Langmuir Turbulence and Solar Radio Bursts

Langmuir waves and turbulence resulting from an electron beam-plasma instability play a fundamental role in the generation of solar radio bursts. We report recent theoretical advances in nonlinear dynamics of Langmuir waves. First, starting from the generalized Zakharov equations, we study the parametric excitation of solar radio bursts at the fundamental plasma frequency driven by a pair of oppositely propagating Langmuir waves with different wave amplitudes. Next, we briefly discuss the emergence of chaos in the Zakharov equations. We point out that chaos can lead to turbulence in the source regions of solar radio emissions. This revised version was published online in August 2006 with corrections to the Cover Date.     

空间环境下的有机热控涂层

本文综述了国外在空间有机热控涂层领域中的研究工作和试验，着重分析了空间极端环境中紫外光辐照和原子氧侵蚀这两大因素对有机热控涂层的影响。     

激光熔敷氧化锆热障涂层微观结构研究

采用5KW连续CO_2激光器对Ni基高温合金上二次重熔NiCoCrAlY和ZrO_2陶瓷层进行了研究。结果表明:激光快速熔化和凝固获得定向外延生长、紧密堆积的柱状晶氧化锆陶瓷层。NiCoCrAlY结合层与柱状晶之间存在氧化铝层,保证了柱状晶与NiCoCrAlY层的联结。激光重熔ZrO_2层由四方相和立方相组成,经快速冷却由高温保留至室温。     

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

High-Frequency Radio Signatures of Solar Eruptive Flares

Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects. This revised version was published online in August 2006 with corrections to the Cover Date.     

航天器空间辐射防护材料与防护结构

电子、质子、重离子、光子等空间辐射环境可在航天器材料或元器件中产生单粒子效应、总剂量效应、表面充放电效应、位移损伤效应、内带电效应等,因此,需要对航天器进行空间辐射防护。本文首先介绍空间辐射防护原理和防护有效性,进而从材料、分系统(或部组件)、航天器3个不同维度,对质量屏蔽防护材料、静电防护材料、抗辐射功能材料、航天器局部辐射防护结构和整星辐射防护结构进行了探讨,最后对未来发展的方向进行了讨论。     

测量透明位相物场的激光纹影-散斑干涉系统(英文)

本文给出了诊断相位场,如燃烧、对流、自由射流、超声速流场和等离子体等的一种激光纹影-散斑干涉系统。利用这套光学系统可在同一瞬时获得流场的散斑图和与之相应的剪切干涉图。作为实验,对一非定常波动的火焰(本生灯)进行了测试,实验表明用散斑照相术有可能得到密度波动的湍流场的定量结果;作为定量测试,对一沿竖直平板的自然对流,同时应用散斑照相和差纹影干涉术进行了定量分析,其结果的一致性很好。本文最后给出了散斑图的傅氏变换空间滤波的全场类似子纹影干涉图的流场显示照片。     

飞机隐身技术综述

本文根据最近几年有关部门对降低军用飞机雷达散射截面(RCS)的研究,对飞机隐身技术的问题作了综合性评述。全文分为二部分,第一部分为飞机隐身技术的发展概况,第二部分概括介绍各种飞机隐身技术的基本内容,最后论述了飞机隐身技术与飞机设计之间的密切关系。     

高焓风洞中钝体近尾流红外辐射测试技术

介绍在JF-10氢氧爆轰驱动高焓激波风洞中开展再人流场红外辐射测量的实验技术。风洞试验状态的驻室总压为19．6MPa，驻室总温为7920K。实验以球头钝锥体为试验模型，测量其近尾流红外辐射能量通量的横向分布。测量采用插入式锑化铟多元红外成像系统，波段范围为2．27-6．0μm。试验数据呈现明显的规律性。试验结果表明：利用这一测量技术能够提供高焓条件下有较高空间分辨率的、较为准确的红外实验数据。