航天器异常与空间环境

本文研究考查了靠近或在地球同步轨道上的ＳＣＡＴＨＡ、ＴＤＲＳ－１卫星以及ＧＰＳ、ＧＯＥＳ卫星组等的各自１０年左右运行时间中,空间环境所导致航天器异常的发生率的年分布特征,月分布特征,地方时分布特征以及不同类型的发生率分布特征。结果表明,由于不同空间环境因素对航天器作用不同,引起异常类型不一样,因此,太阳长周期和短月,地方时周期活动对航天器异常发生率影响无简单的统一规律特征;长周期中的单粒子事件是由     

NMD中导弹预警卫星系统的发展

介绍了美国国家导弹防御系统(NMD)的核心——导弹预警卫星系统自1959年以来的发展和未来趋势，详细阐述了国防支援计划(DSP)与天基红外预警卫星系统(SBIRS)的进展，并探讨了未来美国国家弹道导弹防御计划中导弹预警系统的组成和功能。     

复杂零件加工过程质量控制与改进方法研究

针对航空复杂零件加工过程误差监控、溯源及过程调整问题,提出了一种复杂零件加工过程质量控制与改进方法。在传统SPC质量监控方法的基础上,设计了扩展误差流与MSPC集成的监控策略,并分别设计了单元、多元以及非线性profile的三种控制图;针对因果关系明确的几何定位误差的分解与溯源,建立了基于动态Bayesian网络的因果模型,针对误差源因果关系不明确的受力变形误差的分解与溯源,建立了基于粒子群(PSO)改进的支持向量机的误差溯源方法;在加工过程质量波动调整方面,引入多元工程过程控制(MEPC)理论,建立了MSPC与MEPC集成的加工过程波动调整方法。     

聚酰亚胺薄膜在γ射线辐照下的力学性能退化研究

聚酰亚胺(PI)薄膜在空间高能粒子辐射环境下会发生力学性能退化。文章利用钴源辐照试验装置和热重分析、XPS分析等对均苯型PI薄膜在γ射线辐照下的力学性能退化及其规律进行研究,发现在γ射线辐照下,PI薄膜有明显的总剂量效应和剂量率效应。     

NEPE推进剂中聚乙二醇的结晶性

利用X射线衍射技术研究了NEPE推进剂中聚乙二醇的结晶特性。探讨了填料、化学交联和增逆剂对聚乙二醇结晶的影响，实验结果表明上述几种因素都会显著降低聚乙二醇的结晶性。     

雷达罩的综合优化设计

在分析对比现有的雷达罩设计方法基础上，针对某型直升机机栽雷达罩，研究了雷达罩设计过程中的基本问题、关键技术和综合优化设计方法，运用三维射线追踪法进行了计算机辅助设计，给出了布设防雷击部件的经验公式，讨论了吸波材料选择与喷涂的基本准则。电测结果表明：加罩后的功率传输系数、反射瓣、雷达辐射特性等指标的实测数据与计算值符合较好，满足了设计要求。     

电磁波在电离层中的传输建模分析

电磁波从宇宙空间对地传输过程中,不可避免需要穿过地球电离层,并受到电离层折射、反射、穿透等影响。为研究电离层中电磁波的传播路径,利用IRI2016电离层模型和NRLMSISE-00模型的数据,基于射线追踪算法,综合利用龙格-库塔法,并采用变步长实现了电磁波在电离层多层空间复杂等离子体中的传输计算。同时,还研究了不同频率和纬度的电磁波在电离层的传播途径。研究表明较高频率的电磁波受到电离层的干扰较少,在100MHz时,电磁传播的偏移角度仅为0.795度;电离层的非均匀层状结构决定了电磁波在其中的传输存在多模现象,并受到了光照的影响,在日间和中纬均受电离层的强烈干扰,偏移角度均大于2.2度,较夜间和低、高纬地区的传输偏移更大。     

Search for antihelium: Progress with BESS

In this paper, we report searches for antihelium in cosmic rays using two recently flown magnetic rigidity spectrometers. BESS-TeV had extended rigidity with an MDR of 1.4 TV and had a flight duration of one day. BESS-Polar was optimized for collecting power. It was flown for 8.5 days and had an MDR of 240 GV. The former flight allows us to explore a previously unexplored rigidity band and the latter flight yields a factor of three improvement in the overall BESS limit. No antihelium candidate was found in the rigidity ranges of 1–500 GV, and 0.6–20 GV, among 7 × 10⁴ events taken with BESS-TeV, and 8 × 10⁶ events taken with BESS-Polar, respectively.     

Cosmic ray variations of solar origin in relation to human physiological state during the December 2006 solar extreme events

There is an increasing amount of evidence linking biological effects to solar and geomagnetic disturbances. A series of studies is published referring to the changes in human physiological responses at different levels of geomagnetic activity. In this study, the possible relation between the daily variations of cosmic ray intensity, measured by the Neutron Monitor at the Cosmic Ray Station of the University of Athens (http://cosray.phys.uoa.gr) and the average daily and hourly heart rate variations of persons, with no symptoms or hospital admission, monitored by Holter electrocardiogram, is considered. This work refers to a group of persons admitted to the cardiological clinic of the KAT Hospital in Athens during the time period from 4th to 24th December 2006 that is characterized by extreme solar and geomagnetic activity. A series of Forbush decreases started on 6th December and lasted until the end of the month and a great solar proton event causing a Ground Level Enhancement (GLE) of the cosmic ray intensity on 13th December occurred. A sudden decrease of the cosmic ray intensity on 15th December, when a geomagnetic storm was registered, was also recorded in Athens Neutron Monitor station (cut-off rigidity 8.53 GV) with amplitude of 4%. It is noticed that during geomagnetically quiet days the heart rate and the cosmic ray intensity variations are positively correlated. When intense cosmic ray variations, like Forbush decreases and relativistic proton events produced by strong solar phenomena occur, cosmic ray intensity and heart rate get minimum values and their variations, also, coincide. During these events the correlation coefficient of these two parameters changes and follows the behavior of the cosmic ray intensity variations. This is only a small part of an extended investigation, which has begun using data from the year 2002 and is still in progress.     

利用地面宇宙线强度变化预报地磁暴方法初步研究

分析了Nagoya宇宙线闪烁体望远镜探测数据的变化特点,定性地探讨了CME可能引起的地面宇宙线的变化特征,通过实例证实了地面宇宙线通量的异常波动是地磁暴发生的重要先兆特征,并且将8 h内宇宙线通量与该时间段内平均通量的偏差D8(t)参数应用到宇宙线数据分析中.通过数据分析与讨论,认为D8(t)参数达到一定阈值是地磁暴的重要先兆特征,但不是充分条件,虚假信号仍占多数;D8(t)参数与太阳质子事件探测结果相结合,对于大地磁暴的预报有较好的效果.