3,6-双(1-氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪-1,4-丁二胺盐的制备和热分解动力学及热安全性

利用3,6-双(1-氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪(BTATz)和1,4-丁二胺,在DMSO中合成出了标题化合物。采用元素分析和红外光谱分析,测定了其结构。用DSC和TG/DTG热分析仪,对标题化合物进行了热分解行为及热分解动力学研究。结果表明,化合物的热分解过程只有一个放热阶段,该阶段的非等温热分解反应动力学方程的活化能和指前因子分别为92.95 kJ/mol和1016.58s-1。采用MicroDSCⅢ量热仪中的连续比定压热容测定模式,测定了化合物的比定压热容,比定压热容随温度呈现二次方关系,且298.15 K下的标准摩尔热容为443.22 J/(mol.K)。计算得到化合物的自加速分解温度(TSADT)、热爆炸临界温度(Tb)和绝热至爆时间分别为521.55、536.73 K和36.97 s。     

基于EEC检测系统的t4通道检测研究

飞机性能的提高,对发动机推进控制系统提出了更高的要求。基于EEC检测系统,对t4通道进行了独立检测试验,得出了通道在4种工作状态下t4与S1的特性关系。结合通道原理电路,对试验结果进行了分析。辨识结果证明通道为变结构控制系统。试验证明,EEC检测系统设计合理,安全可靠,抗干扰,具有较高的精确度,对研究EEC内部控制规律具有重要意义。     

Martian CH(4): sources, flux, and detection

Recent observations have detected trace amounts of CH(4) heterogeneously distributed in the martian atmosphere, which indicated a subsurface CH(4) flux of ~2 x 10(5) to 2 x 10(9) cm(2) s(1). Four different origins for this CH(4) were considered: (1) volcanogenic; (2) sublimation of hydrate- rich ice; (3) diffusive transport through hydrate-saturated cryosphere; and (4) microbial CH(4) generation above the cryosphere. A diffusive flux model of the martian crust for He, H(2), and CH(4) was developed based upon measurements of deep fracture water samples from South Africa. This model distinguishes between abiogenic and microbial CH(4) sources based upon their isotopic composition, and couples microbial CH(4) production to H(2) generation by H(2)O radiolysis. For a He flux of approximately 10(5) cm(2) s(1) this model yields an abiogenic CH(4) flux and a microbial CH(4) flux of approximately 10(6) and approximately 10(9) cm(2) s(1), respectively. This flux will only reach the martian surface if CH(4) hydrate is saturated in the cryosphere; otherwise it will be captured within the cryosphere. The sublimation of a hydrate-rich cryosphere could generate the observed CH(4) flux, whereas microbial CH(4) production in a hypersaline environment above the hydrate stability zone only seems capable of supplying approximately 10(5) cm(2) s(1) of CH(4). The model predicts that He/H(2)/CH(4)/C(2)H(6) abundances and the C and H isotopic values of CH(4) and the C isotopic composition of C(2)H(6) could reveal the different sources. Cavity ring-down spectrometers represent the instrument type that would be most capable of performing the C and H measurements of CH(4) on near future rover missions and pinpointing the cause and source of the CH(4) emissions.