Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).     

基于高职院校视角的科研成果转化策略研究

针对高职院校科研成果转化率低的现状,从高职院校自身的视角出发,探讨促进科研成果转化的策略,以提高高职院校科研成果的转化率。     

Energy conversion of the flare due to direct electric fields from the sheared reconnection

In this paper we present a new mechanism of the main energy conversion of the solar flare. Since a flare inducing prominence (flux tube) rises V_z ? 300 km s⁻¹, the plasmas below it cannot continuously eject with Alfvén speeds of V_A = 3000 km s⁻¹ but probably with V_z ≈ ±100 km s⁻¹. Plasma up and downflows with V_A will within a short duration be blocked between the chromosphere where reconnected flux tubes are piling up, and the slowly rising flux rope. Hence the Petschek slow shock mechanism is difficult to be realized as a major energy converting mechanism.     

液相先驱体转化法制备ZrC粉末及合成机理

以氯氧化锆、丙醇、丙三醇和乙酰丙酮等为基本原料合成了锆的有机先驱体溶液,采用液相先驱体转化法在1 500℃制备了ZrC粉末。运用FTIR对锆的先驱体溶液的组成、结构以及形成机理进行了分析,用XRD和EDS分析了粉末的形成机理,用SEM观察了粉末的形貌。结果表明,有机锆的先驱体溶液具有螯和的链状或网状结构;先驱体溶液干燥后的粉末呈蜂窝状结构,在不同热处理温度下获得面心立方的ZrC粉末。经过热力学计算结果表明,C还原锆的氧化物开始生成ZrC的最低温度为1594℃,实验温度低于理论温度,在1500℃时获得面心立方的ZrC材料。     

基于特征映射的涡轮导向叶片精铸模型自动转换研究

通过对涡轮导向叶片及其精铸模型结构特点的分析,以特征映射理论为依据,提取其结构特征、特征内部的约束关系和构成特征的几何元素,将叶片的内外零件模型添加加工余量、工艺附件、收缩率后得到精铸模具设计和制造所需要的模具型腔体模型,从而完成了精铸模具设计各模型间的自动转换,大大缩短了精铸模具的设计周期,具有重要的理论和实践应用价值.     

有翼高超声速再入飞行器气动设计难点问题

有翼高超声速再入飞行器是近年来的研究热点,气动设计是飞行器设计的关键。为了更清楚地认识有翼高超声速再入飞行器气动设计的难点问题,对有翼高超声速再入飞行器的发展、优势及总体任务剖面进行了介绍,从5个方面详细介绍了该类飞行器气动设计的难点问题,包括多约束复杂面对称气动布局设计、高温真实气体效应对气动特性影响、天地差异与天地换算方法、反作用控制系统(RCS)喷流干扰对气动特性的影响以及气动数据不确定度等,简要阐明了这些难点问题对总体设计的重要性以及初步的解决思路,为有翼高超声速再入飞行器气动设计提供了一些参考。     

军品技改项目基准折现率确定方法研究

由于军品项目的特殊性，其基准折现率的确定方法与其他项目有所不同，要用以项目资金加权平均成本为基准，以项目整体风险系数为乘数来增加项目抗风险能力或作为投资风险补偿的基准折现率计算方法，其中，加权平均资金成本采用各种来源资金的资金成本的加权平均值（即全部资金的加权平均值），而在确定风险系数时则应结合军品技改的实际情况，充分考虑项目的风险因素，恰当地确定有关指标和权重。     

太阳能飞行器能源昼夜闭环仿真分析

以能量为核心，建立太阳能飞行器的获能模型；通过对太阳能飞行器飞行剖面特点的分析，设计飞行过程中各个阶段的飞行方案，并建立相应的耗能模型；考虑目前储能电池技术水平，根据产能和耗能模型，建立储能模型，完成了能源闭环模型的设计；参照Zephyr 7太阳能无人机的结构参数对论文建立的模型进行了仿真分析，获取了飞行过程中能量变化规律，同时对飞行姿态进行优化。结果表明：通过对太阳能飞行器昼夜飞行高度的不同设置以及飞行姿态角的优化，太阳能飞行器可以实现跨昼夜持久飞行。     

英汉构词法比较──《现代英语词汇学概论》及《现代汉语》读后感

本文就英汉构词的以下几种形式进行比较：合成、派生、转化、缩合、混合、外来词等。从而找出英汉构词的相似之处，帮助学习英语的人找出掌握英语词汇的捷径。     

Increased urinary excretion rates of serotonin and metabolites during bedrest

Astronauts are often on a voluntarily reduced energy intake during space missions, possibly caused by a metabolic or emotional stress response with involvement of the central serotonergic system (SES). We investigated 24 h urinary excretion (24 h-E) of serotonin (5-HT) and 5-hydroxyindol acidic acid as indicators of the SES in healthy males under two different normocaloric conditions: normal physical activity (NPA) and -6 degree head-down-tilt (HDT). HDT or NPA were randomly arranged with a recovery period of 6 months in between. 24 h-E of hormones varied widely among individuals. Values were higher in HDT compared to NPA. Assuming that the 24 h-E values are, beside being indicators for alterations in the number and metabolism of platelets. Also indicators of central SES, HDT condition seems to activate central SES in a higher degree compared to NPA. Therefore, changes in central SES might be involved in the mechanisms associated with space flight or microgravity, including possible maladaptations such as voluntary undernutrition.