Energy balance in the solar transition region. I - Hydrostatic thermal models with ambipolar diffusion

1990 ◽  
Vol 355 ◽  
pp. 700 ◽  
Author(s):  
J. M. Fontenla ◽  
E. H. Avrett ◽  
R. Loeser
1999 ◽  
Vol 524 (2) ◽  
pp. 1105-1121 ◽  
Author(s):  
Hakeem M. Oluseyi ◽  
A. B. C. Walker II ◽  
Jason Porter ◽  
Richard B. Hoover ◽  
Troy W. Barbee, Jr.

1994 ◽  
Vol 144 ◽  
pp. 315-321 ◽  
Author(s):  
M. G. Rovira ◽  
J. M. Fontenla ◽  
J.-C. Vial ◽  
P. Gouttebroze

AbstractWe have improved previous model calculations of the prominence-corona transition region including the effect of the ambipolar diffusion in the statistical equilibrium and energy balance equations. We show its influence on the different parameters that characterize the resulting prominence theoretical structure. We take into account the effect of the partial frequency redistribution (PRD) in the line profiles and total intensities calculations.


2001 ◽  
Vol 378 (1) ◽  
pp. 257-265 ◽  
Author(s):  
C. Gontikakis ◽  
H. C. Dara ◽  
C. E. Alissandrakis ◽  
Th. G. Zachariadis ◽  
J.-C. Vial

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