螺旋线刃型电解阴极流场的数值模拟与结构优化

为了降低数控电解铣削时阴极流场的波动和不均匀性,提高工件的电解铣削加工精度和表面质量,针对叶轮电解铣削中螺旋线刃阴极结构,建立其流场模型,采用标准K-ε模型对叶轮加工时铣削阴极流场进行了动态模拟,分析了不同的内部流道结构和加工工艺参数对电解液流场速度和压力分布的影响,并结合模拟结果对阴极结构进行了改进。最后以叶轮为加工对象,在数控复合电解铣削加工中心进行了实验。实验结果验证了仿真模拟的有效性和正确性,为铣削用电解阴极结构的设计和改进提供了依据。     

空管人因失效概率的THERP-CREAM预测方法

管制员的人为差错是导致航空器空中相撞的主要原因之一,对空管人因失效概率进行有效预测是一个难题。为此,提出一种基于人误率预测技术（THERP）与认知可靠性和失误率分析模型（CREAM）的组合空管人因失效概率预测方法,基于THERP技术二叉树模型构建事故发展基本脉络,而后基于CREAM方法对各个人误行为触发概率进行修正,从而得出更为准确的概率预测结果。通过对相似事故进行对比分析,结果表明：本文提出的预测方法可识别关键性的事故影响因子,以便制定有针对性的管控措施,从而为研究预测空管人因失效概率提供了一种有效的分析手段。     

成败型产品可靠性评定指标与设计指标的关系

根据研制方与使用方在产品可靠性评定中风险率相等的原则，给出成败型产品可靠性评定指标与可靠性设计指标之间的关系，以及由设计指标确定评定旨标和由评定指标确定设计指标的方法。     

On the motions of RHESSI flare footpoints

The footpoint motions of flare hard X-ray (HXR) sources are directly related to the reconnection scenario of a solar flare. In this work, we tried to extract the information of footpoint motions for a number of flares observed with RHESSI. We found that the RHESSI flare results of the footpoint motions strongly support the classification proposed from the observations of YOHKOH/HXT. Furthermore, it is found that a flare can consist of two types of footpoint motions. We discussed the connections of the footpoint motions with the two-dimensional reconnection models.     

非相干有源诱偏抗反辐射武器效果分析

从反辐射武器导引头瞄准误差的角度,对非相干有源诱偏抗反辐射武器的干扰效果进行分析。     

A study on radio-loud interacting/non-interacting CMEs-associated SEPs and solar flares

We have established a data set of 58 major hybrid SEP events associated with meter-to-decahectometer wavelength (m-to-DH) type II bursts, solar flares, and radio-load CMEs during the period of 1997–2014. The main focus of our study is to address the following two questions: Does the interaction of CMEs play a role in the enhancement of SEP intensity? Is there any difference in the seed population, and parent eruptions in the SEP events with and without CME interactions? Hence, the sample of 58 events is classified into two sets: (i) 35 non-interacting-CME-associated SEP events; (ii) 23 interacting-CME-associated SEP events. All the characteristics of SEPs, their associated CMEs/flares and the relationships between them are statistically analyzed and compared. Some of the basic attributes and relative elemental abundances (Fe/O ratios) of the both the sets are also compared. The results indicate that the seed particles in non-interacting-CME-associated SEP events are mostly from solar wind/coronal materials. But in the case of interacting-CME-associated SEP events, it may be associated with both flare material from preceding flares and coronal materials from solar wind/preceding CMEs. The correlation studies reveal that there are clear correlations between logarithmic peak intensity of SEP events and properties of CMEs (space speed: cc?=?0.56) and solar flares (peak intensity: cc?=?0.40; integrated flux: cc?=?0.52) for non-interacting-CME-associated SEP events. But these correlations are absent for the interacting-CME-associated events. In addition, the results suggest that interaction of primary CMEs with their preceding CMEs plays an important role in the enhancement of peak intensity of SEPs at least for a set of m-to-DH type II bursts associated SEP events.     

不同叶片尾缘结构对流换热特性实验

为了研究不同叶片尾缘结构对对流换热系数的影响规律,设计了三种尾缘结构,并搭建了实验台,采用红外热像仪对叶片尾缘的壁温进行测量。研究结果表明,（1）三种尾缘结构的对流换热系数沿壁面的分布有很大差异,针对实验件I,对流换热系数存在一最大值,且最大值出现的位置随着吹风比的增加而逐渐远离气膜出口;（2）实验件II和III的对流换热系数沿壁面均呈现逐渐降低的趋势,但降低的规律二者又不相同;（3）在相同壁面位置,实验件III的对流换热系数最高,而实验件I的对流换热系数最低,因此可以认为,实验件III所示的尾缘结构更有利于对叶片尾缘更好的冷却。     

确定高速碰撞试验中碎片特性的测试技术

文章介绍了高速碰撞试验中碎片特性的几种测试技术,软捕获技术、照相技术、间接测量技术,及其适用情况。     

Particle acceleration and gamma rays in solar flares: Recent observations and new modeling

Experiments on SMM, GAMMA, Yohkoh, GRANAT, Compton GRO, INTEGRAL, RHESSI and CORONAS-F satellites over the past three decades have provided copious data for fundamental research relating to particle acceleration, transport and energetics of flares and to the ambient abundance of the solar corona, chromosphere and photosphere. We summarize main results of solar gamma-astronomy (including some results of several joint Russian–Chinese projects) and try to appraise critically a real contribution of those results into modern understanding of solar flares, particle acceleration at the Sun and some properties of the solar atmosphere. Recent findings based on the RHESSI, INTEGRAL and CORONAS-F measurements (source locations, spectrum peculiarities, ³He abundance etc.) are especially discussed. Some unusual features of extreme solar events (e.g., 28 October 2003 and 20 January 2005) have been found in gamma-ray production and generation of relativistic particles (solar cosmic rays, or SCR). A number of different plausible assumptions are considered concerning the details of underlying physical processes during large flares: (1) existence of a steeper distribution of surrounding medium density as compared to a standard astrophysical model (HSRA) for the solar atmosphere; (2) enhanced content of the ³He isotope; (3) formation of magnetic trap with specific properties; (4) prevailing non-uniform (e.g., fan-like) velocity (angular) distributions of secondary neutrons, etc. It is emphasized that real progress in this field may be achieved only by combination of gamma-ray data in different energy ranges with multi-wave and energetic particle observations during the same event. We especially note several promising lines for the further studies: (1) resonant acceleration of the ³He ions in the corona; (2) timing of the flare evolution by gamma-ray fluxes in energy range above 90 MeV; (3) separation of gamma-ray fluxes from different sources at/near the Sun (e.g., different acceleration sources/episodes during the same flare, contribution of energetic particles accelerated by the CME-driven shocks etc.); (4) asymmetric magnetic geometry and new magnetic topology models of the near-limb flares; (5) modeling of self-consistent time scenario of the event.     

基于过渡过程安排的PID控制器设计

分析了过渡过程安排法对PID控制的影响,提出了一种基于过渡过程安排法的PID控制器设计的新方法。针对航天器太阳电池板热真空试验,搭建温度控制系统,进行物理仿真实验。实验表明,该方法能够实现快速无超调控制,控制器参数选取方便,适应性、鲁棒性得到增强。