Hot-cold plasma transition region: collisionless case
Marian Karlicky, Frantisek Karlicky

TL;DR
This study investigates the collisionless transition region between hot and cold plasma using 3D PIC simulations, revealing how electromagnetic interactions influence plasma fluxes, temperature distribution, and wave generation in solar atmospheric conditions.
Contribution
It provides new insights into collisionless plasma transition processes, highlighting the role of electromagnetic interactions in shaping plasma fluxes and temperature jumps.
Findings
Cold plasma flux dominates over hot plasma flux.
Electromagnetic interactions cause cold plasma to penetrate hot regions together with protons.
Plasma waves reduce electron escape, supporting temperature jumps.
Abstract
We study processes at the transition region between hot (rare) and cold (dense) plasma in the collisionless regime. We use a 3-dimensional electromagnetic particle-in-cell (3-D PIC) relativistic code. Motivated by the transition region in the solar atmosphere the temperature and density ratio of the plasmas is chosen as 100 and 0.01, respectively. For better understanding of studied processes we make two types of computations: a) without any interactions among plasma particles (free expansion) and b) with the full electromagnetic interactions. In both the cases we found that the flux of cold plasma electrons and protons from colder plasma to hotter one dominates over the flux of hot plasma electrons and protons in the opposite direction. Thus, the plasma in the hotter part of the system becomes colder and denser during time evolution. In the case without any interactions among particles…
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Taxonomy
TopicsLaser-induced spectroscopy and plasma · Dust and Plasma Wave Phenomena · Atomic and Molecular Physics
