Neutron stars: Classification and evolution

The general aproach is considered which describs the evolution of neutron stars in terms of their interaction with surrounding matter. All possible states of neutron stars are classified from this point of view. Classification and evolution of binaries contaning neutron stars are also considered.     

Physical processes in the strong magnetic fields of accreting neutron stars

The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.     

大功率无电极高密度等离子体电磁推进概述

无电极高密度等离子体电磁推进技术已成为未来深空探测、载人航天和货运、太阳能电站以及航天器在轨服务与维护等空间任务中极具竞争力的核心推进技术之一。在梳理不同无电极等离子体电磁加速机制基础上,开展大功率无电极高密度等离子体电磁推进技术性能对比,给出新概念无电极场反构型电磁推进技术向未来超大功率拓展的优势和发展潜力,同步分析了该技术亟需解决的关键基础问题,旨在为中国新概念场反构型电磁推进技术的研发提供理论基础。     

自主火星探测高集成离子与中性粒子分析仪

小型化、高集成化是深空探测载荷发展的主要趋势。在我国自主火星探测计划中,设计了一种高集成化的火星离子与中性粒子分析仪。采用从传感器到电子学进行最大限度共用的设计思路,在一台仪器中实现对离子和能量中性原子进行能量、方向和成分的探测,大大降低了仪器对卫星平台的资源需求。仪器采取静电分析进行离子的方向和能量测量、采取飞行时间方法进行离子成分的测量。中性原子采用电离板电离成带电离子,后端的能量测量和成分测量与离子相同。鉴定件样机已经完成了初步的测试定标,结果表明其满足设计要求。     

Non-stationarity and cross-correlation effects in the MHD solar activity

The analysis of turbulent processes in sunspots and pores which are self-organizing long-lived magnetic structures is a complicated and not yet solved problem. The present work focuses on studying such magneto-hydrodynamic (MHD) formations on the basis of flicker-noise spectroscopy using a new method of multi-parametric analysis. The non-stationarity and cross-correlation effects taking place in solar activity dynamics are considered. The calculated maximum values of non-stationarity factor may become precursors of significant restructuring in solar magnetic activity. The introduced cross-correlation functions enable us to judge synchronization effects between the signals of various solar activity indicators registered simultaneously.     

微藻反应器用于水气净化与产氧的功能验证

将微藻和电去离子技术引入密闭生态系统,设计单元反应器旨在验证其在空气再生、水净化和潜在食物的生产。在反应器中对尿液进行消解和NH4＋硝化转化得到超过90%NH4＋-N硝化为NO-3-N-的培养液适宜于螺旋藻养殖并获得高质量的微藻生物量;此时,CO2的平均吸收速率VCO2=458.6 mL/m3·min、O2产生速率VO2=616.5 mL/m3·min,即螺旋藻的同化系数VCO2/VO2≈0.74,接近人的呼吸系数VCO2/VO2=0.86;EDI法水净化率97%可直接回用。结果表明：该体系能实现CO2吸收、O2释放和螺旋藻生物量的生产,同时将水净化。     

Coronal Heating by Magnetic Explosions

From magnetic fields and coronal heating observed in flares, active regions, quiet regions, and coronal holes, we propose that exploding sheared core magnetic fields are the drivers of most of the dynamics and heating of the solar atmosphere, ranging from the largest and most powerful coronal mass ejections and flares, to the vigorous microflaring and coronal heating in active regions, to a multitude of fine-scale explosive events in the magnetic network, driving microflares, spicules, global coronal heating, and, consequently, the solar wind. This revised version was published online in June 2006 with corrections to the Cover Date.     

网络分析仪法测量稠油介电常数

用网络分析仪在Ｘ波段８～１１．５ＧＨｚ的６个频率点上,对大港、胜利、辽河油田稠油的介电常数进行测量,测量结果可以为微波采油工艺中的井下轴射器的设计及微波能利用率的估算提供理论依据,并对测量结果进行了误差分析。     

原子氧对航天器表面材料作用的数值模拟

对氏地球轨道环境对航天器表面材料的影响和航天器表面材料的低地球轨道环境寿命评定方法进行了介绍;并对低地球轨道环境和地面试验环境下,有无保护涂层的业胺所受冲蚀作用进行了成功的数值模拟,获得了具有工程应用价值的数值计算结果。该工作对航天器的设计具有指导意义。     

等离子体彗尾流线断裂现象的讨论

等离子体Ⅰ型彗尾流线的断裂,已多次被人们见到.本文用MHD的理论,讨论和分析了这种现象,认为这是一种空间等离子体扰动所产生的结果.本文作了定性的分析,及定量的计算,比较满意地解释了这种彗尾中的观测现象.