Optimal placement of two stations in an isotropic Gaussian seismic field reduces equivalent seismic noise ASD by a factor of ~2.3 at 0.3 Hz versus a single station, producing oscillatory features from Bessel-function correlations.
Harms, Living Reviews in Relativity22, 6 (2019)
2 Pith papers cite this work. Polarity classification is still indexing.
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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.
citing papers explorer
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Seismic background mitigation with the Lunar Gravitational-wave Antenna
Optimal placement of two stations in an isotropic Gaussian seismic field reduces equivalent seismic noise ASD by a factor of ~2.3 at 0.3 Hz versus a single station, producing oscillatory features from Bessel-function correlations.
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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.