Multi-component synchrotron self-compton emission from NGC 1275

COS-B gamma-ray data (70–5000 MeV) in the latitude range 10°< |b| <90° are compared with the expected emission from cosmic-ray interactions with interstellar gas. An additional component is found to be necessary to explain the latitude dependence of the emission. Two possible origins for this component are discussed: a gamma-ray halo around the Galaxy and a local emission region.     

Hard X-ray observations of Cygnus X-1 with the MISO telescope

The black hole candidate Cygnus X-1 was observed in the hard X ray - soft γ ray energy range by the MISO telescope on two different occasions: in September 1979 and May 1980. We have measured two hard X-ray states of the source: in 1979 the observed spectrum confirms the superlow state measured in the same period by the HEAO-3 satellite, while in 1980 the MISO X-ray data are consistent with the so called low state of Cygnus X-1. In both occasions, no γ -ray excess has been observed above 200 KeV.     

基于Gamma过程的碳化钨涂层磨损剩余寿命

通过对碳化钨涂层磨损数据的分析,引用Gamma过 程,提出了一种有效融合现场监测数据和先验历史数据的碳化钨涂层磨损剩余寿命预测方法。首先,在历史磨损数据的基础上,确定了Gamma过程参数的先验值;其次,采用贝叶斯方法融合最新磨损监测数据,得到Gamma过程参数的更新值;然后,通过建立碳化钨涂层的实时 可靠度函数,实现剩余寿命预测;最后,通过实例对该方法进行了验证,结果表明精度比采用固定参数下的预测方法有所提高,满足工程实际的需求。     

Radiation from relativistic shocks in turbulent magnetic fields

Using our new 3-D relativistic particle-in-cell (PIC) code parallelized with MPI, we investigated long-term particle acceleration associated with a relativistic electron–positron jet propagating in an unmagnetized ambient electron–positron plasma. The simulations were performed using a much longer simulation system than our previous simulations in order to investigate the full nonlinear stage of the Weibel instability and its particle acceleration mechanism. Cold jet electrons are thermalized and ambient electrons are accelerated in the resulting shocks. Acceleration of ambient electrons leads to a maximum ambient electron density three times larger than the original value as predicted by hydrodynamic shock compression. In the jet (reverse) shock behind the bow (forward) shock the strongest electromagnetic fields are generated. These fields may lead to time dependent afterglow emission. In order to calculate radiation from first principles that goes beyond the standard synchrotron model used in astrophysical objects we have used PIC simulations. Initially we calculated radiation from electrons propagating in a uniform parallel magnetic field to verify the technique. We then used the technique to calculate emission from electrons in a small simulation system. From these simulations we obtained spectra which are consistent with those generated from electrons propagating in turbulent magnetic fields with red noise. This turbulent magnetic field is similar to the magnetic field generated at an early nonlinear stage of the Weibel instability. A fully developed shock within a larger simulation system may generate a jitter/synchrotron spectrum.     

非恒定温度场合弹上性能退化型部件贮存可靠性评估

导弹在贮存期内要反复经历运输、存放、检测、维修和战备值班等过程,其环境温度并不恒定,而是在一定范围内发生动态变化。对性能参数有变化趋势的弹上部件而言,有必要考虑环境温度变化对其可靠性的影响,因此提出一种非恒定温度剖面下的贮存可靠性评估方法。首先,分析产品实际性能退化的特点,选择带有非线性漂移项的Wiener过程描述产品的退化性能,推导出试验环境下产品的寿命分布。然后,采用Gamma分布拟合贮存期间的弹内温度分布。进而利用比例风险模型描述温度变化对产品可靠性的影响,推导弹上性能退化型部件在非恒定温度剖面下的无条件寿命分布,并给出模型参数的极大似然估计。算例表明本方法实际可行。     

激光引致激波传播规律的数值研究

空气光学击穿的激波流场结构的研究是激光与物质相互作用研究领域中的重要组成部分。利用光线追踪法,采用解耦的辐射输运方程,数值求解含能量源项的流体控制方程,对空气光学击穿诱导激波的传播过程和随时间演化规律进行了研究。通过线形拟合,给出了激波传播的后期阶段激波半径随时间的变化关系。流场中的超压波形有几个峰值,由多列压缩-稀疏波组成,并且强度越来越弱。研究结果可为激光应用技术提供一定的理论支持。     

考虑不完全维修的劣化系统最优视情维修策略

 针对实际装备维修工程中系统不能"修如新"以及修后工作时间逐渐缩短的情况,基于Gamma过程建立劣化系统的视情维修(CBM)模型,以定期检测的方式获知系统状态。当系统劣化状态超过预定阈值时采取预防性维修,维修后系统恢复至"如新"与"如旧"之间的某一随机状态;经过若干次预防性维修后,当劣化状态再次超过维修阈值时则进行预防性更换;在对系统进行预防性维修或更换之前若发生劣化故障,则进行故障后更换;通过对检测周期和更换策略联合优化,使得系统长期运行费用率最低。最后通过算例说明CBM模型的可行性,并利用Monte Carlo算法仿真验证模型的正确性。     

光照处理中改进的Gamma矫正方法

在图像处理中，光照始终是影响图像质量的重要因素。为了有效弱化光照对图像质量的影响，利用非线性函数叠加的方法构造了一个合理的Gamma值变化曲线，使Gamma矫正方法充分适应了图像中光照变化的实际情况，并有效防止了Gamma矫正可能产生的图像失真。实验证明该方法在改善图像光照条件、提高图像质量方面具有良好的性能。     

Effect of gamma irradiation on hyperthermal composting microorganisms for feasible application in space

The composting system is the most efficient method for processing organic waste in space; however, the composting activity of microorganisms can be altered by cosmic rays. In this study, the effect of ionizing irradiation on composting bacteria was investigated. Sequence analyses of amplified 16S rRNA, 18S rRNA, and amoA genes were used to identify hyperthermal composting microorganisms. The viability of microorganisms in compost soil after gamma irradiation was directly determined using LIVE/DEAD BacLight viability kit. The dominant bacterial genera were Weissella cibaria and Leuconostoc sp., and the fungal genera were Metschnikowia bicuspidata and Pichia guilliermondii. Gamma irradiation up to a dose of 10 kGy did not significantly alter the microbial population. Furthermore, amylase and cellulase activities were maintained after high-dose gamma irradiation. Our results show that hyperthermal microorganisms can be used to recycle agricultural and fermented material in space stations and other human-inhabiting facilities on the Moon, Mars, and other planets.