硝胺对低燃速丁羟推进剂能量与燃速的影响

从推进剂的能量特性和燃烧性能的角度探索了硝胺（RDX、HMX）在低燃速丁羟推进剂应用的可能性，结果表明：保持固体含量和铝粉含量恒定时，在推进剂中加入一定量的硝胺部分取代AP，可以提高低燃速丁羟推进 理论比冲和显著降低推进剂的燃速压强指数，但加入RDX、HMX降低丁羟推进剂燃速的幅度非常小。     

Ap／RDX推进剂燃速调节实验研究

利用正交试验法研究了CuO、Cr_2O_3和Fe_2O_3三种催化剂对Ap/RDX推进剂燃烧性能的影响,得到了提高燃速的最佳催化剂组合,提出了催化剂对Ap/RDX推进剂的催化机理,该机理可较好地解释许多实验结果。     

GAP贫氧推进剂的常压热分解特性研究

采用DSC方法研究了GAP模拟贫氧推进剂的常压热分解特性．同时考察了TMO催化荆对GAP模拟贫氧推进剂热分解特性的影响。实验结果表明，TMO催化剂对GAP、AP和KP的催化作用不同，复配催化荆可能是GAP贫氧推进荆系统中催化效果较好的催化剂。     

Relative ion Fe,C and O abundances in quiet time particle fluxes in the 23 SC

Using ACE and SOHO data the origin of quiet-time low-energy particle fluxes at 1 AU is studied in the 23rd solar cycle. One of the selection criteria of quiet-time periods is to demand that H/He < 10 provided that periods with noticeable contribution of remnants of gradual events have been excluded from consideration. Our results suggest different origin of 0.03–3 MeV/nucleon particles – different seed populations accelerated and different acceleration processes. During the ascending, maximum and descending phases of solar activity quiet-time ions consist of coronal particles accelerated to suprathermal energies in about a half of the quiet periods, the rest of quiet-time fluxes originates from particle acceleration in processes similar to those in small impulsive solar flares rich in Fe. At solar minimum the bulk solar wind particles serve as seed population.     

小型化高床载过氧化氢整体式催化剂床研究

通过理论分析和试验对一种新型整体式层板催化剂床进行了研究。设计了催化剂床流道结构并对催化剂床的加工工艺进行了初步研究。热试车结果表明，催化剂床性能良好，最高床载可达16．5g／（cm^2·s），分解效率96％，室压粗糙度小于±2％，催化剂床累计工作寿命大于455s，性能未出现下降趋势。     

空间等离子体环境中的高能带电粒子加速机制

空间环境中充满能量从几十keV到几MeV的高能带电粒子,这些粒子可导致在轨航天器表面和内部带电甚至单粒子效应,从而引发航天器故障。高能粒子的产生和日地空间环境中的爆发现象如耀斑、磁层亚暴等密切相关。文章综述了与这些爆发现象相关的磁重联、激波和等离子体波动等加速带电粒子的物理过程。     

提高水反应金属燃料能量性能的理论分析

采用最小自由能热力计算方法,计算了不同配方水反应金属燃料的能量性能,分析了粘合剂、氧化剂、高能添加剂、金属的种类及含量对燃料能量性能的影响。计算结果表明:镁基水反应金属燃料的基础上,添加含能粘合剂(聚叠氮缩水甘油醚(PGAP)、聚3-叠氮甲基-3-甲基氧丁环(PAMMO)、聚二叠氮甲基氧丁环与四氢呋喃共聚物(PBAMO-THF))、高能金属添加剂(Al和Mg-Al合金)及增加金属含量均有利于提高燃料的燃温和理论比冲;氧化剂和高能添加剂的种类、氧粘比(氧化剂与粘合剂质量比)对燃料的燃温和理论比冲影响不明显。采用PBAMO-THF,Al分别取代端羟基聚丁二烯(HTPB)和Mg,金属含量由70%提高到80%时,燃料的理论比冲(水燃比φ=3)由4550.5 N.s/kg提高到5451.0N.s/kg。     

The PAMELA experiment: A space-borne observatory for heliospheric phenomena

PAMELA is a multi-purpose apparatus composed of a series of scintillator counters arranged at the extremities of a permanent magnet spectrometer to provide charge, time-of-flight and rigidity information. Lepton/hadron identification is performed by a silicon–tungsten calorimeter and a Neutron detector placed at the bottom of the device. An Anticounter system is used offline to reject false triggers coming from the satellite. The device was put into orbit on June 15th 2006 in a pressurized container on board the Russian Resurs-DK1 satellite. The satellite is flying along a high inclination (70°), low Earth orbit (350–600 km), allowing to perform measurements in different points and conditions of the geomagnetosphere. PAMELA main goal is a precise measurement of the antimatter ( 80 MeV–190 GeV, e⁺ 50 MeV–270 GeV) and matter (p 80–700 GeV, e⁻ 50 MeV–400 GeV) component of the galactic cosmic rays. In this paper we focus on the capabilites of observations of heliospheric cosmic rays: trapped and semi-trapped particles in the proton and electron belts, solar particle events, Jovian electrons will be studied in the three years of expected mission.     

New insights from cross-correlation studies between solar activity indices and cosmic-ray flux during Forbush decrease events

Observed galactic cosmic ray intensity can be subjected to a transient decrease. These so-called Forbush decreases are driven by coronal mass ejection induced shockwaves in the heliosphere. By combining in situ measurements by space borne instruments with ground-based cosmic ray observations, we investigate the relationship between solar energetic particle flux, various solar activity indices, and intensity measurements of cosmic rays during such an event. We present cross-correlation study done using proton flux data from the SOHO/ERNE instrument, as well as data collected during some of the strongest Forbush decreases over the last two completed solar cycles by the network of neutron monitor detectors and different solar observatories. We have demonstrated connection between the shape of solar energetic particles fluence spectra and selected coronal mass ejection and Forbush decrease parameters, indicating that power exponents used to model these fluence spectra could be valuable new parameters in similar analysis of mentioned phenomena. They appear to be better predictor variables of Forbush decrease magnitude in interplanetary magnetic field than coronal mass ejection velocities.     

中空纤维型自修复复合材料的修复效率及力学性能

以5-亚乙基-2-降冰片烯(ENB)和Grubbs催化剂组成的修复系统为修复剂、以外径为Ф0.9mm的中空玻璃管为载体,通过压力破坏实验和三点弯曲实验研究含有中空玻璃管复合材料的弯曲性能及自修复的效率。结果表明:压力破坏实验给试件带来的损伤程度最大可达到14.67%;已受损的试件在修复系统的作用下,试件的强度能恢复到原强度的99.15%。