4.4 Review

Long term measurements from the Matra Gravitational and Geophysical Laboratory

期刊

EUROPEAN PHYSICAL JOURNAL-SPECIAL TOPICS
卷 228, 期 8, 页码 1693-1743

出版社

SPRINGER HEIDELBERG
DOI: 10.1140/epjst/e2019-900153-1

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资金

  1. MTA EUHUNKP grant
  2. Hungarian National Research, Development and Innovation Office NKFIH [K124366, K104260, K116197, K120660, NK106119, K116375, KH130378]
  3. NCN [UMO-2013/01/ASPERA/ST9/00001]
  4. Momentum (Lendulet) grant of the Hungarian Academy of Sciences [LP2013-60]
  5. PHAROS COST Action [CA16214]
  6. G2net COST Action [CA17137]
  7. Foundation for Polish Science [TEAM/2016-3/19]
  8. European Regional Development Fund
  9. Nitrokemia Zrt.
  10. [GINOP-2.2.1-15-2016-00012]

向作者/读者索取更多资源

The Summary of the long term data taking, related to one of the proposed next generation ground-based gravitational detector's location is presented here. Results of seismic and infrasound noise, electromagnetic attenuation and cosmic muon radiation measurements are reported in the underground Matra Gravitational and Geophysical Laboratory near Gyongyosoroszi, Hungary. The collected seismic data of more than two years is evaluated from the point of view of the Einstein Telescope, a proposed third generation underground gravitational wave observatory. Applying our results for the site selection will significantly improve the signal to noise ratio of the multi-messenger astrophysics era, especially at the low frequency regime.

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