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.     

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。     

焊接方式对铝合金搅拌摩擦焊T 型接头性能的影响

采用4种规格的搅拌头进行了2A70-T6铝合金T型接头搅拌摩擦焊试验,并对焊缝横截面进行了观察以及焊缝抗拉强度的测试.结果表明:焊缝中前进侧熔合过渡区的金属变形比返回侧剧烈,焊缝断裂往往发生在前进侧;在相同的焊接参数下,单道焊缝的焊核宽度与抗拉强度随着搅拌针直径的增大而增大,但增大的幅度较小,并列焊的焊缝抗拉强度仅为单道焊缝的93％左右;为了获取相同宽度的焊核,采用加粗搅拌针单道焊比并列焊更具有优势.     

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。     

基于多相关器的GPS信号质量监测技术

导航卫星的信号质量是影响系统定位性能的一个关键因素,当卫星自身硬件设备或空间传播信号受到干扰时,会导致卫星信号波形失真,用户接收机的伪码相关器产生的相关峰会产生偏差,造成定位精度下降;情况严重时,会使用户失去定位能力。因此,通过对空间信号的监测可以进一步保障系统的服务性能。文中借鉴现有的信号质量监测技术,对GPS信号失真的原因进行了总结,按照TMA、TMB和TMC完成失真信号的建模,并定性分析了对测距的影响。给出基于多相关器的导航信号质量监测方法,使用上述三种模型验证了该判定方法的有效性。     

偏二甲肼组分变化对火箭发动机稳态工作性能的影响

通过建立液体发动机稳态工作模型与热力计算模型,利用最小二乘优化与迭代计算的方法,仿真研究了被空气部分氧化的偏二甲肼(UDMH)对泵压式液体火箭发动机的影响规律。结果表明,随着UDMH中二甲胺、偏腙和水含量的增加,推进剂混合比略有升高,发动机推力、燃烧室压强和燃烧室温度等参数有较明显下降。与传统地单纯分析推进剂能量性能相比,此方法更能准确表征在火箭发动机系统复杂的调节机制作用下,变质推进剂对发动机工作性能的影响。