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JOURNALS // Meždunarodnyj naučno-issledovatel'skij žurnal // Archive

Meždunar. nauč.-issled. žurn., 2018 Issue 6-1(72), Pages 24–28 (Mi irj263)

PHYSICS AND MATHEMATICS

On the quasirelativistic equations for the solar corona plasma and a variant of rationale of its high temperature

Yu. V. Troshchiev

Lomonosov Moscow State University

Abstract: The quasi-relativistic equations are derived from nonrelativistic equations bringing amendments in them. They comprise of the continuity equations, and the conservation laws for impulses and energies both for protons and for electrons. It is so because the hydrodynamic and electric forces acting on them are similar, so, their impulses are also similar. The rife proton velocity in solar corona is $500$ km/s and the consistent electron velocity for such impulse is $0.953$ c, hence, the electrons must be taken into account and they are relativistic. Expressions for the collisional terms are also adapted to relativistic velocities. Heat emitting to warm protons due to friction between electron and proton flows is sufficient to heat plasma. Concentration $n_e$=$10^{10}$ cm$^{-3}$ and amount of scattering energy compensate large free path time.

Keywords: plasma, solar corona, relativistic effects.

DOI: 10.23670/IRJ.2018.72.6.03



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