Where is the base of the Transition Region? Evidence from TRACE,SDO, IRIS and ALMA observations

Classic solar atmospheric models put the Chromosphere-Corona Transition Region (CCTR) at $～2$ Mm above the ${\tau }_{5000}=1$ level, whereas radiative MHD (rMHD) models place the CCTR in a wider range of heights. However, observational verification is scarce. In this work we review and discuss recent results from various instruments and spectral domains. In SDO and TRACE images spicules appear in emission in the 1600, 1700 and 304 Å bands and in absorption in the EUV bands; the latter is due to photo-ionization of H i and He i, which increases with wavelength. At the shortest available AIA wavelength and taking into account that the photospheric limb is $～0.34$ Mm above the ${\tau }_{5000}=1$ level, we found that CCTR emission starts at $～3.7$ Mm; extrapolating to $\lambda =0$, where there is no chromospheric absorption, we deduced a height of $3.0\pm 0.5$ Mm, which is above the value of 2.14 Mm of the Avrett and Loeser model. Another indicator of the extent of the chromosphere is the height of the network structures. Height differences produce a limbward shift of features with respect to the position of their counterparts in magnetograms. Using this approach, we measured heights of $0.14\pm 0.04$ Mm (at 1700 Å), $0.31\pm 0.09$ Mm (at 1600 Å) and $3.31\pm 0.18$ Mm (at 304 Å) for the center of the solar disk. A previously reported possible solar cycle variation is not confirmed. A third indicator is the position of the limb in the UV, where IRIS observations of the Mg ii triplet lines show that they extend up to $～2.1$ Mm above the 2832 Å limb, while AIA/SDO images give a limb height of $1.4\pm 0.2$ Mm (1600 Å) and $5.7\pm 0.2$ Mm (304 Å). Finally, ALMA mm-$\lambda$ full-disk images provide useful diagnostics, though not very accurate, due to their relatively low resolution; values of $2.4\pm 0.7$ Mm at 1.26 mm and $4.2\pm 2.5$ Mm at 3 mm were obtained. Putting everything together, we conclude that the average chromosphere extends higher than homogeneous models predict, but within the range of rMHD models..     

新型凹入式螺旋结构增爆器的实验研究

本实验以脉冲爆震火箭发动机(简称PDREs)系统为实验平台,以液态航空煤油作为燃料,以压缩氧气作为氧化剂,以压缩氮气作为隔离气,分别对安装三种不同截面形式(半圆形、方形、三角形)的凹入式螺旋结构增爆器以及作为基准的Shchelkin螺旋结构增爆器进行了实验研究。实验结果表明,三种不同截面的凹入式增爆器均能有效强化爆燃向爆震转变(DDT)过程,在长径比为12.17的增爆器中均获得了充分发展的爆震波,实现了成功起爆。在流阻损失方面,半圆形凹入式螺旋结构表现出了最好的性能,其推力比Shchelkin螺旋的基准推力高出12个百分点。在多次实验过程中发现,凹入式螺旋结构比Shchelkin螺旋结构更不易烧蚀,工作可靠性更高。     

短切碳纤维增强环氧树脂形状记忆复合材料的制备与性能研究

为实现形状驱动能耗与复合材料力学性能的最佳配合，本文在热致环氧形状记忆聚合物基体中提高增韧剂新戊二醇二缩水醚（NGDE）含量来降低其玻璃化转变温度，同时添加短切碳纤维（SCF）来抵消由增韧剂引起的刚度降低负面效果。通过实验研究了不同NGDE、SCF含量对复合材料形状记忆转变温度、形状记忆性能和力学性能的影响。结果表明，增加NGDE含量可将环氧聚合物基体的形状记忆转变温度从90 ℃降至43 ℃，其储能模量和弯曲模量也随之降低。在11wt%NGDE上添加SCF后，复合材料的玻璃态储能模量、橡胶态储能模量、弯曲模量最高可提高至原始试样的1.9倍、7倍和2.4倍。     

冰晶粒子运动过程中的相变特性

针对冰晶在温暖环境下运动时固液汽耦合的相变现象，基于欧拉法建立了冰晶粒子的运动相变模型和计算方法。计算了冰晶粒子在强迫对流环境下的融化相变过程，与实验结果对比验证了运动相变模型和计算方法的准确性。针对NACA0012翼型计算了冰晶绕流运动时的热力学特性，得到了冰晶粒子到达撞击表面时的融化状态与收集系数。研究了冰晶粒径大小、初始球形度、气流相对湿度和温度对运动相变的影响。结果表明：冰晶粒子运动相变模型可以有效地评估冰晶结冰风险，冰晶粒子的融化速率主要取决于粒子直径、球形度、气流温度、湿度等因素，环境温度为288 K时冰晶粒子的融化时间为27.5 s，而相同条件下环境温度为302 K时的融化时间仅有5.2 s。     

Adjoint-based robust optimization design of laminar flow wing under flight condition uncertainties

It is an inherent uncertainty problem that the application of laminar flow technology to the wing of large passenger aircraft is affected by flight conditions. In order to seek a more robust natural laminar flow control effect, it is necessary to develop an effective optimization design method. Meanwhile, attention must be given to the impact of crossflow(CF) instability brought on by the sweep angle. This paper constructs a robust optimization design framework based on discrete adjoint methods ...     

被动型氢原子钟原子跃迁谱线测试与分析

被动型氢原子钟的原子跃迁谱线特性决定了其稳定度指标.为使其稳定度指标达到最优,通过设计数字式测试电路对氢原子钟物理部分进行探测,获得了不同参数配置下的原子跃迁谱线,并通过数据处理分析其信噪比、增益和线宽等特性,提出了一种参数优化方案,为原子钟闭环参数设置提供了依据.     

内并联型进气道模态转换过程中流道间干扰特性研究

针对组合动力进气道模态转换过程中存在的流道间干扰现象,采用数值模拟方法对一典型内并联型进气道模态转换过程中高/低速流道间的干扰特性展开了深入研究。结果表明：在模态转换过程中,当低速流道结尾激波位于低速流道内部时,高速流道节流至一定程度都将对低速流道形成干扰。该干扰现象出现后,高/低速流道的流动耦合,两流道的流量分配也随之发生变化,甚至导致了进气道流场的失稳。仅当β/α=0.25时,高/低速流道间的干扰造成了进气道流场的失稳且失稳后的振荡流场会先后出现两个不同的发展时期：前一时期的振荡流场的振幅较大但频率较低,约为335Hz；后一时期的振荡流场的振幅较小但频率较高,约为880Hz。