The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

座舱盖系统三维数字化设计流程研究

介绍了某型飞机座舱盖系统的三维数字化设计特点和设计流程。结合在CATIA V5平台虚拟装配环境下的工程设计实例,强调在设计过程中体现面向装配设计和自顶向下的设计思想,对设计流程的各个阶段进行了分析。     

基于FTA方法对某型飞机直流电源系统故障分析

对某型飞机直流电源系统的“一个整流器故障”进行了分析 ,介绍了故障树分析的应用方法 ,并且对实际故障建立了故障树     

Complexity,Forced and/or Self-Organized Criticality,and Topological Phase Transitions in Space Plasmas

The first definitive observation that provided convincing evidence indicating certain turbulent space plasma processes are in states of ‘complexity’ was the discovery of the apparent power-law probability distribution of solar flare intensities. Recent statistical studies of complexity in space plasmas came from the AE index, UVI auroral imagery, and in-situ measurements related to the dynamics of the plasma sheet in the Earth's magnetotail and the auroral zone. In this review, we describe a theory of dynamical ‘complexity’ for space plasma systems far from equilibrium. We demonstrate that the sporadic and localized interactions of magnetic coherent structures are the origin of ‘complexity’ in space plasmas. Such interactions generate the anomalous diffusion, transport, acceleration, and evolution of the macroscopic states of the overall dynamical systems. Several illustrative examples are considered. These include: the dynamical multi- and cross-scale interactions of the macro-and kinetic coherent structures in a sheared magnetic field geometry, the preferential acceleration of the bursty bulk flows in the plasma sheet, and the onset of ‘fluctuation induced nonlinear instabilities’ that can lead to magnetic reconfigurations. The technique of dynamical renormalization group is introduced and applied to the study of two-dimensional intermittent MHD fluctuations and an analogous modified forest-fire model exhibiting forced and/or self-organized criticality [FSOC] and other types of topological phase transitions. This revised version was published online in August 2006 with corrections to the Cover Date.     

A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.     

一种能同时测量喷嘴下游气液流强的两相探针的研制

 针对液体火箭发动机喷注器下游燃料和氧化剂两相流场分布的实验研究，研制了能同时对其流强及混合比进行测量的两相探针，并对其进行了标定。利用两相探针对不同反压下同轴式喷嘴下游的流强和混合比分布所进行的试验研究，证明探针的设计是成功的     

BUILDING A UNIFIED PRODUCT MODEL WITH COMPLEX METHOD

ＢＵＩＬＤＩＮＧＡＵＮＩＦＩＥＤＰＲＯＤＵＣＴＭＯＤＥＬＷＩＴＨＣＯＭＰＬＥＸＭＥＴＨＯＤ￥ＷｕＺｈｏｎｇｋｅ；ＷｕＪｕｎｈｅｎｇ（ＣＡＤ／ＣＡＭＲｅｓｅａｒｃｈＧｒｏｕｐ，ＳｃｈｏｏｌｏｆＳｐａｃｅＴｅｃｈｎｏｌｏｇｙ，ＢｅｉｊｉｎｇＵｎｉｖｅｒｓ...     

EXPERIMENTAL INVESTIGATION ABOUT THE UNSTEADY AERODYNAMIC CHARACTERISTICS OF WINGS

ＥＸＰＥＲＩＭＥＮＴＡＬＩＮＶＥＳＴＩＧＡＴＩＯＮＡＢＯＵＴＴＨＥＵＮＳＴＥＡＤＹＡＥＲＯＤＹＮＡＭＩＣＣＨＡＲＡＣＴＥＲＩＳＴＩＣＳＯＦＷＩＮＧＳＹｕＸｉｎｚｈｉ；ＹａｎｇＹｏｎｇｎｉａｎ；ＷｕＺｅ（Ａｉｒｃｒａ．ｆｔＥｎｇｉｎｅｅｒｉｎｇＤｅｐａ...     

对PIO预测的A值及A准则的分析

从应用的角度详细地介绍了国外预测PIO时使用A值及A准则的情况。进行了计算公式的推导，讨论了准则在推导过程中所采用的假设及其适用情况，重新整理和校核了计算步骤和算例，以便于推广使用。     

复合材料机尾罩减重设计

根据复合材料层压板及夹层结构设计原则提出了某飞机机尾罩复合材料设计方案,结合复合材料强度计算方法进行有限元分析及强度校核。分析结果表明:在满足静强度的前提下,与金属机尾罩相比,复合材料机尾罩重量减少28.4%。