首页> 外文期刊>Optics Communications: A Journal Devoted to the Rapid Publication of Short Contributions in the Field of Optics and Interaction of Light with Matter >Analysis of telescope array receivers for deep-space inter-planetary optical communication link between Earth and Mars
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Analysis of telescope array receivers for deep-space inter-planetary optical communication link between Earth and Mars

机译:地球与火星之间深空行星际光通信链路的望远镜阵列接收机分析

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Optical communication technology shows promising prospects to fulfill the large bandwidth communication requirements of future deep-space exploration missions that are launched by NASA and various other international space agencies. At Earth, a telescope with a large aperture diameter is required to capture very weak optical signals that are transmitted from distant planets and to support large bandwidth communication link. A single large telescope has the limitations of cost, single point failure in case of malfunction, difficulty in manufacturing high quality optics, maintenance, and trouble in providing communication operations when transmitting spacecraft is close to the Sun. An array of relatively smallersized telescopes electrically connected to form an aggregate aperture area equivalent to a single large telescope is a viable alternative to a monolithic gigantic aperture. In this paper, we present the design concept and analysis of telescope array receivers for an optical communication link between Earth and Mars. Pulse-position modulation (PPM) is used at the transmitter end and photon-counting detectors along with the direct-detection technique are employed at each telescope element in the array. We also present the optimization of various system parameters, such as detector size (i.e., receiver field of view), PPM slot width, and the PPM order M, to mitigate the atmospheric turbulence and background noise effects, and to maximize the communication system performance. The performance of different array architectures is evaluated through analytical techniques and Monte-Carlo simulations for a broad range of operational scenarios, such as, Earth-Mars conjunction, Earth-Mars opposition, and different background and turbulence conditions. It is shown that the performance of the telescope array-based receiver is equivalent to a single large telescope; and as compared to current RF technology, telescope array-based optical receivers can provide several orders of magnitude greater data rates for deep-space communication with Mars.
机译:光通信技术显示出有望满足由美国国家航空航天局(NASA)和其他各种国际空间机构发起的未来深空探测任务的大带宽通信要求的前景。在地球上,需要具有大孔径直径的望远镜来捕获从遥远的行星发出的非常微弱的光信号,并支持大带宽通信链路。单个大型望远镜的成本有限,在出现故障时会出现单点故障,难以制造高质量的光学元件,维修以及在发射航天器接近太阳时难以进行通信操作。电连接以形成等效于单个大型望远镜的总孔径区域的相对较小尺寸的望远镜阵列是整体式巨大孔径的可行替代方案。在本文中,我们介绍了用于地球与火星之间的光通信链路的望远镜阵列接收器的设计概念和分析。发射器端使用脉冲位置调制(PPM),阵列中的每个望远镜元件均采用光子计数检测器以及直接检测技术。我们还介绍了各种系统参数的优化,例如检测器尺寸(即接收器视场),PPM缝隙宽度和PPM阶数M,以减轻大气湍流和背景噪声的影响,并最大化通信系统的性能。通过分析技术和蒙特卡洛模拟评估了各种阵列架构的性能,以评估广泛的运行场景,例如地球与火星的合相,地球与火星的对立以及不同的背景和湍流条件。结果表明,基于望远镜阵列的接收器的性能相当于一台大型望远镜。与目前的RF技术相比,基于望远镜阵列的光接收器可以为与火星进行深空通信提供更高的数据量级。

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