Antenna orientations derived from the sinusoidal variation of Galactic noise with the Galactic Center's azimuth match GPS surveys within two standard deviations.
Shefali, PoS, ICRC2025 (these proceedings) 394
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Determining the orientation of radio antennas at the South Pole using Galactic noise measurements
Antenna orientations derived from the sinusoidal variation of Galactic noise with the Galactic Center's azimuth match GPS surveys within two standard deviations.