Fast neutral particles as probes of the extent of Io's exosphere

The spatial extent of ion cyclotron waves at Io has been interpreted as requiring a multistep acceleration and transport process: exospheric ions are accelerated outward (relative to Jupiter) due to the corotation electric field, neutralized due to charge exchange in the surrounding exosphere, and then reionized after traveling far across magnetic field lines, at which point they generate the waves. The trajectories of the particles away from Io are sensitive to the location of their initial ionization. This paper examines the spatial distributions of fast neutrals produced under varying conditions in order to provide constraints on the possible structure and nature of the Io exosphere. While a rapid onset of cyclotron waves at a specific location around Io can be modeled with a single, point-source region of ions, such as might occur over a volcano, the regional extent of the waves suggests multiple or distributed sources.     

KS－熵与混沌层次

有两种不同类型的混沌层次：一种得之于映射维数的增加；另一种则由不变环面分叉产生。通过计算相应的ＫＳ－熵，我们发现前者只是一种几何现象，后者则是本质的混沌层次，即伴随有混沌性的增加。     

TC2002极坐标测量系统在大型天线检测中的应用

单台全站仪极坐标测量系统应用于高精度的测量和安装工作中,必须采用特殊的作业手段和数据处理方法才能达到亚毫米的精度。文中提出了一种坐标转换方法,将其应用于大型多波束天线的安装检测过程中,实测结果表明该方法达到较好的效果。     

Ion cyclotron waves at Io: implications for the temporal variation of Io's atmosphere

When the flowing torus plasma encounters the upper atmosphere of Jupiter's moon, Io, newly created ions are rapidly accelerated by the motional electric field. Many of these ions are reneutralized and form a spray of fast neutrals that travel far away from Io before being reionized by photoionization and impact. These ions, now far from Io, are unstable to the generation of ion cyclotron waves. These waves in turn act as a mass spectrometer allowing Galileo magnetic measurements to be used to probe the composition of the atmosphere of Io and how it varies in time and in space. We now have six Galileo passes by Io on which we have measurements with sufficient cadence to examine the ion cyclotron waves. One of these passes, on Galileo's 32nd orbit has not been discussed previously. These passes provide sufficient observations to begin to distinguish the sources of variability. We find that while the atmosphere of Io varies temporally throughout the mission, it also has a spatial variation in composition at any instant of time.     

一种新的三维地下管线衔接模型算法研究

在城市地下管网中,管线通过管件实现相交、衔接和连通等操作,然而地下管线连接方式种类繁多,管件在面对地下管线复杂多样的连接方式时存在无法完全表达的问题。文中主要研究在三维地下管网建模过程中,管件在不能完全表达管线连接方式时的衔接模型,按衔接管径不同将管线衔接建模分为等径管线衔接建模和异径管线衔接建模两类;提出采用圆管—圆球—圆管的组合进行等径管线衔接建模方法;重点研究异径管线衔接建模,提出一种利用ArcEngine组件对象构建多片圆柱体,圆柱体模拟圆环体,若干首尾相接的渐变径圆环体拟合弯管的算法。研究方法能够高效逼真地构建出等径弯管模型和异径弯管模型,解决了地下管线三维模型衔接处的光滑建模问题。