含能材料低温松弛WLF方程的两种求值法

通过玻璃化转变温度和表观活化能以及由ＶＦＴ方程导得ＷＬＦ方程粘弹系数的两种新计算方法。用该方法分别计算１０个体系的粘弹系数,结果表明,用ＤＳＣ技术可以获得ＷＬＦ方程,３种计算方法获得的粘弹系数符合较好。     

高能推进剂燃烧效率研究和实测比冲预估

采用燃烧残渣中活性铝含量分析、真空爆热和发动机试验等方法，研究了高能推进剂中主要组分对推进剂燃烧效率的影响。研究结果表明：增塑剂的种类和含量是影响效率的主要因素，AP的含量及固体组分的粒度级配也有明显影响；BSF－φ315发动机试车结果证明高能推进剂的的实测比冲效率大于0．94。采用软件计算发动机的实测比中，可预估高能推进剂配方在不同压强及燃速条件下标准试验发动机（BSF－φ165和BSF－φ315）试车的实测比冲值。     

地球同步轨道高能电子增强事件预报方法

分析了地球同步轨道高能电子通量增强事件的发生规律及其与太阳风和行星际磁场参数的关系，并在此基础上建立了基于人工神经网络的高能电子增强事件模式，经实测数据检验，预报模式可以对未来1天的高能电子通量进行预报，误差为8．2％，达到了较高水平．     

新型含能材料──CL－20

综述了ＣＬ－２０结构特征，合成方法及热分解性能，并对其作为固体推进剂氧化剂的能量特性进行了计算分析。结果显示ＣＬ－２０具有能量密度高，感度适中等特点，同时具有较好热稳定性和不同于ＨＭＸ的热分解特性，是一种有潜力的高能量密度材料。     

Self-consistent amplitude profile of ducted VLF transmitter signal due to resonant interaction with energetic electrons in the magnetosphere

Of the various sources of whistler waves in the magnetosphere, the signals from terrestrial VLF transmitters are apparently the simplest for theoretical analysis. The role of these signals in the acceleration and pitch-angle scattering of energetic electrons in the Earth’s radiation belts has not been fully studied quantitatively, despite many decades of relevant research. The main problem in studying this issue is that to calculate the acceleration and pitch-angle scattering of particles, it is necessary to know the spatial profile of the signal amplitude. This is especially critical for phase-trapped particles, for which the energy exchange with the wave is the most significant. At the same time, the wave amplitude profile itself is determined by the interaction of the wave with resonant particles. Thus, we are dealing with a self-consistent problem, which is described by a nonlinear system of equations - a kinetic equation for the distribution function of resonant particles with a self-consistent field, and an equation for the wave field, in which the nonlinear and non-local growth rate is determined by the distribution function of resonant particles. In this paper, we develop an approach to solving this system of equations and the corresponding physical problem using the method of successive approximations.     

Advance of interplanetary physics study in China: 2008—2010

Interplanetary physics study is an important ingredient in space weather research. Considerable progress this aspect has been achieved by the space physics community of China in recent years. This brief report summarizes the latest advances of the interplanetary physics research in China during the period of 2008--2010. This report includes solar corona and solar wind, interplanetary transients, energetic particles, MHD simulation, space plasma, and prediction methods for physical phenomena originating from both solar corona and interplanetary space.      

Numerical investigation of the influence of large turbulence scales on the parallel and perpendicular transport of cosmic rays

In recent analytical investigations it has been demonstrated that the turbulence behavior at large scales has a very strong influence on the perpendicular diffusion coefficient of charged particles. In the present paper we use computer simulations to investigate numerically cross field transport and particle propagation along the mean magnetic field for different turbulence models at large scales. Our results are compared with quasilinear theory and nonlinear diffusion theories. We show that for different forms of the turbulence spectrum at large scales, the perpendicular mean free paths obtained numerically are in agreement with recent predictions made by analytical theory. It is also shown that the parallel diffusion coefficient contains always a strong nonlinear contribution which is, however, independent of the assumed spectrum at large scales.     

Co-rotating particle enhancements out of the ecliptic plane

The characteristics of the recurrent electron (38–53 keV) and ion (>0.5 MeV) enhancements observed by Ulysses from mid-1992 to April 1994 are presented. The magnitude of the ion flux increases reached a maximum at a latitude of 20°S and decreased afterwards by 23%/degree until early 1994. The magnitude of the electron increases showed a similar trend until May, 1993, after which time it became approximately constant, until it started to increase again in early 1994. The electron enhancements have lagged the protons by up to 5 days once Ulysses left the heliospheric current sheet (mid-1993). The electron spectral index tended to harden (a) during the decay of the event and (b) as the latitude increased, up to 50°S. The events have recurred on a 26.0 day period, but with significant phase shifts over the 25 rotations studied. The H/He ratio decreases across the maximum intensity. The mean minimum value for H/He was 3.5±0.3, lower than that measured in previous studies in the ecliptic plane.     

叠氮复合固体推进剂技术研究

分析了航天器和导弹武器系统对固体推进剂提出的新的要求和实现这些要求的技术途径。介绍了国外研制低特征信号叠氮固体推进剂的主要原材料叠氮粘合剂、含能增塑剂、高能高密度氧化剂的发展概况和关键技术。分析认为，由以上材料组成的叠氮复合固体推进剂具有含能量高、密度大、发动机排气羽烟对微波、激光和可见光的透过率高等特征，因此这是一种很有前途的新型推进剂。     

高能氧化剂二硝酰胺铵研究进展

介绍了高能氧化荆二硝酰胺铵（ADN）的特性和应用前景，以及国内外在ADN合成方法、热稳定性、成球造粒、防吸湿性、燃烧性能与应用研究方面所取得的进展。有关资料表明，各国的研究都还处在合成及性能改善阶段，尤其在防吸湿方面尚未取得突破，因而作为一种性能优越的固体推进荆氧化荆，ADN还没有在型号中得到普遍应用。