On bandwidth of solar subsecond bursts in cm-range

The goal is to study parameters of drifting type III bursts, and find out the emission mechanism of these bursts and understand what factors affect instantaneous spectral bandwidth of these bursts.     

浅谈船舶柴油机排放污染及控制对策

本文论述了船舶柴油机废气排放对大气污染的影响，介绍了IMO（国际海事组织）对船舶柴油机排放的控制要求，以及国内外柴油机研究机构和制造公司所采取的对策。     

双栅极空气计数器系统参数优化设计方法

 基于金属材料微裂纹检测传感器系统放电脉冲的形成过程, 建立了离散化放电的数学模型, 提出了传感器系统参数优化设计的一种新方法。实验结果表明, 采用该理论设计的传感器系统参数, 避免了经验公式设计的片面性, 保证了传感器系统无损检测的可靠性和精确性。     

声发射监测钻头折断的实验研究

 金属切削过程中会发出声讯号。用声发射技术监测刀具破损是一个很有潜力的新方法。本文研究了声发射技术在钻头折断在线监测中的应用。实验结果表明,所设计的实验监测系统能可靠地监测钻头的折断,并可提前预报直径大于1.5mm钻头的折断。     

喷射角对涡轮叶栅端壁气膜冷却的气动影响

在大尺寸低速平面叶栅风洞中,对前缘上游有单排气膜孔的涡轮导向叶栅端壁气膜冷却进行了气动实验。在喷射角25°,35°和45°以及吹风比1,2,3下详细测量了叶栅通道中的三维流场,得到了全速度和二次流速度分布,并由此计算了二次流动能的大小。着重研究了喷射角对端壁气膜冷却的气动特性和对叶栅通道中特别是端壁附近的流场结构的影响。数据表明减小喷射角度可以减小通道涡的强度和尺寸,使冷气射流核心更贴近壁面,但同时也明显地增大了壁面附近的气流速度。在高吹风比下,35°喷射时射流将冷气输运到压力边的能力比25°喷射和45°喷射都要强。     

3He-Rich Solar Energetic Particle Events

³He-rich solar energetic particle (SEP) events show huge enrichments of ³He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these events: the particle energy spectra are found to be either power-law or curved in shape, with the ³He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near ∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the new insights found in the last few years.     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.     

不同磁暴条件下GEO卫星表面充电电位分布

文章利用1989-2004年间"Los Alamos"7 颗地球同步轨道卫星的数据对不同磁暴条件下处于地球同步轨道高度等离子体片区域的卫星表面充电电位和热电子(0.03~45 keV)温度随地方时的分布及随磁暴发生时间的变化规律进行统计分析.根据对磁层顶电流修正后的Dst指数(Dst*)将磁暴分成弱磁暴、强磁暴以及超大磁暴.在随地方时的分布上,弱磁暴时卫星最可能在午夜后侧负向强充电(＞800 V);随着磁暴强度的增加,在超大磁暴情况下该区域会沿东西方向扩展到夜晚21时到凌晨4时的区域.在随磁暴发生时间的分布上,弱磁暴下卫星表面充电到高负电位主要发生在Dst*最低点前3 h和后2 h的时刻,强磁暴下主要发生在Dst*最低点时刻,而超大磁暴下主要发生在恢复相,持续时间达十几个小时.表面电位的分布规律和热电子温度的分布规律表现一致:卫星表面负电位超过100 V的区域主要集中在热电子温度大于2 keV的区域,而表面负电位最可能超过800 V的区域主要集中在热电子温度大于2.5 keV的区域.通过统计分析看出,对于那些极可能发生高负电位充电(＞8 kV)情况下的卫星表面电位分布与磁暴的强弱并无明显的相关性,但发现在弱磁暴情况下明显集中在正午前侧区域.     

探月返回飞行器跳跃式再入轨迹优化

基于节点自适应稀疏配点法,提出一种高精度求解探月返回飞行器跳跃式再入轨迹优化问题的方法.该方法的基本策略是:首先,应用节点自适应稀疏配点法对完整的跳跃式再入轨迹进行优化;然后,根据优化得到的控制变量对再入动力学方程进行数值积分;当积分至跳跃轨迹的最高点时,以积分得到的状态变量值作为新的初始条件,对二次再入轨迹重新优化....