A DLR small satellite mission for the investigation of hot spots, vegetation and clouds

Starting from their FIRES proposal [1]the DLR makes a new approach in the design of a small satellite mission dedicated to hot spot detection and evaluation: the BIRD mission. The new approach is characterized by a strict design-to-cost philosophy. A two-channel infrared sensor system in combination with a Wide-Angle Optoelectronic Stereo Scanner (WAOSS) shall be the payload of a small satellite (80kg) considered for piggyback launch. So the launch is not a main cost driver as for other small satellite missions with dedicated launchers. The paper describes the mission objectives, the scientific payload, the spacecraft bus, and the mission architecture of a small satellite mission dedicated to the investigation of hot spots (forest fires, volcanic activities, burning oil wells or coal seams), of vegetation condition and changes and of clouds. The paper represents some results of a phase A study and of the progressing phase B.     

Development of a scheduling algorithm and GUI for autonomous satellite missions

In this paper, a scheduling optimization algorithm is developed and verified for autonomous satellite mission operations. As satellite control and operational techniques continue to develop, satellite missions become more complicated and the overall quantity of tasks within the missions also increases. These changes require more specific consideration and a huge amount of computational resources, for scheduling the satellite missions. In addition, there is a certain level of repetition in satellite mission scheduling activities, and hence it is highly recommended that the operation manager carefully considers and builds some appropriate strategy for performing the operations autonomously. A good strategy to adopt is to develop scheduling optimization algorithms, because it is difficult for humans to consider the many mission parameters and constraints simultaneously. In this paper, a new genetic algorithm is applied to simulations of an actual satellite mission scheduling problem, and an appropriate GUI design is considered for an autonomous satellite mission operation. It is expected that the scheduling optimization algorithm and the GUI can improve the overall efficiency in practical satellite mission operations.     

基于星务管理系统的小卫星自主健康管理系统

为了适应小卫星电子信息系统的快速发展,使卫星能够自行规划工作流程,实现在轨自主管理,需要构建合理有效的小卫星自主健康管理系统。文章以星务管理系统为基础,针对目前健康管理中存在的问题,构建了一套小卫星自主健康管理系统。它包括整星级、系统级和部件级3个层面。设计了自主健康管理执行模块构成整星级层面,其中包括自主健康管理规则库和自主健康管理任务执行模块。文章提出的小卫星自主健康管理系统,可以提高小卫星自主诊断、自主运行能力,最终实现小卫星长寿命、安全可靠运行。     

LARES successfully launched in orbit: Satellite and mission description

On February 13th 2012, the LARES satellite of the Italian Space Agency (ASI) was launched into orbit with the qualification flight of the new VEGA launcher of the European Space Agency (ESA). The payload was released very accurately in the nominal orbit. The name LARES means LAser RElativity Satellite and summarises the objective of the mission and some characteristics of the satellite. It is, in fact, a mission designed to test Einstein's General Relativity Theory (specifically ‘frame-dragging' and Lense-Thirring effect). The satellite is passive and covered with optical retroreflectors that send back laser pulses to the emitting ground station. This allows accurate positioning of the satellite, which is important for measuring the very small deviations from Galilei–Newton's laws. In 2008, ASI selected the prime industrial contractor for the LARES system with a heavy involvement of the universities in all phases of the programme, from the design to the construction and testing of the satellite and separation system. The data exploitation phase started immediately after the launch under a new contract between ASI and those universities. Tracking of the satellite is provided by the International Laser Ranging Service. Due to its particular design, LARES is the orbiting object with the highest known mean density in the solar system. In this paper, it is shown that this peculiarity makes it the best proof particle ever manufactured. Design aspects, mission objectives and preliminary data analysis will be also presented.     

Space experiments of deployable boom and umbrella test satellite (DEBUT)

This paper describes the results of the in-orbit performance testing of deployable and retractable umbrella and boom systems, which will be used as important subsystems of Boomerang/Tether satellites. The umbrella is one of the possible candidates of the aerodynamic braking system for boomerang satellite and the boom is also one of the possible candidates of relative position adjusting mechanism between center of mass and aerodynamic force center of the boomerang satellite and initial release/final recovery mechanism of the tethered satellite. For this technology verification, a small and inexpensive satellite, named DEBUT (Deployable Boom and Umbrella Test satellite), was developed in a short period of 1.5 years elapsing from the start of the detailed design until the launch of the mission. The lithium dry cell batteries were used as the primary power and functioned normally during 10 days mission lifetime.     

Sumbandilasat—An operational technology demonstrator

Technology advances in sensor, digital technology and a standardised modular satellite bus are enabling a new generation of 80 kg micro-satellites with a better than 6.5 m GSD multi-spectral performance, to be specified, built and deployed with a dedicated launch within 12 months. The result of the standardised modular bus is lower cost, higher reliability and fast deployment. Operational remote sensing with a micro-satellite is thus within reach of individual organisations for dedicated missions. Sumbandilasat (pioneer in the Venda language) is a second generation satellite technology building on the expertise obtained in the Sunsat small satellite programme. The components used to build Sumbandilasat are the result of a technology development program of more than 3 years. Sumbandilasat is an operational technology demonstrator with more than 90% newly developed or improved subsystems and a compact refractive imager as a precursor to the MSMISat satellite with the same multi-spectral band set. The scalable, standardised modular satellite bus architecture enables satellites with a mass of 80–450 kg to be adapted to the specific mission requirements with minimum new engineering effort.     

A series of small scientific satellite with flexible standard bus

Japan Aerospace Exploration Agency has a plan to develop the small satellite standard bus for various scientific missions and disaster monitoring missions. The satellite bus is a class of 250–400 kg mass with three-axis control capability of 0.02 accuracy. The science missions include X-ray astronomy missions, planetary telescope missions, and magnetosphere atmosphere missions. In order to adapt the wide range of mission requirements, the satellite bus has to be provided with flexibility. The concepts of modularization, reusability, and product line are applied to the standard bus system. This paper describes the characteristics of the small satellite standard bus which will be firstly launched in 2011.     

Rapid model-based inter-disciplinary design of a CubeSat mission

With an increase in the use of small, modular, resource-limited satellites for Earth orbiting applications, the benefit to be had from a model-based architecture that rapidly searches the mission trade-space and identifies near-optimal designs is greater than ever. This work presents an architecture that identifies trends between conflicting objectives (e.g. lifecycle cost and performance) and decision variables (e.g. orbit altitude and inclination) such that informed assessment can be made as to which design/s to take on for further analysis. The models within the architecture exploit analytic methods where possible, in order avoid computationally expensive numerical propagation, and achieve rapid convergence. Two mission cases are studied; the first is an Earth observation satellite and presents a trade-off between ground sample distance and revisit time over a ground target, given altitude as the decision variable. The second is a satellite with a generic scientific payload and shows a more involved trade-off, between data return to a ground station and cost of the mission, given variations in the orbit altitude, inclination and ground station latitude. Results of each case are presented graphically and it is clear that non-intuitive results are captured that would typically be missed using traditional, point-design methods, where only discrete scenarios are examined.     

An extensible on-board data handling software platform for pico satellites

Miniaturization techniques enable the realization of very small satellites with interesting capabilities in space science. The University of Würzburg contributed in the scope of the cubesat program with its own pico satellite UWE-1, which is in orbit since October 2005. Despite reliable and stable operation of the on-board data handling (OBDH) system during the UWE-1 mission, the successor UWE-2 will be equipped with a more sophisticated, modular and extensible OBDH system, which was designed to facilitate the further development of the UWE satellite platform. The OBDH system was designed for high reliability and stability, but with an easier extension capability. The modular structure of the new system thus supports potential transfer to other satellite platforms.     

卫星GPS组合姿态确定系统方案研究

采用ＧＰＳ定姿技术作为卫星高精度自主姿态确定系统的备份，可以提高系统可靠性。在小型和微小卫星上采用ＧＰＳ定姿技术，保证在满足重量、功耗和其它技术指标的条件下，姿态和轨道控制系统全面满足任务要求。本方案为探索当今姿态和轨道控制系统基本型的研究迈出了一步。     

The GANDER constellation for maritime dissaster mitigation

The development of sea state monitoring from polar-orbiting satellites has recently moved away from the concept of single, multi-sensor platform such as ERS-2, Topex/Poseidon or ENVISAT towards the design of a system that would allow frequent updates from a constellation of small satellites equipped with special-purpose radar altimeters. This new system, called GANDER for Global Altimeter Network Designed to Evaluate Risk, has attracted significant support from a number of important customer segments including the military.

This paper details the design of an altimeter for a Surrey small satellite, and illustrates the major system trade-offs that need to be made. Critical to the viability of the mission will be the development of a radar altimeter capable of operating successfully on a small satellite bus, within a limited volume and power budget. The mission design presents a number of key technological challenges, in order to permit a physically small antenna to be employed, and to minimise the pulse power. This can be achieved by advanced techniques, such as the delay Doppler altimeter concept, which emphasises the needs for high-speed on-board signal processing, phase linearity and pulse-to-pulse phase coherency.

The system design for the GANDER constellation is also described, illustrating how it not only offers a means for maritime disaster mitigation, but also can reduce shipping cost and time.     

基于模糊神经网络的小卫星任务自主调度设计

为了提高小卫星星务软件的自主化、智能化水平，提出一种基于模糊神经网络的小卫星任务自主调度的设计方法。该方法根据小卫星有效载荷和任务的需求，将小卫星的星务软件分解为若干个任务模块。同时，考虑到一些任务执行的紧前关系要求，将若干有紧前关系的任务模块划分为一个任务流程。以任务流程为单位，利用模糊神经网络构建任务流程自主调度决策系统。仿真实验结果表明，该决策系统能够根据小卫星的监测数据，以任务流程的自主调度为基础，最终实现对任务模块的动态自主调度。     

Coronal mass ejection (CME) activity of low mass M stars as an important factor for the habitability of terrestrial exoplanets. I. CME impact on expected magnetospheres of Earth-like exoplanets in close-in habitable zones

Low mass M- and K-type stars are much more numerous in the solar neighborhood than solar-like G-type stars. Therefore, some of them may appear as interesting candidates for the target star lists of terrestrial exoplanet (i.e., planets with mass, radius, and internal parameters identical to Earth) search programs like Darwin (ESA) or the Terrestrial Planet Finder Coronagraph/Inferometer (NASA). The higher level of stellar activity of low mass M stars, as compared to solar-like G stars, as well as the closer orbital distances of their habitable zones (HZs), means that terrestrial-type exoplanets within HZs of these stars are more influenced by stellar activity than one would expect for a planet in an HZ of a solar-like star. Here we examine the influences of stellar coronal mass ejection (CME) activity on planetary environments and the role CMEs may play in the definition of habitability criterion for the terrestrial type exoplanets near M stars. We pay attention to the fact that exoplanets within HZs that are in close proximity to low mass M stars may become tidally locked, which, in turn, can result in relatively weak intrinsic planetary magnetic moments. Taking into account existing observational data and models that involve the Sun and related hypothetical parameters of extrasolar CMEs (density, velocity, size, and occurrence rate), we show that Earth-like exoplanets within close-in HZs should experience a continuous CME exposure over long periods of time. This fact, together with small magnetic moments of tidally locked exoplanets, may result in little or no magnetospheric protection of planetary atmospheres from a dense flow of CME plasma. Magnetospheric standoff distances of weakly magnetized Earth-like exoplanets at orbital distances 相似文献   

An extensible on-board data handling software platform for pico satellites

Miniaturization techniques enable the realization of very small satellites with interesting capabilities in space science. The University of Würzburg contributed in the scope of the cubesat program with its own pico satellite UWE-1, which is in orbit since October 2005. Despite reliable and stable operation of the on-board data handling (OBDH) system during the UWE-1 mission, the successor UWE-2 will be equipped with a more sophisticated, modular and extensible OBDH system, which was designed to facilitate the further development of the UWE satellite platform. The OBDH system was designed for high reliability and stability, but with an easier extension capability. The modular structure of the new system thus supports potential transfer to other satellite platforms.     

ST-5微小卫星与星座及其空间飞行验证——为未来微小卫星的空间应用展现广阔前景

美国NASA于2006年3月22日成功发射三颗ST-5微小卫星,并组成星座,用于空间地磁观测。经过90天飞行演示,于6月20日顺利结束。演示验证很成功。卫星重25kg,功率24W具有通常卫星全部功能。卫星多项先进技术在演示中得到肯定,空间观测获得史无前例的数据。为此,文章介绍了ST-5微小卫星的先进技术和设计经验。ST-5将为今后微小卫星空间应用展现广阔前景。     

国外中继卫星对航天器交会对接的测控通信支持

中继卫星系统的天基测控通信是近代航天技术的重大突破,它能够有效地满足航天器交会对接的测控通信需要。文章分析了美国＂跟踪与数据中继卫星系统＂（TDRSS）和欧洲＂阿特米斯＂（ARTEMIS）中继卫星对＂自动转移飞行器＂（ATV）与＂国际空间站＂（ISS）交会对接任务的测控通信支持,总结了国外中继卫星系统支持航天器交会对接...     

微小卫星热控系统的研究现状及发展趋势

文章针对微小航天器研究现状和发展需求给热控系统设计带来的难点和挑战,从传热学和控制学两个角度,对近年来微小卫星热控领域出现的先进的热量收集、传输和排放装置展开论述;追踪了国内外学者提出的热控发展新的理论和方案。总之,开展各种智能、灵巧的航天器热控部件研究及针对高性能传热装置的控制策略研究是由微小卫星的结构布局和任务特点所决定的必然要求和发展趋势。     

A bistatic SAR mission for earth observation based on a small satellite

The authors present a new scientific space mission consisting of a satellite carrying a receiving- only SAR which receives the signal transmitted by the ENVISAT-1 SAR. The integration of ENVISAT-1 SAR and bistatic radar data offers an improved potentiality of surface classification, three-dimensional observation, and the opportunity of advanced scientific experiments in the field of bistatic scattering. The small satellite nominal orbit and the attitude manoeuvres are designed in order to maintain an adequate overlap between the two radar swaths along the whole orbit, taking into account the ENVISAT-1 attitude and pointing. A preliminary satellite design (2-year lifetime) is then performed to evaluate the orbit decay and to determine the appropriate orbit manoeuvres (every 4 days) to control the satellites relative phase. The numerical simulation shows that a spacecraft of about 584kg is able to meet the mission requirements.     

Orbit design for the Spektr-R spacecraft of the ground-space interferometer

In order to carry out tasks of the RadioAstron mission, a high-apogee orbit was designed. On average, the period of its satellite’s orbit around the Earth is 8.5 days with evolution due to gravitational perturbations produced by the Moon and the Sun. The perigee and apogee of this orbit vary within the limits 7500–70000 km and 270000–333000 km, respectively. The basic evolution of the orbit represents a rotation of its plane around the line of apsides. Over 3 years, the plane normal to the orbit draws on the celestial sphere an oval with a semi-major axis of about 150° and semi-minor axis of about 45°.     

Post mission life plan for FORMOSAT-2

This paper presents the enhancement in mission operations, the mission life state-of-health (SOH) trending analysis, and the post mission life plan of the FORMOSAT-2 (or FS2, Formosa satellite #2, was called ROCSAT-2, or RS2, Republic of China satellite #2, previously) during its five years mission life from 20 May 2004 to 20 May 2009. There are two payloads onboard FS2: a remote sensing instrument (RSI) with nadir ground sampling distance (GSD) of 2 m for panchromatic (PAN) and GSD of 8 m for multi-spectral (MS, 4 bands) as the primary payload, and an imager for sprite and upper atmospheric lightning (ISUAL) as the secondary payload. It was launched on 20 May 2004. The design life is 7 years while the mission life is 5 years. In other words, the end of mission life date of FS2 is 20 May 2009. Generally speaking, FS2 is still at very good condition in its SOH. Post mission life plan for FS2 consists of: the practice of orbit transfer for global coverage and better resolution, the development of gyroless attitude control, and the method for life extension. It is expected that the working life of FS2 can be extended 3–5 years.