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The LOFAR radio telescope detects its first pulsar

机译:LOFAR射电望远镜检测到其第一个脉冲星

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Using its first station of distributed radio antennas, the Low Frequency Array (LOFAR) radio telescope has successfully detected the pulsar PSR B0329+54. The measurement took 15 minutes on 14 June and used only six of the prototype high-band antennas recently installed in the eastern part of the Netherlands. The results demonstrate the technical performance of the antennas.rnLOFAR will be the largest radio telescope ever built, using a new concept based on a vast array of simple omni-directional antennas. The idea is to digitize the signals before sending them to a central digital processor where software will combine them to create the effect of a large conventional antenna. When finished, it will consist of 15000 small antennas, distributed to more than 77 stations in the north east of the Netherlands and nearby parts of Germany. The array will operate at the lowest frequencies that can be observed from Earth, at 10-240 MHz. Plans exist for the extension of the array beyond its initial 100 km scale, by building stations further into Germany and also in the UK, France, Sweden, Poland and Italy.
机译:低频阵列(LOFAR)射电望远镜使用其第一台分布式无线电天线,已成功检测到脉冲星PSR B0329 + 54。该测量在6月14日进行了15分钟,仅使用了最近安装在荷兰东部地区的6个原型高频带天线。结果证明了天线的技术性能。rnLOFAR将成为有史以来最大的射电望远镜,它将使用基于大量简单全向天线的新概念。想法是将信号数字化,然后再将其发送到中央数字处理器,在中央处理器中,软件会将它们组合在一起以产生大型常规天线的效果。完工后,它将由15000根小型天线组成,分布在荷兰东北部和德国附近地区的77多个站点。该阵列将在地球上可以观察到的最低频率(10-240 MHz)下运行。目前已经计划通过在德国,英国,法国,瑞典,波兰和意大利进一步建站,将阵列扩展到最初的100公里范围之外。

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    《CERN courier》 |2007年第8期|9|共1页
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