首页> 外文会议>Conference on Radio Telescopes 27-30 March 2000 Munich, Germany >Active adaptive antennas for radio astronomy; rsults for the RD program toward the square kilometer array
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Active adaptive antennas for radio astronomy; rsults for the RD program toward the square kilometer array

机译:射电天文有源自适应天线;研发计划的结果朝向平方千米阵列

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Various unique concepts are studied for the Square Kilometer Array expected to be operational between 2010 and 2015. We compare telescopes in operation to day with the SKA requirements and among these concepts, emphasize the acitve adaptive aperture antenna. This electronic concept for aperture synthesis has intrinsic capabilityes that may widen avenues of new astronomical research with SKA even further and is topic of active R&D within NFRA. Withing the program, technology demonstrators are built with increasing complexity. As describale side effect of the ongoing studies for SKA, new albiet smaller telescopes are coming into operation earlier. OF these, a new generation low frequency array to be operational in 2005 may result with close ties to the exploration of new technologies in our R&D program together with firm scientific push from the US and Holland. Experimence gained with this telescope are relevant for SKA's mainstream development and in particular the electronic array. Results of these and other research aspects of the R&D program are presented.
机译:针对预计在2010年至2015年之间运行的平方公里阵列,研究了各种独特的概念。我们将日常使用的望远镜与SKA要求进行了比较,在这些概念中,强调了自适应自适应孔径天线。这种用于孔径合成的电子概念具有内在的能力,可能会进一步扩大与SKA进行新天文学研究的途径,并且是NFRA内积极研发的主题。通过该程序,技术演示者的复杂性越来越高。由于SKA正在进行的研究有负面影响,因此,新型的albiet小型望远镜将更早投入使用。其中,新一代低频阵列将于2005年投入运营,这可能与我们研发计划中对新技术的探索以及美国和荷兰的坚定科学推动密切相关。使用该望远镜获得的经验与SKA的主流发展特别是电子阵列有关。介绍了R&D程序的这些以及其他研究方面的结果。

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