Reconstructed 3-d magnetic field structure and hard X-ray two ribbons for 2000 Bastille-day event

The Bastille-day event in 2000 produced energetic 3B/X5.6 flare with a halo CME, which had great geo-effects consequently. This event has been studied extensively and it is considered that it follows the two-ribbon flare model. The flare/CME event was triggered by an erupting filament and TRACE observations showed formation of giant arcade structures during the flare process. Hard X-ray (HXR) two ribbons revealed for the first time in this flare event (Masuda et al., 2001). The reconstruction of 3-D coronal magnetic fields revealed a magnetic flux rope structure, for the first time, from extrapolation of observed photospheric vector magnetogram data and the flux rope structure was co-spatial with portion of the filament and a UV bright lane (Yan et al., 2001a, 2001b). Here we review some recent work related to the flux rope structure and the HXR two ribbons by comparing their locations and the flux temporal profiles during the flare process so as to understand the energy release and particle accelerations. It is proposed that the rope instability may have triggered the flare event, and reconnection may occur during this process. The drifting pulsation structure in the decimetric frequency range is considered to manifest the rope ejection, or the initial phase of the coronal mass ejection. The HXR two ribbons were distributed along the flux rope and the rope foot points coincide with HXR sources. The energy dissipation from IPS observations occurred within about 100 R _⋅ is consistent with the estimate for the flux rope system. This revised version was published online in August 2006 with corrections to the Cover Date.     

斜切反喷管流场的数值模拟

为了在级间分离期间提供反推力，许多固体火箭发动机前端都装有一组斜切反喷管。由于反喷管的气动型面具有许多尖点，并且在超声速区有一个台阶，喷管内存在一系列激波，而且亚声速区和超声速区互相混杂。本文用时间相关法数值模拟了反喷管流场，控制议程用Ｍａｃ Ｃｏｒｍａｃｋ显格式求数值解，边界参数采用物理边界条件和从双特征线方法推导来的有效的特征方法为计算，为于固壁边界点，在不同的区域采用不同的方法对计算方程组求     

On the Coronal Magnetic Field Configuration and Solar Flare/CME Process

The coronal magnetic field configuration is important for understanding the energy storage and release processes that account for flares and/or CMEs. Here we present a model which is based on the work for potential magnetic field problems that only applies the condition at infinity with the boundary condition on the solar surface specified. We also discuss some recent progress on general force-free field models. For some event analyses, we have employed MDI/SOHO longitudinal magnetogram insected into the synoptic magnetogram to obtain whole boundary condition over the solar surface. Globally, the extrapolated global magnetic field structures effectively demonstrate the case for the disk signature of the radio CMEs and the evolution of the radio sources during the CME/flare processes.     

典型城市街道内汽车排放污染物扩散规律的模拟研究

采用自主开发的街道峡谷内污染物扩散模式,对城市中几种典型的街道峡谷内流场和污染物的浓度场进行了模拟研究。模拟结果表明:在一定气象条件下,街道中机动车排放污染物的扩散受街道宽高比、街道两侧建筑物对称性、街道两侧建筑物高度分布及街道两侧的建筑物形状等因素的影响;街道峡谷宽高比接近1时、递升型峡谷以及宽阔街道有利于污染物的扩散。     

利用非交错对称矩阵构造Cartesian认证码

利用特征为2的有限域上非交错对称矩阵构造了一个Cartesian认证码，并计算出其参数。进而，假定编码规则按照均匀的概率分布所选取，计算出了该码被模仿攻击成功的最大概率只和被替换攻击成功的最大概率Ps。     

超音速斜板进气道侧向溢流估算

 本文采用超音速线化理论,算出斜板侧缘附近干扰区内的流场,并根据流量积分方法,导出了关于流量系数的侧向溢流公式。本文还根据Busemann锥型流理论,应用Carafoli方法,得出了估算侧后掠端板影响的方法和图线。理论计算结果与现有的实验数据作了比较,符合程度很好。     

基于知网的汉语语义实例库的建设与应用

为了解决有指导词义消歧任务中的知识源问题,提出并构建了一个基于知网的汉语词义实例库(CSIC),同时开发了一个语义标注平台(SenseTag)。该平台通过方便快捷的人机交互方式显著提高了实例库的建设效率和质量。利用条件随机场模型,从实例库中自动学习消歧知识,进行自动标准在随机选取的部分汉语高频多义词的词义消歧开放测试中,取得了平均正确率85%的较好效果。     

端弯叶片通道出口二次流的研究

实验并且采用考虑粘性的涡传输方程计算端弯压气机叶片通道出口二次流。给出了３种端弯叶片及对应的原始直叶片通道出口气流偏转角的实验值和计算预测值。研究表明：采用上述方程能比较准确地预测出口气流偏转角；叶片后缘减弯可减小流向二次涡强度。     

Variations of the magnetic fields in large solar flares

We present preliminary results from high resolution observations obtained with the Michelson Doppler Imager (MDI) instrument on the SOHO of two large solar flares of 14 July 2000 and 24 November 2000. We show that rapid variations of the line-of-sight magnetic field occured on a time scale of a few minutes during the flare explosions. The reversibility/irreversibility of the magnetic field of both active regions is a very good tool for understanding how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system. This revised version was published online in August 2006 with corrections to the Cover Date.     

利用三维激光测速方法研究悬停状态下的桨尖涡

利用三维多谱勒激光测速仪，对悬停状态下模型旋翼桨叶附近的流场进行了实验测量。研究了悬停状态下桨盘附近的流场特征、旋翼桨尖涡的形成和发展，以及桨尖涡对后续桨叶的影响