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- W2963868504 abstract "The failure of the laser-interferometer gravitational wave antennas to measure the tiny changes of lengths many orders of magnitude smaller than the diameter of a proton raises the question of whether the reason for this failure is a large gravitational wave background noise, and if so, where this background noise is coming from. It is conjectured that it comes from gravitational waves emitted from a magnetohydrodynamic dynamo in the center of the sun, with the large magnetic field from this dynamo shielded by thermomagnetic currents in the tachocline. Using the moon as a large Weber bar, these gravitational waves could possibly be detected by the Poisson diffraction into the center of the lunar shadow during a total solar eclipse." @default.
- W2963868504 created "2019-07-30" @default.
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- W2963868504 date "2015-01-01" @default.
- W2963868504 modified "2023-09-27" @default.
- W2963868504 title "Emission of Gravitational Waves from a Magnetohydrodynamic Dynamo at the Center of the Sun" @default.
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