... time for sound wave to reach photosphere from h1 boundary !h1_bdy_omega !h1_bdy ... time for sound wave to reach photosphere from he4 boundary !he4_bdy_omega !he4_bdy ...
... sound time from center to outer cell boundary div time to photosphere !log_dr_div_cs ... star_age ! time_step ! properties at the photosphere ! Teff ! photosphere_L ! ...
... num_zones ! star_age ! time_step ! properties at the photosphere ! Teff ! photosphere_L ! photosphere_r ! ... properties at the photosphere ! Teff ! photosphere_L ! photosphere_r ! properties at the outermost zone of the model ! ...
... time for sound wave to reach photosphere from h1 boundary !h1_bdy_omega !h1_bdy ... time for sound wave to reach photosphere from he4 boundary !he4_bdy_omega !he4_bdy ...
... A comparison of the influence of the distant photosphere in Inverse Polarity and Normal Polarity prominence models . N.A.J. Schutgens . Astron. ...
... The integration started in the photosphere from point (T = 10 \Gamma4 , ae = 10 \Gamma9 ) with fitting of the apparent radius to the level Ь = 0:01, and was constructed using the dependence T (Ь) up to the onset of convection, 3 determined from the ...
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