导弹目标ISAR成像的仿真

在逆合成孔径雷达（ISAR）成像基本原理及信号处理过程的基础上，根据导弹的飞行弹道、自转和进动模型建立导弹飞行模型，采用自相关快速运动和累积相关运动两种补偿方法，对导弹目标的ISAR二维成像进行了仿真研究。结果表明，导弹的自旋时成像结果及积累时间的影响较大，模型不同，积累时间也不同。     

Gamma-ray detector on board lunar mission Chang’E-1

Gamma-ray spectrometer (GRS) is included in the payload of Chinese first lunar mission Chang’E-1 that will be launched in 2007. Specific objectives of the GRS are to map abundance of O, Si, Fe, Ti, U, Th, K, and perhaps, Mg, Al, and Ca to depths of about 20 cm. There are remarkable advantages for GRS application to remote sensing elemental materials over the entire lunar surface: large effective area and good ability for background rejection. We will describe the design of GRS and present its performance in this paper. Moreover, the GRS calibration will also be introduced.     

基于步进频连续波的近距离主动毫米波圆柱扫描成像系统

为了克服压控振荡器（VCO）输出线性调频（LFM）信号频率线性度较差的缺点,本文提出了基于直接数字合成（DDS）技术产生步进频连续波信号的近距离主动毫米波圆柱扫描成像系统,该系统具有距离分辨率高、频率精度高以及波形产生和波形控制较为简单的优点。首先,本文通过步进频连续波信号的探测原理分析了该信号的一维距离像、距离分辨率以及距离模糊的特点;然后,通过波动方程推导出近距离主动毫米波圆柱扫描成像系统的重构算法;最后,在微波暗室搭建了半实物仿真成像系统,验证了步进频连续波信号在近距离主动毫米波圆柱扫描成像系统中应用的可行性和有效性。     

Solar X-ray Monitor (XSM) on-board Chandrayaan-2 orbiter

The remote X-ray fluorescence spectroscopy is a powerful technique to investigate the elemental abundances in the atmosphere-less planetary bodies. The experiment involves measuring spectra of fluorescent X-rays from lunar surface using a low energy X-ray detector onboard an orbiting satellite. Since the flux of fluorescent X-ray lines critically depend on the flux and spectrum of the incident solar X-rays, it is essential to have simultaneous and accurate measurement of X-ray from both Moon and Sun. In the context of Moon, this technique has been employed since early days of space exploration to determine elemental composition of lunar surface. However, so far it has not been possible to exploit it to its full potential due to various reasons. Therefore it is planned to continue the remote X-ray fluorescence spectroscopy experiment on-board Chandrayaan-2 which includes both lunar X-ray observations and solar X-ray observations as two separate payloads. The lunar X-ray observations will be carried out by Chandra Large Area Soft x-ray Spectrometer (CLASS) experiment; whereas the solar X-ray observations will be carried out by a separate payload, Solar X-ray Monitor (XSM). Here we present the overall design of the XSM instrument, the present development status as well as preliminary results of the laboratory model testing. XSM instrument will have two packages namely – XSM sensor package and XSM electronics package. XSM will accurately measure spectrum of Solar X-rays in the energy range of 1–15 keV with energy resolution ∼200 eV @ 5.9 keV. This will be achieved by using state-of-the-art Silicon Drift Detector (SDD), which has a unique capability of maintaining high energy resolution at very high incident count rate expected from Solar X-rays. XSM onboard Chandrayaan-2 will be the first experiment to use such detector for Solar X-ray monitoring.     

An Overview of the Instrument Suite for the Deep Impact Mission

A suite of three optical instruments has been developed to observe Comet 9P/Tempel 1, the impact of a dedicated impactor spacecraft, and the resulting crater formation for the Deep Impact mission. The high-resolution instrument (HRI) consists of an f/35 telescope with 10.5 m focal length, and a combined filtered CCD camera and IR spectrometer. The medium-resolution instrument (MRI) consists of an f/17.5 telescope with a 2.1 m focal length feeding a filtered CCD camera. The HRI and MRI are mounted on an instrument platform on the flyby spacecraft, along with the spacecraft star trackers and inertial reference unit. The third instrument is a simple unfiltered CCD camera with the same telescope as MRI, mounted within the impactor spacecraft. All three instruments use a Fairchild split-frame-transfer CCD with 1,024× 1,024 active pixels. The IR spectrometer is a two-prism (CaF₂ and ZnSe) imaging spectrometer imaged on a Rockwell HAWAII-1R HgCdTe MWIR array. The CCDs and IR FPA are read out and digitized to 14 bits by a set of dedicated instrument electronics, one set per instrument. Each electronics box is controlled by a radiation-hard TSC695F microprocessor. Software running on the microprocessor executes imaging commands from a sequence engine on the spacecraft. Commands and telemetry are transmitted via a MIL-STD-1553 interface, while image data are transmitted to the spacecraft via a low-voltage differential signaling (LVDS) interface standard. The instruments are used as the science instruments and are used for the optical navigation of both spacecraft. This paper presents an overview of the instrument suite designs, functionality, calibration and operational considerations.     

A hybrid X-ray imaging spectrometer for NeXT and the next generation X-ray satellite

We propose a new type of wide band X-ray imaging spectrometer as a focal plane detector of the super mirror onboard on future X-ray missions including post Astro-E2. This camera is realized by the hybrid of back illumination CCDs and a back supportless CCD for 0.05–10 keV band, and a Micro Pixel Gas Chamber detecting X-rays at 10–80 keV.     

空间大气成分探测傅立叶变换红外光谱仪

文章阐述了用于空间大气成分探测傅立叶变换红外光谱仪的国外发展状况，主要介绍了几种国外先进的高分辨率空间大气探测用傅立叶变换红外光谱仪的结构、应用范围和技术指标，比较了这几种设备的优缺点和技术特点。     

太阳,地球,卫星相关模拟源设计

“风云二号”自旋稳定地球同步气象卫星，以地球脉冲作为姿态控制基准，以太阳脉冲作为图像扫描基准，太阳、地球、卫星三者之间的相对关系在连续不断地运动变化。为了验证扫描成像原理和在地面测试卫星的成像质量，需对三者的相对关系进行研究。在此基础上，研制出太阳、地球、卫星相关模拟源，成功地用电子信号准确模拟“风云二号”卫星在静止轨道上感受到的不断变化的太阳、地球信号，使卫星的成像测试顺利进行，同时发现了卫星设计中存在的问题。     

星载合成孔径雷达的运动效应

对星载合成孔径雷达的运动效应进行了详细的分析，给出了雷达回波的多普勒参数和距离徒动特性的一般关系式。详细论证了卫星运动对多普勒参数和成像的影响，导出了描述速度误差、加速度误差和姿态误差的一系列定量计算公式，并就运动误差的补偿方法进行了阐述。     

非真空收集器质谱检漏标定技术

从理论上导出了非真空收集器质谱检漏漏率的几种标定公式 ,并对漏率标定的各种方法进行了利弊分析。经综合考虑认为 :为实现快速的高精度的漏率标定 ,采用标准气量直接加注法进行漏率的标定是比较适宜的