Quiet sun XUV and EUV spectroscopy

The two XUV–EUV spectrometers on SOHO have collected a large amount of data in the 6000–10⁶ K solar plasma temperature range. These data have allowed us to greatly enhance our knowledge of the processes acting in the solar atmosphere, from the chromosphere to the corona. Some results on the quiet Sun structure (network, quiet Sun versus coronal hole), on the dynamics (velocities, waves, transient events), and the main characteristics of the quiet Sun atmosphere are presented and discussed.     

Radio Emissions from Solar Active Regions

Solar active region coronae are known for strong magnetic fields permeating tenuous plasma, which makes them an ideal astronomical laboratory for magnetohydrodynamics research. It is, however, relatively less known that this physical condition also permits a very efficient radiation mechanism, gyro-resonant emission, produced by hot electrons gyrating in the coronal magnetic field. As a resonant mechanism, gyro-emission produces high enough opacity to fully reveal the coronal temperature, and is concentrated at a few harmonics of the local gyrofrequency to serve as an excellent indicator of the magnetic field. In addition, the polarization of the ubiquitous free–free emission and a phenomenon of depolarization due to mode coupling extend the magnetic field diagnostic to a wide range of coronal heights. The ability to measure the coronal temperature and magnetic field without the complications that arise in other radiative inversion problems is a particular advantage for the active region radio emissions available only at these wavelengths. This article reviews the efforts to understand these radiative processes, and use them as diagnostic tools to address a number of critical issues involved with active regions.     

Magneto-gravity Waves Trapped in the Lower Solar Corona

The possibility of trapped magneto-gravity waves in the lower solar corona with an open magnetic field is discussed. Intensity variations and/or Doppler shifts of relevant UV, EUV and x-ray spectral lines in the chromosphere, transition region and lower corona may reveal the existence of such low-frequency modes (with periods longer than ∼ 1.5 hour). The spectrum may be either discrete or continuous depending on the reflection property of the narrow transition region. These modes can be utilized to probe the dynamics of the upper chromosphere, transition region and lower corona; they may also play an important role in coronal heating. This revised version was published online in June 2006 with corrections to the Cover Date.     

某型飞机发电机供电系统一起典型故障的分析

分析了在维修过程中某型飞机发电机供电系统的一起典型故障的原因,详述该故障排除的过程,以及通过此故障的排除获得的两点启示。     

卫星电源系统短路暂态特性分析及对策

针对卫星电源系统短路故障导致母线电压跌落、业务中断甚至整星失效的问题,分别采用电路模型和数学模型的方法对短路后母线电压的暂态特性进行分析,指出故障持续过程经历母线电容放电、太阳电池阵动作、放电调节器动作、蓄电池经二极管直接供电这4个阶段,分析了各阶段母线电压的暂态响应及转换条件。随后,研究了发生稳态电压跌落的条件及其影响因素。针对航天器通常使用的快速熔断器保护,分析了母线电压跌落受熔断I~2T、短路通路阻抗、蓄电池内阻、蓄电池开路电压的影响程度。依据暂态特性的分析,提出接地优化方法以及蓄电池开路电压、短路通路阻抗和欠压保护点的配合设计方法,使得短路暂态过程母线电压跌落程度满足系统关键单机运行的需求。     

Experimental Investigation of the Effects of Various Plasma Actuator Configurations on Lift and Drag Coefficients of a Circular Cylinder Including the Effects of Electrodes

In this paper, the effects of the existence of plasma actuator electrodes and also various configurations of the actuator for controlling the flow field around a circular cylinder are experimentally investigated. The cylinder is made of PVC (Polyvinyl Chloride) and considered as a dielectric barrier. Two electrodes are flush-mounted on the surface of the cylinder and are connected to a DC high voltage power supply for generation of electrical discharge. Pressure distribution results show that the existence of the electrodes and also the plasma are able to change the pressure distribution around the cylinder and consequently the lift and drag coefficients. It is found that the effect of the existence of the electrodes is comparable with the effect of plasma actuator in controlling the flow field around the cylinder and this effect is not reported by other researchers. Eventually it is concluded that the existence of the electrodes or any extra objects on the cylinder and also the existence of the plasma are capable of changing the flow field structure around the cylinder so that the behavior of the lift and drag coefficients of the cylinder will be changed significantly.     

适用于航天领域的高效叠加式升压变换器

叠加式升压变换器（SBC）的部分功率不通过开关电路,而通过叠加支路直接供给负载,因此可实现较高的效率,适用于航天场合。为了避免输入输出电流断续,采用的变压器为双边磁化的隔离脉冲单元,它与电感、输出滤波电容以及叠加支路共同组成SBC变换器。根据电感位置的不同,分别提出了SBC-Ⅰ、SBC-Ⅱ和SBC-Ⅲ的基本结构与生成规则。基于生成规则推衍出9种SBC变换器,并从电流特性、输入输出电压关系、主电路传递函数、变压器的磁偏问题以及效率的角度对这9种变换器进行分析比较。最后选择一种性能最优的变换器,通过600 W的实验样机验证理论分析结果。     

叶栅等离子体流动控制布局优化和影响规律

为提高流动控制能力,基于高负荷压气机叶栅的流场特性和等离子体气动激励特性,对等离子体流动控制的激励布局进行优化,通过选取典型激励布局,实验揭示了不同因素对等离子体气动激励抑制叶栅流动分离的影响.结果表明:吸力面激励布局中,靠近前缘流向激励的作用效果强于展向激励和尾缘激励,沿流向分布多组电极的激励效果最佳;端壁激励布局中,横向激励的作用效果明显强于流向激励;组合激励布局中,基于端壁横向激励和吸力面流向激励的组合布局的激励效果最佳.等离子体气动激励的作用效果随着激励电压的增大而增强,随着攻角的增大其作用效果先增强后变弱;变定常激励为非定常激励,通过耦合流动的不稳定性,可以提高等离子体气动激励流动控制效果.      

高温气冷堆核电站主氦风机驱动电机绝缘系统评定技术研究

设计了一套在0.1 MPa氦气和空气环境下测试绝缘系统电气绝缘性能的试验装置,完成了0.1 MPa气压下氦气和空气中主氦风机驱动电机绝缘系统模型的局部放电起始电压(PDIV)、起晕电压、匝间冲击、绝缘电阻和工频击穿电压对比试验。试验结果表明:在0.1 MPa气压下,绝缘系统在氦气环境下的部分绝缘性能较空气中大幅下降,氦气环境下绝缘系统的PDIV值约为空气中的50%,起晕电压值约为空气中的20%~25%, 闪络(击穿)电压约为空气中的50%。