控化程度低、生产效率低等问题，开展了本体新工艺的研制。在分析复合舵机本体结构特点和加工难点的基础上，采用了数控加工与精密研磨相结合的加工方法，设计了加工工艺流程和专用装夹工装，配置了本体活塞孔精密研磨所需研磨膏，通过试验验证了工艺流程的可行性。工艺验证结果表明，本体活塞孔圆柱度不大于0.002mm，表面粗糙度在Ra0.05μm以下，在内窥镜下观察无可见划痕。自配研磨膏在研磨加工中使用效果显著，所设计工艺流程合理可行。     

Detailed magnetic structure and stochastic threshold

Non-linear evolution of reconnection is too slow to explain-by itself-fast phenomena such as internal disruptions in tokamaks or flares in the solar atmosphere. It has been proposed that the change in topology could lead to field line stochastization, and hence to highly increased transport. An important objection to this idea is that the increase of transport coefficients should smoothly follow the amplitude of the perturbation, while the observations show a catastrophic transition. We have shown 1) that the shape of the structures (and not only their size or amplitude) evolve during non-linear evolution 2) that the stochastic threshold can be strongly influenced by the detailed shape. Therefore, sharp transitions can appear during the evolution, due to the combination of these two effects. We will first consider an idealized situation, namely the two-waves problem in slab geometry, for which we will study the effect of the separatrix shape on the stochastic threshold. In the second part, we will present an application to the internal disruption in tokamaks, with anm=1 perturbation in a toroidal magnetic configuration. In the last part, we will discuss possible applications of the studies on shape effects to the behaviour of trapped particles in structures of the solar atmosphere.     

CO2焊外加纵向磁场的数值计算

针对CO2焊时与电极同轴的单个轴对称空心圆柱线圈在励磁电流作用下产生的外加磁场，采用积分方程法建立了磁控CO2焊外加纵向磁场的计算模型，对CO2焊外加磁场进行了数值计算，该方法具有模型简单、计算速度快和精度高等优点，并与实际测量结果进行了比较。计算及实验结果表明，利用所建模型计算得出的外加纵向磁场分布是准确的、可靠和有效的。     

Latitude and solar-cycle dependence of radial IMF intensity

I describe a simple procedure for extrapolating the observed solar magnetic field into the heliosphere, which averages the asymptotic fields computed using the standard source surface and current sheet models. The resultant field is characterized by strong latitudinal gradients (maintained by volume currents outside the source surface) and by abrupt reversals in direction at the current sheets. The model yields good agreement with the observed long-term variation of the radial IMF component in the ecliptic, and is used to predict the variation of |B _r | along the latitudinal trajectory of Ulysses during 1990–1994. As found in earlier studies, the magnitude ofB _r at any latitude is determined largely by the strength and relative orientation of the Sun's dipole moment.     

X波段波导端头裂缝的数值分析

用矩量法(MOM)导出求解X波段波导端头裂缝口面等效磁流的公式。在此基础上,计算波导不同频率下的反射系数和驻波系数等参数。给出了BJ-100波导端头裂缝口参数的计算结果,据此讨论了裂缝长度、宽度、厚度与谐振频率的关系。另外检验了圆头与方头裂缝的等效性,并给出了波导端头裂缝谐振频率的近似设计公式。分析结果表明,该算法简单,计算结果与测试值吻合较好。