火焰辐射光场成像光线采样特性

为了研究全光相机对火焰等半透明介质的光场采样并优化全光相机的参数,基于近轴光学,建立了全光相机的逆向光线追迹模型。在此基础上,针对弥散介质沿采集方向的半透明特性,提出了像素采样锥形角以及物方采样角度等评价光线角度采样的性能指标,据此分析了全光相机像素和微透镜的位置对光场采样特性的影响,以及全光相机光学参数变化对光线方向采样性能的影响。结果表明:采集火焰辐射光场时,较小的微透镜直径有利于提高光场采样的单方向性,并减小主镜头入瞳直径,而较小的主镜头焦距有利于增大物方采样角度。     

Driving major solar flares and eruptions: A review

This review focuses on the processes that energize and trigger M- and X-class solar flares and associated flux-rope destabilizations. Numerical modeling of specific solar regions is hampered by uncertain coronal-field reconstructions and by poorly understood magnetic reconnection; these limitations result in uncertain estimates of field topology, energy, and helicity. The primary advances in understanding field destabilizations therefore come from the combination of generic numerical experiments with interpretation of sets of observations. These suggest a critical role for the emergence of twisted flux ropes into pre-existing strong field for many, if not all, of the active regions that produce M- or X-class flares. The flux and internal twist of the emerging ropes appear to play as important a role in determining whether an eruption will develop predominantly as flare, confined eruption, or CME, as do the properties of the embedding field. Based on reviewed literature, I outline a scenario for major flares and eruptions that combines flux-rope emergence, mass draining, near-surface reconnection, and the interaction with the surrounding field. Whether deterministic forecasting is in principle possible remains to be seen: to date no reliable such forecasts can be made. Large-sample studies based on long-duration, comprehensive observations of active regions from their emergence through their flaring phase are needed to help us better understand these complex phenomena.     

多媒体流处理器中缓冲器的体系结构设计

传统微处理器体系结构不能很好地匹配媒体处理应用的特点.针对处理器与存储器之间日益增长的性能间隙问题,分析了传统微处理器对媒体处理应用的通讯瓶颈;通过分析Cache存储器的特点,得出了传统的Cache结构并不适合现代媒体处理应用的结论,讨论了目前针对处理器通讯瓶颈的一些解决办法;提出了一种以大容量流寄存器堆替代Cache作为中间缓冲器,并能适合于媒体处理应用的金字塔存储层次体系结构设计.该体系结构具有三级并行数据带宽存储层次,即片外SDRAM、全局寄存器堆和局部寄存器堆.三级并行存储层次所能提供的带宽依次提高一个数量级,带宽之比为1∶16∶256,从而可以有效地支持卫星遥感图像预处理对数据带宽的需求.      

关于大众传媒在高校音乐传播中作用的调查及思考

为了解大众传媒所传播的音乐信息及其在大学生中所产生的效应,笔者在南京三所不同类型的高校进行了一次问卷调查,对问卷中反映的问题进行初步探讨。     

遥测数据传递介质的选择

遥测数据需要传递 ,传递介质的选择是一个重要问题。对我国遥测数据传递介质的沿革、现状进行了分析 ,对国外的发展趋势作了介绍 ,提出了硬盘记录 ,光盘传递的新思路     

热防护系统的硅纤维隔热层复合传热数值计算

鉴于热防护系统的硅纤维隔热层是各向异性的非灰体材料，其复合传热计算是复杂且耗时的，提出了一种简便方法用于硅纤维这类各向异性非灰体材料的复合传热计算。该方法借鉴了医学领域断层摄影法（局部X射线检测法）中对光沿各向异性散射介质传播分析的思路，得到了各向异性扩散的热辐射方程（RTE—D）并把该方程用于求解非灰体半透明介质的辐射热通量。计算结果与文献中基于辐射传递方程（RTE）求得辐射热流的复合传热数值结果相比较，其最大相对误差为1．5％，并且其计算时间也由Pentium Ⅱ的3297．66分钟缩短为PentiumⅣ的约5分钟。最后，该方法被用于真实热环境下刚性隔热瓦L1900（高空隙率硅纤维隔热材料）的复合传热计算，计算结果与实验数据有较高吻合度。数据结果表明，各向异性的扩散近似被用于求解非灰体半透明介质的辐射热通量的方法用在热防护系统的硅纤维隔热层复合传热数值计算中是简便高效的。     

Space Tweetup – from a participant to a Mars Tweetup organizer and a new format of space communication

In September 2011, the European Space Agency (ESA) and the German Space Agency (DLR) organized the first European SpaceTweetup during the German Aerospace day. One of the authors was one of 60 participants at this SpaceTweetup in Cologne and experienced the concept of a Tweetup and the engagement of the participants from the inside view.     

新兴媒体影响下的大学生思想状况调查研究

在全球化的文化背景下,公共传媒对传统的思想道德、文化底线产生着强大的冲击,而青年学生又是公共传媒的主要受众群体和组成部分。基于当前形势,针对新兴媒体对大学生思想政治教育所产生的影响开展了相应的调查和研究,提出了新形势下高校大学生思想政治教育的思路。调查结果显示:新兴媒体已经对大学生的学习、生活产生了较大的影响,高校应该开辟多种渠道以适应新兴媒体对高等院校思想政治教育所提出的新要求。     

中国电视节目生产的本土化策略

研究中国电视节目生产中实施"本土化"策略的方式和意义。从电视媒体的生存环境入手,结合跨国媒体集团以及国内几家电视台本土化策略成功运用的案例,进行系统综合分析。使人们对电视节目的"本土化"有一个比较客观、理性的认识。那些能体现本土特色的电视节目才真正具有市场竞争力,才能吸引观众的眼球。     

Effect of surface roughness on microwave brightness temperature from lunar surface: Numerical analysis with a hybrid method

A hybrid method, combining the radiative transfer theory and the method of moments (MoM), is proposed to study the potential effect of the lunar surface roughness on the microwave brightness temperature. The total upward emission reaching the lunar surface from below media is calculated by the radiative transfer theory, and then the brightness temperature is obtained by weighting the bidirectional transmission coefficients which is computed using the MoM. The method is validated by both flat and rough surface models with analytic solutions. With the hybrid method, brightness temperatures from simulated lunar model are calculated and compared to those from a flat layered model. The comparisons show that the effect of rough surface on brightness temperature cannot be ignored and also depends on many other factors, such as observation angle and polarizations. For vertical polarization, an optimal observation angle may exist to reduce the effect of surface roughness. These results indicate that the knowledge of lunar surface roughness is important in microwave remote sensing to the Moon and may probably provide a guide to lunar projects in future.