利用可靠性模型确定电子测量设备检定周期的方法

周期检定是保障计量器具能够准确可靠地开展测量活动的重要手段。检定周期的长度影响计量器具测量活动的可靠性和计量工作的经济性。本文通过建立电子测量设备测量可靠性与使用时间关系的数学模型提出了利用可靠性模型确定电子测量设备检定周期的可靠性评估法。该方法可以有效地保证电子测量设备检定周期制定的科学性。     

可靠性预计与分配的作用研究

阐述了可靠性预计与分配对装备作战能力、生存力、部署机动能力、维修人力和使用保障费用等方面的重要作用,以及它在战争中取胜的重要性。同时指出了在民用产品方面加强可靠性预计与分配可以有效提高产品的市场竞争力。     

RTCADO-178B标准与相关国军标的对照分析

RTCA的DO-178B标准是国际认可的开发准则,将DO-178B与我国的国标进行了对照分析,给出了异同。     

文献A Successful Strategy for Satellite Development and Testing点评

文章对美国在1998-2002年执行"快,好,省"采购改革方案期间航天器故障率上升146%的3个原因进行了分析与点评.这3个原因包括:对标准、规范严格遵循的意识下降;航天元器件复合度激增;系统工程管理失控.文章对抑制故障率上升的对策进行归纳,其中最重要的一条是:卫星研制工作必须严谨,一丝不苟地按照相关标准进行(环境)试验.     

变量相关情况下基于马尔可夫链样本模拟的线抽样可靠性灵敏度分析方法

针对变量具有相关性的可靠性灵敏度分析问题,提出了一种变量相关情况下基于马尔可夫链样本模拟的线抽样可靠性灵敏度分析方法。在所提方法中,首先将相关变量等价转换为独立正态变量,然后采用基于马尔可夫链样本模拟的线抽样方法,求解失效概率对等价独立正态变量分布参数的偏导数,最后利用等价变换前后变量分布参数之间的解析关系和复合函数求导法则,求得失效概率对相关变量分布参数的可靠性灵敏度。为了解所提方法的效率和精度,对所提方法的可靠性灵敏度估计值进行了方差分析。由于所提方法采用马尔可夫链快速产生失效域中的条件样本,这些失效域中的样本可用来准确获取重要方向,并可作为线抽样的随机样本,因而该方法具有很高的抽样效率。算例结果表明,所提方法是一种计算相关变量可靠性灵敏度的高效率、高精度方法。     

某型导弹伸缩翼展开可靠性评估

与固定翼相比,伸缩翼能够有效减少飞机弹仓的空间占用,但由于伸缩翼存在运动机构,其带来的可靠性下降成为不可忽视的问题。为探究新型机构的可靠度,本文从理论方面计算某型伸缩翼展开机构的定位可靠性;采用 Adams 对伸缩翼展开过程进行仿真,结合 Adams/Insight 模块计算在考虑摩擦力条件下的卡滞可靠性,并对伸缩翼卡滞失效原因进行分析。结果表明：异物的存在使伸缩翼的定位可靠性显著降低,适当增加上下翼弹簧的预载荷能够有效减小伸缩翼展开机构的卡滞失效,上下翼弹簧在上翼质心产生的附加力矩会降低伸缩翼的卡滞可靠性。     

Heat storage and electricity generation in the Moon during the lunar night

One of the biggest challenges of the exploration of the Moon is the survival of the crew and the lunar assets during the lunar night. The environmental conditions on the lunar surface and its cycle, with long periods of darkness, make any long mission in need of specific amounts of heat and electricity to be successful. We have analyzed two different systems to produce heat and electricity on the Moon's surface. The first system consists of Thermal Wadis, sources of thermal power that can be used to supply heat to protect the exploration systems from the extreme cold during periods of darkness. Previous results showed that Wadis can supply enough heat to keep lunar devices such as rovers above their minimum operating temperature (approximately 243 K). The second system studied here is the Thermal Energy Storage (TES), which is able to run a heat engine during the lunar night to produce electricity. When the Sun is shining on the Moon's surface, the system can run the engine directly using the solar power and simultaneously heat a thermal mass. This thermal mass is used as a high temperature source to run the heat engine during the night. We present analytical and numerical calculations for the determination of an appropriate thermal mass for the TES system.     

Equatorial Ionospheric Anomaly (EIA) and comparison with IRI model during descending phase of solar activity (2005–2009)

The ionospheric variability at equatorial and low latitude region is known to be extreme as compared to mid latitude region. In this study the ionospheric total electron content (TEC), is derived by analyzing dual frequency Global Positioning System (GPS) data recorded at two stations separated by 325 km near the Indian equatorial anomaly region, Varanasi (Geog latitude 25°, 16^/ N, longitude 82°, 59^/ E, Geomagnetic latitude 16°, 08^/ N) and Kanpur (Geog latitude 26°, 18^/ N, longitude 80°, 12^/ E, Geomagnetic latitude 17°, 18^/ N). Specifically, we studied monthly, seasonal and annual variations as well as solar and geomagnetic effects on the equatorial ionospheric anomaly (EIA) during the descending phase of solar activity from 2005 to 2009. It is found that the maximum TEC (EIA) near equatorial anomaly crest yield their maximum values during the equinox months and their minimum values during the summer. Using monthly averaged peak magnitude of TEC, a clear semi-annual variation is seen with two maxima occurring in both spring and autumn. Results also showed the presence of winter anomaly or seasonal anomaly in the EIA crest throughout the period 2005–2009 only except during the deep solar minimum year 2007–2008. The correlation analysis indicate that the variation of EIA crest is more affected by solar activity compared to geomagnetic activity with maximum dependence on the solar EUV flux, which is attributed to direct link of EUV flux on the formation of ionosphere and main agent of the ionization. The statistical mean occurrence of EIA crest in TEC during the year from 2005 to 2009 is found to around 12:54 LT hour and at 21.12° N geographic latitude. The crest of EIA shifts towards lower latitudes and the rate of shift of the crest latitude during this period is found to be 0.87° N/per year. The comparison between IRI models with observation during this period has been made and comparison is poor with increasing solar activity with maximum difference during the year 2005.     

基于BM3803的1553B总线通信软件设计

在某卫星地面检测设备中使用BM3803处理器来模拟卫星中的总线控制端对远程终端进行检测,构建了比传统的Windows+1553B_PCI板卡方案实时性更强的卫星数据仿真平台。首先向BM3803移植了实时操作系统μC/OS II,设计了适用于BM3803的板级支持包,保证了软件的可在轨更新和任务的实时性,确定了用户任务与硬件高度分离的软件结构。在设计μC/OS II的用户任务时,充分利用BM3803和B61580的校验功能,提高了软件的可靠性。最后令本设计和Windows+1553B_PCI板卡方案完成相同的用户任务,对比可得本设计有更好的实时性,可满足卫星高层通信协议对实时性的要求。     

基于学科链的卫星系统工程方法与实践

目前,绝大多数的卫星系统都是按照分系统来设计的,这种方法的弊端在于分系统内部重复的功能模块对整星而言是冗余的。因此,为了摒除按照分系统设计的卫星系统缺点以提高系统可靠性,我们设计了一个全新的卫星系统,其基于学科功能链。按照学科功能链,我们将卫星系统划分为控制学科链、结构热学科链、电子学学科链、载荷学科链,显著提高了卫星系统的性能、可靠性和功能密度,同时有效降低了研制成本,缩短了研制周期。最终,基于学科链的卫星系统已成功应用于北斗导航全球系统的首发卫星上。本文阐述了基于学科链设计的核心思想和四个主要的学科链内涵。