Non-equilibrium ionization by a periodic electron beam. I. Synthetic coronal spectra and implications for interpretation of observations
Elena Dzifcakova, Jaroslav Dudik, Simon Mackovjak

TL;DR
This study explores how a periodic high-energy electron beam affects synthetic coronal spectra, revealing persistent non-equilibrium ionization states and complex spectral behaviors that challenge traditional equilibrium-based interpretations.
Contribution
It introduces a model of periodic electron beams impacting coronal plasma, demonstrating non-equilibrium ionization effects and multithermal spectra in synthetic observations.
Findings
Spectra are almost always multithermal under periodic beams.
Ionization equilibrium assumptions often lead to misinterpretation of spectra.
Instantaneous spectra show rapid intensity changes in certain lines.
Abstract
Context. Coronal heating is currently thought to proceed via the mechanism of nanoflares, small-scale and possibly recurring heating events that release magnetic energy. Aims. We investigate the effects of a periodic high-energy electron beam on the synthetic spectra of coronal Fe ions. Methods. Initially, the coronal plasma is assumed to be Maxwellian with a temperature of 1 MK. The high-energy beam, described by a kappa-distribution, is then switched on every period for the duration of P/2. The periods are on the order of several tens of seconds, similar to exposure times or cadences of space-borne spectrometers. Ionization, recombination, and excitation rates for the respective distributions are used to calculate the resulting non-equilibrium ionization state of Fe and the instantaneous and period-averaged synthetic spectra. Results. Under the presence of the periodic electron…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
