The Diagnostic Potential of Transition Region Lines under-going Transient Ionization in Dynamic Events
J. G. Doyle, A. Giunta, A. Singh, M. S. Madjarska, H. Summers, B. J., Kellett, M. O'Mullane

TL;DR
This paper explores how transient ionization affects ultraviolet spectral lines during solar flares, demonstrating that it can significantly enhance certain emission lines and improve diagnostics of flare plasma conditions.
Contribution
It introduces a method to account for transient ionization effects in UV spectral diagnostics, enhancing the interpretation of solar flare observations.
Findings
Transient ionization can increase O V 1371A line emissivity by 2-4 times.
Line enhancement occurs rapidly, within the first fraction of a second.
The rise time and enhancement depend mainly on electron density.
Abstract
We discuss the diagnostic potential of high cadence ultraviolet spectral data when transient ionization is considered. For this we use high cadence UV spectra taken during the impulsive phase of a solar flares (observed with instruments on-board the Solar Maximum Mission) which showed excellent correspondence with hard X-ray pulses. The ionization fraction of the transition region ion O V and in particular the contribution function for the O V 1371A line are computed within the Atomic Data and Analysis Structure, which is a collection of fundamental and derived atomic data and codes which manipulate them. Due to transient ionization, the O V 1371A line is enhanced in the first fraction of a second with the peak in the line contribution function occurring initially at a higher electron temperature than in ionization equilibrium. The rise time and enhancement factor depend mostly on the…
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