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1.
D. Koschny V. Dhiri K. Wirth J. Zender R. Solaz R. Hoofs R. Laureijs T.-M Ho B. Davidsson G. Schwehm 《Space Science Reviews》2007,128(1-4):167-188
ESA’s Rosetta mission was launched in March 2004 and is on its way to comet 67P/Churyumov-Gerasimenko, where it is scheduled
to arrive in summer 2014. It comprises a payload of 12 scientific instruments and a Lander. All instruments are provided by
Principal Investigators, which are responsible for their operations.
As for most ESA science missions, the ground segment of the mission consists of a Mission Operations Centre (MOC) and a Science
Operations Centre (SOC). While the MOC is responsible for all spacecraft-related aspects and the final uplink of all command
timelines to the spacecraft, the scientific operations of the instruments and the collection of the data and ingestion into
the Planetary Science Archive are coordinated by the SOC. This paper focuses on the tasks of the SOC and in particular on
the methodology and constraints to convert the scientific goals of the Rosetta mission to operational timelines. 相似文献
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在简要论述微波遥感定标技术工作特点的基础上,着重分析星载有源微波遥感定标技术基本原理和关键技术,比较了各种定标方法特点,提出了若干建议。 相似文献
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大迎角下导弹气动耦合控制系统分析 总被引:1,自引:0,他引:1
工程设计中,基于三通道自独立的前提来设计导弹控制器的常用方法,一般是将耦合项作为随机干扰来处理,这种方法不但具有一定的盲目性和不确定性,而且还丰厚明显的理论缺陷:耦合的存在改变了原系统的性能,严重时甚至会影响系统的稳定性。因此,只有当耦合影响很微弱时,这种方法才有实际应用价值。现分别从稳定裕度和气动参数两个方面,论述了气动交连耦合是造成大迎角飞行导弹控制系统不稳定的重要原因,并由此得出结论:对于大迎角下气动耦合强烈的导弹,其控制系统需考虑采用解耦控制,以便行这有效地变不稳定系统为稳定系统。 相似文献
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陈惠萍 《中国民航学院学报》1990,8(4):38-46
对湍流目标进行检测,是多卜勒效应在现代机载气象雷达中的应用。鉴于目前在新型机载气象雷达中普遍装备了湍流信号处理电路,本文就有关的湍流目标及其检测原理和方法作简要介绍。 相似文献
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以作者所开发的计算机考试系统为例,阐述了大二进制对象数据类型(BLOB)使用方法,包括将一个大对象(文本、图像、声音等)存入一个BLOB变量中、通过BLOB变量读写数据库中的大对象等内容。 相似文献
9.
Giammarco Cialone Andrea Gianfermo Alessandra Di Cecco Silvia Mari Santi Cassisi Fabio Santoni Fabrizio Piergentili 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):800-811
Binary or multiple stellar systems, constituting almost a third of the content of the Milky Way, represent a high priority astronomical target due to their repercussions on the stellar dynamical and evolutionary parameters. Moreover the spectral study of such class of stars allows to better constrain the evolutionary theories of the Galactic stellar populations. By resolving the members of stellar systems through photometric observations we are able to perform more detailed measurements to infer their mass. In this paper we investigate the feasibility of a cubesat based mission including an optical payload to directly optically discriminate the members of a selected sample of binary systems. The scientific targets, consisting 11?M class dwarf stars binary systems, have been extracted from the already studied Riaz catalogue. These subset has been selected considering the star distance, the members angular separation, and the distance from the Galactic plane (due to limit the background and foreground contamination). The satellite concept is based on a 6 unit Cubesat embedding some commercial off the shelf components and an ad hoc designed optical payload occupying almost 4 units. The optical configuration has been chosen in order to fit the angular resolution requirements, as derived from the target characteristics. Moreover, according to the optical analysis and the computed field of view some requirements on the attitude control system have been inferred and fulfilled by the component selection. The paper is organized as in the following: a brief scientific introduction is made; consequently the project is described with particular attention to the optical design and the standard sub-systems; finally the conclusions are drawn and the future perspectives are investigated. 相似文献
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