大气臭氧地基遥感反演的退卷积方法

本文提出了一种大气臭氧地基遥感信息处理的新方法,它利用非线性退卷积方法和等效仪器函数提高光谱分辨率,利用非线性最小二乘法进行大气臭氧反演计算,可以显着提高大气臭氧遥感的可探测高度和精度。      

用固体吸附/分光光度法同时监测空气中的肼、一甲肼和偏二甲肼

介绍了用一甲肼浓缩采样采集空气中三肼混合气体,用分光光度法分别测出肼、一甲肼和偏二甲肼各组分的含量。测定结果通过标准气验证,相对误差小于１７％,各组份回收率均大于８０％。本方法适用于空气中低浓度三肼废气的测定。     

Study on Satellite-to-ground Laser Communications with Existence of Atmosphere

The laser beam used to establish a communication channel between satellite and ground segments has a small divergence angle and a tiny spot on the Earth’s surface, which may lead to the fail of the system. So it’s important to study the deflection of laser beam by the Earth’s atmosphere and find a way to calibrate this error. Both theoretical analysis and real data processing method are used to obtain the mathematical model for divergence angle of laser communication beam and its correction function. Then the model has been applied to the data, which was used to describe the atmosphere state by traditional ground segments to obtain the critical elevation angle. According to the results of calculation, our conclusion will be that the correction should be done when the critical elevation happens.      

脉冲展宽对深空激光通信的影响与补偿研究

深空激光通信系统下行链路的脉冲位置调制PPM（Pulse Position Modulation）信号在经过大气信道传输和单光子探测器接收时,将出现脉冲展宽效应,引起通信系统性能下降。分析了大气信道中的淡积云云层散射、大气湍流与气溶胶散射和单光子探测器的抖动特性所引起的脉冲展宽效应。在此基础上,仿真分析了淡积云云层物理厚度对不同PPM调制阶数下通信速率的影响,并研究了单光子探测器引起的脉冲展宽产生的抖动损失。为补偿脉冲展宽的影响,提出了一种基于时隙似然比解调的补偿方法,通过仿真验证了该方法能够有效降低深空PPM激光通信链路中脉冲展宽对通信误码率的影响。该研究对分析和提升深空PPM激光通信系统的链路性能具有一定的参考意义。     

基于MPX4115的小型无人机气压高度测量系统设计

从气压高度测量的原理出发,介绍了基于MPX4115传感器,以C8051F020单片机为飞控计算机的小型无人机高度测量系统的组成和工作原理,并详细论述了测量系统的电路设计;利用压力校验仪对MPX4115传感器进行了辨识,保证了系统对压强的测量准确度;对高度-大气压强公式进行了数据拟合,并设计了计算程序,有效地解决了C8051F020单片机计算能力不足的问题;该系统具有体积小、功耗低、速度快、电路简单可靠等优点。     

有限时间收敛的阻力加速度跟踪进入制导律

摘要：针对地球或火星的大气层进入过程提出一种具有有限时间收敛性质的阻力加速度跟踪鲁棒制导律.将再入动力学方程抽象为一类带有不确定性及扰动的非线性系统,并针对该类系统提出一种基于滑模控制的有限时间鲁棒控制律.将所提出的理论方法应用于阻力加速度跟踪制导律的设计中,设计可使阻力加速度在有限时间内跟踪上标称值的制导律.仿真验证方法的有效性和先进性.     

面向非结构混合网格高精度阻力预测的梯度求解方法

针对非结构混合网格的特点,通过改进传统的Green-Gauss梯度求解方法,提出了一种可提高非结构混合网格黏性计算精度的节点型Green-Gauss梯度求解方法。利用改进后的方法,完成了DLR-F4翼身组合体算例的计算和对比分析。改进后的梯度求解方法残差收敛更好,下降量级更多,阻力系数和试验吻合更好,激波区域压力分布和分离区域流场细节的模拟更精确,说明改进后的梯度求解方法有效提高了程序的鲁棒性和阻力预测精度,验证了方法的有效性。采用改进后的方法对第5届AIAA阻力预测研讨会的通用研究模型（CRM）进行了详细的模拟分析,结果表明：改进的梯度求解方法更加适用于非结构混合网格的黏性计算,计算精准度达到国际同类CFD软件水平,进一步验证了改进方法的可靠性。     

仿生减阻翼型的气动性能

利用一种基于滑移边界理论的仿生肋条结构的模化方法,对仿生减阻翼型的气动性能开展了数值模拟研究。结果显示:肋条结构同时布置在翼型压力面和吸力面湍流区域时,仿生减阻翼型的阻力可降低1.73%~3.07%,升阻比可提高2.10%~4.08%,其中黏性阻力的减小是总阻力下降的主要原因。对流场分析表明,仿生减阻翼型的速度曲线出现一定抬升,使得湍流边界层中的黏性子层增厚,进而导致了仿生减阻翼型气动性能的提升。      

ROPP反演软件算法及其精度分析

介绍了ROPP反演软件中无线电掩星反演的算法与精度分析. 采用COSMIC卫星2008年1 月1日全天的附加相位数据, 反演得到折射率、温度、压强与湿度等参数, 并与CDAAC 相应结果进行对比. 实验结果表明, 在30km高度以下, 折射率、压强和湿度的相对 误差在2%以内, 温度误差不超过2K.      

Thick galactic cosmic radiation shielding using atmospheric data

NASA is concerned with protecting astronauts from the effects of galactic cosmic radiation and has expended substantial effort in the development of computer models to predict the shielding obtained from various materials. However, these models were only developed for shields up to about 120 g/cm² in mass thickness and have predicted that shields of this mass thickness are insufficient to provide adequate protection for extended deep space flights. Consequently, effort is underway to extend the range of these models to thicker shields and experimental data is required to help confirm the resulting code. In this paper empirically obtained effective dose measurements from aircraft flights in the atmosphere are used to obtain the radiation shielding function of the Earth's atmosphere, a very thick, i.e. high mass, shield. Obtaining this result required solving an inverse problem and the method for solving it is presented. The results are shown to be in agreement with current code in the ranges where they overlap. These results are then checked and used to predict the radiation dosage under thick shields such as planetary regolith and the atmosphere of Venus.