SUSCEPTIBILITY OF ELECTROMAGNETIC FIELDS IN THE SOLAR SYSTEM TO GRAVITATIONAL WAVE EFFECTS FROM RELATIVISTIC BINARY STAR SYSTEMS
Authors:
1.
Vladimir State University
2.
Eigenvector LLC
3.
Eigenvector LLC
Type:
Сonference abstract
Published:
27.12.2024
Subject area:
1.3.1
1.3.4
1.6.9
523-1/-8
52-423
52
53
520
521
523
524
52-1
52-6
37.00
41.19
41.00
29.35
29.31
29.33
29.27
29.05
03.03.03
03.05.01
03.06.01
223
2
6144
614
6135
SCI004000
SCI033000
SCI032000
SCI005000
1.3.4
1.6.9
523-1/-8
52-423
52
53
520
521
523
524
52-1
52-6
37.00
41.19
41.00
29.35
29.31
29.33
29.27
29.05
03.03.03
03.05.01
03.06.01
223
2
6144
614
6135
SCI004000
SCI033000
SCI032000
SCI005000
Language:
English
Keywords:
gravitation; gravitational waves; Earth; (stars:) binaries: general; relativistic processes; atmospheric effects; methods: statistical
Abstract (English):
Using an eigenvector and signal component analyzer (eigenoscope), the problem of identifying the impact of gravitational waves of relativistic binary star systems (RBSS) with large and small eccentricity on the vertical component of the electric field strength ($E_\text{z}$) in the Earth's atmospheric surface layer in the infra-low frequency (ILF) range at high harmonics of the EDS circulation frequencies has been solved. The results were obtained using monitoring data at four spatially separated $E_\text{z}$ observation stations. A model is proposed to explain the effect of the gravitational wave influence of relativistic binary star systems on the vertical component of the Earth's electric field strength in the surface layer of the atmosphere, previously discovered by the authors. The model considers as the mechanism the disturbance of the Earth's orbit by gravitational waves from relativistic binary star systems, leading to small displacements of the Earth relative to the free space charge in the troposphere. The estimates of the amplitude of the $E_\text{z}$ components, spectrally localized at the frequencies of gravitational waves of relativistic binary star systems, obtained on the basis of the presented model do not contradict the experimental results.
Using an eigenvector and signal component analyzer (eigenoscope), the problem of identifying the impact of gravitational waves of relativistic binary star systems (RBSS) with large and small eccentricity on the vertical component of the electric field strength ($E_\text{z}$) in the Earth's atmospheric surface layer in the infra-low frequency (ILF) range at high harmonics of the EDS circulation frequencies has been solved. The results were obtained using monitoring data at four spatially separated $E_\text{z}$ observation stations. A model is proposed to explain the effect of the gravitational wave influence of relativistic binary star systems on the vertical component of the Earth's electric field strength in the surface layer of the atmosphere, previously discovered by the authors. The model considers as the mechanism the disturbance of the Earth's orbit by gravitational waves from relativistic binary star systems, leading to small displacements of the Earth relative to the free space charge in the troposphere. The estimates of the amplitude of the $E_\text{z}$ components, spectrally localized at the frequencies of gravitational waves of relativistic binary star systems, obtained on the basis of the presented model do not contradict the experimental results.
Keywords:
gravitation; gravitational waves; Earth; (stars:) binaries: general; relativistic processes; atmospheric effects; methods: statistical
gravitation; gravitational waves; Earth; (stars:) binaries: general; relativistic processes; atmospheric effects; methods: statistical
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