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PULSARPLANE: A FEASIBILITY STUDY FOR MILLISECOND RADIO PULSAR NAVIGATION

机译:脉冲平面:微妙的无线电脉冲导航的可行性研究

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Stars have been used -in what is called celestial navigation- since thousands of years by mankind. Stars were observed with navigational tools such as the sextant and its predecessors from the 16th century and in the modern times with star trackers. Celestial navigation was used extensively in aviation until the 1960s, and in marine navigation until quite recently. While outside the Earth's atmosphere, intercontinental ballistic missiles (ICBMs) are believed to continue to utilize celestial navigation to verify their flight path steered by incrtial navigation systems: the main reason being that signals from Global Navigation Satellites Systems could be jammed at times the use of ICBMs is most critical. Recently the interest in celestial navigation has sparked again with an emphasis on deep space navigation using pulsars. Pulsars arc fast rotating neutron stars that emit electromagnetic radiation, which is received anywhere in our solar system as a scries of very stable fast periodic pulses with periods in between milliseconds and up to 10 seconds. Pulsars can provide stable frequency standards and the variance of the millisecond pulsars -the most stable astronomical clocks- is comparable to that of atomic clocks. Pulses, emitted by a pulsar in a wide frequency range, can be received at regular intervals corresponding to a beam (or beams) being emitted from a rotating neutron star. The pulsar emits radiowaves and particles along its magnetic axis. From a far distance the reception of the electromagnetic waves can be compared with that of a light house. A number of studies have been performed on navigating using pulsar signals;the first study was performed by NASA in 1974 focused on radio pulsars, but in later years most attention was given to X-ray pulsars. Radio pulsar navigation - utilizing signals which could be detected on Earth - has not received much attention, since the signal strength of radio pulsars was deemed too weak to be useful. Advances in signal processing, analog/RF circuit design as well as antenna design, however, could enable faster and more accurate detection of pulsar signals, using a smaller antenna size. The objective of this paper is to investigate the feasibility of a navigation system inside the Earth's atmosphere using signals from millisecond radio pulsars. The study is part of the research project PulsarPlane under the European 7th Framework Programme as a pioneering idea, i.e. technologies and concepts that have the potential to bring step changes in the second half of this century and beyond.
机译:自从人类数千年以来,就一直使用恒星-在所谓的天体导航中。使用导航工具(例如16世纪的六分体及其前身)和现代的恒星追踪器观测恒星。直到1960年代,天体导航才在航空领域得到广泛应用,直到最近,海天导航也一直在海洋中使用。虽然洲际弹道导弹(ICBM)不在地球大气层中,但仍会继续利用天体导航来验证由非特异导航系统控制的飞行路径:主要原因是全球导航卫星系统的信号有时可能会被干扰洲际弹道导弹至关重要。最近,对天体导航的兴趣再次引起关注,重点是使用脉冲星的深空导航。脉冲星是快速旋转的中子星,它们发出电磁辐射,并以非常稳定的快速周期脉冲(在毫秒到10秒之间的周期)的形式在我们的太阳系中的任何地方接收。脉冲星可以提供稳定的频率标准,而毫秒级脉冲星的变化(最稳定的天文钟)可与原子钟相媲美。脉冲星在宽频率范围内发出的脉冲可以以规则的间隔接收,该间隔对应于从旋转中子星发出的一个或多个波束。脉冲星沿着其磁轴发射无线电波和粒子。从远处可以将电磁波的接收与灯塔的接收进行比较。在使用脉冲星信号导航方面已经进行了许多研究; 1974年,美国国家航空航天局(NASA)进行了第一项研究,重点是射电脉冲星,但是在随后的几年中,人们对X射线脉冲星的关注最多。无线电脉冲星导航-利用可以在地球上检测到的信号-并未引起足够的重视,因为无线电脉冲星的信号强度被认为太弱而无用。但是,信号处理,模拟/ RF电路设计以及天线设计方面的进步可以使用更小的天线尺寸实现更快,更准确的脉冲星信号检测。本文的目的是研究使用毫秒无线电脉冲星产生的信号在地球大气内部导航系统的可行性。这项研究是欧洲第七框架计划下的PulsarPlane研究项目的一部分,是一个开创性的想法,即具有可能在本世纪下半叶及以后发生重大变化的技术和概念。

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