高空气球热力学模型与上升过程仿真分析

基于对高空气球热力学环境的分析,建立了热力学与动力学耦合的高空气球动力学模型;并采用该模型对某高空气球的上升与驻留过程进行仿真分析.结果表明:高空气球上升过程中内部氦气存在"超冷"现象,其中平流层区域"超冷"明显,氦气平均温差为-19 K;由于"超冷",其上升速度曲线呈双"V"形变化;强太阳辐射与弱对流环境使驻留过程中氦气呈现"超热"现象,平衡时氦气平均温度比环境温度高39 K,球内氦气超压648.8 Pa.数值仿真的速度、平均温度变化规律与相关飞行试验数据相吻合,说明该仿真模型是有效的.      

NASA用“飞碟”试验火星着陆技术

<正>6月28日,为试验未来火星着陆所需技术,美国航宇局(NASA)将一个飞碟状飞行器送到高空并使其降落,但降落伞在展开时出现了缠绕问题。飞行器最终溅落在太平洋上。称为"低密度超音速减速器"(LDSD)的飞行器由一个橄榄球场大小的巨型氦气球搭载升空,约2.5小时后在约36.6千米高空与气球分离,随后由火箭发动机加速到3.8倍音速,并飞到54.9千米高度。此后,伴随着高度下降,它展开了名为"超     

锡林浩特市火山地质公园平台山顶近地面大气电场变化特征

大气电场强度是大气电学的重要参数.大气电场的准确测量对雷暴和地震的监测、预警等具有重要的意义.利用2015年8月27日气球搭载大气电场仪测量近地面大气电场实验得到的电场数据，分析在特殊地形表面近地面500m高度内大气电场强度随高度的变化特征.结果表明:晴天条件下，火山喷发形成的熔岩平台山顶上空近地面大气电场强度随高度增加呈指数递减，大气电场的数值和变化范围均较大，尤其是近地面100m高度内，大气电场值达到1kV·m-1以上.此外，还通过经验公式得出了近火山灰石地表的大气电导率.受空气中重离子的影响，其电导率远小于全球大气电导率的平均值.实验结果丰富了在特殊地形下大气电场的测量结果，揭示了中国内蒙古锡林浩特地区火山山顶近地面大气电场强度随高度的变化特征.      

乌鲁木齐地区电离层环境长期变化特性研究

电离层环境变化对电子信息系统具有重要影响,其可能引起短波通信质量下降甚至中断,导致导航信号闪烁和误差增加等. 研究电离层环境特性对于评估空间环境对通信、雷达及导航装备的影响具有重要意义. 本文根据乌鲁木齐电波环境观测站50余年数据,研究了乌鲁木齐地区电离层F层临界频率、F层底高、Es层临界频率的日变化、季节变化和长期变化情况,同时根据HWM07高空风场模型研究了乌鲁木齐地区高空风场的昼夜和季节变化特性.      

临近空间环境下封闭方腔内耦合换热特性

以临近空间浮空器载荷舱为应用背景,对复杂热边界条件下含热源的三维封闭方腔内自然对流、表面辐射和导热的耦合问题进行了数值模拟。综合考虑对流换热、长波辐射、太阳辐射等因素的影响,建立了临近空间热环境模型。通过Fluent软件用户自定义函数（UDF）引入外部非定常的辐射-对流耦合热边界条件,对腔内换热特性的昼夜变化进行研究,并分析了腔壁厚度、发射率和导热系数对其的影响。数值结果表明,腔内平均温度昼夜变化很小,约为12.9 K,但温度场分布随太阳方位变化而变化;腔内对流换热较弱,同一时刻最大温差约为71.3 K;腔壁热阻和发射率增加会削弱自然对流的强度。      

昼夜温度变化对燃油箱空余空间氧浓度的影响

燃油箱空余空间氧浓度变化规律的确定是惰化系统的设计基础，但影响燃油箱空余空间氧浓度因素很多，当前人们对于昼夜温度变化这一实际现象还缺少必要的分析计算。为此，以某型飞机中央翼燃油箱为研究对象，依据FAR25适航条款中昼夜温度变化的相关规定，建立理论仿真模型，利用实验数据对模型进行验证，探讨燃油箱空余空间氧浓度与昼夜温度变化之间的对应关系，并分析昼夜温度变化范围、载油率、初始氧浓度、溶解氧析出等因素对燃油箱空余空间氧浓度的影响，提出满足适航条款要求的夜间停机前燃油箱初始氧浓度限值。研究结果表明:昼夜温度的变化范围、载油率、初始氧浓度等因素对燃油箱空余空间氧浓度变化规律影响程度有所不同；停机前燃油箱初始氧浓度限值应该低于最低氧浓度限值0.5%~1%。研究成果将对惰化系统设计、燃油箱可燃性暴露时间计算具有较好的参考价值。      

液体姿控发动机76km高空模拟试验系统性能仿真

为研究液体姿控发动机76 km高空模拟试验系统的工作性能,建立了考虑燃气相变的试验系统集中参数动态仿真模型。模型由真空抽气系统、冷凝管束和液氮外流程3个子模型组成。根据燃气、霜、液氮之间的传热和传质过程将各子模型耦合在一起。以四氧化二氮/甲基肼双组元姿控发动机为实例,计算了稳态和脉冲点火试验时系统的工作参数,分析了关键设计参数对其工作性能的影响。结果表明:试验系统能够为最大流量6.4 g/s(推力约16.5 N)的发动机提供脉冲和6×10~4s长程稳态试验环境;在长程稳态试验中,冷凝管束霜层将依次饱和,失去对二氧化碳和水蒸汽的抽吸能力,导致真空舱压力逐渐升高;在脉冲点火试验中,真空舱压力将随发动机工作而脉冲波动,15 ms开关脉冲时的压力波动幅度约70%。研究结果为液体姿控发动机高空模拟试验系统的设计与改进提供了参考。     

真空条件下多孔平板发汗冷却试验研究

发汗冷却是解决高速飞行器关键部位热防护问题的有效途径。以不同材料的多孔平板为研究对象，以水为冷却剂，利用自行设计搭建的试验平台对多孔平板发汗冷却过程进行瞬态试验测量，得到了不同热流加热环境下不同材料多孔平板内外壁温度变化，并分析冷却剂对不同材料的冷却效果。结果表明:发汗冷却极大降低了多孔平板内外壁温度，起到了有效的主动热防护作用。对于镍、铜金属多孔平板，保持冷却剂水流量约3.5 g/s，在热流密度小于120 kW/m2的条件下，多孔平板内外壁温度稳定在30~50℃。对于陶瓷多孔平板，保持冷却剂水流量约0.32 g/s，在热流密度小于220 kW/m2的条件下，多孔平板内外壁温度基本稳定在30~40℃。在高热流密度315 kW/m2的条件下，对于镍、铜金属和陶瓷多孔平板，发汗冷却时平板内壁温度变化不大，外壁温度分别稳定在约260℃、110℃和130℃。外壁冷却剂处于完全汽化状态，且冷却剂汽化相变位置在多孔平板内部。若无发汗冷却，多孔平板内外壁温度快速升高，其平衡温度较有发汗冷却时大幅提高，进一步表明发汗冷却的巨大应用潜力。      

基于钠激光雷达观测数据的中间层顶大气温度分布特性研究

作为中间层和热层的边界层,中间层顶存在多种能量交换方式,是大气能量耦合的重要区域。本文利用部署于中国科学院廊坊临近空间大气探测站的钠荧光多普勒激光雷达2013年的观测数据,研究了廊坊上空中间层顶区域大气温度的年度和季节分布特性,并分析了影响温度分布的多种因素。年平均温度廓线图显示,中间层顶位于约97.5 km高度处,温度约191.2 K。受放热化学反应的影响,年平均温度廓线91 km高度处出现了一个198 K的相对温度高点。中间层顶区域大气温度的季节分布受太阳辐射和大气动力学因素综合影响,夏季在大气动力学影响下,中间层顶高度较低,位于88 km高度处,温度也较低,约177 K;冬季太阳辐射起主导作用,中间层顶位于99 km高度处,温度为181 K。通过拟合月平均温度分析了中间层顶区域大气温度年变化和半年变化的振幅和相位特征。结果显示,中间层顶区域上部温度分布主要受太阳辐射的影响;在中间层顶区域下部,大气波动主导了温度分布。      

卫星热平衡试验的温度预测与仿真模型

为了解决卫星热平衡试验中涉及的温度预测与变工况仿真试验问题,建立起星载仪器温度变化的双层集总参数模型,这一动态特性模型采用简单的嵌套结构,模型参数可以方便地运用系统辨识算法从卫星热平衡试验数据中获取,应用这一模型可以对不同星载仪器的温度变化进行分别的预测与仿真计算,从而大大减少了温度预测与仿真工作的计算量.对比研究表明:温度预测与仿真计算的结果与实际热平衡试验的结果一致.     

Modeling and analysis of floating performances of stratospheric semi-rigid airships

In recent years, the study of semi-rigid airship has revived with the development of airships. Semi-rigid airships have some characteristics of rigid airships and non-rigid airships. Due to the flexibility of the envelope of the non-rigid airship, the variation of the temperature of the inner gas will lead to its structure deformation and affect its flight altitude. This paper develops the structural mechanics model, thermodynamic model and dynamic model of the semi-rigid airship, based on which nonlinear finite element analysis is employed for geometrically nonlinear deformation of the airship upper film in consideration of thermodynamics and structural mechanics coupling. Based on the thermal-structural interaction, the thermal characteristics and flight performances of the airship during floating flight are investigated. The 3-D solar radiation and temperature distribution of the airship skin and the temperature variation of the inner gas are presented to investigate the thermal performance of the airship, flight velocity, acceleration and flight altitude are simulated to investigate the flight performance, and the variations of the volume and pressure difference of the inner gas are calculated to provide a basis for structure design. The results of the simulation can be referenced for the design of the semi-rigid airship, and can be used for the further study on the attitude control of the airship during its floating flight.     

Soviet-Indian research of cosmic radiation by high altitude balloons

The report presents some results on the cosmic radiation intensity research carried out with the high-altitude balloons for the period of 1977–1979. The intensity of gamma-radiation with the energy above 40 MeV was measured in two balloon flights at an altitude of 4–7 g/cm² of residual atmosphere in the vicinity of the geomagnetic equator. A temporal analysis of the intensity to discover fluctuations with periods in the range of 4–60 min was made. Quasi-periodic fluctuations of gamma-radiation intensity with 5 min periods, amplitude ～20% and duration of several hours were discovered. Possible mechanisms of such fluctuation appearance are discussed.The report gives the results of measuring downward, upward and horizontal electron fluxes in the vicinity of the equator. The obtained data and the data provided by satellites are compared. The report discusses the prospects of further joint Soviet-Indian research of cosmic gamma-radiation.     

Low altitude dose measurements from APEX, CRRES and DMSP

Dosimeter data taken on the APEX (1994–1996), CRRES (1990–1991) and DMSP (1984–1987) satellites have been used to study the low altitude (down to 350 km) radiation environment. Of special concern has been the inner edge of the inner radiation belt due to its steep gradient. We have constructed dose models of the inner edge of the belt from all three spacecraft and put them into a personal computer utility, called APEXRAD, that calculates dose for user-selected orbits. The variation of dose for low altitude, circular orbits is given as a function of altitude, inclination and particle type. Dose-depth curves show that shielding greater than 1/4 in Al is largely ineffectual for low altitude orbits. The contribution of outer zone electrons to low altitude dose is shown to be important only for thin shields and to have significant variation with magnetic activity and solar cycle.     

Feasibility study of a sea-anchored stratospheric balloon for long-duration flights

Sea-anchored balloons are stratospheric super-pressure balloons that are anchored to the sea. The sea-anchored balloon is a simple system that has the capability for long-duration flights, fixed-point observations, flexible launch windows, easy telemetry links to ground stations, and quick recoveries. Such balloons are not required to fly through the jet stream while tethered to the ground or sea, because the tether is deployed from a reel on the balloon after reaching a floating altitude. In this study, the feasibility of the sea-anchored balloon is investigated, with particular emphasis on the tether strength, balloon altitude, and system mass, based on the present technological level of the tether’s specific strength. Although the wind distribution with altitude is a dominant factor for feasibility, a sea-anchored balloon with an altitude of about 25 km would be feasible if the velocity of the jet stream is sufficiently low. The sea-anchored balloon can be simply flight-tested, since additional ground facilities and special flight operations are not necessary.     

A comprehensive numerical model investigating the thermal-dynamic performance of scientific balloon

The increase of balloon applications makes it necessary for a comprehensive understanding of the thermal and dynamic performance of scientific balloons. This paper proposed a novel numerical model to investigate the thermal and dynamic characteristics of scientific balloon in both ascending and floating conditions. The novel model consists of a dynamic model and thermal model, the dynamic model was solved numerically by a computer program developed with Matlab/Simulink to calculate the velocity and trajectory, the thermal model was solved by the Fluent program to find out the balloon film temperature distribution and inner Helium gas velocity and temperature field. These models were verified by comparing the numerical results with experimental data. Then the thermal and dynamic behavior of a scientific balloon in a real environment were simulated and discussed in details.     

USV test flight by stratospheric balloon: Preliminary mission analysis

The Unmanned Space Vehicle test flights will use a 7 m 1300 kg aircraft. The first three launches will take place at the Italian Space Agency ASI base in Trapani–Milo, Sicily, through a stratospheric balloon that will drop the aircraft at a predefined height. After free fall acceleration to transonic velocities, the parachute deployment will allow a safe splash down in the central Mediterranean Sea. The goal of this article is to show the preliminary analysis results for the first USV flight.We carried out a statistical study for the year 2000–2003, evaluating the typical summer and winter launch windows of the Trapani–Milo base.First, in the center Mediterranean, we define safe recovery areas. They cannot be reached during the balloon ascending phase so, after a sufficiently long floating part able to catch the open sea, the balloon will go down to the release height (24 km). The simulation foresees a 400,000 m³ balloon and 3 valves for the altitude transfer.A safe splash down must occur far enough from the nearest coast: the minimum distance is considered around 25 km. The vehicle should be released at a distance, from the nearest coast, greater than this minimum amount plus the USV model maximum horizontal translation, during its own trajectory from balloon separation to splash down. In this way we define safe release areas for some possible translations.Winter stratospheric winds are less stable. The winter average flight duration is 7 h and it is probably too long for the diurnal recovery requirement and its scheduled procedures.Comparing past stratospheric balloons flights and trajectories computed using measured meteorological data (analysis), with their predictions made using forecast models and soundings, we obtain the standard deviation of the trajectory forecast uncertainty at the balloon–aircraft separation. Two cases are taken into account: predictions made 24 and 6 h before the launch.Assuming a Gaussian latitudinal uncertainty distribution for the prediction 6 h before the launch, we are able to identify the forecast trajectories that have a probability greater than 97% to reach the safe release areas.Simulating the summer windows trajectories for the years from 2000 to 2003 and for the favorable ground wind days, we obtain the number of trajectories with the desired forecast probabilities.     

Measurements of upper atmosphere wind and temperature from meteorological rocket experiments during winter 1979

This institute conducted a series of meteorological rocket experiments for the upper-atmospheric sounding in the winter of 1979. Within the overlap altitude range with balloon flights, a comparison of the results with the standard radiosonde data indicated that the rocket-borne system was reliable. The measurements from foru rocket flights for the region between 20 and 30 km showed a degree of compatibility to each other while those for above 30 km differed considerably from one another. At low latitude, the temperature profiles in the winter stratosphere in general showed a reasonably good agreement with the U.S. Standard Atmospheric Supplements, 1966 (USSAS 66). A temperature of 2–24°C lower than the USSAS 66, however, was recorded in the lower mesosphere. Above 30 km the maximum diurnal variation in temperature was 9°C or so. In the winter, the wind profile showed the westerlies and the maximum wind velocity of 92.1 Msec^?1 was obtained from these experiments at the height of 60 km.     

A balloon-borne sun-tracking multichannel photometer for atmospheric aerosol measurements

A balloon borne multichannel photometer for measurement of atmospheric scattering in the near ultraviolet and the visible wavelength regions has been developed at the Physical Research Laboratory, Ahmedabad for study of the size distribution and number density of aerosols at tropospheric and lower stratospheric altitudes. The instrumentation involves tracking the sun in elevation and scanning in azimuth. The payload was recently flown on a 100 kg. balloon from the Hyderabad Balloon Facility on 18 April 1984. The balloon reached a float altitude of 35 km and good quality data has been obtained from an altitude of 6 km upto float altitude. Data analysis is still in progress. The present paper details the instrument design and presents a few illustrations of the instrument performance from this flight.