发动机尾焰注水降温数值计算与试验研究

针对火箭发动机尾焰注水流场,组织并实施了火箭发动机系留点火及燃气流场注水降温缩比试验,研究了燃气冲击射流流场和注水作用下两相流场的分布状态以及降温效果。并通过研究在高温高速对流冲击作用下气液两相流的传热和传质理论,在Mixture多相流模型的基础上添加质量和能量源项,建立了多组分气液两相流非定常数值计算模型,通过对比试验结论,结果表明：所建立的数值计算模型具有较高的计算精度和可靠性,能够准确地反映物理现象。利用数值计算模型研究了注水后燃气、液态水和水蒸气三种主要组分在流场中的组成,通过与自由射流对比得到了注水燃气流场的包络线长度与宽度变化,注水对燃气流场降温效果显著。     

Water movement on the convex surfaces of porous media under microgravity

A plant growth system for crop production under microgravity is part of a life supporting system designed for long-duration space missions. A plant growth in soil in space requires the understanding of water movement in soil void spaces under microgravity. Under 1G-force condition, on earth, water movement in porous media is driven by gradients of matric and gravitational potentials. Under microgravity condition, water movement in porous media is supposed to be driven only by a matric potential gradient, but it is still not well understood. We hypothesized that under microgravity water in void spaces of porous media hardly moved comparing in void spaces without obstacles because the concave surfaces of the porous media hindered water movement. The objective of this study was to investigate water movement on the convex surfaces of porous media under microgravity. We conducted parabolic flight experiments that provided 20–25?s of microgravity at the top of a parabolic flight. We observed water movement in void spaces in soil-like porous media made by glass beads and glass spheres (round-bottomed glass flasks) in the different conditions of water injection under microgravity. Without water injection, water did not move much in neither glass beads nor glass spheres. When water was injected during microgravity, water accumulated in contacts between the particles, and the water made thick fluid films on the particles surface. When the water injection was stopped under microgravity, water was held in the contacts between the particles. This study showed that water did not move upward in the void spaces with or without the water injection. In addition, our results suggested that the difficulty of water movement on the convex (i.e. particle surfaces) might result in slower water move in porous media under microgravity than at 1G-force.     

利用低轨道卫星间微波信号探测反演温湿廓线

通过同时测量微波信号的折射和吸收信息,低地球轨道卫星间（LEO-LEO）微波掩星探测技术能够独立反演温度和水汽廓线。通过仿真手段,首先,正演模拟了微波信号穿过大气层后由折射和吸收效应分别导致的相位延迟和振幅衰减,在此基础上,对温度、水汽和云中液态水反演廓线进行了个例分析,然后,统计分析了温度和水汽在不同纬度带的反演性能,以及云对反演精度的影响。结果表明：温度在约35 km以上存在明显正偏差,高纬度的最大,中纬度次之,低纬度最小。水汽反演误差在约4 km以下明显增大,低纬度的最大,中纬度次之,高纬度最小。有云存在时,需要去除云的吸收作用,否则温度和水汽会出现明显的正偏差。上述研究为进一步发展LEO-LEO掩星探测计划提供了理论参考依据。     

Verification of shielding effect by the water-filled materials for space radiation in the International Space Station using passive dosimeters

The dose reduction effects for space radiation by installation of water shielding material (“protective curtain”) of a stack board consisting of the hygienic wipes and towels have been experimentally evaluated in the International Space Station by using passive dosimeters. The averaged water thickness of the protective curtain was 6.3 g/cm². The passive dosimeters consisted of a combination of thermoluminescent detectors (TLDs) and plastic nuclear track detectors (PNTDs). Totally 12 passive dosimeter packages were installed in the Russian Service Module during late 2010. Half of the packages were located at the protective curtain surface and the other half were at the crew cabin wall behind or aside the protective curtain. The mean absorbed dose and dose equivalent rates are measured to be 327 μGy/day and 821 μSv/day for the unprotected packages and 224 μGy/day and 575 μSv/day for the protected packages, respectively. The observed dose reduction rate with protective curtain was found to be 37 ± 7% in dose equivalent, which was consistent with the calculation in the spherical water phantom by PHITS. The contributions due to low and high LET particles were found to be comparable in observed dose reduction rate. The protective curtain would be effective shielding material for not only trapped particles (several 10 MeV) but also for low energy galactic cosmic rays (several 100 MeV/n). The properly utilized protective curtain will effectively reduce the radiation dose for crew living in space station and prolong long-term mission in the future.     

透光脉动值在絮凝实验研究中的应用

通过理论分析和实验研究，以流动原水为研究对象，首次考察了PAM、PAC、PAF和PFS几种絮凝剂在絮凝过程中的透光脉动值变化。结果表明，不同种类絮凝剂投加条件下所形成的絮凝体具有不同的特性，能及时得到絮凝体破碎和重组的有关信息。     

大连春季一次平流海雾天气过程分析

本文从天气形势背景、水文气象条件等方面分析2012年4月下旬发生在大连地区的一次平流海雾过程;重点探讨大连地区春季海雾的形成机制与大雾形成的水汽来源等问题。在东南风的引导下,暖湿空气流经冷的海面是成雾的主要机制;天气形势稳定少动是这次大雾天气持续时间较长的主要原因。     

中国空间地球科学发展现状及未来策略

空间地球科学是以空间对地观测为主要信息获取手段,研究地球系统的各圈层及之间的相互作用、过程与演变,对地球进行系统研究的综合性交叉学科.为纪念空间科学学会成立40周年,本文系统回顾了中国空间地球科学的发展历程,分析当前面临的机遇与挑战,进而提出中国空间地球科学未来发展的建议.     

FY-2C星辐射定标及其结果分析

介绍了风云二号(FY-2)C星发射前后红外与水汽波段的地面真空辐射定标、星上黑体定标和地面辐射校正场定标,以及可见光波段的地面太阳定标、积分球定标、地面辐射校正场定标和太阳像的原理与方法.给出了C星不同波段不同定标法的结果.分析表明,C星采用的定标方法均有效,并互为补充和验证.为进一步提高定标精度,还可对环境温度模拟、二次曲线拟合、减小积分球定标误差和光谱响应等作相应的改进.     

Development of a micro-balance system for dust and water vapour detection in the Mars atmosphere

Quartz crystal piezoelectric sensors are suitable for deposition analyses that need very high sensitivity. Due to the wide working ranges and high performances, micro-balances can measure the mass settling in average Mars conditions during a period of months before saturation is reached. This ensures a proper use for short and long term water and dust deposition monitoring. Micro-balances have been studied, calibrated and used for the GIADA (grain impact analyser and dust accumulator) experiment for the ESA-Rosetta space mission. Experience on micro-balance performance study by dust deposition has been acquired and water vapour deposition studies are in progress in a Martian atmosphere simulation chamber. Preliminary results show that micro-balances are capable to detect up to partial pressure values corresponding to parts per billion of the typical Martian atmosphere.