Cosmological Plasma Filaments Instability and Universe Climate Systems (Published)
The language of differential geometry used to study instability of inhomogeneous plasma filaments by those techniques where the curve’s motion is fully described by Frenet torsion and curvature. The case studied is time depending frame changes according to free motions of charged particles. Longitudinal modes describing low-frequency waves in plasma in the medium are obtained by applying chaotic flows which describe cosmological perturbations to Magneto-Hydrodynamic (MHD) equations of inhomogeneous plasma.
Keywords: Alfven waves., Frenet frame, Inhomogeneous plasma, Instability