Generation of low-frequency kinetic waves at the footpoints of pre-flare coronal loops
Kryshtal Alexandr, Voitsekhovska Anna, Cheremnykh Oleg, Ballai Istvan,, Verth Gary, Fedun Viktor

TL;DR
This paper investigates how low-frequency kinetic plasma waves can be generated at the footpoints of coronal loops in the pre-flare phase, using specific solar atmosphere models and plasma parameters, to predict flare onset.
Contribution
It demonstrates that the VAL (F) model supports low-frequency wave instability driven by sub-Dreicer electric fields and plasma inhomogeneities, advancing understanding of flare precursors.
Findings
Low-frequency wave instability occurs in the VAL (F) model.
Kinetic Alfven and ion-acoustic waves can be excited by sub-Dreicer electric fields.
Wave generation can happen with Coulomb conductivity or Bernstein turbulence.
Abstract
In this study we discuss the excitation of low frequency plasma waves in the lower-middle chromosphere region of loop footpoints for the case when the plasma can be considered in a pre-flare state. It is shown, that among the known semi-empirical models of the solar atmosphere, only the VAL (F) model together with a particular set of basic plasma parameters and amplitudes of the electric and magnetic fields supports generation of low frequency wave instability. Our results show that it is possible to predict the onset of the flare process in the active region by using the interaction of kinetic Alfven and kinetic ion-acoustic waves, which are solutions of the derived dispersion equation. The VAL (F) model allows situations when the main source of the aforementioned instability can be a sub-Dreicer electric field and drift plasma movements due to the presence of spatial inhomogeneities.…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
