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Radio Communication Attempts and Possible Signal Detections for the CUAVA-1 CubeSat

Presented by:

Iver Cairns

Iver H. Cairns

    University of Sydney and CUAVA

 

Guifre Morales Calves

    University of Tasmania

 

Xueliang Bai

    University of Sydney and CUAVA

 

Tony Monger

    University of Sydney and CUAVA

 

Patrick Oppel

    University of Sydney and CUAVA

 

Youngho Eun

    University of Sydney and CUAVA

 

Flynn Bryant

    University of Sydney and CUAVA

 

Oscar Ansted

    University of Sydney and CUAVA

 

James Unicomb

    Saber Astronautics

 

Alix Murdoch

    Saber Astronautics

 

Andreas Antoniades

    Saber Astronautics and CUAVA

 

Jason C. Held

    Saber Astronautics and CUAVA

 

Simon Ellingsen

    University of Tasmania

 

Joon Wayn Cheong

    University of New South Wales - Sydney, CUAVA, and ACSER


Andrew G. Dempster

    University of New South Wales - Sydney, CUAVA, and ACSER

The CUAVA-1 satellite was deployed into space on 6 October 2021. This paper summarises attempts to detect CUAVA-1’s radio beacons and other radio signatures. We attempted to detect CUAVA-1’s radio beacons near 437 MHz using ground stations at the universities of Sydney and New South Wales, at Saber Astronautics, and via the global amateur SatNOGS network. While some signals with the correct centre frequency, periodicity, and Doppler signatures were detected during one pass, they could not be decoded. Some other passes showed an occasional signal at the correct Doppler-shifted frequency. In contrast, beacons from other satellites (e.g., TauSat-1) were detected routinely. Direct transmission of commands on the uplink frequency also led to no observable results. Accordingly, the putative CUAVA-1 beacon signals are currently considered to be noise. We also observed CUAVA-1 using the University of Tasmania’s radio dishes in the frequency range 2.2 to 2.3 GHz, hoping for signals at harmonics of microprocessor clock or communication system frequencies. During one pass signals with the correct Doppler signature were observed at a center frequency of 2221.50 MHz, close to but 36 MHz away from the 5th harmonic of the downlink frequency. These signals have not been observed again and are currently interpreted in terms of either interference or another satellite. In summary, neither beacons or other radio signals are considered to have been detected from CUAVA-1 to date and the satellite is considered lost.

Category:

Space missions

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