Magnetic Noise Mitigation Strategies for the Einstein Telescope Infrastructure
The Einstein Telescope (ET) will be a third-generation Gravitational Wave (GW) detector that will tackle cutting-edge technological challenges. The ET will be constructed at a depth of 200–300 m to isolate it from vibrations caused by seismic waves and human activities, which are sources of noise fo...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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MDPI AG
2025-01-01
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| Edice: | Galaxies |
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| On-line přístup: | https://www.mdpi.com/2075-4434/13/1/9 |
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