Longitudinal distribution of thermospheric densities and ionization rates in the upper atmosphere of Mars at mid-latitude using MGS ACC data

The Accelerometer Experiment (ACC) onboard Mars Global Surveyor (MGS) measured 1600 density profiles in the upper atmosphere of Mars during aerobraking. These measurements reveal large-scale and small-scale structure in the thermosphere of Mars. Here, the measurements of mass density for 115 orbits (#P0670–P0789) from November 1 to 30, 1998, under spring equinox and medium solar activity conditions (average F_10.7 ∼ 137) during phase 2 of the aerobraking in the thermosphere of Mars at different altitudes and longitudes are presented for northern mid-latitude (17–42°N) in the dayside atmosphere using ACC onboard MGS. From these mass densities, the neutral densities of different gases are derived from their mixing ratios. Using these neutral densities, the longitudinal distribution of photoionization rates and photoelectron impact ionization rates are calculated at wavelength range 1–102.57 nm due to EUV and soft X-ray radiation under photochemical controlled region using Analytical Yield Spectrum approach (AYS). These conditions are appropriate for MGS Phase 2 aerobraking period from which the accelerometer data is used. Under the photochemical equilibrium condition, the electron density near the peak varies as the square root of the total peak ionization rate. Using this fact, an attempt is being made to estimate the mean primary and secondary peak electron density by averaging the longitudinal variations of total peak ionization rates in the northern mid-latitude (17–42°N) ionosphere of Mars, as there is no radio science measurement at this latitude region by MGS.     

RNSS上行L频段新划分的回顾及风险评述

从国际频率划分规定的角度，回顾了2000年世界无线电通信大会（WRC-2000）对1300～1350MHz频段做出卫星无线电导航业务新划分的背景、研究过程、最终划分结果及相关条款等历史状况，同时对卫星无线电导航业务上行信号使用该频段存在的限制和风险进行了分析及评述。     

可视化技术在分析新型蓄冷材料——笼型化合物(Clathrate)溶解过程中的应用(一)

混浊液内部的流动 ,由于微粒子之间的相互作用以及因浊度高不易进行内部观察 ,所以无论是分析还是可视化实验都相当困难 ,存在着许多未弄清的问题。通过采用折射率匹配 (Refractive IndexMatching)技术 ,使透明的微粒子与透明的溶媒的折射率近乎相同 ,做成一种透明的“混浊液” ,从而使混入其中的示踪粒子的运动轨迹能被摄像机捕捉到 ,并以微粒子的沉降和温度的干涉所引起的流动现象为焦点 ,利用图像速度测量法来处理分析所拍摄到的可视化图像 ,成功地获得了定量的混浊液内部的速度场 ,为进一步揭示混浊液内部自然对流的流动机理提供了实验依据。     

The Effects of Transverse Magnetic Field and Density Variations on the Particle Energy Spectra in a Reconnecting 3D Current Sheet

Electron and proton acceleration by a super-Dreicer electric field is further investigated in a non-neutral reconnecting current sheet (RCS) with a variable plasma density. The tangential B _z and transverse magnetic field components B _x are assumed to vary with the distances x and z from the X nullpoint linearly and exponentially, respectively; the longitudinal component (a ‘guiding field’) is accepted constant. Particles are found to gain a bulk of their energy in a thin region close to the X nullpoint where the RCS density increases with z exponentially with the index λ and the tangential magnetic field B _x also increases with z exponentially with the index α. For the RCS with a constant density (λ = 0), the variations of the tangential magnetic field lead to particle power-law energy spectra with the spectral indices γ₁ being dependent on the exponent α as: for protons and for electrons in a strong guiding field (β > 10⁻²) and for electrons in a moderate or weak guiding field (β > 10⁻⁴). For the RCS with an exponential density increase in the vicinity of the X nullpoint (λ≥ 0) there is a further increase of the resulting spectral indices γ that depends on the density exponent index λ as for protons and for electrons in weaker guiding fields and as for electrons in stronger guiding fields. These dependencies can explain a wide variety (1.5–10) of particle spectral indices observed in solar flares by the variations of a magnetic field topology and physical conditions in a reconnecting region. This can be used as a diagnostic tool for the investigation of the RCS dynamics from the accelerated particle spectra found from hard X-ray and microwave emission.     

CT图像环状伪影校正方法

CT图像环状伪影是由探测器像元响应不理想等因素造成的,它导致CT重建图像的降质,影响了图像的后续处理和量化分析.提出了一套完整的算法完成CT伪影校正:基于探测器像元通道响应不一致性的校正,通过偏置和增益校正对硬件响应不一致性进行补偿;基于投影正弦图的校正,通过数字滤波提取正弦图上残余的线状伪影,属于CT图像重建前的一种预处理校正方法;基于重建图像的校正,通过坐标变换将直角坐标系中的环状伪影变为极坐标系中的线状伪影进行处理,属于一种图像后处理方法.这些算法已经用于基于YXLON XRS232 9″图像增强器的CT重建,在保证图像质量的基础上环状伪影得到有效校正.      

一种基于嵌入式图像处理的工程车辆导向装置

分析了架桥施工中运梁车工作的特点,针对其在车辆导向方面所存在的主要问题,并结合现场需求,设计了一种基于单片机实现的嵌入式图像处理的新型车辆辅助导向装置,完成了相关硬件平台的设计,给出了在单片机系统中实现视频采集、图像处理、车辆跑偏判断和报警输出等关键技术细节的具体方法.实验结果表明,该辅助导向装置满足了运梁车在轨道梁上的行驶要求.该装置已应用于现场实际,其设计和实现方法对于其他大型工程车辆导向装置的研发具有较高的参考价值.      

CCD互相关粒子图像测速及其在对抗流流场测量中的应用

在常规自相关粒子图像测速（ＰＩＶ）系统的基础上,发展了一个采用ＣＣＤ像机的互相关粒子图像测速系统。用这一新系统测量了对抗流流场的结果表明,这一技术克服了自相关粒子图像测速技术在测量具有滞止点的流场中的困难。实验说明,与自相关粒子图像测速技术相比,这一技术更快捷有效。     

目标图像的显示及后期处理技术

:通过对由图象输入设备获得的目标图象文件的分析 ,论述了利用计算机来完成此类图象的显示方法。此外还论述了利用抛物插值算法来实现目标图像的后期处理———图象局部放大显示的原理及方法。     

星载SAR图像斑点抑制与质量评估系统

结合星载合成孔径雷达(SAR)单视图像斑点噪声抑制技术与质量评估,并基于为科学数据可视化及数学分析提供完备计算环境的IDL(Interactive Data Language)语言,完成了在IDL环境下开发的SAR图像斑点抑制与质量评估系统,获得了高空间分辨率和高辐射分辨率的星载SAR图像.      

基于解析小波的光流计算方法

在基于小波变换的光流计算中,实值小波系数的相位振荡和多分辨率计算的累计误差是影响光流计算精度的两个主要原因.通过引入解析小波以降低相位振荡的影响,同时结合M估计子能够有效抑制参数估计产生的大误差项,提出一种多尺度多分辨率的光流计算方法.实验表明,与现有的基于小波变换的光流计算方法相比,提出的方法不论在光流计算的精度还是可计算范围上都有很大程度的提高.