Long term measurements from the Mátra Gravitational and Geophysical Laboratory
Abstract 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...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ván, P. [verfasserIn] Barnaföldi, G. G. [verfasserIn] Bulik, T. [verfasserIn] Biró, T. [verfasserIn] Czellár, S. [verfasserIn] Cieślar, M. [verfasserIn] Czanik, Cs. [verfasserIn] Dávid, E. [verfasserIn] Debreceni, E. [verfasserIn] Denys, M. [verfasserIn] Dobróka, M. [verfasserIn] Fenyvesi, E. [verfasserIn] Gondek-Rosińska, D. [verfasserIn] Gráczer, Z. [verfasserIn] Hamar, G. [verfasserIn] Huba, G. [verfasserIn] Kacskovics, B. [verfasserIn] Kis, Á. [verfasserIn] Kovács, I. [verfasserIn] Kovács, R. [verfasserIn] Lemperger, I. [verfasserIn] Lévai, P. [verfasserIn] Lökös, S. [verfasserIn] Mlynarczyk, J. [verfasserIn] Molnár, J. [verfasserIn] Singh, N. [verfasserIn] Novák, A. [verfasserIn] Oláh, L. [verfasserIn] Starecki, T. [verfasserIn] Suchenek, M. [verfasserIn] Surányi, G. [verfasserIn] Szalai, S. [verfasserIn] Tringali, M. C. [verfasserIn] Varga, D. [verfasserIn] Vasúth, M. [verfasserIn] Vásárhelyi, B. [verfasserIn] Wesztergom, V. [verfasserIn] Wéber, Z. [verfasserIn] Zimborás, Z. [verfasserIn] Somlai, L. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2019 |
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| Übergeordnetes Werk: |
Enthalten in: European physical journal special topics - Berlin : Springer, 2007, 228(2019), 8 vom: Sept., Seite 1693-1743 |
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| Übergeordnetes Werk: |
volume:228 ; year:2019 ; number:8 ; month:09 ; pages:1693-1743 |
| Links: |
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| DOI / URN: |
10.1140/epjst/e2019-900153-1 |
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| Katalog-ID: |
SPR02207760X |
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| 245 | 1 | 0 | |a Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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| 520 | |a Abstract 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 Gyöngyösoroszi, 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. | ||
| 700 | 1 | |a Barnaföldi, G. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bulik, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Biró, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Czellár, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Cieślar, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Czanik, Cs. |e verfasserin |4 aut | |
| 700 | 1 | |a Dávid, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Debreceni, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Denys, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Dobróka, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Fenyvesi, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Gondek-Rosińska, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Gráczer, Z. |e verfasserin |4 aut | |
| 700 | 1 | |a Hamar, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Huba, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Kacskovics, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Kis, Á. |e verfasserin |4 aut | |
| 700 | 1 | |a Kovács, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Kovács, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Lemperger, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Lévai, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Lökös, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Mlynarczyk, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Molnár, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Singh, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Novák, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Oláh, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Starecki, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Suchenek, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Surányi, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Szalai, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Tringali, M. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Varga, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasúth, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Vásárhelyi, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Wesztergom, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Wéber, Z. |e verfasserin |4 aut | |
| 700 | 1 | |a Zimborás, Z. |e verfasserin |4 aut | |
| 700 | 1 | |a Somlai, L. |e verfasserin |4 aut | |
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10.1140/epjst/e2019-900153-1 doi (DE-627)SPR02207760X (SPR)e2019-900153-1-e DE-627 ger DE-627 rakwb eng 530 ASE 31.00 bkl 33.00 bkl Ván, P. verfasserin aut Long term measurements from the Mátra Gravitational and Geophysical Laboratory 2019 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract 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 Gyöngyösoroszi, 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. Barnaföldi, G. G. verfasserin aut Bulik, T. verfasserin aut Biró, T. verfasserin aut Czellár, S. verfasserin aut Cieślar, M. verfasserin aut Czanik, Cs. verfasserin aut Dávid, E. verfasserin aut Debreceni, E. verfasserin aut Denys, M. verfasserin aut Dobróka, M. verfasserin aut Fenyvesi, E. verfasserin aut Gondek-Rosińska, D. verfasserin aut Gráczer, Z. verfasserin aut Hamar, G. verfasserin aut Huba, G. verfasserin aut Kacskovics, B. verfasserin aut Kis, Á. verfasserin aut Kovács, I. verfasserin aut Kovács, R. verfasserin aut Lemperger, I. verfasserin aut Lévai, P. verfasserin aut Lökös, S. verfasserin aut Mlynarczyk, J. verfasserin aut Molnár, J. verfasserin aut Singh, N. verfasserin aut Novák, A. verfasserin aut Oláh, L. verfasserin aut Starecki, T. verfasserin aut Suchenek, M. verfasserin aut Surányi, G. verfasserin aut Szalai, S. verfasserin aut Tringali, M. C. verfasserin aut Varga, D. verfasserin aut Vasúth, M. verfasserin aut Vásárhelyi, B. verfasserin aut Wesztergom, V. verfasserin aut Wéber, Z. verfasserin aut Zimborás, Z. verfasserin aut Somlai, L. verfasserin aut Enthalten in European physical journal special topics Berlin : Springer, 2007 228(2019), 8 vom: Sept., Seite 1693-1743 (DE-627)523571909 (DE-600)2267176-6 1951-6401 nnns volume:228 year:2019 number:8 month:09 pages:1693-1743 https://dx.doi.org/10.1140/epjst/e2019-900153-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 33.00 ASE AR 228 2019 8 09 1693-1743 |
| spelling |
10.1140/epjst/e2019-900153-1 doi (DE-627)SPR02207760X (SPR)e2019-900153-1-e DE-627 ger DE-627 rakwb eng 530 ASE 31.00 bkl 33.00 bkl Ván, P. verfasserin aut Long term measurements from the Mátra Gravitational and Geophysical Laboratory 2019 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract 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 Gyöngyösoroszi, 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. Barnaföldi, G. G. verfasserin aut Bulik, T. verfasserin aut Biró, T. verfasserin aut Czellár, S. verfasserin aut Cieślar, M. verfasserin aut Czanik, Cs. verfasserin aut Dávid, E. verfasserin aut Debreceni, E. verfasserin aut Denys, M. verfasserin aut Dobróka, M. verfasserin aut Fenyvesi, E. verfasserin aut Gondek-Rosińska, D. verfasserin aut Gráczer, Z. verfasserin aut Hamar, G. verfasserin aut Huba, G. verfasserin aut Kacskovics, B. verfasserin aut Kis, Á. verfasserin aut Kovács, I. verfasserin aut Kovács, R. verfasserin aut Lemperger, I. verfasserin aut Lévai, P. verfasserin aut Lökös, S. verfasserin aut Mlynarczyk, J. verfasserin aut Molnár, J. verfasserin aut Singh, N. verfasserin aut Novák, A. verfasserin aut Oláh, L. verfasserin aut Starecki, T. verfasserin aut Suchenek, M. verfasserin aut Surányi, G. verfasserin aut Szalai, S. verfasserin aut Tringali, M. C. verfasserin aut Varga, D. verfasserin aut Vasúth, M. verfasserin aut Vásárhelyi, B. verfasserin aut Wesztergom, V. verfasserin aut Wéber, Z. verfasserin aut Zimborás, Z. verfasserin aut Somlai, L. verfasserin aut Enthalten in European physical journal special topics Berlin : Springer, 2007 228(2019), 8 vom: Sept., Seite 1693-1743 (DE-627)523571909 (DE-600)2267176-6 1951-6401 nnns volume:228 year:2019 number:8 month:09 pages:1693-1743 https://dx.doi.org/10.1140/epjst/e2019-900153-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 33.00 ASE AR 228 2019 8 09 1693-1743 |
| allfields_unstemmed |
10.1140/epjst/e2019-900153-1 doi (DE-627)SPR02207760X (SPR)e2019-900153-1-e DE-627 ger DE-627 rakwb eng 530 ASE 31.00 bkl 33.00 bkl Ván, P. verfasserin aut Long term measurements from the Mátra Gravitational and Geophysical Laboratory 2019 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract 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 Gyöngyösoroszi, 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. Barnaföldi, G. G. verfasserin aut Bulik, T. verfasserin aut Biró, T. verfasserin aut Czellár, S. verfasserin aut Cieślar, M. verfasserin aut Czanik, Cs. verfasserin aut Dávid, E. verfasserin aut Debreceni, E. verfasserin aut Denys, M. verfasserin aut Dobróka, M. verfasserin aut Fenyvesi, E. verfasserin aut Gondek-Rosińska, D. verfasserin aut Gráczer, Z. verfasserin aut Hamar, G. verfasserin aut Huba, G. verfasserin aut Kacskovics, B. verfasserin aut Kis, Á. verfasserin aut Kovács, I. verfasserin aut Kovács, R. verfasserin aut Lemperger, I. verfasserin aut Lévai, P. verfasserin aut Lökös, S. verfasserin aut Mlynarczyk, J. verfasserin aut Molnár, J. verfasserin aut Singh, N. verfasserin aut Novák, A. verfasserin aut Oláh, L. verfasserin aut Starecki, T. verfasserin aut Suchenek, M. verfasserin aut Surányi, G. verfasserin aut Szalai, S. verfasserin aut Tringali, M. C. verfasserin aut Varga, D. verfasserin aut Vasúth, M. verfasserin aut Vásárhelyi, B. verfasserin aut Wesztergom, V. verfasserin aut Wéber, Z. verfasserin aut Zimborás, Z. verfasserin aut Somlai, L. verfasserin aut Enthalten in European physical journal special topics Berlin : Springer, 2007 228(2019), 8 vom: Sept., Seite 1693-1743 (DE-627)523571909 (DE-600)2267176-6 1951-6401 nnns volume:228 year:2019 number:8 month:09 pages:1693-1743 https://dx.doi.org/10.1140/epjst/e2019-900153-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 33.00 ASE AR 228 2019 8 09 1693-1743 |
| allfieldsGer |
10.1140/epjst/e2019-900153-1 doi (DE-627)SPR02207760X (SPR)e2019-900153-1-e DE-627 ger DE-627 rakwb eng 530 ASE 31.00 bkl 33.00 bkl Ván, P. verfasserin aut Long term measurements from the Mátra Gravitational and Geophysical Laboratory 2019 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract 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 Gyöngyösoroszi, 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. Barnaföldi, G. G. verfasserin aut Bulik, T. verfasserin aut Biró, T. verfasserin aut Czellár, S. verfasserin aut Cieślar, M. verfasserin aut Czanik, Cs. verfasserin aut Dávid, E. verfasserin aut Debreceni, E. verfasserin aut Denys, M. verfasserin aut Dobróka, M. verfasserin aut Fenyvesi, E. verfasserin aut Gondek-Rosińska, D. verfasserin aut Gráczer, Z. verfasserin aut Hamar, G. verfasserin aut Huba, G. verfasserin aut Kacskovics, B. verfasserin aut Kis, Á. verfasserin aut Kovács, I. verfasserin aut Kovács, R. verfasserin aut Lemperger, I. verfasserin aut Lévai, P. verfasserin aut Lökös, S. verfasserin aut Mlynarczyk, J. verfasserin aut Molnár, J. verfasserin aut Singh, N. verfasserin aut Novák, A. verfasserin aut Oláh, L. verfasserin aut Starecki, T. verfasserin aut Suchenek, M. verfasserin aut Surányi, G. verfasserin aut Szalai, S. verfasserin aut Tringali, M. C. verfasserin aut Varga, D. verfasserin aut Vasúth, M. verfasserin aut Vásárhelyi, B. verfasserin aut Wesztergom, V. verfasserin aut Wéber, Z. verfasserin aut Zimborás, Z. verfasserin aut Somlai, L. verfasserin aut Enthalten in European physical journal special topics Berlin : Springer, 2007 228(2019), 8 vom: Sept., Seite 1693-1743 (DE-627)523571909 (DE-600)2267176-6 1951-6401 nnns volume:228 year:2019 number:8 month:09 pages:1693-1743 https://dx.doi.org/10.1140/epjst/e2019-900153-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 33.00 ASE AR 228 2019 8 09 1693-1743 |
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Ván, P. @@aut@@ Barnaföldi, G. G. @@aut@@ Bulik, T. @@aut@@ Biró, T. @@aut@@ Czellár, S. @@aut@@ Cieślar, M. @@aut@@ Czanik, Cs. @@aut@@ Dávid, E. @@aut@@ Debreceni, E. @@aut@@ Denys, M. @@aut@@ Dobróka, M. @@aut@@ Fenyvesi, E. @@aut@@ Gondek-Rosińska, D. @@aut@@ Gráczer, Z. @@aut@@ Hamar, G. @@aut@@ Huba, G. @@aut@@ Kacskovics, B. @@aut@@ Kis, Á. @@aut@@ Kovács, I. @@aut@@ Kovács, R. @@aut@@ Lemperger, I. @@aut@@ Lévai, P. @@aut@@ Lökös, S. @@aut@@ Mlynarczyk, J. @@aut@@ Molnár, J. @@aut@@ Singh, N. @@aut@@ Novák, A. @@aut@@ Oláh, L. @@aut@@ Starecki, T. @@aut@@ Suchenek, M. @@aut@@ Surányi, G. @@aut@@ Szalai, S. @@aut@@ Tringali, M. C. @@aut@@ Varga, D. @@aut@@ Vasúth, M. @@aut@@ Vásárhelyi, B. @@aut@@ Wesztergom, V. @@aut@@ Wéber, Z. @@aut@@ Zimborás, Z. @@aut@@ Somlai, L. @@aut@@ |
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Ván, P. |
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Ván, P. ddc 530 bkl 31.00 bkl 33.00 Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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530 ASE 31.00 bkl 33.00 bkl Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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Ván, P. |
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Ván, P. Barnaföldi, G. G. Bulik, T. Biró, T. Czellár, S. Cieślar, M. Czanik, Cs. Dávid, E. Debreceni, E. Denys, M. Dobróka, M. Fenyvesi, E. Gondek-Rosińska, D. Gráczer, Z. Hamar, G. Huba, G. Kacskovics, B. Kis, Á. Kovács, I. Kovács, R. Lemperger, I. Lévai, P. Lökös, S. Mlynarczyk, J. Molnár, J. Singh, N. Novák, A. Oláh, L. Starecki, T. Suchenek, M. Surányi, G. Szalai, S. Tringali, M. C. Varga, D. Vasúth, M. Vásárhelyi, B. Wesztergom, V. Wéber, Z. Zimborás, Z. Somlai, L. |
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Ván, P. |
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long term measurements from the mátra gravitational and geophysical laboratory |
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Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
| abstract |
Abstract 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 Gyöngyösoroszi, 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. |
| abstractGer |
Abstract 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 Gyöngyösoroszi, 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. |
| abstract_unstemmed |
Abstract 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 Gyöngyösoroszi, 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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Long term measurements from the Mátra Gravitational and Geophysical Laboratory |
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https://dx.doi.org/10.1140/epjst/e2019-900153-1 |
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Barnaföldi, G. G. Bulik, T. Biró, T. Czellár, S. Cieślar, M. Czanik, Cs Dávid, E. Debreceni, E. Denys, M. Dobróka, M. Fenyvesi, E. Gondek-Rosińska, D. Gráczer, Z. Hamar, G. Huba, G. Kacskovics, B. Kis, Á. Kovács, I. Kovács, R. Lemperger, I. Lévai, P. Lökös, S. Mlynarczyk, J. Molnár, J. Singh, N. Novák, A. Oláh, L. Starecki, T. Suchenek, M. Surányi, G. Szalai, S. Tringali, M. C. Varga, D. Vasúth, M. Vásárhelyi, B. Wesztergom, V. Wéber, Z. Zimborás, Z. Somlai, L. |
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Barnaföldi, G. G. Bulik, T. Biró, T. Czellár, S. Cieślar, M. Czanik, Cs Dávid, E. Debreceni, E. Denys, M. Dobróka, M. Fenyvesi, E. Gondek-Rosińska, D. Gráczer, Z. Hamar, G. Huba, G. Kacskovics, B. Kis, Á. Kovács, I. Kovács, R. Lemperger, I. Lévai, P. Lökös, S. Mlynarczyk, J. Molnár, J. Singh, N. Novák, A. Oláh, L. Starecki, T. Suchenek, M. Surányi, G. Szalai, S. Tringali, M. C. Varga, D. Vasúth, M. Vásárhelyi, B. Wesztergom, V. Wéber, Z. Zimborás, Z. Somlai, L. |
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10.1140/epjst/e2019-900153-1 |
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2024-07-04T01:41:18.258Z |
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| score |
7.3998976 |