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Table 1.

Simulation data for the solar corona and the transition region of the equilibrium atmosphere background.

Solar corona Transition region
T0 [K] 106 5000
ΔTy [K cm−1] 0 1.98 × 10−2
ρ0 [g cm−3] 10−16 10−11
H [Mm] 100 0.5

Notes. The quantity T0 is the temperature at the base domain, ΔTy is the temperature gradient (constant) in the gravity direction, ρ0 is the plasma density at the base domain, and H is the height domain. For both cases we take γ = 5/3 (specific heats ratio), g(y = 0) = 2.74 × 104 cm s−2 (gravitational acceleration at the base domain), R = 696 Mm (solar radius), R = 16.6289196 × 107 erg (K g)−1 (particular gas constant that results of considering a totally ionized hydrogen atmosphere).

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