Impact Cratering Theory and Modeling for the Deep Impact Mission: From Mission Planning to Data Analysis

The cratering event produced by the Deep Impact mission is a unique experimental opportunity, beyond the capability of Earth-based laboratories with regard to the impacting energy, target material, space environment, and extremely low-gravity field. Consequently, impact cratering theory and modeling play an important role in this mission, from initial inception to final data analysis. Experimentally derived impact cratering scaling laws provide us with our best estimates for the crater diameter, depth, and formation time: critical in the mission planning stage for producing the flight plan and instrument specifications. Cratering theory has strongly influenced the impactor design, producing a probe that should produce the largest possible crater on the surface of Tempel 1 under a wide range of scenarios. Numerical hydrocode modeling allows us to estimate the volume and thermodynamic characteristics of the material vaporized in the early stages of the impact. Hydrocode modeling will also aid us in understanding the observed crater excavation process, especially in the area of impacts into porous materials. Finally, experimentally derived ejecta scaling laws and modeling provide us with a means to predict and analyze the observed behavior of the material launched from the comet during crater excavation, and may provide us with a unique means of estimating the magnitude of the comet’s gravity field and by extension the mass and density of comet Tempel 1.     

线性回归模型的贝叶斯决策方法

决策影响图分析法是决策问题一种新的图示表征求解方法，它用无有向回路的有向图来表征决策信息的关系，运用这一决策分析的新方法，对一类线性回归模型，从决策的角度进行探讨和求解，并将结果推广到更加一般的情形。     

飞机机翼表面水滴撞击特性计算

根据飞机防冰系统的研制需要，以机翼为对象，对水滴撞击特性的数值计算进行研究，建立了计算模型，研究了计算方法，用相应的计算程序，在广泛的飞行，气象及多种翼型条件下，对水滴撞击特性作了计算，计算结果与国外权威机构公布的数据相比吻合性好，给出了部分计算结果，并对水滴撞击特性计算的应用作了简要分析。     

高速可编程PCM遥测帧同步器

依据国际最新测地面站的发展方向，给出了一种新型高码率可编程ＰＣＭ遥测帧同步器的方案设计，既采用了高速可编程全数字化相关检测技术及新颖的滑动窗口技术，又采用了状态机变量设计和微程序设计，并基于ＰＬＤ技术，完成了整个高速可编程ＰＣＭ遥测帧同步器的软、硬件设计、实验表明，该方案切实可行。     

图形点阵式液晶显示器MGLS-160128在智能化仪表中的应用

本文介绍了图形点阵式液晶显示器MGLS－160128在实际测量中硬件连接和软件设计思想。具有较强的实用价值。     

基于MATLAB的自动控制系统仿真与分析

本文在给出机器人行走系统的数学模型的基础上，利用 MATLAB对控制系统进行仿真，同时详细地分析了控制系统，给出了系统的时域性能指标、开环频率特性及根轨迹，说明了系统设计的有效性。     

精密车削细长轴的几点措施

本文针对长径比大于80：1的细长轴精密加工问题，从车刀角度、车削方法、车床尾座、跟刀架等方面提出了改进措施，从而满足了加工要求，提高了生产效率。     

“Oblique” Bernstein modes in solar preflare plasma: Generation of second harmonics

Process of second harmonics generation due to development of corresponding instability has been investigated for pure electron weakly oblique Bernstein mode. This mode was supposed to be modified by taking into account the influence of pair Coulomb collisions and weak large-scale electric field in flare loop. Investigated area was located near the loop foot-point in the “lower–middle” chromosphere of active region. It has been shown, that for the Fontenla–Avrett–Loeser model of solar atmosphere the investigated process of second harmonics generation starts at the extremely low threshold values of subdreicer electric field, well before the beginning of “preheating” phase of flare process.     

Relative ion Fe,C and O abundances in quiet time particle fluxes in the 23 SC

Using ACE and SOHO data the origin of quiet-time low-energy particle fluxes at 1 AU is studied in the 23rd solar cycle. One of the selection criteria of quiet-time periods is to demand that H/He < 10 provided that periods with noticeable contribution of remnants of gradual events have been excluded from consideration. Our results suggest different origin of 0.03–3 MeV/nucleon particles – different seed populations accelerated and different acceleration processes. During the ascending, maximum and descending phases of solar activity quiet-time ions consist of coronal particles accelerated to suprathermal energies in about a half of the quiet periods, the rest of quiet-time fluxes originates from particle acceleration in processes similar to those in small impulsive solar flares rich in Fe. At solar minimum the bulk solar wind particles serve as seed population.     

Space and velocity distributions of neutron stars in the Milky Way

We study the long term dynamics of isolated neutron stars (NSs) for different initial conditions. From the resulting phase-space distributions, we estimate the fraction of NSs bound to the Milky Way. We also estimate the surface and spatial density of NSs in the solar neighborhood and the mean velocity of NSs in the Galactic disk. Estimates of the sky density of NSs towards specific lines of sight, i.e. the Galactic center and the Magellanic Clouds, are also given.