基于粒子群优化算法的不完全数据的处理

不完全信息下的数据挖掘是一个困难的问题,但它在实际决策中是不可避免的。在介绍几种处理方法的基础上,提出了基于粒子群优化算法的处理方法。对适应函数进行了讨论,实例表明该方法比较有效。     

采用非均匀反弹特性壁面的粒子分离器研究

为了在不改变流道几何型面的基础上实现对较大粒径砂尘轨迹的有效组织,借助数值仿真技术,对一类典型无旋式惯性粒子分离器流道内两相流场展开了模拟研究。通过对典型工况下粒子分离器内砂尘轨迹的追踪和细致分析,首先获得了壁面反弹主导下的较大粒径砂尘的三类基本运动模式及其主要特征。而后以此为基础,充分利用2024铝合金、7020橡胶以及45钢3种典型壁面在反弹特性上的差异,同时结合原流道型面,完成了一种基于非均匀壁面的粒子分离器方案设计。计算表明:通过对鼓包迎风面等关键区域的壁面材质的特殊设计,可在不降低气动性能的前提下实现AC砂及C砂分离效率的显著提升,其增幅分别为6.0%和13.7%。      

Are small-scale field-aligned currents and magnetosheath-like particle precipitation signatures of the same low-altitude cusp?

We examined some 75 observations from the low-altitude Earth orbiting DMSP, Ørsted and CHAMP satellites which were taken in the region of the nominal cusp. Our objective was to determine whether the actually observed cusp locations as inferred from magnetosheath-like particle precipitation (“particle cusp”) and intense small-scale magnetic field variations (“current cusp”), respectively, were identical and were consistent with the statistically expected latitude of the cusp derived from a huge number of charged particle spectrograms (“statistical cusp”).     

Spectroscopic analysis of the solar flare event on 2002 August 3 with the use of RHESSI and RESIK data

We use simultaneous observations from RESIK and RHESSI instruments to compare plasma properties of a major solar flare in its rise and gradual phase. This event occurred on 2002 August 3 (peak time at 19:06 UT). The flare had a very good coverage with RESIK data and well-resolved soft and hard X-ray sources were seen in RHESSI images. Spectra of X-ray radiation from RHESSI images are studied and compared with RESIK measurements in different flare phases. Result shows large differences in flare morphology and spectra between flare rise and gradual phase.     

Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.     

Using gamma-ray burst prompt emission to probe relativistic shock acceleration

It is widely accepted that the prompt transient signal in the 10 keV–10 GeV band from gamma-ray bursts (GRBs) arises from multiple shocks internal to the ultra-relativistic expansion. The detailed understanding of the dissipation and accompanying acceleration at these shocks is a currently topical subject. This paper explores the relationship between GRB prompt emission spectra and the electron (or ion) acceleration properties at the relativistic shocks that pertain to GRB models. The focus is on the array of possible high-energy power-law indices in accelerated populations, highlighting how spectra above 1 MeV can probe the field obliquity in GRB internal shocks, and the character of hydromagnetic turbulence in their environs. It is emphasized that diffusive shock acceleration theory generates no canonical spectrum at relativistic MHD discontinuities. This diversity is commensurate with the significant range of spectral indices discerned in prompt burst emission. Such system diagnostics are now being enhanced by the broad-band spectral coverage of bursts by the Fermi Gamma-Ray Space Telescope; while the Gamma-Ray Burst Monitor (GBM) provides key diagnostics on the lower energy portions of the particle population, the focus here is on constraints in the non-thermal, power-law regime of the particle distribution that are provided by the Large Area Telescope (LAT).     

激励频段对航天器随机振动载荷的影响

在航天器随机振动等效准静态载荷计算中,高频因对随机振动载荷的贡献较小而可以被截去,但目前截止频率的选择还未有完全确定。为确定随机振动环境下的计算频段,文章设计了不同动态特性的组件进行不同截止频率的随机振动试验,并根据试验数据分析研究了不同特性组件在不同振动频段下应变的变化规律。研究结果认为,对于一般组件,随机振动的计算截止频率可取为组件主频率的1.5倍。针对非均匀输入加速度谱的随机振动载荷计算问题,文章提出分频段的分析方法。按3个基本频段计算随机振动载荷,分析得到了不同频段对总随机振动载荷贡献大小和规律,以及截止频率误差的影响因素和影响大小。算例表明,分频段法可以用于不同状态输入加速度谱的随机振动载荷计算。