卫星时分多址信号高精度快速时频差联合估计方法

针对传统时频差估计方法对时分多址(TDMA)信号进行参数估计时会出现不同用户相互影响、估计精度差,以及计算复杂度高不利于系统实时信号处理等问题,文章提出一种高精度快速时频差联合估计方法.首先,基于循环平稳特征对主站接收数据进行信号检测;然后,基于小波阈值去噪和短时电平和进行TDMA信号时隙分离;在此基础上,基于不同调制信号特征参数设计多级分类器,对每个分离的信号时隙进行调制样式判别,进而分选不同用户对应的信号时隙;接着,利用主站分选的各个用户信号分别与辅站信号进行时频差粗值估计;根据粗时频差估计值减小细化时差搜索范围,以获取精细时频差估计值;最后,利用二阶曲面拟合方法进一步提升参数估计精度.仿真结果表明:文章所提方法能够有效实现TDMA信号高精度快速时频差联合估计,可为后续卫星频谱感知体系的建设提供理论支撑.     

1. Transport of Mass,Momentum and Energy in Planetary Magnetodisc Regions

The rapid rotation of the gas giant planets, Jupiter and Saturn, leads to the formation of magnetodisc regions in their magnetospheric environments. In these regions, relatively cold plasma is confined towards the equatorial regions, and the magnetic field generated by the azimuthal (ring) current adds to the planetary dipole, forming radially distended field lines near the equatorial plane. The ensuing force balance in the equatorial magnetodisc is strongly influenced by centrifugal stress and by the thermal pressure of hot ion populations, whose thermal energy is large compared to the magnitude of their centrifugal potential energy. The sources of plasma for the Jovian and Kronian magnetospheres are the respective satellites Io (a volcanic moon) and Enceladus (an icy moon). The plasma produced by these sources is globally transported outwards through the respective magnetosphere, and ultimately lost from the system. One of the most studied mechanisms for this transport is flux tube interchange, a plasma instability which displaces mass but does not displace magnetic flux—an important observational constraint for any transport process. Pressure anisotropy is likely to play a role in the loss of plasma from these magnetospheres. This is especially the case for the Jovian system, which can harbour strong parallel pressures at the equatorial segments of rotating, expanding flux tubes, leading to these regions becoming unstable, blowing open and releasing their plasma. Plasma mass loss is also associated with magnetic reconnection events in the magnetotail regions. In this overview, we summarise some important observational and theoretical concepts associated with the production and transport of plasma in giant planet magnetodiscs. We begin by considering aspects of force balance in these systems, and their coupling with the ionospheres of their parent planets. We then describe the role of the interaction between neutral and ionized species, and how it determines the rate at which plasma mass and momentum are added to the magnetodisc. Following this, we describe the observational properties of plasma injections, and the consequent implications for the nature of global plasma transport and magnetodisc stability. The theory of the flux tube interchange instability is reviewed, and the influences of gravity and magnetic curvature on the instability are described. The interaction between simulated interchange plasma structures and Saturn’s moon Titan is discussed, and its relationship to observed periodic phenomena at Saturn is described. Finally, the observation, generation and evolution of plasma waves associated with mass loading in the magnetodisc regions is reviewed.     

通过任务驱动教学模式提高教师实践技能

根据数控加工任务驱动教学的改革与实践,提出通过任务驱动教学过程提高教师实践技能的方法,在数控加工任务驱动中,当教师准备课程时,通过试做任务(目标零件)、完成任务(加工目标零件),可有效地提高实践技能.这为适应工学结合教学改革,提高教师实践技能素质,做了有益的探索.     

基于CS8900A的工业级嵌入式网络接口实现

介绍了工业级以太网络控制芯片CS8900A—IQ3在嵌入式Internet中的应用，以实例详细对比说明了其在8位和16位两种运行模式下的硬件和软件实现。     

Mathematical modeling of heat transfer process in a variable domain

In this paper, a brief review and generalization of studies on the heat transfer and heat conduction problem in a variable domain are presented. The equations of the process, where the boundary displacement velocity is the control, are obtained taking into account heat inflow. This article was submitted by the authors in English.     

高校科研工作量考核中的抽样调查及统计分析方法

针对科研工作量考核中的考核标准确定及考核结果的分析等问题进行了研究，主要包括：根据分层抽样原理，采用Ｂｒｅｗｅｒ方法设计了制订考核标准值的抽样调查方案；确定科研工作量的分布情况以及有关特征值，掌握学校科研工作的现状；利用方差分析法，确定不同职称系列承担科研工作的差异例用回归分析预测法和干涉因子灰色预测法，掌握科研工作量的变化情况及和学校政策的相互关系。一实际应用结果表明，该方法能比较客观地确定科研工作量的考核标准，同时为学校制订相关政策提供了依据。     

不同介质下高速铣削钛合金时切屑的变形研究

开展了不同介质下钛合金切屑变形的高速铣削试验研究,分析比较了不同介质、不同铣削速度对切屑宏观和微观形貌的影响及其原因,得出了干铣削、空气油雾和氮气油雾介质下切屑变形的各自特点以及切屑变形随速度而变化的规律。     

大功率无电极高密度等离子体电磁推进概述

无电极高密度等离子体电磁推进技术已成为未来深空探测、载人航天和货运、太阳能电站以及航天器在轨服务与维护等空间任务中极具竞争力的核心推进技术之一。在梳理不同无电极等离子体电磁加速机制基础上,开展大功率无电极高密度等离子体电磁推进技术性能对比,给出新概念无电极场反构型电磁推进技术向未来超大功率拓展的优势和发展潜力,同步分析了该技术亟需解决的关键基础问题,旨在为中国新概念场反构型电磁推进技术的研发提供理论基础。     

ExoMars 2016 Schiaparelli Module Trajectory and Atmospheric Profiles Reconstruction

On 19^th October 2016 Schiaparelli module of the ExoMars 2016 mission flew through the Mars atmosphere. After successful entry and descent under parachute, the module failed the last part of the descent and crashed on the Mars surface. Nevertheless the data transmitted in real-time by Schiaparelli during the entry and descent, together with the entry state vector as initial condition, have been used to reconstruct both the trajectory and the profiles of atmospheric density, pressure and temperature along the traversed path.The available data-set is only a small sub-set of the whole data acquired by Schiaparelli, with a limited data rate (8 kbps) and a large gap during the entry because of the plasma blackout on the communications.This paper presents the work done by the AMELIA (Atmospheric Mars Entry and Landing Investigations and Analysis) team in the exploitation of the available inertial and radar data. First a reference trajectory is derived by direct integration of the inertial measurements and a strategy to overcome the entry data gap is proposed. First-order covariance analysis is used to estimate the uncertainties on all the derived parameters. Then a refined trajectory is computed incorporating the measurements provided by the on-board radar altimeter.The derived trajectory is consistent with the events reported in the telemetry and also with the impact point identified on the high-resolution images of the landing site.Finally, atmospheric profiles are computed tacking into account the aerodynamic properties of the module. Derived profiles result in good agreement with both atmospheric models and available remote sensing observations.     

高能(450 kV)X射线参考辐射场附加过滤研究

利用MCNP程序对450kV X光机建立模型，计算各参考辐射质下的原级谱、平均光子能量。对ISO 4037-1中已有范围的管电压与附加过滤片厚度关系曲线进行二次拟合，确定模拟厚度范围。利用MCNP计算各附加过滤组合下的平均光子能量值，并与外推法得出的平均光子能量值进行对比，将相对偏差最小时的附加过滤作为最终确定值。从部分能量点的模拟与测量结果的对比可看出，模拟得出的平均光子能量在2%以内与PTB及中国计量院测量结果保持一致，附加过滤最大相对偏差为18%。