复合绝热管气囊成型工艺设计和实验

对两端收口复合绝热管进行了工艺方案分析,确定气囊成型工艺为优选工艺方案,在此基础上阐述了气囊成型工艺设计的原则,依据这个原则开展了典型样件的研制.结果表明：方案选择合理,工艺设计完整、可靠,产品满足各项指标要求.     

基于参数优化的截尾序贯检验法

截尾序贯概率比检验法和序贯网图检验法（SMT）是在序贯概率比检验法（SPRT）的基础上发展起来的2种方法,可进一步控制试验次数。但是这些截尾序贯方法的停止边界仍有待优化,本文以最常见的截尾SPRT为例,说明决定停止边界的参数的取值直接影响了最大试验样本量,且存在最佳取值。并以此为基础,对SMT和传统的SPRT进行了综合比较,发现截尾SMT并不优于传统的截尾SPRT,它不过是一种广义形式的截尾序贯检验法,SPRT的研究重点应该是截尾形式的构造。最后本文提供了一种曲线形式的截尾序贯检验法.     

地球物理导航中位场下延的迭代正则化方法研究

地磁、重力数据下延是制备地球物理导航基准图的重要内容,而它通常是一个不适定问题,采用常规代数方法求解并不奏效;对此,结合航空地球物理测量和地球物理导航的特点,研究了迭代正则化方法(包括迭代Tikhonov法、Landweber迭代法和截断奇异值分解(TSVD)法)在位场下延中的应用.首先给出了位场下延和迭代正则化的基本理论,然后采用理论位场模型验证了迭代正则化方法在位场下延中的应用可行性,最后分析了迭代正则化方法的下延精度、计算时间和边界效应等性能.由分析结果可知,迭代Tikhonov方法具有最好的综合下延性能,应优先在实际的位场下延中使用.     

Robotic Instrument for Grinding Rocks Into Thin Sections (GRITS)

We have developed a rock grinding and polishing mechanism for in situ planetary exploration based on abrasive disks, called Grinding Rocks Into Thin Sections (GRITS). Performance characteristics and design considerations of GRITS are presented. GRITS was developed as part of a broader effort to develop an in situ automated rock thin section (ISARTS) instrument. The objective of IS-ARTS was to develop an instrument capable of producing petrographic rock thin sections on a planetary science spacecraft. GRITS may also be useful to other planetary science missions with in situ instruments in which rock surface preparation are necessary.     

Mars Sample Return: Do Australians trust NASA?

Mars Sample Return (MSR) represents an important scientific goal in space exploration. Any sample return mission will be extremely challenging from a scientific, economic and technical standpoint. But equally testing, will be communicating with a public that may have a very different perception of the mission. A MSR mission will generate international publicity and it is vital that NASA acknowledge the nature and extent of public concern about the mission risks and, perhaps equally importantly, the public’s confidence in NASA’s ability to prepare for and manage these risks. This study investigated the level of trust in NASA in an Australian population sample, and whether this trust was dependent on demographic variables. Participants completed an online survey that explored their attitudes towards NASA and a MSR mission. The results suggested that people believe NASA will complete the mission successfully but have doubts as to whether NASA will be honest when communicating with the public. The most significant finding to emerge from this study was that confidence in NASA was significantly (p < 0.05) related to the respondent’s level of knowledge regarding the risks and benefits of MSR. These results have important implications for risk management and communication.     

直线度测量中采样间距与偏差形状关系的理论研究

从频域理论上对直线度测量中采样间距与偏差形状的吻合关系进行了较为深入的理论分析，提出在相同的采样误差条件下，随着采样点数的增加，测量误差将随之下降。因此，直线度测量采样间距的选择应按测量准确度要求来确定。     

A sample collector for robotic sample return missions I: Temperature effect on collected mass

Sample return is playing an increasingly important role in solar system exploration. Among the possible mission on the horizon, are sample return from asteroids, comets, the Moon and Mars. A collector initially intended for near-Earth asteroids is the touch-and-go-impregnable-pad (TGIP). Here we explore the effect of temperature on its collection capabilities. Temperatures expected on near-Earth asteroid mission targets range from −43 to 36 °C. Experiments were conducted at −75, −50, −25, 23, 65, and 105 °C. It was found that the mass of sample collected by the TGIP increased almost linearly to 23 °C and then leveled off at higher temperatures. We also found that the collector did not lose its ability to collect samples after being subjected to −75 °C temperatures (essentially frozen) and then thawed. These experiments have shown that the TGIP can operate effectively at temperatures expected on near-Earth asteroids, especially if collection is performed on the sunward side of the asteroid.     

A sample collector for robotic sample return missions II: Radiation tests

Sample return from small solar system objects is playing an increasingly important part in solar system exploration. Critical to such missions is a robust, simple, and economic sample collector. We have developed a collector such as this for near-Earth asteroid sample return missions that we have termed the Touch-and-Go Impregnable Pad (TGIP). The collector utilizes a silicone substrate that is pushed into the dust and gravel surface layer of the asteroid. As part of a systematic evaluation of the TGIP, we have investigated the resilience of this substrate to ionizing radiations. Several miniature versions of the collector, containing typically ∼3 g of the collection substrate, were exposed to 0.564 MeV beta particles from a ⁹⁰Sr source and a 6 MeV electron beam in a linear accelerator to simulate the wide range of energies of solar and galactic ionizing radiation. Various radiation levels up to eight times greater than expected on a six-year asteroid mission (in the case of beta radiation) and 50 times greater than expected (in the case of the 6 MeV electron radiation) were administered to the substrate. After irradiation, the efficiency of the substrate in collecting samples of mock regolith was compared with that of collectors that had not been irradiated. No difference beyond experimental uncertainty was observed and we suggest that the operational TGIP will not be affected adversely by radiation doses expected during a typical six-year inner solar system mission.     

Traverses for the ISECG-GER design reference mission for humans on the lunar surface

This study explores the Design Reference Mission (DRM) architecture developed by Hufenbach et al. (2015) as a prelude to the release of the 2018 Global Exploration Roadmap (GER) developed by the International Space Exploration Coordination Group (ISECG). The focus of this study is the exploration of the south polar region of the Moon, a region that has not been visited by any human missions, yet exhibits a multitude of scientifically important locations – the investigation of which will address long standing questions in lunar research. This DRM architecture involves five landing sites (Malapert massif, South Pole/Shackleton crater, Schrödinger basin, Antoniadi crater, and the South Pole-Aitken basin center), to be visited in sequential years by crew, beginning in 2028. Two Lunar Electric Rovers (LER) are proposed to be tele-robotically operated between sites to rendez-vous with crew at the time of the next landing. With engineering parameters in mind we explore the feasibility of tele-robotic operation of these LERs between lunar landing sites, and identify potential high interest sampling locations en-route. Additionally, in-depth sample collection and return traverses are identified for each individual landing site across key geologic terrains that also detail crew Extra-Vehicular Activity (EVA). Exploration at and between landing sites is designed to address a suite of National Research Council (2007) scientific concepts.     

广义Weibull分布参数的收缩估计

在右删失样本下,研究了双参数广义Weibull分布参数的极大似然估计。针 对在小样本或高度删失样本下参数估计效果差的问题,引入了收缩估计方法,将先验信息与 样本信息相结合,用于改善参数估计。分别在单参数和双参数含有先验信息两种情形下,给 出了分布参数的收缩估计。以定数截尾样本为例,利用Monte\|Carlo方法对收缩估计与极 大似然估计进行了比较,模拟结果表明在一定的条件下,收缩估计具有更优的统计性质。数 值算例表明,在小样本或高度截尾样本下,双参数广义Weibull分布参数的收缩估计具有较 好的效果。