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’’.     

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.     

影响招生计划制定因素的个案分析

通过沈阳航空工业学院2005年招生计划制定的个案，对影响招生计划制定的多重因素作了全面分析和深入研究，旨在说明招生计划的制定不是简单的数量增减，而是一门需要进行综合分析的科学，揭示出影响制定招生计划的外部因素即经济发展环境，以及学校发展定位、就业质量、生源质量等内部因素。     

自动校相技术在现代测控雷达中的实现

介绍自动校相技术的程序设计及其在工程中的应用，详细叙述了该软件关键部分的设计技术。     

厌氧胶在液体火箭发动机上的应用研究

简要叙述了厌氧胶在航空和汽车制造业方面的使用,指出了厌氧胶具有的优越防松性能,可以成为取代目前仍在使用的传统的保险丝锁紧方式的途径之一,并重点介绍了厌氧胶在液体火箭发动机上的应用试验研究的内容和方法,给出了试验结论,最后提出了厌氧胶在今后液体火箭发动机应用上应重点解决的几个问题。     

LU—ADI方法在求解跨声速翼型绕流问题中的应用

本文利用LU-ADI方法求解了跨声速范围内的Euler、NS方程。研究了边界的处理和某些求解方法的改进。     

基于DSP和FPGA的GPS伪随机码并行快速捕获方案设计

讨论了高动态下GPS伪随机码并行搜索的基本原理,以及自适应门限确定方法与搜索过程中应注意的问题。提出了一种基于高速DSP和FPGA的全数字解扩接收机方案,阐述了工作流程,并给出了系统的结构框图,经测试验证实现了伪随机码并行快速捕获的功能。     

有关误差的基本概念与表示

阐述了“测量误差”、“测量不确定度”及“测量准确度，，等计量学基本概念，明确指出了这些概念的内涵、表达方法及使用中应注意的问题，并讨论了它们的联系与区别。     

N2O/丙烷火箭发动机研制

为进行N2O/丙烷(C3H8)火箭发动机(NOP)试验,在亚拉巴马大学(UAH)新建了一座发动机试车台,装备了台架式推进剂供应系统、10001bsf(4448.22N)的推力架和数据采集系统.研究了N2O催化分解点火方案,对几种催化剂材料进行了评估.Shel1-405和钴基的ZSM-5性能良好,可使N2O充分分解,并点燃碳氢燃料,如丙烷.试验表明,纯N2O通过Shel1-405时,催化分解反应在400°F(204℃)时进行,如果加入少许碳氢燃料(例如丙烷或丙烯),此温度将下降到大约200°F(93℃).NOP发动机在L*=3m时,在混合比4.89到8.68之间进行了试验.在合适的热损失模型下,试验数据与理论计算结果相吻合.使NOP发动机稳定工作的范围基本确定为N2O流量＜0.270 1bm/sec(0.122kg/s),混合比在5～6之间.用辐射测量仪来测量发动机排气温度和羽流成分,用羽流皮托管校验推力数据.     

K—ε两方程模型的改进及其应用

本文对标准的k-ε两方程模型进行了改进。摒弃了v_t=C_μ(k~2/ε)的假定,而从雷诺应力方程和Rodi的简化假设出发,得出了计算v_t的新表达式(10)。算例表明,它对时均速度u的计算结果比标准k-ε模型更精确。