射线剂量标准装置校准的新方法

在简要介绍 JC- 型射线剂量标准装置工作原理及组成的基础上 ,详细论述了其校准的新方法 ,并给出了检测数据的处理方法     

太阳能热动力发电系统吸热器腔体辐射计算

空间太阳能热动力发电系统是一种新型的空间电力系统，吸热器是热动力发电系统关键部件之一，吸热器腔体的热辐射将直接影响到吸热腔的热损失和吸热器的传热，建立了太阳能热动力发电系统吸热器腔体辐射模型，结合换热管的传热模型计算了吸热器的传热过程，得到了吸热器热损失，换热管最大温度，工质出口温度等结果，并进行了比较，分析、计算结果可以用于吸热器的设计。     

双锥—圆筒红外辐射源特性的蒙特卡罗解

本文考虑了红外辐射源腔内的镜反射成份,采用镜-漫混合反射模式,用蒙特卡罗法求定空腔的定向有效发射率。在通解的数学模型基础上,还针对500K双锥-圆筒热管空腔求得其典型解,分析了空腔辐射特性与锥角的关系。利用本文提供的方法也可计算其他腔形的辐射特性。     

空间对接机构太阳外热流的计算与分析

根据空间对接机构的结构特点,在简化物理模型的基础上,用太阳窗口和蒙特卡洛(MC)法计算不同空间位置、不同轨道高度、不同表面辐射特性的机构内部构件太阳辐射外热流,并给出了相应的计算流程。分析了飞行角β和表面辐射特性等因素对太阳热流的影响。研究结果对对接机构以及其他复杂系统的热控涂层选择有一定的参考价值。     

两点源干扰下被动雷达导引头测角性能分析

两点源干扰是干扰雷达导引头的重要手段。但在实际应用中，两点源的功率不可能完全相等，这就为被动雷达导引头对抗两点源干扰提供了契机。本文通过数学推导得出了：在远场，当导引头无模糊测角范围满足一定要求，只要保证足够的数据积累点数，导引头进行数据和累取均值，其结果并不指向两源的“重心”或“质心”而是指向两源中功率较大者。     

针对跟踪雷达的反辐射导弹发射时机告警

介绍一种反辐射导弹发射时机警设备的基本原理和实施方案。根据雷达收到的载机和反辐射导弹回波信号特征，综合成ｅｘｐ（Ｊ２π（ｆｏ＋ｆｄ）ｔ）信号和ｅｘｐ（ｊ２π（ｆｏ＋ｆｄ＋ａｔ／２）ｔ）信号的数学模型。分雷达跟踪波门内外两种情况进行５１２点快傅里叶变换（ＦＦＴ）谱分析，从频域上把载机和导弹区分开来，达到反辐射导弹发射时机靠警的目的。最后给出了仿真结果，结果是令人满意的。     

含非均匀辐射气体空腔辐射特性计算研究

文章发展了求解积分辐射传输方程组的方法来计算充满非均匀辐射性气体封闭腔的辐射特性的方法,讨论了辐射空间分布及光谱分布的计算方法,并编制了相应的计算机程序.计算了某型发动机轴对称喷管的辐射分布,并与采用通常的辐射换热经验公式的计算结果进行了比较.     

圆柱形黑体腔热辐射及其在光纤中的传输

分析了圆柱形黑体腔腔内视在发射率的分布及腔体发射率，讨论了斜光线在光纤中的耦合与传输，并导出了光纤中传输的辐射功率表达式和光电探测器输出电流表达式。探测器输出电流的表达式表明，光电流的大小除随黑体腔温度变化外，还与探测器的下限、上限截止波长有关。下限、上限截止波长的间隔愈大，则光电流愈大，故在接收辐射功率时，探测器前不加窄带滤波片。文中还给出了光电流随温度变化的理论曲线和实验曲线，两者基本吻合。     

Structural dynamic responses of a stripped solar sail subjected to solar radiation pressure

The stripped solar sail whose membrane is divided into separate narrow membrane strips is believed to have the best structural efficiency. In this paper, the stripped solar sail structure is regarded as an assembly made by connecting a number of boom-strip components in sequence. Considering the coupling effects between booms and membrane strips, an exact and semi-analytical method to calculate structural dynamic responses of the stripped solar sail subjected to solar radiation pressure is established. The case study of a 100 m stripped solar sail shows that the stripped architecture helps to reduce the static deflections and amplitudes of the steady-state dynamic response. Larger prestress of the membrane strips will decrease stiffness of the sail and increase amplitudes of the steady-state dynamic response. Increasing thickness of the boom will benefit to stability of the sail and reduce the resonant amplitudes. This proposed semi-analytical method provides an efficient analysis tool for structure design and attitude control of the stripped solar sail.     

Effect of severe geomagnetic storm conditions on atomic oxygen greenline dayglow emission in mesosphere

Severe geomagnetic storms and their effects on the 557.7 nm dayglow emission are studied in mesosphere. This study is primarily based on photochemical model with the necessary input obtained from a combination of experimental observations and empirical models. The model results are presented for a low latitude station Tirunelveli (8.7°N, 77.8°E). The volume emission rates are calculated using MSISE-90 and NRLMSISE-00 neutral atmospheric models. A comparison is made between the results obtained from these two models. A positive correlation amongst volume emission rate (VER), O, O₂ number densities and Dst index has been found. The present results indicate that the variation in emission rate is more for MSISE-90 than in NRLMSISE-00 model. The maximum depletion in the VER of greenline dayglow emission is found to be about 30% at 96 km during the main phase of the one of the geomagnetic storms investigated in the case of MSISE-90 (which is strongest with Dst index −216 nT). The O₂ density decreases about 22% at 96 km during the main phase of the same geomagnetic storm.The NRLSMSISE-00 model does not show any appreciable change in the number density of O during any of the two events. The present study also shows that the altitude of peak emission rate is unaffected by the geomagnetic storms. The effect of geomagnetic storm on the greenline nightglow emission has also been studied. It is found that almost no correlation can be established between the Dst index and variations in the volume emission rates using the NRLMSISE-00 neutral model atmosphere. However, a positive correlation is found in the case of MSISE-90 and the maximum depletion in the case of nightglow is about 40% for one of the storms. The present study shows that there are significant differences between the results obtained using MSISE-90 and NRLMSISE-00.