基于GAN网络的红外图像生成技术

当将人工智能技术应用于军事领域中的目标识别任务时，针对由红外图片采集的局限性而造成的训练数据不足的问题，提出了基于生成对抗网络以生成红外图像的方法，实现了数据集的扩充。对基本的生成对抗网络进行了改进，将网络的输入由随机噪声变为真实图片，使之实现了图片到图片的风格转换，即彩色图片转变为红外图片。经过网络模型的搭建和训练，实验结果表明，该方法能够有效生成清晰和高质量的红外图片，解决了由红外数据不足而造成的网络训练不充分的问题。     

An empirical solar radiation pressure model for satellites moving in the orbit-normal mode

We present a family of empirical solar radiation pressure (SRP) models suited for satellites orbiting the Earth in the orbit normal (ON) mode. The proposed ECOM-TB model describes the SRP accelerations in the so-called terminator coordinate system. The choice of the coordinate system and the SRP parametrization is based on theoretical assumptions and on simulation results with a QZS-1-like box-wing model, where the SRP accelerations acting on the solar panels and on the box are assessed separately. The new SRP model takes into account that in ON-mode the incident angle of the solar radiation on the solar panels is not constant like in the yaw-steering (YS) attitude mode. It depends on the elevation angle of the Sun above the satellite’s orbital plane. The resulting SRP vector acts, therefore, not only in the Sun-satellite direction, but has also a component normal to it. Both components are changing as a function of the incident angle. ECOM-TB has been used for precise orbit determination (POD) for QZS-1 and BeiDou2 (BDS2) satellites in medium (MEO) and inclined geosynchronous Earth orbits (IGSO) based on IGS MGEX data from 2014 and 2015. The resulting orbits have been validated with SLR, long-arc orbit fits, orbit misclosures, and by the satellite clock corrections based on the orbits. The validation results confirm that—compared to ECOM2—ECOM-TB significantly (factor 3–4) improves the POD of QZS-1 in ON-mode for orbits with different arc lengths (one, three, and five days). Moderate orbit improvements are achieved for BDS2 MEO satellites—especially if ECOM-TB is supported by pseudo-stochastic pulses (the model is then called ECOM-TBP). For BDS2 IGSOs, ECOM-TB with its 9 SRP parameters appears to be over-parameterized. For use with BDS2 IGSO spacecraft we therefore developed a minimized model version called ECOM-TBMP, which is based on the same axis decomposition as ECOM-TB, but has only 2 SRP parameters and is supported by pseudo-stochastic parameters, as well. This model shows a similar performance as ECOM-TB with short arcs, but an improved performance with (3-day) long-arcs. The new SRP models have been activated in CODE’s IGS MGEX solution in Summer 2018. Like the other ECOM models the ECOM-TB derivatives might be used together with an a priori model.     

纵向波纹隔热屏气膜冷却特性实验

针对加力燃烧室纵向波纹隔热屏气膜冷却效果开展了细致的实验研究,利用红外热像仪测量了隔热屏壁面的温度分布,分析了隔热屏板型、吹风比、开孔率等参数对气膜冷却效率的影响。实验中板型选取了平板和纵向波纹隔热屏,吹风比变化范围是0.5~3.0,开孔率变化范围是1.4%~3.7%。结果表明:相比于平板隔热屏的气膜冷却效率沿程逐渐增加,纵向波纹隔热屏的气膜冷却效率随波纹板的起伏而起伏且大于平板隔热屏;随着吹风比的增加气膜冷却效率逐渐加大,在吹风比为3.0时达到最大值;气膜冷却效率在波峰处低,波谷处高,整体上随波纹板的起伏而波动,吹风比越小,气膜冷却效率随波纹板的起伏变化越明显;高吹风比(吹风比为2.0~3.0)下,气膜冷却效率沿程变化与增幅较为缓慢;整体上,随着开孔率的增加气膜冷却效率逐渐加大,小开孔率(开孔率为1.4%、2.7%)下的气膜冷却效率相差不大,但在次流背风侧,开孔率小的气膜冷却效率要小于开孔率大的气膜冷却效率。      

The adjusted optical properties for Galileo/BeiDou-2/QZS-1 satellites and initial results on BeiDou-3e and QZS-2 satellites

Solar Radiation Pressure (SRP) is the dominant non-gravitational perturbation for GNSS (Global Navigation Satellite System) satellites. In the absence of precise surface models, the Empirical CODE Orbit Models (ECOM, ECOM2) are widely used in GNSS satellite orbit determination. Based on previous studies, the use of an a priori box-wing model enhances the ECOM model, especially if the spacecraft is a stretched body satellite. However, so far not all the GNSS system providers have published their metadata. To ensure a precise use of the a priori box-wing model, we estimate the optical parameters of all the Galileo, BeiDou-2, and QZS-1 (Quasi Zenith Satellite System) satellites based on the physical processes from SRP to acceleration. Validation using orbit prediction proves that the adjusted parameters of Galileo and QZS-1 satellites exhibit almost the same performance as the corresponding published and “best guess” values. Whereas, the estimated parameters of BeiDou-2 satellites demonstrate an improvement of more than 60% over the initial “guess” values. The resulting optical parameters of all the satellites are introduced into an a priori box-wing model, which is jointly used with ECOM and ECOM2 model in the orbit determination. Results show that the pure ECOM2 model exhibits better performance than the pure ECOM model for Galileo, BeiDou-2 GEO and QZS-1 orbits. Combined with the a priori box-wing model the ECOM model (ECOM+BW) results in the best Galileo, BeiDou-2 GEO and QZS-1 orbits. The standard deviation (STD) of satellite laser ranging residuals reduce by about 20% and 5% with respect to the pure ECOM2 model for Galileo and BeiDou-2 GEO orbits, while the reductions are about 40% and 60% for QZS-1 orbits in yaw-steering and orbit-normal mode respectively. BeiDou-2 IGSO and MEO satellite orbits do not benefit much from the a priori box-wing model. In summary, we suggest setting up a unified SRP model of ECOM+BW for Galileo, QZS-1, and BeiDou-2 orbits based on the adjusted metadata. In addition, we estimate the optical parameters of BeiDou-3e and QZS-2 satellites using a limited number of tracking stations. Results regarding the unified SRP model indicate the same advantages, the STD of satellite laser ranging residuals reduces by about 30% and 20% for QZS-2 and BeiDou-3e orbits respectively over orbit products without a priori model. The estimation procedure is effective and easy to apply to the new emerging satellites in the future.     

基于DNET的空中红外目标抗干扰识别算法

复杂空战背景下针对人工干扰的博弈是红外空空导弹精确探测制导技术发展面临的瓶颈和核心技术。针对人工干扰对空中红外目标产生的遮蔽、黏连、相似等干扰现象，以及目标机动和相对运动造成的形状、尺度、辐射特性剧烈变化等实际问题，提出一种基于信息特征提取的深度卷积神经网络DNET空中红外图像目标抗干扰识别算法。首先，DNET网络对大尺度特征图像采用密集连接模块，在前部通道保存每一层的网络输出，在网络末端引入特征注意力机制，获得每个特征通道的信息特征识别权重。然后，加入多尺度密集连接模块，并与多尺度特征融合检测结合，提高对大尺度变化情况下的目标特征提取能力。实验结果表明，在伴随红外诱饵干扰的实时检测条件下，红外目标由点目标变化为成像目标，直至充满视场的整个过程中，本文抗干扰识别算法的识别精确度、召回率及识别速度分别达到99.36%、96.95%、132 fps，具备识别精确度和召回率高、识别速度快等优点，并具有良好的鲁棒性。     

基于红外波段船载星光定向仪白昼恒星探测技术

摘要： 白昼恒星探测技术是船载星光定向仪海上应用的关键技术之一.本文基于实测星图给出白昼恒星探测技术的理论公式和实现方案.该技术针对实测红外星图中的背景噪声、伪星点、坏像素、对灰度背景的适应性问题，分别设计星图滤波算法、多帧伪星点剔除算法、坏像素索引表以及多梯度渐进积分时间调整算法.通过外场观星和组合导航实验验证该技术的有效性和精度.     

27-day variation in solar-terrestrial parameters: Global characteristics and an origin based approach of the signals

The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ～27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ～27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation.     

临近空间大气中波红外辐射特性的数值分析研究

介绍了临近空间大气环境特点及其非局域热平衡状态的辐射传输计算方法。利用战略高高度辐亮度代码SHARC（Strategic high-altitude radiance code），计算了3—5 μm波段不同观测条件、光学现象及大气环境下的临近空间大气背景辐射。分析结果表明：临近空间中波红外辐射随观测天顶角的增大而增强，随太阳天顶角的增大而减弱；在38 km及75 km附近，临边背景辐射存在极大值；纬度越高，临边背景辐射的季节变化特征越明显。OH夜气辉和极光对背景辐射有重要增强作用。     

PBT弹性体微相分离及对其力学性能的影响研究

为了获得微相分离对宽温PBT叠氮聚醚弹性体力学性能的影响规律,用红外光谱分析法(FT-IR)和动态热力学分析法(DMA)研究了PBT叠氮聚醚弹性体产生微相分离的机理和影响因素。用调节硬段含量、交联参数的方法调控其微相分离,控制适当的微相分离程度可显著改善推进剂的力学性能。研究结果表明:在二元醇扩链的弹性体体系中,当硬段含量约为15%时,弹性体发生相对最大比例的微相分离,体现出较佳的综合力学性能。通过微相分离的调控可获得宽温范围内综合力学性能较好的叠氮聚醚推进剂用粘合剂基体材料。     

高能(450 kV)X射线参考辐射场附加过滤研究

利用MCNP程序对450kV X光机建立模型，计算各参考辐射质下的原级谱、平均光子能量。对ISO 4037-1中已有范围的管电压与附加过滤片厚度关系曲线进行二次拟合，确定模拟厚度范围。利用MCNP计算各附加过滤组合下的平均光子能量值，并与外推法得出的平均光子能量值进行对比，将相对偏差最小时的附加过滤作为最终确定值。从部分能量点的模拟与测量结果的对比可看出，模拟得出的平均光子能量在2%以内与PTB及中国计量院测量结果保持一致，附加过滤最大相对偏差为18%。