导航卫星原子钟舱温度控制方法及其验证

原子钟是导航卫星的重要组成部分,可为卫星系统提供高准确及高稳定度的时间频率源.原子钟工作性能与环境温度变化密切相关,为保证其在轨连续、稳定运行,热控系统需为其提供良好的工作温度环境.本文以某导航卫星原子钟舱温度控制为研究内容,给出原子钟舱热控设计方案、控制算法,并进行仿真分析和试验验证.在轨遥测数据表明,卫星原子钟舱热控方案和控制算法设计合理,仿真分析及试验结果有效,各原子钟在轨工作温度满足要求,原子钟温度稳定度满足并优于设计指标近一个数量级.     

现场可修系统的可靠性数据处理

用随机点过程模型来处理航空产品现场可修系统的可靠性数据时,存在系统故障修复次数少,数据不齐全的问题。为此,对符合非时齐泊松过程模型的数据作为“修复如新”处理时,所所应满足的条件及适用范围作了分析,通过数字仿真对精度的计算,在工作应用中,当系统修复次数小于或等于３时,可将“修复如旧”的系统当作“修复如新”的模型处理,但要注意参数ｍ的影响;对残存比率法应用于可修系统数据处理时的可能性进行了讨论。仿真结     

影响氢原子钟长期稳定度的系统效应分析

进一步改进氢钟的频率稳定度,需要了解影响频率稳定度的各个过程及其影响的相对大小。讨论影响氢钟频率稳定度的各种系统过程。这种分析能够使钟的研制者和用户去识别稳定度的限制因素并加以选择以便改进。     

Are Boltzmann plots of hydrogen Balmer lines a tool for identifying a subclass of S1 AGN?

It is becoming clear that we can define two different types of nearby AGN belonging to the Seyfert 1 class (S1), on the basis of the match of the intensities of their Broad Balmer Lines (BBL) with the Boltzmann Plots (BP). These two types of S1 galaxies, that we call BP-S1 and NoBP-S1, are characterized, in first approximation, by Broad Line Regions (BLR) with different structural and physical properties. In this communication, we show that these features can be well pointed out by a multi-wavelength analysis of the continuum and of the broad recombination Hydrogen lines, that we carry out on a sample of objects detected at optical and X-ray frequencies. The investigation is addressed to verify whether BP-S1 are the ideal candidates for the study of the kinematical and structural properties of the BLR, in order to derive reliable estimates of the mass of their central engine and to constrain the properties of their nuclear continuum spectrum.     

Kapton抗原子氧侵蚀的Al2O3涂层研究

在原子氧侵蚀地面模拟设备中对Kapton和利用反应溅射制备的Al2O3涂层进行了原子氧暴露实验,并采用XPS和SEM等分析手段对暴露前后试样表面的物理和化学变化进行了研究。结果表明,Kapton试样遭受了严重的侵蚀,质量损失较大;Al2O3涂层质量变化很小,对基体提供了良好的保护作用。XPS分析结果表明,Kapton的羰基与原子氧作用时形成CO2,随后CO2气体脱附。反应溅射的Al2O3涂层是富Al的,初始暴露时由于氧化反应而质量有少许增加,随时间延长,涂层变得完全符合化学计量。     

An investigation of the solar cycle impact on the lower thermosphere O(S) nightglow emission as observed by WINDII/UARS

The yearly variation of the integrated emission rate of the O(¹S) nightglow in the lower thermosphere is studied and the solar cycle impact is examined from the observations of the Wind Imaging Interferometer (WINDII) operated on the Upper Atmosphere Research Satellite (UARS). More than 300,000 volume emission rate profiles of the O(¹S) nightglow observed by WINDII for 40°S–40°N latitudes during November 1991–August 1997 over half of a solar cycle are utilized. These profiles are vertically integrated for the altitude range of 80–100 km and the equivalent column integrated emission rates are then zonally averaged for bins with 10° latitude and 3 month intervals. It is found that for each latitude the O(¹S) nightglow emission rate appears to increase with increasing solar F10.7 cm flux, following a linear relationship. This characterizes the solar cycle impact on the O(¹S) nightglow, while the solar influence is modulated by a seasonal variation. Based on these variations, an empirical formula is derived for predicting the three-month averages of the O(¹S) nightglow integrated emission rate. The standard error of the estimated values from the formula is smaller than 30 Rayleigh.     

考虑备件约束的多部件串联系统使用可用度计算方法

使用可用度是衡量装备系统保障效能的重要指标,而备件供应是保障活动中的关键,故在计算系统的使用可用度时有必要考虑备件约束对其的影响。在现有的使用可用度计算方法中,马尔可夫更新理论很少用于分析考虑备件的系统,基于库存理论的可用度计算模型没有考虑备件供应延误对系统更换维修活动的影响。为了解决以上问题,首先将整个系统故障与维修过程分为故障系统的更换维修和故障件的维修周转2个子过程,并分析了2个子过程之间的影响关系;然后给出一种考虑备件约束的多部件串联系统使用可用度计算模型;最后实例分析表明,该模型可以方便地计算多部件串联系统的使用可用度,且与库存理论中的计算模型相比,该模型计算结果与仿真结果更为接近。     

本地标准时间频率的产生与保持

近年来,地方协调时UTC(BIRM)守时能力稳步提升,截至目前,UTC(BIRM)与UTC的相对频率偏差优于3E-14,时间偏差优于20ns。本文概括介绍了守时系统的组成,本地频率驾驭与主备同步技术,以及TA(BIRM)算法研究等。