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10~50MHz地基低频射电天文数字接收机及上位机软件研制
许丙强1; 白宇1; 路光1; 平劲松2,3; 王明远2,3; 杨文军4; 王震4; 严发宝1,5
2023
Source Publication地球物理学报
ISSN0001-5733
Volume66Issue:3Pages:891-904
Contribution Rank4
Abstract低频段(<50 MHz)射电观测,是研究射电爆发、恒星形成、宇宙初期状态的重要手段,而我国对该频段相关仪器研究较少.本文从关键器件选型、仿真与设计、接口和通讯、功能模块等方面,对组成地基低频射电观测系统的核心部件——数字接收机与上位机软件进行论述.数字接收机由采集卡和工控机构成,采集卡配置包含AD9265芯片和K7系列现场可编程门阵列(Field Programmable Gate Array, FPGA).数字接收机探测频率覆盖1~62.5 MHz,接收功率范围-78~-6 dBm,拥有先进的频率分辨率(15.3 kHz)和时间分辨率(0.5~32 ms).为满足射电观测显示与存储需求,研发了具有针对性的上位机软件解决方案.软件支持高速串行计算机扩展总线标准(Peripheral Component Interconnect express, PCIe)数据传输协议,支持实时频谱显示、数据存储和交互操作,具有全频带内强度图显示与图像自动保存功能.自主研制的数字接收机与上位机软件已成功应用于新疆奇台观测站低频(10~50 MHz)射电观测设备,该设备自2021年6月投入运行,捕获多次太阳射电暴事件.将观测结果与澳大利亚Learmonth观测设备对比分析,结果表明,新疆奇台站低频射电观测系统探测精度更为精细、探测频率更低,性能指标位于国际前列.系统后期可开展星-地协同观测,推动我国低频段射电研究.
Other AbstractRadio observation in low frequency band (<50 MHz) can be widely used to study the radio burst, star formation and the early evolution of the universe in the astronomical society. However, there is not enough research on the development of new instruments with better performance in this field in China. In this paper, we studied the core module of observing system, i. e. the digital receiver (including key device selection, simulation and design, interface and communication, and functional modules) and host computer software. The digital receiver is composed of acquisition card and industrial computer. The acquisition card is equipped with AD9265 chip and K7 series Field Programmable Gate Array (FPGA). The designed system works in the frequency range of 1 similar to 62. 5 MHz, with a dynamic range of -78 to -6 dBm. The frequency resolution is 15. 3 kHz and the time resolution ranges from 0. 5 to 32 ms. A software is then developed, which realizes Peripheral Component Interconnect express (PCIe) data transmission protocol, real-time spectrum display, data storage and interactive operation, and storage of full-band quicklook. The independently developed digital receiver and PC software have been successfully applied to low frequency (10 similar to 50 MHz) radio observation in Xinjiang Qitai Observation Station since June 2021. Several solar radio bursts have been captured. Compared with Learmonth's observation, the results show that the detection accuracy of low frequency radio observation system at Qitai station in Xinjiang is better with lower frequency limit and more fine structures. In the future, satellite-ground cooperative observation can be carried out to promote the research of low frequency radio in China.
Keyword低频射电 地基观测 数字接收机 太阳射电爆发
DOI10.6038/cjg2022Q0015
Indexed BySCI
Language英语
WOS IDWOS:000945003800003
CSCD IDCSCD:7423615
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6600
Collection射电天文研究室_行星科学研究团组
Corresponding Author严发宝
Affiliation1.山东大学空间科学研究院空间电磁探测技术实验室
2.中国科学院国家天文台射电部
3.中国科学院大学空间与天文学院
4.中国科学院新疆天文台
5.山东大学机电与信息工程学院
Recommended Citation
GB/T 7714
许丙强,白宇,路光,等. 10~50MHz地基低频射电天文数字接收机及上位机软件研制[J]. 地球物理学报,2023,66(3):891-904.
APA 许丙强.,白宇.,路光.,平劲松.,王明远.,...&严发宝.(2023).10~50MHz地基低频射电天文数字接收机及上位机软件研制.地球物理学报,66(3),891-904.
MLA 许丙强,et al."10~50MHz地基低频射电天文数字接收机及上位机软件研制".地球物理学报 66.3(2023):891-904.
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