Long term measurements from the M’atra Gravitational and Geophysical Laboratory. (arXiv:1811.05198v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Van_P/0/1/0/all/0/1">P. Ván</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barnafoldi_G/0/1/0/all/0/1">G. G. Barnaföldi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bulik_T/0/1/0/all/0/1">T. Bulik</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Biro_T/0/1/0/all/0/1">T. Biró</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Czellar_S/0/1/0/all/0/1">S. Czellár</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cieslar_M/0/1/0/all/0/1">M. Cieślar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Czanik_C/0/1/0/all/0/1">Cs. Czanik</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+David_E/0/1/0/all/0/1">E. Dávid</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Debreceni_E/0/1/0/all/0/1">E. Debreceni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Denys_M/0/1/0/all/0/1">M. Denys</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dobroka_M/0/1/0/all/0/1">M. Dobróka</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fenyvesi_E/0/1/0/all/0/1">E. Fenyvesi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gondek_Rosinska_D/0/1/0/all/0/1">D. Gondek-Rosińska</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Graczer_Z/0/1/0/all/0/1">Z. Gráczer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hamar_G/0/1/0/all/0/1">G. Hamar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huba_G/0/1/0/all/0/1">G. Huba</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kacskovics_B/0/1/0/all/0/1">B. Kacskovics</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kis_A/0/1/0/all/0/1">Á. Kis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kovacs_I/0/1/0/all/0/1">I. Kovács</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kovacs_R/0/1/0/all/0/1">R. Kovács</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lemperger_I/0/1/0/all/0/1">I. Lemperger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Levai_P/0/1/0/all/0/1">P. Lévai</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lokos_S/0/1/0/all/0/1">S. Lökös</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mlynarczyk_J/0/1/0/all/0/1">J. Mlynarczyk</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Molnar_J/0/1/0/all/0/1">J. Molnár</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Singh_N/0/1/0/all/0/1">N. Singh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Novak_A/0/1/0/all/0/1">A. Novák</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Olah_L/0/1/0/all/0/1">L. Oláh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Starecki_T/0/1/0/all/0/1">T. Starecki</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Suchenek_M/0/1/0/all/0/1">M. Suchenek</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Suranyi_G/0/1/0/all/0/1">G. Surányi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Szalai_S/0/1/0/all/0/1">S. Szalai</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tringali_M/0/1/0/all/0/1">M. C. Tringali</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Varga_D/0/1/0/all/0/1">D. Varga</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vasuth_M/0/1/0/all/0/1">M. Vasúth</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vasarhelyi_B/0/1/0/all/0/1">B. Vásárhelyi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wesztergom_V/0/1/0/all/0/1">V. Wesztergom</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Weber_Z/0/1/0/all/0/1">Z. Wéber</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zimboras_Z/0/1/0/all/0/1">Z. Zimborás</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Somlai_L/0/1/0/all/0/1">L. Somlai</a>
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 Gy”ongy”osoroszi, 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 nose ratio of the multi-messenger astrophysics era,
especially at the low frequency regime.
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 Gy”ongy”osoroszi, 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 nose ratio of the multi-messenger astrophysics era,
especially at the low frequency regime.
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