硅基太赫兹频率源关键技术研究进展综述

随着太赫兹技术的发展,由于太赫兹THz(Terahertz)频段具有丰富的频谱资源和相对宽的带宽优势,因此太赫兹频率源表现出广泛的应用前景,如超高速短距无线/有线通信、雷达、医疗、成像和遥感传感器等.本文总结了硅基太赫兹频率源的最新研究成果和存在的问题,概述了近二十年来太赫兹倍频器、太赫兹振荡器、太赫兹天线、太赫兹辐射...     

气象海洋卫星地面遥感站

气象海洋卫星地面遥感站主要是用于接收各类气象、海洋、环境卫星的遥感原始数据,并实现数据存储及相关数据处理,从中提取可用的空间环境资料。5.2m天线根据轨道预报捕获并跟踪目标,接收L/S/X三频段射频信号,将信号放大变频后送解调器,解调器从中频信号中恢复出原始遥感数据帧,由记录器对数据进行存储,快视设备实时对原始数据进行去格式处理后显示遥感图像,通过网络传输给各个用户。     

Some problems of selection and evaluation of the Martian suit enclosure concept

One of the most important tasks for preparation of a future manned mission to Mars is to create a space suit, which ensures efficient and safe operation of the man on the planet surface.

The concept of space suit (SS) utilisation on the Mars surface will be determined mainly by the Mars mission scenario. Currently the preference is given to utilisation of robotics with the crew driving a Mars rover vehicle, whereby the suit will be used solely as an additional safety means.

However, one cannot exclude the necessity of a durable self-contained stay of the man outside a pressurised compartment, to pick up, for instance, soil samples or do certain repair work in case of an emergency.

The requirements to the Mars suit and especially to the personal self-contained life support system (LSS) will depend in many respects on the Mars environmental conditions, the space vehicle system concept and performance characteristics, the airlock and its interface design, the availability of expendable elements for the LSS, etc.

The paper reviews principal problems, which have to be solved during development of the Martian suit. A special attention is paid to the issue of suited man mobility during traversing on the planet surface.

The paper also reviews the arguments for application of a suit semi-rigid design concept and evaluates potentialities of using certain elements of the existing “Orlan” type suit.

The paper presents results of a number of studies on selection of the planetary SS enclosure concept and on experimental evaluation of mobility of the lower torso and leg enclosures in conjunction with a specially designed prototype model (tentative model) of the SS enclosure.     

遥感卫星扰振对TDICCD相机图像影响的仿真与分析

随着传输型遥感卫星结构的扩大化及灵活性的增强,对图像品质产生影响的扰振越来越受到重视。当遥感卫星在轨进行成像时,相机的图像品质会由于星上活动部件的运动的影响而下降。文章从调制传递函数（Modulation Transfen Function,MTF）角度出发,对不同工况下太阳翼转动驱动机构（BAPTA）和动量轮对图像品质的影响进行了仿真和评估。同时,针对高分辨率相机成像品质影响,从动力学仿真方面对星体扰振的幅值和频率进行了有限元分析,确定了扰振源的频率和幅值。最后,根据仿真分析结果,提出了星上扰振控制方案建议。     

Future earth observation missions for oceanographic applications: Indian perspectives

Significant progress has been achieved in India in demonstrating the utility of remote sensing data for various oceanographic applications during the last one decade. Among these, techniques have been developed for retrieval of ocean surface waves, winds, wave forecast model, internal waves, sea surface temperature and chlorophyll pigments. Encouraged from these results as well as for meeting the specific and increasing data requirements on an assured basis by oceanographers, India is making concerted efforts for developing and launching state-of-the-art indigenous satellites for ocean applications in the coming years.

The first in the series of ocean satellites planned for launch is Oceansat-1 (IRS-P4) by early 1999. Oceansat-1 carries on-board an Ocean Colour Monitor (OCM) and a Multi-frequency Scanning Microwave Radiometer (MSMR). OCM will have 8 narrow spectral bands operating in visible and near- infrared bands (402–885 nm) with a spatial resolution of 360 m and swath of 1420 km. The MSMR with its all weather capability is configured to have measurements at 4 frequencies viz., 6.6, 10.65, 18 & 21 GHz in dual polarisation mode with a spatial resolution of 120, 80, 40 & 40 km, respectively with an overall swath of 1360 km. The Oceansat-1 with repetitivity of once in two days will provide global data for retrieval of various oceanographic and meteorological parameters such as chlorophyll (primary productivity), sea surface temperature and wind speed, besides a host of other parameters of relevance to meteorology.

A full fledged satellite for ocean applications known as Oceansat-2 (IRS-P7) is also planned for launch during 2002. This satellite with payload mix of microwave (Scatterometer, Altimeter & Passive Microwave Radiometer), Thermal (TIR) and Optical (OCM) sensors, will provide greater in-sight into the global understanding of ocean dynamics/resources. This mission is expected to provide a complete set of oceanographic measurements, which are useful for providing operational oceanographic services.

Efforts are also on towards development of missions having multi-frequency, multipolarisation and multi-look angle microwave payloads including Synthetic Aperture Radar (SAR) and advanced millimeter wave sounders, besides development of imaging spectrometers by 2005.

A well-knit plan has been initiated in India for utilisation of planned Oceansat data. Important efforts initiated in this direction include SATellite Coastal and Oceanographic Research and Ocean Information Services, which are being carried out on an integrated basis aiming at providing services to the down stream users. The paper highlights these efforts in India towards providing an operational ocean information services in the coming years.     

LOCSS and its implementation on the basis of a small satellite cluster

A problem of providing users with the necessary remote sensing data in the visible and near IR spectral bands has been considered. The solution of the problem plans increase of spatial and spectral resolution for imaging from space, high periodicity of surveying the same sites on the Earth's surface and spaceborne data delivery to users in real time.

This problem solution proposed is to use a cluster of small satellites and to implement the Local Space Service (LOCSS) program. The main aspects of this concept are as follows:

• • optimization of remote sensing instrumentation parameters;

• • image data compression onboard a small spacecraft;

• • compressed data downlinking via the low rate radio channel;

• • direct reception of the image data by users at small cheap receiving stations; and

• • image data decompression and processing using personal computers and special processors.

     

新一代无源微波遥感器及其在地球同步卫星上的应用研究

星载无源微波遥感已发展成为观测大气与地球表面的重要手段，地球同步气象卫星上使用的微波遥感仪器必须是新一代先进的遥感器；它应兼备传统的无源微波大气探测仪及微波成像仪的双重功能。本文叙述了国际上新一代星载无源微波遥感器的研究现状和发展趋势，讨论了在地球同步气象卫星上装载无源微波遥感仪器的可行性及其关键技术，并研究了其频率的选择问题。     

中波红外面阵遥感相机相对辐射定标方法研究

为了促进中波红外面阵遥感相机遥感数据的应用,提出了一种在轨相对辐射定标方法。该方法根据两点定标原理,以中波红外面阵遥感图像数据为基础,利用在轨其他卫星数据获得相机入瞳处辐亮度,计算出非均匀性系数,从而实现在轨相对辐射定标。它为同类红外面阵遥感相机在轨相对辐射定标提供了一种新的思路,同时也可作为星上黑体标的一种校验手段。     

WorldView系列卫星设计状态分析与启示

WorldView 系列卫星是目前世界商业卫星中分辨率较高的光学遥感卫星。文章从卫星总体设计角度介绍了WorldView 系列卫星技术指标,分析了卫星敏捷机动工作能力、构形布局设计、平台和载荷一体化设计和微振动抑制设计等,梳理出国外先进遥感卫星的发展趋势,以此为基础提出了对我国新一代光学遥感卫星的设计启示。     

高速率遥感卫星接收与处理系统的设计与实现

为成功接收搭载分米级分辨率的SAR（Synthetic Aperture Radar,合成孔径雷达）载荷低轨遥感卫星数据,验证卫星载荷工作状态和性能,本项目研发一套Ka/S双频段遥感卫星接收与处理机动站。针对窄波束高动态卫星跟踪、多通道高速率遥感数据星地传输的重难点,本文着重从窄波束高动态目标卫星跟踪、超高速高性能全数字解调以及高精度双模式自适应盲均衡等关键技术进行研究。通过试验验证技术路径正确、措施有效,可为后续相关系统研制提供技术参考。     

低背景红外辐射源校准技术

介绍了以低温绝对辐射计(Absolute Cryogenic Radiometer)作为标准探测器的低背景红外辐射源校准技术的原理、设备、关键技术以及校准结果不确定性的分析方法,同时阐述了该技术的先进性和重要性。     

基于直方图修改的卫星遥感图像无损隐藏传输

针对星上低速率数据的传输问题,提出了一种基于直方图修改技术的卫星遥感图像无损隐藏传输方法。该方法通过对星上高速率遥感图像相邻像素差的直方图进行修改,将低速率数据嵌入到原始高速率遥感载体图像中,并利用卫星高速数传系统进行下传。地面接收端可以从载体图像中正确提取低速率数据,并无损恢复原始高速率遥感图像数据。该方法在不增加卫星数传系统复杂度和信息传输速率的前提下,提高了卫星数传系统的利用率,增强了数据传输的隐蔽性。实验结果表明,本文算法在保证良好的不可见性的情况下,获得了较高的纯载荷嵌入容量。与其它无损嵌入方法相比,在峰值信噪比和纯载荷嵌入容量方面都有很大的优势。     

遥感卫星立体影像传感器模型综述

文章首先介绍了遥感卫星立体影像传感器模型的主要类型;然后从模型数学表达式、对影像的处理精度和应用范围等几个方面对目前几种主流传感器模型进行了分析;最后比较了不同传感器模型的优缺点,对遥感卫星立体影像处理模型的选择提出了建议。     

空间光学遥感器系统偏振测试方法探讨

随着光学遥感器的不断发展,对光学遥感器的性能要求也不断提高。遥感器系统偏振特性也逐渐为人们所重视。特别是对辐射灵敏度要求较高的光学遥感器。文章首先分析了光学遥感器偏振特性的表述及与遥感器系统辐射灵敏度的关系。讨论了系统偏振影响的因素和系统偏振补偿设计的几种考虑。最后提出了遥感器系统偏振灵敏度测试方法和应用实例。     

“风云三号”D星电离层光度计

“风云三号”D星电离层光度计（IPM）是我国首次利用天基方式对电离层进行全天候定量化光学遥感观测的载荷。该载荷通过观测电离层夜/日间OI 135.6 nm气辉辐射强度、日间N₂LBH带气辉辐射强度,可以反演获取夜间电子总含量（TEC）、F2层峰值电子密度（NmF2）及日间O/N₂比等关键电离层环境信息。该载荷具备夜间高灵敏度观测的突出优势,非常适合电离层精细结构和微小变化观测,配置了夜间和日间两种工作模式,可以实现对电离层关键环境信息的全天候监测。文章主要对该电离层光度计的观测目标、观测原理、系统组成和在轨观测结果进行介绍。     

星载激光雷达高精高稳探测卫星系统保证技术

激光雷达探测精度高,具备全天时工作和垂直探测能力,在大气环境天基遥感领域应用广泛。基于CO_2柱线浓度激光遥感探测原理,分析了积分路径差分吸收星载激光雷达测量系统的激光波长、能量精度和稳定性及光轴指向精度等关键指标要求和功能模块配置,重点开展了星载激光雷达光机头部稳定安装、良好机热环境保障及星敏载荷一体化布局等整星层面系统设计保证,仿真结果初步表明设计方案可行。同时,提出了激光雷达波长、能量精度及稳定性实时监测、卫星对地光轴指向高精度测定和星地载荷光轴指向测量误差标定的地面试验验证要求,以确保系统设计的有效性,为激光雷达遥感卫星的研制提供了技术参考。     

Remote sensing in the information age

A large percentage of the public today perceives the majority of applications of Earth observation data from satellite and aircraft altitudes to be focused on the understanding and management of the renewable and non-renewable resources of the Earth and its environment. Originally conceived as a tool for gathering intelligence information, remote sensing has just fully emerged from its military womb to the public domain. Advances in the technology, a variety of indirect benefits that could be derived from space exploration, commercialization of remote sensing and the drive of the value-added companies - all of these hold promise for new opportunities for many other novel applications of Earth observation data and related information. In the advent of the more advanced, user-friendly, cost effective, and problem solving operations being championed by the private sector, particularly in the industrialized countries, it appears that the commercial future for remote sensing programmes and related information generated in the process is promising. This paper examines how the information age is influencing the metamorphosis of remote sensing technology particularly through international legal instruments and converging technologies. In spite of the progress attained to-date, of international concern is possible radio frequency interference between remote sensing satellite and communication satellite services. There is also a major knowledge gap between the providers of raw remote sensing data and the user community, particularly those interested in the new high-level information. A resolution of these issues will enhance the contributions of remote sensing to the information economy.     

Chandrayaan-1 mission to the Moon

Chandrayaan-1 is the first Indian planetary exploration mission that will perform remote sensing observation of the Moon to further our understanding about its origin and evolution. Hyper-spectral studies in the 0.4– region using three different imaging spectrometers, coupled with a low energy X-ray spectrometer, a sub-keV atom analyzer, a 3D terrain mapping camera and a laser ranging instrument will provide data on mineralogical and chemical composition and topography of the lunar surface at high spatial resolution. A low energy gamma ray spectrometer and a miniature imaging radar will investigate volatile transport on lunar surface and possible presence of water ice in the polar region. A radiation dose monitor will provide an estimation of energetic particle flux en route to the Moon as well as in lunar orbit. An impact probe carrying a mass spectrometer will also be a part of the spacecraft. The 1 ton class spacecraft will be launched by using a variant of flight proven indigenous Polar Satellite Launch Vehicle (PSLV-XL). The spacecraft will be finally placed in a 100 km circular polar orbit around the Moon with a planned mission life of two years.     

基于MTFC的遥感图像复原方法

遥感图像在成像过程中受到大气、光学系统、探测器、平台运动和电路等因素的影响,引起图像退化,图像复原算法可以改善遥感图像像质,提高图像信息的解译能力。文章介绍了调制传递函数补偿（modulation transfer function compensation,MTFC）算法的原理,从遥感成像的链路环节出发,分析了MTFC的原理,提出了一种星上实时遥感图像MTFC复原算法。通过卷积系数和抑噪参数的优化设计,在提高图像清晰度的同时能较好地抑制噪声;对不同卷积和抑噪参数的图像复原效果进行了对比,从主观和客观两个方面对复原图像进行了评价。实验结果表明,该算法能有效提高图像像质,增强图像的高频部分,采用不同类型的卫星遥感图像验证了算法的适应性。