Abstract
In this paper, we study the propagation of jets with some characteristics of Type II spicules into the solar corona using a thermomechanical (TM) approximation. Embedding two plasmas with different densities (one representing the chromospheric plasma and the other the coronal plasma) in cylindrical sections, we use iterative processes to calculate the final temperatures due to the mixture between both plasmas. The resulting process dissipates heat that could represent a potential source of the solar corona’s high temperatures (106 K).
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