飞机电机、电器产品濕热试验分析报告

一九七一年由三机部、六院组织编制了《飞机电机、电器产品通用技术条件》初稿。关于产品周期交变湿热试验的方法,原则上沿用一机部标准(JD839—66),试验时间、绝缘电阻等项标准之确定,则缺乏试验依据,因此难以统一。遵照毛主席“一切经过试验”的教     

类IXV飞行器初期再入制导与姿态控制方法研究

摘要： 针对类IXV飞行器无翼式升力体构型及采用RCS/尾襟翼组合控制特点,研究其初期再入段的高精度制导与姿态控制方法.设计带过程约束的数值预测 校正制导律以提高制导系统的鲁棒性及精确性;根据其执行机构配置特点,设计基于RCS的航向控制律及基于RCS/气动舵的纵、横向复合控制律,并采用鲁棒伺服LQR技术进行控制参数快速设计.通过蒙特卡洛打靶仿真来验证算法的精度及鲁棒性.     

第32届机构间空间碎片协调委员会会议在京召开

2014年5月12-15日,第32届机构间空间碎片协调委员会（IADC）会议在北京召开,中国国家航天局、意大利航天局、法国国家空间研究中心、加拿大航天局、德国航空航天中心、欧洲航天局、印度空间研究组织、日本宇宙航空研究开发机构、美国航空航天局、俄罗斯联邦航天局、英国国家航天局等11个正式成员机构,亚太空间合作组织以及作为IADC观察员的韩国航天局参加了此次会议,外交部、中科院等国内有关部门代表也应邀出席了此次会议。参加会议的国内外代表共150多人。     

一种跟随式大磁矩磁力矩器高反电势抑制技术

摘要： 提出一种可以实现大磁矩磁力矩器磁棒电流续流时间自动调节的控制方法,该方法既可以抑制大磁矩磁力矩器高反电势的产生,又无需增加功率器件为磁棒电流提供续流回路,大幅减小控制线路的体积及热设计难度,同时可以满足输出磁矩在小幅值内频繁变换方向的使用要求.     

MX导弹第二级发动机

引言MX导弹第二级发动机用来提供飞行第二阶段的动力,以及飞行第一阶段和第二阶段的滚转控制力矩。MX导弹第二级发动机的直径为92英寸(2337毫米),长220.4英寸(5598毫米),毛重60234磅(27322公斤),其基本结构如图1所示。经过16个月的系统论证(SD)和头4个月的全尺寸工程研制(FSED),第二级发动机业已进行了优化,以便满足系统要     

基于Tersoff-Brenner势的航天器群图形编队研究

从分子动力学模拟角度提出了一种分布式航天器群导航控制方法,可使行星中心开普勒轨道上的航天器群在有限的感知信息条件下自发实现图形编队.该法基于人工势场技术,主要分为两个部分：改造自C-W方程的外围全局汇聚势场和基于Tersoff-Brenner势的局部塑形势场.前者将各航天器导引至预设汇聚点附近,后者进一步使各航天器自我调整彼此相对位置,最终编成期望构型.此外,引入一速度依赖型耗散项以确保任意初始分布条件下图形编队均收敛.通过地球同步轨道上航天器群正四面体构型（含中心,即金刚石结构单元）编队仿真,验证了所提方法的有效性和优越性.将编队脚本简单修改,该法还可方便用于其它类碳元素同素异形体构型的塑造,如石墨晶体结构单元正六边形等.     

《宇航计测技术》撰稿须知CSCD

一、征稿范围无线电、时间频率、电磁学、电离辐射、化学和光学等计量标准的设计、研制和计量测试技术、仪器仪表的检定维修技术、误差分析及数据处理技术;石英晶体器件的设计和研制、电子技术应用、自动化测量、计量产品介绍、国内外计量信息、计量测试动态及发展趋势等。     

Some ecological mechanisms to generate habitability in planetary subsurface areas by chemolithotrophic communities: the Río Tinto subsurface ecosystem as a model system

Chemolithotrophic communities that colonize subsurface habitats have great relevance for the astrobiological exploration of our Solar System. We hypothesize that the chemical and thermal stabilization of an environment through microbial activity could make a given planetary region habitable. The MARTE project ground-truth drilling campaigns that sampled cryptic subsurface microbial communities in the basement of the Río Tinto headwaters have shown that acidic surficial habitats are the result of the microbial oxidation of pyritic ores. The oxidation process is exothermic and releases heat under both aerobic and anaerobic conditions. These microbial communities can maintain the subsurface habitat temperature through storage heat if the subsurface temperature does not exceed their maximum growth temperature. In the acidic solutions of the Río Tinto, ferric iron acts as an effective buffer for controlling water pH. Under anaerobic conditions, ferric iron is the oxidant used by microbes to decompose pyrite through the production of sulfate, ferrous iron, and protons. The integration between the physical and chemical processes mediated by microorganisms with those driven by the local geology and hydrology have led us to hypothesize that thermal and chemical regulation mechanisms exist in this environment and that these homeostatic mechanisms could play an essential role in creating habitable areas for other types of microorganisms. Therefore, searching for the physicochemical expression of extinct and extant homeostatic mechanisms through physical and chemical anomalies in the Mars crust (i.e., local thermal gradient or high concentration of unusual products such as ferric sulfates precipitated out from acidic solutions produced by hypothetical microbial communities) could be a first step in the search for biological traces of a putative extant or extinct Mars biosphere.     

遥测的过去现在和将来

本文回顾了二十年前的遥测技术,与目前的技术作了比较,并对将来的遥测作出了推测。评述的内容包括:遥测系统的特性、设备的单元价格、遥测在过去、目前的应用情况以及未来可能获得的应用。本文中关键的字眼是“选择”。二十年前,用户在设备和技术方面都没有什么选择的余地,但现在的技术提供了一个广泛的选择范围;有迹象表明,今后在性能、价格以及遥测作为数据采集和处理手段方面会有更广泛的选择。     

A sulfur-based survival strategy for putative phototrophic life in the venusian atmosphere

Several observations indicate that the cloud deck of the venusian atmosphere may provide a plausible refuge for microbial life. Having originated in a hot proto-ocean or been brought in by meteorites from Earth (or Mars), early life on Venus could have adapted to a dry, acidic atmospheric niche as the warming planet lost its oceans. The greatest obstacle for the survival of any organism in this niche may be high doses of ultraviolet (UV) radiation. Here we make the argument that such an organism may utilize sulfur allotropes present in the venusian atmosphere, particularly S(8), as a UV sunscreen, as an energy-converting pigment, or as a means for converting UV light to lower frequencies that can be used for photosynthesis. Thus, life could exist today in the clouds of Venus.