端羧基聚丁二烯(CTPB)推进剂的进展

用作优良粘合剂组份的端羧基聚丁二稀聚合物,由于其均匀的分子结构和化学反应性提供给推进剂良好的力学性能。本文是关于新的端羧基聚丁二稀和推进剂的进展。作者们共同研究的新CTPB 已从工业基地日本合成橡胶公司推荐给推进剂制造者。对日本合成橡胶公司的端羧基聚丁二稀的特性,特别是关于分子结构和粘合剂性能方面已进行了试验研究。     

Engineering challenges to the long term operation of the International Space Station

The U.S. Congress has maintained an intense interest in the ISS program since its inception. In the Appropriations Act of 1997, the Senate of the United States included language directing National Aeronautics and Space Administration (NASA) to have the National Research Council (NRC) under take a study that evaluates the engineering challenges posed by extravehicular activity (EVA) requirements, United States and non-United States space launch requirements, the potential need to upgrade or replace equipment and components after Assembly Complete, and the requirement to decommission and disassemble the facility. NASA and the NRC decided the focus should be on the anticipated challenges in the continuous operation and maintenance of the ISS after assembly of the on-orbit facility has been completed. This would encompass the operational years, from late 2004 (if the current schedule holds) to 2020-2025. This executive summary overviews the results of this NRC study. It focuses on the U.S. operation of the ISS after Assembly Complete, including cooperative efforts by the United States and Russia. The paper summarizes the primary findings and recommendations in each of the areas considered during this two-year NRC study.     

Pc5 Oscillation Analysis by the Satellite and Ground-Based Data

Large amplitude Pc5 event was observed in the space and on ground on August 3, 2001, about three hours after contact of the strong discontinuity in the solar wind with the magnetosphere according to data from ACE and Wind satellites. The Pc5 amplitude was as high as 15 nT in the tail of magnetosphere and about 5 nT at the ground based stations. In the magnetosphere Pc5 waves were observed by Cluster and Polar satellites, which occupied positions in the morning part of the near tail at the close field lines but were parted by distance of 11.5 Re, mainly along the x-axis of the GSM coordinate system. Both compressional and transverse components of the Pc5 wave activity were observed in the space, with the transverse component having the larger amplitude. Time delay between the Cluster and Polar satellites was about 8 minutes, which could be interpreted as a wave propagation from the geomagnetic tail to the Earth with the 150 km/s group velocity. The ground-based Pc5 activity was analysed by using data from the Image magnetometer network. Doubtless demonstrations of a field line resonant structure were found in variations of amplitude and polarization with latitude. Finnish chain of search coil magnetometers observed modulated Pc1 emission simultaneously with the Pc5 wave train. A possibility of non-linear impact of Pc5 wave energy on the plasma and waves in the magnetosphere is discussed.     

The Main Results and the Perspectives in the Researches at SSRT

In this report briefly presented the contemporary state of the experimental base of Radio Astrophysical Observatory (RAO) of the Institute of Solar-Terrestrial Physics (ISTP), the methodology of radioheliographic monitoring of the solar corona, the SSRT database, the RAO Web-pages, factors limiting the effective use of SSRT. Here are formulated the original results of the basic directions of the solar activity researches and the problems solutions on SSRT: (1) active regions at various development stages, morphology, modeling,signs of energy accumulation and flares buildup, forecast of powerful flares; (2) scenario, topology and the fine temporal picture of flares development, signs of primary energy release, radio emission mechanisms, scatter effects of radio emission in turbulent corona, energetic particles fluxes; (3) filaments; (4) CME with the localization of their initiation at the solar disk background, development scenario of filament activation + CME +flare; (5) coronal holes, and (6) bright coronal points.      

大直径交点孔螺旋铣精加工技术研究

在飞机装配过程中经常需要进行大直径交点孔的精加工。交点孔的直径大、材料工艺性差导致精加工时切削力大、振动大,不同耳片间初孔不同心导致刀具受力不均易引偏,装配制孔作业环境复杂导致大型加工设备使用困难。目前主要加工方法为使用自动进给钻进行多次的扩孔和铰孔,制孔效率低、使用刀具种类多、成本高。螺旋铣孔是航空航天领域出现的制孔新方法,在难加工材料大直径孔加工中,与传统的钻、扩、铰工艺相比具有更好的制孔质量和效率,尤其在扩孔加工时,螺旋铣孔刀具不会被初孔引偏,优势明显。基于便携式螺旋铣孔装备,开展了大直径交点孔扩孔精加工试验,检测了加工孔的尺寸精度和孔壁表面质量,并进一步研究了孔壁表面完整性,结果表明,孔径尺寸精度优于±0.05 mm,孔壁粗糙度优于R_a1.6μm,验证了采用螺旋铣孔方法实现飞机装配交点孔精加工的可行性。     

Detailed modeling of aluminum particle combustion——From single particles to cloud combustion in Bunsen flames

A numerical model for aluminum cloud combustion which includes the effects of interphase heat transfer, phase change, heterogeneous surface reactions, homogeneous combustion,oxide cap growth and radiation within the Euler–Lagrange framework is proposed. The model is validated in single particle configurations with varying particle diameters. The combustion process of a single aluminum particle is analyzed in detail and the particle consumption rates as well as the heat release rates due to the v...