Application of Spatio-Temporal Spectral Analysis for Detection of Seismic Waves in Gravitational-Wave Interferometer

被引:0
|
作者
Szymko, Robert [1 ]
Denys, Mateusz [2 ]
Bulik, Tomasz [3 ,4 ]
Idzkowski, Bartosz [4 ]
Kutynia, Adam [4 ]
Nikliborc, Krzysztof [4 ]
Suchinski, Maciej [4 ]
机构
[1] Univ Warsaw, Fac Phys, Pasteura 5, PL-02093 Warsaw, Poland
[2] Polish Acad Sci, Inst Phys, Lotnikow Ave 32-46, PL-02668 Warsaw, Poland
[3] Polish Acad Sci, Ctr Int Res Agenda, Nicolaus Copernicus Astron Ctr, AstroCeNT Particle Astrophys Sci & Technol, Rektorska 4, PL-00614 Warsaw, Poland
[4] Univ Warsaw, Astron Observ, Ujazdowskie Ave 4, PL-00478 Warsaw, Poland
来源
GALAXIES | 2021年 / 9卷 / 03期
关键词
virgo; seismicity; seismic sensor; fourier analysis; newtonian noise; spatio-temporal spectral analysis; NOISE;
D O I
10.3390/galaxies9030050
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Mixed spatio-temporal spectral analysis was applied for the detection of seismic waves passing through the west-end building of the Virgo interferometer. The method enables detection of a passing wave, including its frequency, length, direction, and amplitude. A thorough analysis aimed at improving sensitivity of the Virgo detector was made for the data gathered by 38 seismic sensors, in the two-week measurement period, from 24 January to 6 February 2018, and for frequency range 5-20 Hz. Two dominant seismic-wave frequencies were found: 5.5 Hz and 17.1 Hz. The presented method can be applied for a better understanding of the interferometer seismic environment, and by identifying noise sources, help the noise-hunting and mitigation work that eventually leads to interferometer noise suppression.
引用
收藏
页数:15
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