Simulation data for the solar corona and the transition region of the equilibrium atmosphere background.
|Solar corona||Transition region|
|ΔT/Δy [K cm−1]||0||1.98 × 10−2|
|ρ0 [g cm−3]||10−16||10−11|
Notes. The quantity T0 is the temperature at the base domain, ΔT/Δy 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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