A Further Study of the Mixing of Relativistic Ideal Gases with Relative Relativistic Velocities: The Hot Plasma in the Sun’s Corona, the Type II Spicules and CMEs.

Abstract

Abstract The Redefined Relativistic Thermodynamics and the conservation of the 4-vector energy-momentum predict a tremendous increment of the temperature after mixing two gases with relative sub-relativistic velocity. This phenomenon can be used to describe the heating of a cold clump with shocked jets material and to predict an improving of the ignition in a Tokamak by injecting a plasma with a sub-relativistic velocity. First, by using the same effect, the mixing of the type II spicule and Coronal Mass Ejections with the plasma of a cold Sun’s corona will explain the increase temperature of the Sun’s corona. Second, considering, in agreement with the observations, that a part of the type II spicule, fall off into the Chromosphere and that the rest of the type II spicule that shocks with the Sun’s corona possesses a higher average relative velocity, the mixing of such a part and the plasma in the Sun’s corona will maintain the high temperature of the Sun’s corona. Moreover, the shock of Coronal Mass Ejections with the Sun’s corona it is a energy source to maintain the high temperature of the Sun’s corona too.