Comparison of Antarctic riometer radio wave absorption and THEMIS mission energetic electron fluxes

Simultaneous observations of in situ plasma properties in the tail of the Earth’s magnetosphere and of ground based instruments, lying on the same geomagnetic field lines, have recently proved to yield significant new results. In most cases magnetosphere ionosphere interactions during the night-time northern hemisphere conditions are studied. Here, observations of energetic electrons in the tail of the Earth’s magnetosphere made by the THEMIS mission satellites are compared with auroral radio wave absorption determined by riometers in the Antarctic for sunlit conditions. Days for which satellites and riometers are connected by the same geomagnetic field line are selected using a geomagnetic field model. The six days analysed show clear associations between fluxes and absorptions in some cases. However, these do not necessarily correspond to conjugacy intervals. Hours of positive associations are 1.65 times those for negative associations, all hours and days considered (1.42–3.6 on five days and 0.58 on the other day). These computations are assumed appropriate since the footprints of the satellites used approximately follow corrected geomagnetic parallels for all six days studied. The use of a finer parameterization of geomagnetic models to determine conjugacy may be needed.     

单壁碳纳米管低能区光吸收性质

采用半经验方法,通过紧束缚理论建立一维近似模型,研究了单壁碳纳米管的态密度,解释了单壁碳纳米管光吸收谱低能阶段出现的3个吸收峰的形成原因。     

涡扇发动机排气系统红外特征

采用反向蒙特卡罗法(Reverse Monte-carlo,简称RMC)结合窄带模型计算了模型涡扇发动机(不带加力)排气系统的红外辐射强度。考虑了金属壁面的发射和反射以及燃气中CO2,CO和H2O等组分的吸收、发射和透射,组分的吸收系数由NASA SP3080数据库获得,并对判断射线归宿的过程进行了改进,开发了计算程序。实验测量了模型涡扇发动机排气系统的中波红外光谱辐射强度及其空间辐射强度分布。结果表明:计算得到的3～5μm波段内的光谱辐射强度以及空间辐射强度分布与实验值吻合较好,最大误差为10%左右,本文的计算方法能比较准确地反映涡扇发动机排气系统在非加力状态下的中波红外辐射特征。     

长寿命卫星热控涂层性能退化及其对卫星热特征的影响

分析了卫星热控涂层在轨运行时所面临的复杂的空间辐照环境,在国 内外试验数据的基础上,给出了热控涂层在空间辐照环境作用下的退化模型,得到了退化前 后热控涂层光学性能变化的表达式,预测了几种常用热控涂层在空间环境下的退化结果。并 以一颗地球同步轨道模拟星为例,分析热控涂层性能退化对卫星热特征尤其是对卫星红外辐 射特性的影响。
     

红外动态目标模拟器光学系统的设计

设计了一种用于红外导引头性能测试的红外动态目标模拟器,利用数字微镜阵列(DMD)对黑体红外辐射进行反射调制,并由光学准直系统实现红外场景生成系统与红外导引头的光学耦合。用光学设计软件（ZEMAX）对准直光学系统进行了设计和优化,准直光学系统成像质量良好,接近衍射极限,点列图直径小于艾里斑直径,畸变小于0.1%。结果表明该系统环境适应性强,能很好地用于红外导引头动态图像的校准。     

碳纤维/ 氰酸酯复合材料尺寸稳定性能

对碳纤维/氰酸酯复合材料的吸湿、空间放气、吸湿变形性能进行了研究,并与传统碳纤维/环氧复合材料的性能进行对比。研究表明:氰酸酯基复合材料的吸湿性能优于碳纤维/环氧树脂复合材料,且其各项空间环境性能均与环氧树脂基复合材料相当。     

直接敏感地平的空天飞行器惯性/天文组合方法

传统的惯性/天文位置组合导航系统中,由于天文定位观测输出耦合了水平观测平台基准误差,往往存在系统噪声与量测噪声不完全独立的问题.针对此问题,分析了利用天文观测量修正惯性系下陀螺漂移的原理,提出了一种直接敏感地平进行天文解析定位及组合滤波的空天飞行器自主导航定位方案,并建立了相应的组合滤波模型.所提出的方法采用星敏感器和陀螺仪构造惯性基准,并在此基础上进行基于红外地平仪的天文定位解算,最后进行惯性/天文组合定位.该方案充分利用了星光敏感器在惯性系下姿态测量精度高的优点,并使惯性/天文组合定位滤波中状态噪声和观测噪声完全独立,仿真结果验证了该定位方法的有效性.     

Improved rainfall estimation over the Indian region using satellite infrared technique

The GOES Precipitation Index (GPI) technique (Arkin, 1979) for rainfall estimation has been in operation for the last three decades. However, its applications are limited to the larger temporal and spatial scales. The present study focuses on the augmentation on GPI technique by incorporating a moisture factor for the environmental correction developed by Vicente et al. (1998). It consists of two steps; in the first step the GPI technique is applied to the Kalpana-IR data for rainfall estimation over the Indian land and oceanic region and in the second step an environmental moisture correction factor is applied to the GPI-based rainfall to estimate the final rainfall. Detailed validation with rain gauges and comparison with Tropical Rainfall Measuring Mission (TRMM) merged data product (3B42) are performed and it is found that the present technique is able to estimate the rainfall with better accuracy than the GPI technique over higher temporal and spatial domains for many operational applications in and around the Indian regions using Indian geostationary satellite data. Further comparison with the Doppler Weather Radar shows that the present technique is able to retrieve the rainfall with reasonably good accuracy.     

InGaAs探测器热电制冷方法研究

InGaAs探测器在短波红外领域具有良好的探测率,对空间遥感和探测有重要的价值。为了实现空间红外仪器的高灵敏度要求,使用热电制冷技术设计了探测器制冷系统,使探测器稳定地工作在合适的温度,以相对较小的体积和功耗代价显著地提高红外仪器的探测灵敏度。