Indian tracking and data acquisition facilities for low Earth andgeosynchronous satellites

To support its satellite program, the Indian Space Research Organization (ISRO) has an extensive infrastructure of ground support facilities throughout the country and abroad. The major elements include the ISRO Telemetry Tracking and Command Network (ISTRAC), the National Remote Sensing Agency (NRSA), and the Indian National Satellite (INSAT) control facilities. These facilities and their important role in supporting the Indian Space Program are described. The locations of the principal ISRO space control facilities within India are shown     

遥感影像中电磁特性数据挖掘

从数据挖掘和遥感信息提取的概念出发,提出了遥感影像中电磁特性数据挖掘的思想,从电子信息装备试验对电磁特性数据的需求和SAR影像数据处理的需求出发,重点完成了基于电磁特性的地物分类和面向对象的遥感影像电磁特性数据挖掘,其中面向对象的遥感影像电磁特性数据挖掘包含遥感影像准备与数据预处理、影像分割、对象的层次结构、规则建立、电磁特性数据获取、信息提取等六个部分,最后把理论方法进行了实践,为大批量获取遥感影像中的电磁特性数据提供了方法支持。     

用大面积源检定核应急机载/车载伽玛能谱仪

人工核素大面积源标准是核工业航测遥感中心等单位经过十余年研究建立的新型计量保障标准,使用该标准,可对监测核应急伽玛辐射环境的机载/车载伽玛能谱仪进行检定.使用大面积源标准检定,可以有效地弥补因机载/车载伽玛能谱仪系统的角响应影响因素复杂而难于模拟计算的缺陷,为监测核应急伽玛辐射环境的机载/车载伽玛能谱仪提供了量值传递的保障.本文介绍了大面积源检定的原理和技术方法.     

CCRS C/X-airborne synthetic aperture radar: An Rand D tool for the ERS-1 time frame

The airborne synthetic-aperture radar (SAR) system developed for the Canada Centre for Remote Sensing (CCRS) is described. It consists of two radars, at C-band and X-band. Each radar incorporates the following features: dual-channel receivers and dual-polarized antennas; a high quality, 7-look, real-time processor; a sensitivity time control for range-dependent gain control; a motion-compensation system for antenna steering in azimuth and elevation; and baseband I and Q signal phase rotation. The system also uses a high-power transmitter with a low-power back-up. The SAR maps to either side of the aircraft, at high or low resolution, at incidence angles which in high resolution span 0° to 80°. Radar operating parameters, data products, key specifications and the motion compensation scheme used are presented. Properties of the real-time imagery are discussed and examples of C-band SAR data in the three operating modes are given     

Arctic sea ice mapping with satellite radars

The drastic reduction of Arctic sea ice in recent years demands ice monitoring over various spatial and temporal scales. Sea ice backscatter signatures from field measurements and from model analyses are obtained at L-band and C-band frequencies. Based on these signatures, capabilities for Arctic sea ice mapping are determined for current and future satellite active microwave sensors including synthetic aperture radars (SAR) and scatterometers. This study includes L-band and C-band radars such as the ERS (European Remote Sensing), Envisat (Environmental Satellite), RADARSAT-1 and 2, ALOS (Advanced Land Observing Satellite), and DESDnyl (Deformation, Ecosystem Structure, and Dynamics of Ice). SARs with resolutions from 10 to 100 m, and the SMAP (Soil Moisture Active-Passive) scatterometer with resolutions from 1 to 10 km.     

Multipath and ground clutter analysis for a UWB noise radar

An ultrawideband (UWB) random-noise radar operating in the 1-2 GHz frequency band has been developed and field-tested up to a 200 m range at the Environmental Remote Sensing Laboratory (ERSL) of the University of Nebraska. A unique heterodyne correlation technique based on a delayed transmitted waveform using a photonic delay line has been used to inject coherence within this system. The performance of this radar in the presence of ground reflections is investigated analytically and experimentally, and the mitigating effects of UWB waveform on multipath-induced interference are analyzed. In addition, the ground clutter statistics, in a look-down mode, are theoretically established and experimentally verified. The performance of this radar in detecting clutter embedded targets with small radar cross section (RCS) is also experimentally examined.     

REMS: The Environmental Sensor Suite for the Mars Science Laboratory Rover

The Rover Environmental Monitoring Station (REMS) will investigate environmental factors directly tied to current habitability at the Martian surface during the Mars Science Laboratory (MSL) mission. Three major habitability factors are addressed by REMS: the thermal environment, ultraviolet irradiation, and water cycling. The thermal environment is determined by a mixture of processes, chief amongst these being the meteorological. Accordingly, the REMS sensors have been designed to record air and ground temperatures, pressure, relative humidity, wind speed in the horizontal and vertical directions, as well as ultraviolet radiation in different bands. These sensors are distributed over the rover in four places: two booms located on the MSL Remote Sensing Mast, the ultraviolet sensor on the rover deck, and the pressure sensor inside the rover body. Typical daily REMS observations will collect 180 minutes of data from all sensors simultaneously (arranged in 5 minute hourly samples plus 60 additional minutes taken at times to be decided during the course of the mission). REMS will add significantly to the environmental record collected by prior missions through the range of simultaneous observations including water vapor; the ability to take measurements routinely through the night; the intended minimum of one Martian year of observations; and the first measurement of surface UV irradiation. In this paper, we describe the scientific potential of REMS measurements and describe in detail the sensors that constitute REMS and the calibration procedures.     

40G以太网在航电系统中的应用初探

随着飞机整体性能的提升，航电系统的发展日新月异，对总线网络提出了越来越高的要求。基于远端内存直接访问技术传输机制的以太网以其高带宽、低延时以及生态开放性的特点，在航电系统总线中逐渐得到推广。本文介绍了航电总线网络的发展，对典型的航电总线进行了对比分析，开展了10G/40GE交换工程样机的研制和测试工作，为下一代航电系统总线网络的选型提供了参考。     

In-orbit demonstration of rendezvous laser radar for unmanned autonomous rendezvous docking

The National Space Development Agency of Japan (NASDA) performed unmanned autonomous rendezvous docking (RVD) experiments using the Engineering Test Satellite VII (ETS-VII) in 1998 and 1999. In these experiments, a rendezvous laser radar (RVR) was used as the primary navigation sensor during the final approach phase (relative distances from 500 m to 2 m). The RVR functioned properly, and its characteristics, which are measurement accuracy, optical propagation, and acquisition/tracking, satisfied the requirements. The experimental results show that RVR is effective for autonomous rendezvous docking.     

The Indian Space Program

The Indian Space Program is described. The main objectives of the program are to provide operation space services to the nation, especially in the fields of communications and remote sensing, and to use modern space technology for the benefit of the Indian people. Some applications of the Indian Space Program are remote sensing, imagery, communications, broadcasting, and surveys of natural resources for water, crop, forest, land, minerals, and ocean. The emphasis is on the development and operation of indigenous satellites and launch vehicles for providing these space services     

火星中继应答机技术现状及发展

火星中继已作为火星探测重要组成部分,被美国NASA(National Aeronautics and Space Administration,国家航空航天局)和ESA(European Space Agency,欧空局)广泛应用于火星EDL(Entry,Descent and Landing,进入、下降和着陆)以及火星表面探测中。针对该情况,介绍了火星中继系统的组成和工作情况。结合NASA和ESA火星探测的成功经验和成果,重点对火星轨道器和着陆器的中继应答机的性能进行了梳理和分析,并对该技术的后续发展进行了展望。基于此,可为我国自主火星探测提供借鉴和参考。     

飞机维修保障远程技术支援系统建设方案初探

现阶段部队外场新换装飞机使用维修保障支持难度大、外场服务保障能力有限等问题日益凸显。依托信息化技术的发展,建立飞机维修保障远程技术支援系统,是解决上述问题的有效途径。本文从飞机维修保障远程技术支援系统组成及功能、系统构成及关键技术和系统工作流程三方面对系统建设方案进行了初步探索。     

载人月球探测深空站布局体系

针对载人月球探测,在我国现有深空测控资源的基础上,结合其他航天组织,如NASA (National Aeronautics and Space Administration,美国国家航空航天局)、ESA(European Space Agency,欧空局)等分布在全球的深空测控资源,提出了全球深空站布局体系.该体系包括我国深空站在内的8个地面站,大体形成“南四北四,均匀分布”的格局.并以美国“重返月球”计划深空站布局为参照,对比分析了布局体系的测控覆盖、三向测量和干涉测量共视弧段,讨论了布局干涉测量不同观测站三角的测角精度,可以为后续载人月球探测任务提供支持和参考.     

James Webb Space Telescope: Project Overview

The James Webb Space Telescope (JWST) project at the NASA, Goddard Space Flight Center (GSFC) is responsible for the development, launch, flight, and science operations for the telescope. The project is in phase B with its launch scheduled for no earlier than June 2013. The project is a partnership among NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA). The JWST mission team is fully in place, including major ESA and CSA subcontractors. This provides an overview of the planned JWST science, current architecture focusing on the instrumentation, and mission status, including technology developments, and risks.     

FADS系统迭代算法的收敛性分析

嵌入式大气数据传感系统采用分布在飞行器前端周线上的压力传感器阵列测量的压力推导大气参数的.介绍了采用迭代法推导大气参数的方法,针对迭代过程中出现的发散问题,提出采用小扰动线性化分析法解决多变量叠代算法的收敛性分析.最后应用Matlab仿真验证,仿真结果表明,在一般的超声速状态下(马赫数小于4.5),该算法是收敛的.     

基于EMD-CS的脉冲星周期超快速估计

面向X射线脉冲星周期估计的压缩感知（CS）中测量矩阵尺寸大,进而导致计算量大。针对这一问题,提出了一种基于经验模态分解-压缩感知（EMD-CS）的脉冲星周期超快速估计方法。将不同畸变度的脉冲轮廓进行EMD分解,得到一系列固有模态函数（IMF）。由于IMF包含了不同时间尺度的局部特征信号,脉冲轮廓畸变度这一微弱局部特征可体现在某些IMF中。采用迭代剔除法剔除冗余的IMF,剩下的IMF构成了测量矩阵。由于IMF的数量较少,采样率大幅减少。利用EMD-CS可实现X射线脉冲星周期超快速估计。通过计算复杂度分析结果可知,采样率与计算量呈正比关系。仿真结果中表明,EMD-CS的采样率为0.25%,仅为FFT-CS的1/29,因而计算量更小。     

The Japanese Experiment Module

This paper describes Japanese Experiment Module (JEM) which is a Japanese contribution to International Space Station (SS) Program. First half of phase B study of JEM was completed last March successfully. JEM primary function and basic configuration has been established. JEM consists of a Pressurized Module (PM), an Exposed Facility (EF), a scientific/equipment airlock, a local remote manipulator, and an Experimental Logistic Module (ELM). With all those hardware elements, JEM will accommodate general scientific and technology development research (some of which are to utilize the advantage of microgravity environment), and also accommodate control panels for the Space Station Mobile Remote Manipulator System and attached payloads.     

嵌入式大气数据传感系统的改进算法

简要介绍了嵌入式大气数据传感系统及其空气动力学模型,提出了求解动、静压和修正参数的改进算法.改进算法首先应用Moore-Penrose广义逆矩阵对非线性方程组进行简化.然后采用改进迭代算法和BP神经网络求解动、静压和修正系数.改进算法在精度、可靠性和实时性上都能满足系统的要求.应用BP神经网络,达到系统要求的精度所需要的计算时间只相当于原有算法的5%,具有更大的实时性优势.     

Plasma instabilities and their simulations in the equatorial F region – Recent results

In this paper the developments made in the last five years on numerical simulation/modeling studies of a complex nighttime equatorial spread F phenomenon are reviewed. Emphasis is given to the Indian work and necessary comparisons are done with other international works on this field. Investigations involving the important aspects, namely the confinement of the plasma bubble in the bottomside of the ionosphere, linear and nonlinear effects of molecular ions in the development of plasma bubbles, interaction of two modes as a seed perturbation are discussed in detail. This revised version was published online in August 2006 with corrections to the Cover Date.     

Ground-to-satellite laser communication experiments

Ground-to-satellite laser communication experiments between the optical ground station located in Koganei, central Tokyo, and a low earth orbit (LEO) satellite were jointly performed by the Japan Aerospace Exploration Agency and the National Institute of Information and Communications Technology. In 18 trials during three non-consecutive months, the satellite was acquired and tracked 61 % of the time, when clear or partly-clear conditions were predominant. The optical link was maintained for about 6 minutes when the satellite was visible in spite of the high angular velocity of the satellite. In 3 of the 18 trials, the link was not interrupted due to clouds during the six-minute transit. The failures (39% of the time) occurred when cloudy or rainy conditions were predominant. Fluctuation in the uplink received signal power was minimized by using multiple laser beam transmissions. The measured uplink and downlink bit error ratios were 10^-7-10^-4. These results demonstrate the applicability of free-space laser communication for not only geostationary earth orbit-LEO optical links but also ground-to-LEO optical links.