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ORIGINAL RESEARCH article

Front. Astron. Space Sci.
Sec. Astronomical Instrumentation
Volume 11 - 2024 | doi: 10.3389/fspas.2024.1420066

General Heterogeneous Real-Time Baseband Backend System Scheme Applied to QTT Based on RFSoC+GPU

Provisionally accepted
Qingsong Zhang Qingsong Zhang Maozheng Chen Maozheng Chen *Jian Li Jian Li *
  • Xinjiang Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences (CAS), Ürümqi, China

The final, formatted version of the article will be published soon.

    This paper proposes a heterogeneous real-time baseband astronomical backend solution centered on RFSoC and combined GPU. The solution implemented the integration of the high-performance, completely configurable RF signal link to digitize, process, and transmit increasingly massive radio astronomy signals and provided a highly flexible and scalable scheme for the QTT backend. The RFSoC-based integration RF pre-processing front-end directly digitizes dual-polarization signals at the sampling rate of 2048MHz and converts them to dual-16-channel data streams for parallel mixing and polyphase decimation filtering. The generated baseband data with 256MHz center frequency and 100MHz bandwidth is packaged and output to the GPU server through the 100GbE Interface. Complete processes of direct RF sampling, pre-processing, and high-speed transmission are implemented at the receiver. The GPU server executes real-time post-processing at the remote end. The dynamic configuration of two observation modes can be achieved with frequency resolutions of 3.051kHz and 0.763kHz. The H2CO absorption line observations with the Nanshan 26-meter radio telescope verified the system's performance and the design's rationality. This paper explores and confirms the RFSoC's applicability on the backend. The flexible and efficient QTT backend scheme was planned based on the proposed real-time baseband pattern by expanding multi-RFSoC and GPU computing nodes.

    Keywords: Astronomical backend, QTT, RFSoC, RF signal link, heterogeneous

    Received: 19 Apr 2024; Accepted: 27 Jun 2024.

    Copyright: © 2024 Zhang, Chen and Li. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

    * Correspondence:
    Maozheng Chen, Xinjiang Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences (CAS), Ürümqi, China
    Jian Li, Xinjiang Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences (CAS), Ürümqi, China

    Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.