Open AccessModified data on geoeffective solar flares and seismic noise variations
Author(s) -
Н. А. Сычева,
Л. М. Богомолов
Publication year - 2021
Publication title -
iop conference series. earth and environmental science
Language(s) - English
Resource type - Journals
eISSN - 1755-1307
pISSN - 1755-1315
DOI - 10.1088/1755-1315/929/1/012033
Subject(s) - induced seismicity , seismology , solar flare , geology , flare , noise (video) , swarm behaviour , geophysics , astrophysics , physics , mathematical optimization , mathematics , artificial intelligence , computer science , image (mathematics)
The problem of the relationship between strong magnetic swarms caused by solar flares and variations in seismicity is considered. The data on the temporal dependences of the parameters of seismic noise (average level, and standard deviation, RMS) recorded by the stations of the KNET seismic network have been used as the output data of monitoring the territory of the Bishkek geodynamic proving ground (Northern Tien Shan). The signatures of the influence of a magnetic swarm that occurred after an ultra-strong solar flare on September 6, 2017 have been established. The results obtained on the increase in seismic noise after this super-strong eruptive event are consistent with the results of studies on the influence of magnetic swarms on changes in regional seismicity.