Characteristics of the three simulations and their main results.
|heating||source terms||model||(×103 km)||(s)|
|Equilibrium atmosphere||&||LTE (chromos.) & Λ (acc. flow)|
|atmosphere||(transition: ζ)||collisional radiative|
Notes. “W–Λ” corresponds to our reference case. Hmax: maximum extension reached by the post-shock medium; τcycle: cycle duration; “Window”: fixed rigid non-porous transparent interface; Λ: optically thin radiative cooling; : one solar luminosity enters the simulation box from the inner boundary; Modified Saha: Brown (1973).
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