天问一号着陆器大底分离触发条件设计方法

针对天问一号着陆器防热大底分离触发条件确定问题,利用数学仿真的方法分析气动特性、防热大底相对着陆器姿态运动等因素对分离安全性的影响,给出可安全分离的触发条件.不同分离触发马赫数的仿真结果表明,较大分离马赫数的碰撞风险较高,但防热大底长期运动趋势由弹道系数决定,相比着陆器下降更快.根据伞降过程着陆器姿态运动及伞绳力特点,...     

创造具有自身特色的经营策略：———论云南航空公司的经营策略

阐述了在国内外航空市场的竞争压力下航空公司应采取的措施。针对过去和未来一段时期内国际航空市场的变化，结合云南航空公司的实际情况，分析了国内航线和国际航线运营状况，提出了具有其自身特色的发展战略和经营策略。     

基于Gauss-Newton法的L1数据拟合

在数据拟合中，当个别数据存在较大测量误差时，采用Ｌ１准则对数据进行拟合要优于最小二乘准则。本文通过建立Ｌ１准则与最小二乘准则之间的关系，给出了一种基于Ｇａｕｓｓ－Ｎｅｗｔｏｎ法的Ｌ１数据拟合自满。计算结果表明，该方法易于理解，便于编程，具有一定的理论意义和现实意义。     

Sulfur “concrete” for lunar applications – Sublimation concerns

Melting sulfur and mixing it with an aggregate to form “concrete” is commercially well established and constitutes a material that is particularly well-suited for use in corrosive environments. Discovery of the mineral troilite (FeS) on the moon poses the question of extracting the sulfur for use as a lunar construction material. This would be an attractive alternative to conventional concrete as it does not require water. However, the viability of sulfur concrete in a lunar environment, which is characterized by lack of an atmosphere and extreme temperatures, is not well understood. Here it is assumed that the lunar ore can be mined, refined, and the raw sulfur melded with appropriate lunar regolith to form, for example, bricks. This study evaluates pure sulfur and two sets of small sulfur concrete samples that have been prepared using JSC-1 lunar stimulant and SiO₂ powder as aggregate additions. Each set was subjected to extended periods in a vacuum environment to evaluate sublimation issues. Results from these experiments are presented and discussed within the context of the lunar environment.     

四边Bézier曲面与三角B-B曲面的光滑拼接

 <正> 三角B-B曲面具有许多类似于四边B（?）zier曲面的性质,如果将二者结合使用,则可以处理比较复杂的问题,有重要的实用意义。最近,刘鼎元教授给出了四边B（?）zier曲面片G¹拼接的充分必要条件,并给出了G^拼接的两个充分条件:简单连接条件和升阶连接条件。本文将升阶连接条件用于四边B（?）zier曲面和三角B-B曲面的G¹拼接。结合使用简单连接条件,解决了在一般G¹连续的四边B（?）zier曲面中嵌入G¹连续的三角B-B曲面片的问题。     

基于DSP的UAV飞控计算机设计与半物理仿真

飞行控制计算机(FCC)作为飞行控制系统的核心，担负着多种任务。随着系统功能的日益增多，飞行包线的不断扩大，模拟式FCC已经越来越不能满足系统要求。针对目前FCC向数字式、智能化方向发展，本文利用高速DSP芯片，结合复杂可编程器件(CPLD)，设计出一种集高可靠性、高集成度、高精度于一体的新型FCC，最后在此基础上外加了数据采集卡组成闭环半物理系统，并进行了仿真。仿真结果表明，本文这一全新尝试完全可行，且应用前景将非常广泛。     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

The History and Dynamics of Comet 9P/Tempel 1

Since its discovery in 1867, periodic comet 9P/Tempel 1 has been observed at 10 returns to perihelion, including all its returns since 1967. The observations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary nucleus. The successful nongravitational acceleration model did not assume any change in the comet’s ability to outgas from one apparition to the next and the outgassing was assumed to reach a maximum at perihelion. The success of this model over the 1967–2003 interval suggests that the comet’s spin axis is currently stable. Rough calculations suggest that the collision of the impactor released by the Deep Impact spacecraft will not provide a noticeable perturbation on the comet’s orbit nor will any new vent that is opened as a result of the impact provide a noticeable change in the comet’s nongravitational acceleration history. The observing geometries prior to, and during, the impact will allow extensive Earth based observations to complement the in situ observations from the impactor and flyby spacecraft.     

双(口恶)唑啉化合物改性热固性树脂的研究

采用自制2,2′-(1,3-苯)双(4,5-二氢)(口恶)唑分别与热塑性酚醛树脂或二氨基二苯甲烷(DADPM)进行聚合反应制得了聚醚酰胺树脂(PEAR)和聚氨基酰胺树脂(PAAR).实验表明PEAR的冲击强度达到6 kJ/m2以上,弯曲强度达到100MPa以上,且电绝缘性能优良,可作为H级绝缘材料使用;PAAR的冲击强度最高达到22kJ/m2,弯曲强度达到202 MPa,电绝缘性能较PEAR稍差,但仍然可作为H级绝缘材料使用,另外还可望作为无卤阻燃材料使用.以这两种高性能热固性树脂为基体可制备出性能优良的玻璃布复合材料.