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。     

The iron Kα-line diagnostics of the rotating black hole metric in Seyfert galaxies

Observations of Seyfert galaxies in X-ray region reveal the wide emissive lines in their spectra, which can arise in inner parts of accretion disks, where the effects of General Relativity (GR) must be taken into account. A spectrum of a solitary emission line of a hot spot in Kerr accretion disk is simulated depending on the radial coordinate r and the angular momentum a = J/M of a black hole, under the assumption of equatorial circular motion of a hot spot. It is shown that the characteristic two-peak line profile with the sharp edges arises at a large distance (about r ≈ (3–10) r_g). The inner regions emit the line, which is observed with one maximum and extremely wide red wing. We present results of simulations for the isothermal and Shakura–Sunayev disks.     

胡适红学研究十项失误

胡适先生在红学研究中存在失误,希望后来研究者不要重蹈覆辙。通过对一些红学研究材料的举证分析。提出胡适先生在红学研究中的十项失误,并给予纠正。勿需多言是胡适先生对红学的巨大贡献。     

SDD-1算法的研究与改进

SDD-1算法是分布式数据库查询优化的一种算法,研究SDD-1算法的过程,分析SDD-1算法的优缺点,并针对该算法的不考虑最后一点传输代价的缺点提出了改进的SDD-1算法。     

高超音速技术发展概述

简述了美国高超音速飞行器计划的研制背景,介绍了乘波者飞行器的构型特点与热应力松弛设计考虑,初步探讨了高超音速验证飞行器的典型代表X-51A和HTV-2验证飞行失败的原因与遇到的技术困难。     

低纬100—200km间电子数密度的变化

利用光化平衡模式计算了低纬100—200km间白天电子数密度的变化。求得E-F₁谷区的谷深,谷宽、谷高的变化特征。获得如下结果:a.太阳活动明显影响电子数密度随高度及太阳天顶角的变化,发现太阳活动指数与电子数密度间不仅存在正相关,而且存在负相关;b.太阳活动明显影响E-F₁谷区的形态。在一定太阳活动条件下,对同一太阳赤纬和地理纬度,谷深、谷宽与太阳天顶角的关系难以用一简单函数来表示;c.太阳耀斑、地磁活动对该区电子密度有明显影响;d.在讨论100—200km间电子密度时不能忽略O⁺（2P）和NO的光电离率。     

基于混合算法的涡轴发动机稳态性能仿真模型

以自由涡轮式涡轴发动机为研究对象,建立了涡轴发动机的稳态性能仿真模型,提出了基于天牛须算法和N+1点残量法的求解发动机模型的混合算法(BAS-N+1混合算法),利用发动机台架试车数据对仿真计算结果进行了验证。结果表明,该稳态性能仿真模型各参数的求解误差在3%以内。与PSO-N+1混合算法相比,BASN+1混合算法求解精度更高,收敛更快。BAS-N+1混合算法既保留了智能算法对初猜值误差的包容性,也拥有接近经典迭代算法的收敛速度和精度,能够实现涡轴发动机稳态仿真模型的高精度大范围快速收敛。     

新型遥感图像增强技术

基于方向辅助信号和所需带宽,提出一种基于各向异性BEMD的遥感图像融合增强算法。首先,给定的方向辅助信号和其对应负信号加到原始信号中去,构建两个待分解信号;然后,应用传统BEMD把两个待分解信号进行分解,获取的分量相加得到对应的IMFs,辅助信引同时在相加的过程中被移除,同时该过程有效地避免了边界效应和模式混叠,该方法...     

Ocean Observation from Haiyang Satellites

In 2018, China successfully launched three new Haiyang (which means ocean in Chinese, referred to as HY) satellites which are an ocean color observation satellite HY-1C (operational), an ocean dynamics environment satellite HY-2B (operational) and the China-France ocean satellite CFOSAT (experimental). In 2019, all the three satellites had finished their commissioning phases and were declared operational. HY-2A satellite continues to operate in-orbit, and its operational status is basically normal. So in 2020, China has 4 Haiyang satellites in-orbit, China's ocean satellites enter into a new operational application phase. The operation of the ground application system of Chinese ocean satellites is stable. In 2019, Beijing, Hainan, Mudanjiang, and Hangzhou ocean satellite ground stations had received the data of HY-1C, HY-2A, HY-2B, and CFOSAT 5012 orbits and 26.46 TB data had been distributed to both domestic and international users. Chinese ocean satellite data has played an important role in marine disaster prevention and mitigation, development and management of marine resources, maintenance of marine rights and interests, marine environment protection, scientific researches, and blue economy development.     

Spatial asymmetry in topside ion density and vertical E × B plasma drift velocity within 75°E–95°E

The ion density measured by the Ionospheric Plasma and Electrodynamics Instrument (IPEI) on board the ROCSAT -1 over the 75°E and 95°E meridian at 600km altitude has been utilized to examine the latitudinal and longitudinal distribution within the Indian sector, in particular, the north-south and east-west asymmetries of the equatorial ionization anomaly (EIA). A longitudinal gradient in ion density at 600?km higher towards 95°E develops during the noontime and afternoon hours when the EIA is at its peak. The density gradient persists till evening hours when pre-reversal enhancements occur. The vertical E?×?B plasma drift velocity measured simultaneously by ROCSAT -1 for the same space-time configuration has also been studied. In addition to diurnal, seasonal and solar activity variations in E?×?B drift velocity, the longitudinal gradient is also observed. The EIA at the altitude of 600?km peaks at different latitudes and are mostly asymmetric about the magnetic equator. From midnight till 0800 LT, the ion density across the equator is nearly uniform in the equinoxes. But in the solstices, the density exhibits a north-south gradient. In the June solstice, density is higher in the northern hemisphere and decreases gradually towards south. The gradient in density reverses in December solstice. Normally, the EIA peaks within 1200 LT and 1600 LT while around 2000 LT, pre-reversal enhancement of ionization occurs affecting the EIA evening structure. The strength of the EIA also exhibits seasonal, year-to-year and hemispheric variations. The longitudinal asymmetry of drift velocity along 75°E and 95°E longitude sectors is the contributing factor behind the observed longitudinal asymmetry in ion density. Significant positive correlation between the strength of the EIA and E?×?B drift is observed in both longitudes.