太阳耀斑硬X射线能谱演变特征

太阳硬X射线是耀斑高能电子束流与太阳大气相互作用产生的韧致辐射,根据简单的太阳耀斑环物理模型,假定具有流量与能谱同步变化的高能电子束流从耀斑环顶部注入,计算了硬X射线辐射在不同的靶物质密度区的能谱演变特征。结果表明:硬X射线辐射在低大气密度靶区呈现软一硬一硬的能谱演变特征,在高密度靶区硬X射线能谱则具有软一硬一软的变化特征。高能电子束流持续时间影响谱型转变区域在耀斑环中的高度。     

Magnetospheric and ionospheric manifestations of interplanetary foreshocks

The geometry of a typical interplanetary shock front in the vicinity of the Earth’s orbit predicts that the leading edge of the foreshock region comes into contact with the magnetosphere a few hours ahead of geomagnetic sudden impulses (SI). There is reason to believe that the interaction of the magnetosphere with the foreshock leads to magnetic and ionospheric disturbances, which can be detected by ground-based instruments. We searched for specific precursors of SIs in data from the Scandinavian riometer network and in the short period geomagnetic pulsation data from mid-latitude magnetometers. We found that SIs were preceded by the following three features: (1) an increase in riometric absorption, (2) excitation of Pcl magnetic pulsations and (3) a spectral broadening of the Pc3 magnetic pulsations. Our observations may be useful for the study of acceleration processes in the solar wind. These observations are also of potential forecasting interest.     

双损耗Al2O3基多孔吸波材料的制备及其吸波性能

基于片状Al₂O₃陶瓷互锁结构强度高的特点,制备出夹杂石墨的高气孔率的Al₂O₃多孔陶瓷,并通过原位还原在多孔骨架中制备出Ni微粒,形成一种轻质的双损耗陶瓷基吸波材料。通过XRD、FE-SEM和EDS研究了还原温度对多孔吸波材料的组成、微观形貌、元素分布和吸波性能的影响。结果表明,还原温度升温至700 ℃可将多孔网络中Ni完全还原,形成以堆叠互锁Al₂O₃为基,夹杂片状石墨和孔表面覆盖Ni微粒的双损耗轻质吸波材料。当复合材料厚度为6.5 mm时,最小反射损耗为-35.01 dB,有效吸收带宽达到1.75 GHz。片状Al₂O₃锁定的石墨片构筑的导电网络,Ni微粒与基体之间的极化效应等共同促进复合材料良好的微波吸收性能。     

连续型和非连续型蜂窝芯材的共振吸声结构性能研究

以芳纶纸蜂窝、内嵌树脂隔板和微穿孔面板为原料,制备了连续和非连续双自由度共振吸声结构,对两种共振吸声结构的力学性能和吸声系数进行对比研究。结果表明：连续蜂窝芯材所制备共振吸声结构的压缩和拉伸性能高于非连续型共振吸声结构,其中非稳定型压缩强度和拉伸强度高19%,稳定型压缩强度高32%,稳定型压缩模量高43%,剪切性能基本相当;两层蜂窝芯材容易出现孔格错位（非连续型共振吸声结构）,引起错位区域的微孔堵塞,使该结构的共振吸收峰与理论值出现较大差异。     

Plastic wrinkling model and characteristics of shear enforced Ti-alloy thin-walled tubes under combination die constraints and differential temperature fields

Plastic wrinkling predictions and shear enforced wrinkling characteristics of Ti-alloy thin-walled tubes under combination die constraints have become key problems urgently in need of solutions in order to improve forming quality in their shear bending processes under differential temperature fields. To address this, a wrinkling wave function was developed by considering their shear bend deformation characteristics. Based on this wave function and the thin shell theory, an energy prediction model for this type of wrinkling was established. This model enables considera-tion of the effects of shear deformation zone ranges, material parameters, loading modes, and fric-tion coefficients between tube and dies on the minimum wrinkling energy. Tube wrinkling sensitive zones (WSZs) can be revealed by combining this wrinkling prediction model with a thermal-mechanical coupled finite element model for simulating these bending processes. The reliability of this wrinkling prediction model was verified, and an investigation into the tube wrinkling char-acteristics was carried out based on the experimental conditions. This found that the WSZs are located on either a single side or both sides of the maximum shear stress zone. When the friction coefficients between the tube and the various dies coincide, the WSZs are located on both sides. The larger the value of the tube inner corner radius and/or the smaller the value of the outer corner radius, the smaller the wrinkling probability. With an increase in the value of the moving die dis-placement, the wrinkling probability increases at first, and then decreases.     

原子吸收光谱法测定热电池隔离粉中镁

提出用一氧化二氮－乙炔火焰原子吸收光谱法测定热电池隔离粉中镁。介绍镁的最佳测定条件并具有良好线性范围的浓度，并对样品消化处理条件、干扰因素进行了综合考虑。该方法灵敏度高、重现性好，同时具有方法步骤简单、操作容易掌握等特点，达到了实验室分析质量控制的要求。     

红外气体分析中环境影响的补偿方法研究

环境温度、总压影响是红外气体分析中难以有效解决的主要问题之一，本文以二氧化碳气体为测量对象，采用实验手段，单片机和数据自理技术建立了环境温度、总压对红上气体分析影响的补偿数学模型和求解方法，并进行了实验验证，研究的内容为红外气体分析中影响影响的外补偿开始辟了一条新的途径，具有广阔的应用前景。     

大气行星波影响低频电波吸收变化的机制

本文根据冬季中低纬低电离层中、低频（ＬＦ）电波振幅扰动与高纬平流层中大气行昨波活动密切相关的观测事实，分析研究了可能引起低电离层对ＬＦ电波吸收变化诸因素的作用后，提出了一种能较好地解释观测现象的物理机制，大气行星波可通过两种方式改变大气离化率ｑ，因而引起低电离层中电子密度Ｎ扰动，进而改变由Ｎ大小决定的电离层电波吸收值，结果导致ＬＦ电波振幅发生相应变化。文中给出了描述这一物理计算公式和某些计算结果。     

平流层飞艇的能源技术和平衡分析

平流层飞艇作为近空间对地观测平台的一种实现方案，主要依靠自身庞大体积产生的静浮力而不像其它飞行器依靠相对空气运动产生升力，所以飞艇能够以较慢的速度飞行甚至能够在空中长期保持定点悬停即相对地面静止。具有长时间在平流层自主飞行的能力，是平流层飞艇设计的一个重要目标。文章对平流层飞艇能源系统的构成、部件及能源平衡分析方法作了介绍。     

末端能量管理段迭代校正轨道算法研究

针对航天器进入末端能量管理段接口处时位置和航迹偏角存在大范围摄动的问题，提出一种使用迭代校正法的轨道快速生成算法。该算法可以根据航天器的具体初始状态，自动选择直接进场或者间接进场策略，快速生成可行的参考轨迹。首先通过跟踪轨迹地面投影实现侧向制导；根据末端能量管理段的起始点与终点的高度与速度约束生成参考动压-高度剖面，并跟踪此剖面实现纵向制导。然后采用迭代校正计算快速确定航向校准柱的位置与最终半径两个参数用以调整航程，保证航天器在末端的所有状态满足自动着陆段接口的边界约束。仿真结果校验了该算法可以根据航天器的具体状态快速生成符合约束条件的末端能量管理段飞行轨道，具有很好的鲁棒控制性能。