先进树脂基复合材料的发展和应用

先进树脂基复合材料在航空领域应用日益广泛,继铝、钢、钛之后,已迅速发展成为四大航空结构材料之一. 本文主要介绍先进树脂基复合材料在航空工业的应用、复合材料的发展现状以及先进复合材料的发展趋势.     

先进树脂基复合材料研究进展

主要介绍了先进复合材料树脂基体、成形技术研究和应用的最新发展；简要分析了先进树脂基复合材料今后的发展趋势；提出了先进树脂基复合材料的发展重点。     

先进树脂基复合材料的发展

综述了先进树脂基复合材料的发展现状和在航空工业中的应用,讨论分析了我国先进树脂基复合材料发展应注意的问题。     

先进航空发动机树脂基复合材料技术现状与发展趋势

介绍了先进树脂基复合材料在国内外航空发动机上的应用需求与发展现状,讨论了国内航空发动机树脂基复合材料研制遇到的问题.最后分析了航空发动机树脂基复合材料在原材料、低成本技术、设计工具与体系、适航要求等方面亟待解决的问题.     

先进树脂基复合材料的技术现状及发展方向

综述了国内外先进树脂基复合材料的发展、应用现状 ,提出了先进树脂基复合材料技术今后的发展方向。     

环境湿度对先进树脂基复合材料成型质量的影响

叙述了环境相对湿度与先进树脂基复合材料产品废品率的关系,通过扩大水污染试验,说明了环境相对湿度对先进树脂基复合材料产品性能的影响.     

先进复合材料国防科技重点实验室的航空树脂基复合材料研发进展

归纳先进复合材料国防科技重点实验室在航空先进树脂基复合材料方面的应用和研究进展.研制出超薄热塑性无纺织物层间增韧技术以实现提高复合材料的CAI性能.设计出的多夹层结构具有多层吸收拓展频带的作用,使多夹层隐身复合材料的吸收频宽达1 ～ 18GHz.高韧性树脂基复合材料和耐高温复合材料技术得到发展,并形成预浸料-热压灌成型、液态成型和自动化制造技术体系.发展复合材料固化、树脂流动、固化变形等模拟优化技术,并建立复合材料数据库技术.建立先进复合材料国防科技重点实验室可在支撑航空装备研制,在航空复合材料创新引领、体系主导、基础支撑和保障应用方面发挥作用.     

国外航空结构材料发展概况——先进复合材料(Ⅰ)

国外航空结构材料发展概况——先进复合材料（Ⅰ）中国航空信息中心张和善１复合材料应用和发展概述按照复合材料的基体不同，先进复合材料主要分为树脂基、金属基、陶瓷基和碳碳复合材料。此外还有纤维增强金属层板复合材料。当前树脂基复合材料技术基本成熟，已在军机和...     

热压罐/VARTM组合成型新工艺设计

热压罐/VARTM组合成型新工艺是树脂基复合材料成型工艺的一个新发展,特别适用于平面、立体织物增强高粘度树脂基复合材料的液体注射成型,可以应用于航空、航天等先进复合材料制造领域.     

专注航空复合材料构件研发——访北京航空制造工程研究所飞机工艺研究室(101室)主任曹正华

航空工业树脂基复合材料构件研究与开发中心(北京航空制造工程研究所101室,以下简称101室)作为国内知名的树脂基复合材料技术研发基地,长期以来坚持跟踪世界先进复合材料技术,为我国航空产品采用先进复合材料结构提供了强大的技术支持.     

Magnetic fields in the ionosphere of Venus

This review surveys the observations of the ionospheric magnetic fields of Venus as observed on the Pioneer Venus Orbiter and the models that have been developed to describe them over the last decade. The models for the large-scale ionospheric field have developed to the advanced stage of one-dimensional, self-consistent, multi-fluid MHD models which provide a detailed picture of the field in the subsolar region for specific upper boundary conditions. In contrast, the models for the small-scale fields and the nightside fields have only reached a rudimentary stage. Much challenging work remains to be done on the origin of the ionospheric flux ropes and nightside ionospheric hole fields. On the whole, the subject of the ionospheric fields would greatly benefit from 3-dimensional global MHD models with self-consistent treatments of the ionosphere.     

Asteroid surface materials: Mineralogical characterizations from reflectance spectra

The interpretation of diagnostic parameters in the spectral reflectance data for asteroids provides a means of characterizing the mineralogy and petrology of asteroid surface materials. An interpretive technique based on a quantitative understanding of the functional relationship between the optical properties of a mineral assemblage and its mineralogy, petrology and chemistry can provide a considerably more sophisticated characterization of a surface material than any matching or classification technique for those objects bright enough to allow spectral reflectance measurements. Albedos derived from radiometry and polarization data for individual asteroids can be used with spectral data to establish the spectral albedo, to define the optical density of the surface material and, in general, to constrain mineralogical interpretations.Mineral assemblages analogous to most meteorite types, with the exception of ordinary chondritic assemblages, have been found as surface materials of Main Belt asteroids. C1- and C2-like assemblages (unleached, oxidized meteoritic clay minerals plus opaques such as carbon) dominate the population (80%) throughout the Belt, especially in the outer Belt. A smaller population of asteroids exhibit surface materials similar to C3 (CO, CV) meteoritic assemblages (olivine plus opaque, probably carbon) and are also distributed throughout the Belt. The relative size (diameter) distributions for these two populations of objects are consistent with an origin by sequential accretion from a cooling nebula (C2 as surface layers, C3 as interior layers or cores). Based on information from meteoritic analogues and on qualitative models for the behavior of these materials during a heating episode, it seems unlikely that these C2- and C3-like asteroidal bodies have experienced any significant post-accretionary heating event either near surface or in the deep interior.The majority of remaining studied asteroids (20) of 65 asteroids exhibit spectral reflectance curves dominated by the presence of metallic nickel-iron in their surface materials. These objects are most probably the several end products of an intense thermal event leading to the melting and differentiating of their protobodies. These thermalized bodies are concentrated toward the inner part of the Asteroid Belt but exist throughout the Belt.The size of the proto-asteroid has apparently exercised control over the post-accretionary thermal history of these bodies. The available evidence indicates that all asteroids larger than about 450 km in (present) diameter have undergone a significant heating episode since their formation. The post-accretionary thermal history of the asteroidal parent bodies was apparently affected by both distance from the Sun and body size.The C2-like materials which dominate the main asteroid belt population appear to be relatively rare on earth-approaching asteroids. This suggests that most of these Apollo-Amor objects are not randomly derived from the main belt, but (a) may derive from a single event in recent time (10⁷ yr), (b) may derive from a favorably situated source body, (c) may derive from a particular, compositionally anomalous region of the belt, or (d) may derive from an alternate source (e.g. comets).     

Electric Fields and Magnetic Fields in the Plasmasphere: A Perspective From CLUSTER and IMAGE

The electric field and magnetic field are basic quantities in the plasmasphere measured since the 1960s. In this review, we first recall conventional wisdom and remaining problems from ground-based whistler measurements. Then we show scientific results from Cluster and Image, which are specifically made possible by newly introduced features on these spacecraft, as follows. 1. In situ electric field measurements using artificial electron beams are successfully used to identify electric fields originating from various sources. 2. Global electric fields are derived from sequences of plasmaspheric images, revealing how the inner magnetospheric electric field responds to the southward interplanetary magnetic fields and storms/substorms. 3. Understanding of sub-auroral polarization stream (SAPS) or sub-auroral ion drifts (SAID) are advanced through analysis of a combination of magnetospheric and ionospheric measurements from Cluster, Image, and DMSP. 4. Data from multiple spacecraft have been used to estimate magnetic gradients for the first time.