SSRT: First results of millisecond spike observations

We present the results of the first observations of spike-like phenomena with the Siberian Solar Radio Telescope (SSRT) in the one-dimensional mode at the frequency of 5.7 GHz with high spatial and temporal resolutions.     

Modeling coronal streamers and their eruption

Numerical solutions of the time-dependent MHD equations are used to generate ambient coronal streamer structures in a corona characteristic of that near solar minimum. The streamers are then disrupted by slow photospheric shear motion at the base of magnetic field lines within the closed field region, which is currently believed to be responsible for producing at least some CMEs. In contrast to several other simulations of this phenomena, the polytropic index is maintained at a value of 5/3 through the addition of coronal heating. Observations are used as a guide in determining the thermodynamic structure and plasma beta in the ambient corona. For a shear speed of 2.5 km/sec, the streamer configuration evolves slowly for about 65 hours before erupting outward with the formation of a CME. The bright CME leading edge travels outward at a speed of about 240 km/sec, and the sheared field lines follow at a somewhat slower speed. A closed magnetic field region is ejected as the magnetic field lines that were opened by the CME reconnect and reform the streamer.     

Aczel不等式的推广

在Mitrinovie,D.S.著的《解析不等式》中介绍了有名的Aczel不等式、Popoviciu不等式、Bellman不等式,但后者的不等式的条件不妥当,且也没有给出等式成立的充要条件。本文进一步推广Aczel不等式,并改进了Popoviciu不等式与Bellman不等式的条件,也给出了等式成立的充要条件,且把Aczel不等式推广到复向量空间中,也推广到相反的不等式。     

数据资料与模型

本文论述了数据资料在数学建模中的作用,介绍了数据资料的收集、选取及利用数据资料建立数学模型的方法。     

“风云”系列气象卫星的发展现状及其展望

介绍了我国第一代极地气象卫星“风云一号”（FY－1）系列和静止气象卫星“风云二号”（FY－2）系列的发展历程、主要性能。FY－1系列包括4颗卫星及其相应的地面数据接收、处理和应用系统。介绍了FY－2后续卫星及FY-3的发展计划。最后还介绍了遥感卫星遥感器辐射校正场计划。     

Modeling the (upper) solar atmosphere including the magnetic field

The atmosphere of the Sun is highly structured and dynamic in nature. From the photosphere and chromosphere into the transition region and the corona plasma-β changes from above to below one, i.e., while in the lower atmosphere the energy density of the plasma dominates, in the upper atmosphere the magnetic field plays the governing role – one might speak of a “magnetic transition”. Therefore the dynamics of the overshooting convection in the photosphere, the granulation, is shuffling the magnetic field around in the photosphere. This leads not only to a (re-)structuring of the magnetic field in the upper atmosphere, but induces also the dynamic reaction of the coronal plasma, e.g., due to reconnection events. Therefore the (complex) structure and the interaction of various magnetic patches is crucial to understand the structure, dynamics and heating of coronal plasma as well as its acceleration into the solar wind.

The present article will emphasize the need for three-dimensional modeling accounting for the complexity of the solar atmosphere to understand these processes. Some advances on 3D modeling of the upper solar atmosphere in magnetically closed as well as open regions will be presented together with diagnostic tools to compare these models to observations. This highlights the recent success of these models which in many respects closely match the observations.     

阶跃光纤端面球透镜耦合的最佳耦合效率

采用光纤端面球透镜耦合方式,是提高半导体光源与阶跃折射率光纤之间耦合效率的简单实用的方法。对半导体光源与阶跃折射率光纤之间,采用光纤端面球透镜耦合方式的耦合效率进行了深入研究,得出了最大耦合效率及对应的球透镜最佳半径的计算公式。     

基于51系列单片机平台的64位数据显示

分析了51系列单片机在KeilC开发环境中64位数据的显示问题。51系列单片机为8位，其常用的开发环境KeilC最大支持32的整数，因此无法显示64位的整数。对此作了分析，提出了两种解决办法：计算法和查表法。结合实例，对其原理和实现过程作了详细的分析，并用C语言实现了这两种算法，给出了源程序和流程图．     

光线跟踪Bezier曲面

 本文提出了一种光线跟踪Bezier曲面的求交算法。该算法通过建立曲面树形存贮结构及网格面的包围盒,实现光线曲面片的相交测试;曲面片的交替二叉离散最终实现交点计算,有效的提高了相交测试效率,改善了曲面四叉、二叉离散求交特性。具有结构简单、有效性强、易于实现等特点,是光线跟踪曲面求交的一种算法。     

高精度ENO格式在射流数值模拟中的应用

本文分析了ENO格式的特点，并应用于全NS方程的迁移项和压力顶，模拟了轴对称和三维射流。首先对轴对称自由射流为算例比较了高阶TVD格式和ENO格式，证实了ENO格式捕获复杂激波波系的能力；其次计算了四喷管湍射流干扰流场，给出了相应的计算结果；最后计算了四股射流流入圆管内的流场，给出了物理量沿壁面和截面的分布。