Gamma-rays from Active Galactic Nuclei: Emission processes and particle acceleration

It is argued that the high-energy X-ray and -ray emission from flaring blazars is beamed radiation from the relativistic jet supporting the relativistic beaming hypothesis and the unified scenario for AGNs. Most probably the high-energy emission results from inverse Compton scattering by relativistic electrons and positrons in the jet of radiation originating external to the jet plus pair annihilation radiation from the jet. Future positive TeV detections of EGRET AGN sources will be decisive to identify the prominent target photon radiation field. Direct -ray production by energetic hadrons is not important for the flaring phase in -ray blazars, but the acceleration of energetic hadrons during the quiescent phase of AGNs is decisive as the source of secondary electrons and positrons through photo-pair and photo-pion production. Injection of ultrahigh energy secondary electrons and positrons into a stochastic quasilinear acceleration scheme during the quiescent AGN phase leads to cooling electron-positron distribution functions with a strong cut-off at low but relativistic energy that under certain local conditions may trigger a plasma instability that gives rise to an explosive event and the flaring -ray phase.     

用最优估计法从飞行试验数据估计飞机迎角及测量误差

本文采用最优估计方法——信息平方根滤波和平滑算法,利用飞行数据对J-7原型机安装的92/BJ311型风标式迎角传感器的迎角测量误差进行了估计,给出了飞行迎角的校准公式。状态估计系统方程采用六自由度非线性方程。飞行动作采用推拉机动方法.飞行试验结果与风洞值进行了比较分析,证明飞行试验获得的误差修正系数和零偏误差是合理的。     

Background-sensitive event selection in the search for gamma-ray sources

Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-known time signature of the source as its signal, has been developed (Özel and Mayer-Haβelwander, 1983). In an iterative procedure based on the improvement of source signal, generalized zones around the source are defined, from which gamma rays should be accepted to construct the optimum light curve of the source. These zones depend on the energy of the probed gamma rays, on the spatial structure and intensity of the background around the source, on the (estimated and/or tentative) intetnsity of the source and finally on the observing instrument's angular and energy response functions. The method, when applied to simulated and observed COS-B data demonstrated its feasibility and merits over the previonsly used circular event-acceptance cones method which was the basis of searches for gamma ray emission from radio pulsars (see for example Kniffen et al., 1974; Ögelman, et al. 1976; Kanbach, et al., 1977; and references therein). Present method does not introduce “trials” which usually reduce the significance of the results obtained, fully accounts the available knowledge on the topography of gamma ray sky, makes use of all the information about the sky, source and the instrument and therefore is the proper way of handling gamma ray data in pulsar-type searches.Presently, method is applied in the analyses of COS-B data in the context of searches for gamma ray emitting X-ray and radio pulsars. Results will be published elsewhere.     

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     

地面和机载Ku波段定向天线的标定方法

提出了一种以地球同步轨道卫星作为参考物、利用GPS位置对Ku波段地面及机载定向天线进行快速标定的方法;研究了将地心大地坐标变换到地心空间直角坐标参数和将地心空间直角坐标变换到站心极坐标的计算方法;给出了定向天线的标定实施步骤。测试结果表明,地面定向天线标定角度误差可达0.1°,机载定向天线标定角度误差可达1°,该标定精度可以满足大部分应用需求。     

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。