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Ionization equilibrium in soft X-ray-emitting solar flares (1974)

Phillips, K. J. H. ; Neupert, W. M. ; Thomas, R. J.

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Publication Date: 2011-08-16

Description: Studies of the 1.9-A line produced by highly ionized iron during a solar flare indicate that this emission occurs under conditions approaching a steady-state ionization equilibrium. Time-dependent and steady-state ionization equilibrium values are used for calculation of 1.9 A line fluxes per unit flare emission. The results are compared with those obtained by observations of some four solar flares, showing that the calculations from time-dependent equilibrium values approximate the observed line flux values with the same accuracy as the calculations from steady-state equilibrium values only when the electron densities are equal to or greater than 10 billion per cu cm.

Keywords: SPACE RADIATION

Type: Solar Physics; 36; June 197

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