Suppr超能文献

用于车辆导航的射电脉冲星信号的到达时间(TOA)和信噪比(SNR)准确性研究。

Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation.

作者信息

Kabakchiev Hristo, Behar Vera, Kabakchieva Dorina, Kisimov Valentin, Stefanova Kamelia

机构信息

Faculty of Mathematics and Informatics, Sofia University, 1164 Sofia, Bulgaria.

IICT, 1113 Sofia, Bulgaria.

出版信息

Sensors (Basel). 2023 Aug 7;23(15):7010. doi: 10.3390/s23157010.

Abstract

It is known that X-ray and gamma-ray pulsars can only be observed by spacecraft because signals from these pulsars are impossible to be detected on the Earth's surface due to their strong absorption by the Earth's atmosphere. The article is devoted to the theoretical aspects regarding the development of an autonomous radio navigation system for transport with a small receiving antenna, using radio signals from pulsars, similar to navigation systems for space navigation. Like GNSS systems (X-ray and radio), they use signals from four suitable pulsars to position the object. These radio pulsars (out of 50) are not uniformly distributed but are grouped in certain directions (at least 6 clusters can be determined). When using small antennas (with an area of up to tens of square meters) for pulsar navigation, the energy of the pulsar signals received within a few minutes is extremely insufficient to obtain the required level of SNR at the output of the receiver to form TOA estimation, ensuring positioning accuracy up to tens of kilometers. This is one of the scientific tasks that is solved in the paper by studying the relationship between the SNR of the receiver output, which depends on the size of the antenna, the type of signal processing, and the magnitude of the TOA accuracy estimate. The second scientific task that is solved in the paper is the adaptation of all the possible approaches and algorithms suggested in the statistical theory of radars in the suggested signal algorithm for antenna processing and to evaluate the parameters of the TOA and DS pulsar signals, in order to increase the SNR ratio at the receiver output, while preserving the dimensions of the antenna. In this paper, the functional structure of signal processing in a pulsar transport navigation system is proposed, and the choice of the observed second and millisecond pulsars for obtaining a more accurate TOA estimate is discussed. The proposed estimates of positioning accuracy (TOA only, no phase) in an autonomous pulsar vehicle navigation system would only be suitable for the navigation of large vehicles (sea, air, or land) that do not require accurate navigation at sea, air, or desert. Large-sized antennas with an area of tens of square meters to hundreds of square meters can be installed in such vehicles.

摘要

众所周知,X射线和伽马射线脉冲星只能通过航天器进行观测,因为这些脉冲星发出的信号在地球表面会被大气层强烈吸收,从而无法被探测到。本文致力于研究一种用于小型接收天线运输工具的自主无线电导航系统的理论方面,该系统利用脉冲星的无线电信号,类似于太空导航的导航系统。与全球导航卫星系统(X射线和无线电)一样,它们使用来自四颗合适脉冲星的信号来定位目标。这些射电脉冲星(在50颗中)并非均匀分布,而是在某些方向上成组分布(至少可以确定6个星团)。当使用小型天线(面积达数十平方米)进行脉冲星导航时,在几分钟内接收到的脉冲星信号能量极其不足,无法在接收机输出端获得所需的信噪比水平以形成到达时间(TOA)估计,从而确保定位精度达到数十公里。这是本文通过研究接收机输出信噪比之间的关系来解决的科学任务之一,该信噪比取决于天线尺寸、信号处理类型以及到达时间精度估计的大小。本文解决的第二个科学任务是在天线处理的建议信号算法中采用雷达统计理论中提出的所有可能方法和算法,并评估到达时间和色散(DS)脉冲星信号的参数,以便在保持天线尺寸的同时提高接收机输出端的信噪比。本文提出了脉冲星运输导航系统中信号处理的功能结构,并讨论了选择观测到的秒脉冲星和毫秒脉冲星以获得更精确到达时间估计的问题。自主脉冲星车辆导航系统中提出的定位精度估计(仅到达时间,无相位)仅适用于不需要在海上、空中或沙漠进行精确导航的大型车辆(海上、空中或陆地)。在这类车辆中可以安装面积从数十平方米到数百平方米的大型天线。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a153/10422519/40cefff394d9/sensors-23-07010-g001.jpg

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验