The South Pole's low seismic noise, existing infrastructure, and geographic position make it a strong candidate site for a long-baseline atom interferometer to detect decihertz gravitational waves and strengthen global triangulation.
Wave model depends on local site parameters such as ground density and wave speed which need to be measured locally
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Opportunities for Gravitational Wave Physics at the South Pole
The South Pole's low seismic noise, existing infrastructure, and geographic position make it a strong candidate site for a long-baseline atom interferometer to detect decihertz gravitational waves and strengthen global triangulation.