pith. sign in

arxiv: 2604.24014 · v1 · submitted 2026-04-27 · 🌌 astro-ph.IM

The Operation Control System for the Tianlai Experiment

Pith reviewed 2026-05-08 01:38 UTC · model grok-4.3

classification 🌌 astro-ph.IM
keywords Tianlai experimentremote control system21cm intensity mappingoperation controlelectromagnetic interferenceremote observing stationLAN network
0
0 comments X

The pith

The Tianlai experiment uses a local network for remote secure control of its radio array to reduce on-site staffing and travel.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The authors present the design of an operation control system for the Tianlai 21cm intensity mapping experiment at a remote site chosen for its clean electromagnetic environment. Devices connect through a local area network so that operators can log in securely from elsewhere and issue commands to manage power switches, steer dish antennas, adjust analog and digital components, and run the full array. The design stresses online access, simplicity, flexibility, strict limits on electromagnetic interference, and security features. This approach aims to cut the human effort and costs of keeping the array running while protecting data quality.

Core claim

We have designed the Tianlai operation control system to be remotely controllable from the start. All devices sit on a local area network, and one controls them by securely logging into a server on that network to issue commands. The system handles the power switch, the steering of the dish antennas, the analog and digital parts of the array, and overall array operation. Emphasis is placed on online accessibility, simplicity, flexibility, electromagnetic interference control, and security.

What carries the argument

A local area network that links the array devices, with remote secure login to a central server used to send commands for power, antenna steering, and component operation.

Load-bearing premise

The local area network and remote login can be implemented without adding electromagnetic interference or security vulnerabilities at the remote site.

What would settle it

Extended remote operation of the Tianlai array that produces 21 cm data with no detectable rise in electromagnetic noise and no successful unauthorized access to the control server.

Figures

Figures reproduced from arXiv: 2604.24014 by Fengquan Wu, Jixia Li, Shijie Sun, Xuelei Chen, Yougang Wang.

Figure 1
Figure 1. Figure 1: Location of the station house, the existing antenna site (Site A), future FRB outriggers (Site B, C), and global view at source ↗
Figure 2
Figure 2. Figure 2: The various parts and signal flow of the Tianlai experiment. view at source ↗
Figure 3
Figure 3. Figure 3: A schematic of the local area network and the various components. view at source ↗
Figure 4
Figure 4. Figure 4: Various devices and servers are connected to PDUs which are remotely manageable through the LAN. view at source ↗
Figure 5
Figure 5. Figure 5: Main power control schematic in antenna site. view at source ↗
Figure 6
Figure 6. Figure 6: GUI of the dish antenna controller these are deployed in the login server. Each of the cylinder and dish arrays also has both a correlator to generate interferometric visibilities, and an FRB backend to search for FRBs. Due to different hardware architectures, each of these 4 digital backend has its own control server. Below, each of these programs are presented. 6.1 Channel Equalization While all signal c… view at source ↗
Figure 7
Figure 7. Figure 7: Local oscillator program logic. RS-232 protocol. This socket is also connected to the 32p SPS. We developed the program lo.py to adjust the frequency and signal output level of the LO. This program runs on the login server, which connects to the serial port server through LAN, and then the serial server forwards the command to the LO. Using lo.py, we can check current setting, set the LO frequency and atte… view at source ↗
Figure 8
Figure 8. Figure 8: The program logic of the automatic observation. view at source ↗
Figure 10
Figure 10. Figure 10: Dish correlator program logic. data, meta parameters such as the frequency value, site information, CNS information, etc. are also saved in the attributes of the HDF5. The Tianlai dish correlator backend is controlled by the program dev trigger 32chn.py, which is run on the control server of the dish correlator as shown in view at source ↗
Figure 9
Figure 9. Figure 9: Program logic for cylinder correlator. the GPU server are working properly. If everything is Okay, one can finally starts the observation by running the script roach vis 192ch.py. Each GPU server processes the correlation data for four fixed frequency channels. The data of the same frequency channel are sent to the same UDP port in the control server. In the program roach vis 192ch.py, as shown in view at source ↗
Figure 11
Figure 11. Figure 11: Logos drawn by AI. Fengquan Wu leads the design and construction of the Tianlai systems, Fengquan Wu, Shijie Sun and Yougang Wang deployed the devices and instruments. Xuelei Chen is the leader of the Tianlai project and made detailed revision of the paper. All authors read and approved the final manuscript. SOFTWARE AVAILABILITY The software described in this paper is available freely from the authors up… view at source ↗
read the original abstract

The Tianlai 21cm intensity mapping experiment is located at the Hongliuxia Observing Station, which is a remote site with excellent electromagnetic environment. To facilitate the operation of the Tianlai experiment while reducing the required human power and travel cost, we have designed the system to be remotely controllable from the start. In this paper, we present the basic design of the operation control system, including the control network, and the controlling mechanisms for the power switch, the steering of the dish antenna, the analog and digital components of the array, and the operation of the array. In the design of this system of operation control, we emphasize the following points: online accessible, simplicity, flexibility, strict control of electromagnetic interference (EMI) and security. The various devices are connected in a local area network (LAN), and one can control them remotely by securely logging into a server on the LAN and issue commands. We describe the functions of the programs designed for the control. Similar design and the various hardware and software components may also be applicable or of reference value to other remote observing stations.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 3 minor

Summary. The paper describes the design of an operation control system for the Tianlai 21cm intensity mapping experiment at the remote Hongliuxia site. It outlines a LAN-based architecture allowing secure remote login to a central server for issuing commands, along with dedicated control programs for power switches, dish antenna steering, analog/digital array components, and overall array operations. The design prioritizes online accessibility, simplicity, flexibility, strict EMI control, and security to minimize on-site human presence and travel costs.

Significance. If the described architecture functions as intended, it would enable cost-effective remote operation of a sensitive radio astronomy array while maintaining low EMI, a key requirement for 21cm observations. The emphasis on simplicity and flexibility could make the approach reusable at other isolated observing stations. As a design paper, its value lies in providing a concrete reference architecture rather than new measurements or proofs; the lack of implementation metrics or validation data confines its impact to the conceptual and methodological level.

major comments (1)
  1. [Control network and remote access descriptions] The central claim that the system was 'designed from the start' with strict EMI control is load-bearing, yet the manuscript gives only high-level descriptions of the LAN topology and remote-login server without specifying cable shielding, filtering, grounding, or device placement strategies that would prevent network hardware from introducing EMI (see the sections on control network and hardware control programs).
minor comments (3)
  1. A block diagram or schematic of the LAN topology and server connections would substantially improve clarity of the remote-access architecture.
  2. The descriptions of the control programs list functions but omit example command sequences, pseudocode, or flowcharts that would illustrate how simplicity and flexibility are achieved in practice.
  3. No references are provided to comparable remote-control systems used at other radio observatories, which would help situate the design choices.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for their careful reading of the manuscript and constructive feedback. We address the single major comment below and will incorporate the suggested clarifications in a revised version.

read point-by-point responses
  1. Referee: The central claim that the system was 'designed from the start' with strict EMI control is load-bearing, yet the manuscript gives only high-level descriptions of the LAN topology and remote-login server without specifying cable shielding, filtering, grounding, or device placement strategies that would prevent network hardware from introducing EMI (see the sections on control network and hardware control programs).

    Authors: We agree that the current description of EMI mitigation remains high-level and that additional specifics would better substantiate the design claim and increase the paper's utility as a reference. In the revised manuscript we will expand the control network and hardware control program sections to detail the concrete measures employed, including use of shielded cables, grounding and filtering at interfaces, and device placement choices intended to minimize EMI from network hardware. revision: yes

Circularity Check

0 steps flagged

No significant circularity; purely descriptive design paper

full rationale

The paper presents a descriptive account of the Tianlai experiment's operation control system architecture, including LAN topology, remote login mechanisms, and control programs for power, antennas, and array components. No derivations, equations, predictions, or fitted parameters appear anywhere in the text. The central claim—that the system was designed with emphases on remote accessibility, simplicity, flexibility, EMI control, and security—is supported directly by the design description itself rather than by any reduction to prior inputs, self-citations, or self-definitional steps. No load-bearing self-citation chains or uniqueness theorems are invoked. This is a standard engineering design paper whose content is self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

No mathematical models, parameters, or new entities; this is an engineering design description.

pith-pipeline@v0.9.0 · 5494 in / 921 out tokens · 50213 ms · 2026-05-08T01:38:34.322052+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

67 extracted references · 13 canonical work pages

  1. [1]

    Chen, X. L. 2012. The Tianlai Project: a 21CM Cosmology Experiment.International Journal of Modern Physics Conference Series,12, 256–263

  2. [2]

    D., Wang, X., & Chen, X

    Xu, Y. D., Wang, X., & Chen, X. L. 2015. Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array.The Astrophysical Journal,798(1), 40

  3. [4]

    Yan, Z.-s., Ye, Y., & Zhang, Y. 2025. Overview of the telescope observation management and con- trol system bus. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.3076404

  4. [5]

    Wang, J., Luo, M., Wu, W., et al. 2013. Study of central control system for FAST.Experimental Astronomy, 36(3), 569–589

  5. [6]

    C., & Mutel, R

    Downey, E. C., & Mutel, R. L. 1996. The University of Iowa Automated Telescope Facility. In Astronomical Society of the Pacific Conference Series

  6. [7]

    J., Epand, D., Bresina, J., et al

    Boyd, L. J., Epand, D., Bresina, J., et al. 1993. Automatic Telescope Instruction Set 1993. International Amateur-Professional Photoelectric Photometry Communications,52, 23

  7. [8]

    Kong, D.-Q., Wang, S.-G., Wang, J.-Q., et al. 2014. A new calibration model for pointing a radio telescope that considers nonlinear errors in the azimuth axis. Research in Astronomy and Astrophysics,14(6), 733– 740

  8. [9]

    Tong, L., Sun, Y., Yang, X., et al. 2024. Design and application of an autonomous Master Control System for a multi-layer magnetic and helioseismic telescope. Astronomical Techniques and Instruments,1(3), 187– 196

  9. [10]

    Huang, Y., Hao, L., Lee, K., et al. 2024. An observation control system for radio telescopes based on Python and C++ languages.Astronomical Techniques and Instruments,1(6), 307–315

  10. [11]

    Wang, N., Xu, Q., Ma, J., et al. 2023. The Qitai radio telescope.Science China Physics, Mechanics, and Astronomy,66(8), 289512

  11. [12]

    Zhang, D., Zhao, R.-B., Yan, Z., et al. 2023. Distributed Control Software for the Active Surface System of Tian-ma Radio Telescope.Research in Astronomy and Astrophysics,23(11), 115024

  12. [13]

    Dong, J., Jin, H., Ye, Q., et al. 2016. The active surface control system for the Tian Ma Telescope. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2230560

  13. [14]

    Jiang, P., Yue, Y., Gan, H., et al. 2019. Commissioning progress of the FAST.Science China Physics, Mechanics, and Astronomy,62(5), 959502

  14. [15]

    Li, H., & Jiang, P. 2020. An open-loop control algorithm of the active reflector system of FAST. Research in Astronomy and Astrophysics,20(5), 065

  15. [16]

    YANG, F., WANG, M., DONG, L., et al. 2023. Design of feed switching system for large aperture fully movable radio telescope.Chinese Journal of Engineering Design,30(5), 617–625

  16. [17]

    Xu, Q., Yi, L., Li, L., et al. 2018. A rapid feed switching mechanism design for NSRT. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2309941

  17. [18]

    Prestage, R. M. 2006. The Green Bank Telescope. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.670472

  18. [19]

    Liu, F., He, J., Chen, Z., et al. 2013. Design of an Ethernet Based Control System for the CSRH Antenna Arrays.Astronomical Research and Technology,10, 99

  19. [20]

    Liu, F., Yan, Y., Wang, W., et al. 2019. A dig- ital correlation receiver for the Mingantu Spectral Radioheliograph.Publications of the Astronomical Society of Australia,36, e043

  20. [21]

    Deng, X., Wu, W., Luo, M., et al. 2012. Real time control system of Active Reflector of FAST. DOI: 10.1109/RTC.2012.6418102

  21. [22]

    Shen, T.-C., Galeas, P., Carrasco, S., et al. 2022. EtherCAT as an alternative of the next generation real-time control system for telescopes. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2629232

  22. [23]

    J., Bridger, A., Chaudhuri, S

    Williams, S. J., Bridger, A., Chaudhuri, S. R., et al

  23. [24]

    In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

    The SKA observation control system. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2231770

  24. [25]

    Chiozzi, G., Gustafsson, B., Jeram, B., et al

  25. [26]

    In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

    CORBA-based Common Software for the ALMA project. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.461036

  26. [27]

    Huang, Y., Wu, X.-P., Zheng, Q., et al. 2016. The radio environment of the 21 Centimeter Array: RFI detection and mitigation.Research in Astronomy and Astrophysics,16(2), 36. Astronomical Techniques and Instruments,0(0), 0–1, 202515

  27. [28]

    Zheng, Q., Wu, X.-P., Johnston-Hollitt, M., et al

  28. [29]

    Radio Sources in the NCP Region Observed with the 21 Centimeter Array.The Astrophysical Journal,832(2), 190

  29. [30]

    Yan, Y., Chen, Z., Wang, W., et al. 2021. Mingantu Spectral Radioheliograph for Solar and Space Weather Studies.Frontiers in Astronomy and Space Sciences,8, 20

  30. [31]

    Deng, Y., Wang, D., Hua, J., et al. 2025. The Overview and Trial Observations of AIMS.Research in Astronomy and Astrophysics,25(7), 075020

  31. [32]

    X., Zuo, S

    Li, J. X., Zuo, S. F., Wu, F. Q., et al. 2020. The Tianlai Cylinder Pathfinder array: System func- tions and basic performance analysis.Science China Physics, Mechanics, and Astronomy,63(12), 129862

  32. [33]

    Q., Li, J

    Wu, F. Q., Li, J. X., Zuo, S. F., et al. 2021. The Tianlai dish pathfinder array: design, operation, and performance of a prototype transit radio interferome- ter.Monthly Notices of the RAS,506(3), 3455–3482

  33. [34]

    Q., Chen, Z

    Liu, T., Wu, F. Q., Chen, Z. P., et al. 2014. Design of a wideband feed for the Tianlai project proceedings of the XXXIst URSI general assembly and scientific symposium to be held in Beijing, China (CIE), August 17–23, 2014. DOI:10.1109/URSI- GASS.2014.6930029

  34. [35]

    P., Wang, R

    Chen, Z. P., Wang, R. L., Peterson, J., et al

  35. [36]

    In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

    Design and analysis of a large cylinder an- tenna array in Tianlai. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2232570

  36. [37]

    J., Anderson, C

    Cianciara, A. J., Anderson, C. J., Chen, X. L., et al

  37. [38]

    Simulation and Testing of a Linear Array of Modified Four-Square Feed Antennas for the Tianlai Cylindrical Radio Telescope.Journal of Astronomical Instrumentation,6(3), 1750003–40

  38. [39]

    H., Wang, Q

    Niu, C. H., Wang, Q. X., MacMahon, D., et al. 2019. The design and implementation of a ROACH2+GPU based correlator on the Tianlai dish array.Research in Astronomy and Astrophysics,19(7), 102

  39. [40]

    X., Zhang, K., et al

    Wang, Z., Li, J. X., Zhang, K., et al. 2024. Design and implementation of a scalable correlator based on ROACH2 + GPU cluster for tianlai 96-dual- polarization antenna array.Frontiers in Astronomy and Space Sciences,11, 1407870

  40. [41]

    F., Ansari, R., et al

    Zhang, J., Zuo, S. F., Ansari, R., et al. 2016. Sky re- construction for the Tianlai cylinder array.Research in Astronomy and Astrophysics,16(10), 158

  41. [42]

    F., Pen, U

    Zuo, S. F., Pen, U. L., Wu, F. Q., et al

  42. [43]

    An Eigenvector-Based Method of Radio Array Calibration and Its Application to the Tianlai Cylinder Pathfinder.The Astronomical Journal, 157(1), 34

  43. [44]

    F., Li, J

    Zuo, S. F., Li, J. X., Li, Y. C., et al. 2021. Data pro- cessing pipeline for Tianlai experiment.Astronomy and Computing,34, 100439

  44. [45]

    Phan, A., Das, S., Stebbins, A., et al. 2022. AlgoSCR: an algorithm for solar contamination removal from radio interferometric data.Monthly Notices of the RAS,512(3), 3520–3537

  45. [46]

    Perdereau, O., Ansari, R., Stebbins, A., et al

  46. [47]

    Monthly Notices of the RAS,517(3), 4637–4655

    The Tianlai dish array low-z surveys forecasts. Monthly Notices of the RAS,517(3), 4637–4655

  47. [48]

    F., Wu, F

    Yu, K. F., Wu, F. Q., Zuo, S. F., et al. 2023. A Simulation of Calibration and Map-making Errors of the Tianlai Cylinder Pathfinder Array.Research in Astronomy and Astrophysics,23(10), 105008

  48. [49]

    F., Zuo, S

    Yu, K. F., Zuo, S. F., Wu, F. Q., et al

  49. [50]

    Application of Regularization Methods in the Sky Map Reconstruction of the Tianlai Cylinder Pathfinder Array.Research in Astronomy and Astrophysics,24(2), 025002

  50. [51]

    J., Ansari, R., et al

    Das, S., Anderson, C. J., Ansari, R., et al. 2018. Progress in the construction and testing of the Tianlai radio interferometers. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. DOI:10.1117/12.2313031

  51. [52]

    F., Liu, W., et al

    DAI, C., ZUO, S. F., Liu, W., et al. 2019. A Method to Detect Radio Frequency Interference Based on Convolutional Neural Networks. In Astronomical Society of the Pacific Conference Series

  52. [53]

    Y., Liu, J

    Zhang, J. Y., Liu, J. X., Wu, F. Q., et al

  53. [54]

    Beam Measurements of the Tianlai Dish Radio Telescope Using an Unmanned Aerial Vehicle [Antenna Applications Corner].IEEE Antennas and Propagation Magazine,63(6), 98–109

  54. [55]

    2025, arXiv e-prints, arXiv:2508.01413 4

    Li, J. X., Suo, N. B., Xu, S. Z., et al. 2025. Measurement of the Primary Beam of the Tianlai Cylindrical Antenna Using an Unmanned Aerial Vehicle.arXiv e-prints, , arXiv:2508.01413

  55. [56]

    X., Wu, F

    Li, J. X., Wu, F. Q., Sun, S. J., et al. 2021. Reflections and standing waves on the Tianlai cylinder array. Research in Astronomy and Astrophysics,21(3), 059

  56. [57]

    J., Li, J

    Sun, S. J., Li, J. X., Wu, F. Q., et al. 2022. The Electromagnetic Characteristics of the Tianlai Cylindrical Pathfinder Array.Research in Astronomy and Astrophysics,22(6), 065020

  57. [58]

    Kwak, J., Podczerwinski, J., Timbie, P., et al

  58. [59]

    16www.ati.ac.cn

    The Effects of the Local Environment on a Compact Radio Interferometer I: Cross-Coupling in the Tianlai Dish Pathfinder Array.Journal of Astronomical Instrumentation,13(1), 2450002. 16www.ati.ac.cn

  59. [60]

    F., Sun, S

    Liu, Y. F., Sun, S. J., Yu, K. F., et al. 2025. Beamforming in Interferometer Arrays with Cross- couplings.arXiv e-prints, , arXiv:2510.10067

  60. [61]

    J., Deng, F

    Yu, Z. J., Deng, F. R., Sun, S. J., et al. 2022. A Fast Radio Burst Backend for the Tianlai Dish Pathfinder Array.Research in Astronomy and Astrophysics, 22(12), 125007

  61. [62]

    J., Deng, F

    Yu, Z. J., Deng, F. R., Sun, S. J., et al

  62. [63]

    The FRB-searching Pipeline of the Tianlai Cylinder Pathfinder Array.Research in Astronomy and Astrophysics,24(8), 085010

  63. [64]

    C., Wu, F

    Zhu, J. C., Wu, F. Q., Zhang, C., et al. 2021. 21cm Global Spectrum Measuring Instrument For Lunar- Orbit Satellite Array

  64. [65]

    J., de Lera Acedo, E., Wu, F

    Sun, S. J., de Lera Acedo, E., Wu, F. Q., et al. 2024. Calibration Error in 21-Centimeter Global Spectrum Experiment.Universe,10(6), 236

  65. [66]

    Q., Xu, S

    Xu, J. Q., Xu, S. Z., Zhang, C., et al. 2025. Progress in the Ground Testing for a Cosmic Dawn Global Spectrum Measurement System.URSI Radio Science Letters,7, 26

  66. [67]

    C., Xu, J

    Zhang, C., Zhu, J. C., Xu, J. Q., et al. 2025. Precision Calibration Techniques and Preliminary Observational Results of a High-Input-Impedance Receiver System for Global Spectrum Detection of the Cosmic Dawn.URSI Radio Science Letters,7, 23

  67. [68]

    B., Wu, F

    Suo, N. B., Wu, F. Q., He, K., et al. 2024. The electrical design of a membrane antenna for a lunar- based low-frequency radio telescope.Astronomical Techniques and Instruments,1(4), 227–238. Astronomical Techniques and Instruments,0(0), 0–1, 202517