Observations of the Sun at Vacuum- Ultraviolet Wavelengths from Space. Part I: Concepts and Instrumentation

Space Science Reviews - Studies of the high-temperature solar atmosphere are to a large extent based on spectroscopic observations of emission lines and continuum radiation in the...     

基于混合验前分布的制导精度评定方法

如何合理有效地利用验前信息是小子样评定中的关键问题。针对导弹制导精度评定,提出了一种根据验前数据构造验前分布的方法,并结合验前信息可信度给出了一种混合验前分布。通过对参数验后估计的分析,该方法能够有效避免验前信息“淹没”现场信息的情况,而验前信息可信度则通过验后边缘分布得到。通过对验后估计均方差(MSE)的分析,给出了验前信息利用的一些基本原则,为工程应用提供了指导。     

Reduction in clamping force due to applied longitudinal load to aerospace structural bolted plates

The main purpose of the present work is to experimentally and numerically study why and how the magnitude of the bolt clamping force reduces in the aerospace structural bolted plates when they are subjected to a longitudinal tensile load. In the experimental method, a holed plate of aluminium alloy 7075-T6 was clamped using a single bolt fastener, and then tested under an increasing static longitudinal tensile load. The bolt clamping magnitude was determined by using the measured axial compressive strains of a steel bush placed between the nut and plate. Two clamped specimens with different initial clamping forces were studied. In each specimen the actual clamping forces were determined during the longitudinal loading on the plate. In the numerical method, a three-dimensional (3D) finite element model was generated in order to simulate and quantify the bolt clamping force in the plate model loaded in tension. Both experimental and numerical results showed that the clamping force reduces considerably in the aluminium bolted plates under the longitudinal tensile loading. This is because of the transverse contraction of the plate material that causes the clamped material to release from the initial compression, and as a result, the clamping force to relax.     

The Galactic Environment of the Sun: Interstellar Material Inside and Outside of the Heliosphere

Interstellar material (ISMa) is observed both inside and outside of the heliosphere. Relating these diverse sets of ISMa data provides a richer understanding of both the interstellar medium and the heliosphere. The galactic environment of the Sun is dominated by warm, low-density, partially ionized interstellar material consisting of atoms and dust grains. The properties of the heliosphere are dependent on the pressure, composition, radiation field, ionization, and magnetic field of ambient ISMa. The very low-density interior of the Local Bubble, combined with an expanding superbubble shell associated with star formation in the Scorpius-Centaurus Association, dominate the properties of the local interstellar medium (LISM). Once the heliosphere boundaries and interaction mechanisms are understood, interstellar gas, dust, pickup ions, and anomalous cosmic rays inside of the heliosphere can be directly compared to ISMa outside of the heliosphere. Our understanding of ISMa at the Sun is further enriched when the circumheliospheric interstellar material is compared to observations of other nearby ISMa and the overall context of our galactic environment. The IBEX mission will map the interaction region between the heliosphere and ISMa, and improve the accuracy of comparisons between ISMa inside and outside the heliosphere.     

The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons

The Solar Wind Around Pluto (SWAP) instrument on New Horizons will measure the interaction between the solar wind and ions created by atmospheric loss from Pluto. These measurements provide a characterization of the total loss rate and allow us to examine the complex plasma interactions at Pluto for the first time. Constrained to fit within minimal resources, SWAP is optimized to make plasma-ion measurements at all rotation angles as the New Horizons spacecraft scans to image Pluto and Charon during the flyby. To meet these unique requirements, we combined a cylindrically symmetric retarding potential analyzer with small deflectors, a top-hat analyzer, and a redundant/coincidence detection scheme. This configuration allows for highly sensitive measurements and a controllable energy passband at all scan angles of the spacecraft.     

C/C复合材料密度的CT定量无损检测技术

讨论了利用水模试样和石墨试样标定CT检测过程中影响CT值的因素(系统噪声、产品尺寸、检测参数、摆放位置等)对CT值的影响,然后利用C/C复合材料试样建立CT值和材料密度的拟合曲线和拟合公式.结果表明系统噪声、产品尺寸、检测参数、摆放位置等对CT值的影响很小,C/C复合材料织物和复合物CT值和材料密度的拟合公式分别为P=(T+793)/659和P=(T+100)/860,说明利用CT值可以对C/C复合材料的密度进行定量定义.     

航空发动机研制中量化评估方法探索

本文参考国内外重大项目研制中所采取的先进的、科学的量化评估方法,对在航空发动机研制中采用量化评估方法进行了探索,对用于航空发动机的技术成熟度定义、可行性量化评估方法、风险量化评估方法均进行了较为详细的描述,每种方法均给出了实例。     

单喷嘴气-气喷注器推力室燃烧流场相似性

 设计了单喷嘴容热式气-气喷注器推力室,喷注器采用同轴剪切式,氢气/氧气作为推进剂。在同一燃烧室采用了0.92~6.10 MPa范围内7个室压工况,并在同一室压下采用不同燃烧室尺寸工况进行了试验研究,在变化室压和推力室尺寸时,推进剂种类、温度、混合比和喷注速度保持不变,燃烧室尺寸变化时保持几何相似,采用燃烧室壁面测温方法对比了不同工况下内流场的相似性。研究结果表明：不同室压和不同推力室尺寸工况下的推力室内流场具有相似性。     

一种模糊决策专家系统的模型

目前决策型专家系统主要适合于解决精确的或不确定性决策问题,还存在模糊决策问题,如最佳方案选择问题。统一考虑决策问题中的不确定性和模糊性,提出了一种能统一处理带有不确定性和模糊性决策问题的单目标决策型专家系统模型。针对构造决策专家系统所涉及的具体问题,本文从知识表示、知识获取、模糊谓词计算、规则匹配、系统求解方式等几个方面介绍所提出的模型。     

The Galileo Heavy element monitor

The Heavy Ion Counter on the Galileo spacecraft will monitor energetic heavy nuclei of the elements from C to Ni, with energies from 6 to 200 MeV nucl^-1. The instrument will provide measurements of trapped heavy ions in the Jovian magnetosphere, including those high-energy heavy ions with the potential for affecting the operation of the spacecraft electronic circuitry. We describe the instrument, which is a modified version of the Voyager CRS instrument.