Open AccessA 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.
Author(s) -
R. E. González-Narváez,
E. E. Díaz-Figueroa,
G. Ares de Parga
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1239/1/012002
Subject(s) - physics , astrophysics , corona (planetary geology) , plasma , coronal mass ejection , coronal hole , solar prominence , mixing (physics) , astronomy , mechanics , solar wind , astrobiology , quantum mechanics , venus , magnetic field
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.